Front entrance of the school

SN 2005E (aka 2005-1032) is a supernova first observed in January 2005 that scientists conclude is a new type of cosmic explosion. The explosion originated in the galaxy NGC 1032, approximately 100 million light years away.Location: RA 02° 39' 14.34" Dec+01hr 05' 55.0" [Epoch J2000]

Approx. 850

SN Goenka

Type II/Ib

SN 1979C was a supernova about 50 million light-years away in Messier 100, a spiral galaxy in the constellation Coma Berenices. The Type II supernova was discovered April 19, 1979 by Gus Johnson, a school teacher and amateur astronomer. This type of supernova is known as a core collapse and is the result of the internal collapse and violent explosion of a large star. A star must have at least 9 times the mass of the Sun in order to undergo this type of collapse.

SMS Roon

SMS Tb 98 M

SMS V25 was a V25-class torpedo boat of the Imperial German Navy that served during the First World War. The ship was built by AG Vulcan at Stettin in Prussia (now Szczecin in Poland), and was completed in June 1914. The ship was sunk by a British mine on 13 February 1915.

SN 2002cx

SO-239

title

First supernova detected by the X-rays released very early on in its formation.

SN Medical College

SNoW (Japanese singer)

In mathematics, SO(5), also denoted SO5(R) or SO(5,R), is the special orthogonal group of degree 5 over the field R of real numbers, i.e. (isomorphic to) the group of orthogonal 5×5 matrices of determinant 1.

SN 2006X was a Type Ia supernova about 65 million light-years away in Messier 100, a spiral galaxy in the constellation Coma Berenices. The supernova was independently discovered in early February 2006 by Shoji Suzuki of Japan and Marco Migliardi of Italy.SN 2006X is particularly significant because it is a Type Ia supernova. These supernovae are used for measuring distances, so observations of these supernovae in nearby galaxies are needed for calibration.

* surfaced
* submerged

* at surfaced
* at submerged

SN 2003H

First observed between August 4 and August 6, 1181, Chinese and Japanese astronomers recorded the supernova now known as SN 1181 in eight separate texts. One of only eight supernovae in the Milky Way observable with the naked eye in recorded history, it appeared in the constellation Cassiopeia and was visible in the night sky for about 185 days.The radio and X-ray pulsar J0205+6449 (also known as 3C 58), which rotates about 15 times per second, is possibly the remnant from this event. If the supernova and pulsar are associated, the star is still rotating about as quickly as it did when it first formed. This is in contrast to the Crab pulsar, known to be the remnant of the SN 1054 supernova in the year 1054, which has lost two-thirds of its rotational energy in essentially the same time span. Recent radio surveys of 3C 58, however, indicate that this supernova remnant may be much older and thus not associated with SN 1181.

yes

*1921: Teodo
*1924: Barbana
*1926: Barbana G
*1940: Empire Airman

SN 1961i was a supernova that was discovered in June 1961 in the Messier 61 (NGC 4303) galaxy, by Milton L. Humason at the Palomar Observatory, the brightest of 16 supernovae found at Palomar that year. Although it was originally consider by Fritz Zwicky to be the prototype of a type III supernova, subsequent researchers have classified it as a type II supernova.

Pendekar, Pahlawan, Panglima dan Perwira

SMS Victoria Louise was the lead ship of her class of protected cruisers, built for the German Imperial Navy (Kaiserliche Marine) in the late 1890s. She was laid down at the AG Weser shipyard in 1895, launched in March 1897, and commissioned into the German fleet in February 1899. She was named after Princess Victoria Louise, the daughter of Kaiser Wilhelm II.

SN 2003gd was a type II-P supernova occurring in the spiral galaxy Messier 74 in the constellation Pisces. SN 2003gd was discovered on 12 June 2003 by Robert Evans, using a 0.31m reflector, and its discovery was confirmed on 13 June 2003 by R. H. McNaught using the 1.0m telescope at the Siding Spring Observatory.

scout cruiser

SN 2005ap

*5 × torpedo tubes
*10 torpedoes
*1 × deck gun

first supernova in

This gene encodes a member of the sorting nexin family. Members of this family contain a phox domain, which is a phosphoinositide binding domain, and are involved in intracellular trafficking. This protein does not contain a coiled coil region, like some family members, but does contain an SH3 domain near its N-terminus. This protein interacts with the cytoplasmic domains of the precursor but not the processed forms of a disintegrin and metalloprotease domain 9 and 15. This protein binds the beta-appendage domain of adaptor protein 2 and may function to assist adaptor protein 2 in its role at the plasma membrane. This protein interacts with activated Cdc42-associated kinase-2 to regulate the degradation of epidermal growth factor receptor protein.

Record-breaking supernova SN UDS10Wil in the CANDELS Ultra Deep Survey

SN 1895B

NGC 4490

Hypergiant in NGC 1260 Galaxy

Sekolah Menengah Sains Sabah

SN 2010lt is a supernova located in the galaxy UGC 3378 in Camelopardalis. It was discovered by amateur astronomers Kathryn Aurora Gray, her father Paul Gray, of Fredericton, New Brunswick, Canada and David J. Lane of Stillwater Lake, Nova Scotia, Canada. Upon discovery, Kathryn Aurora Gray became the youngest person to ever discover a supernova, being 10 years old when she did so. The previous record was held by the 14-year-old Caroline Moore.

SN 1990U was a type Ic supernova event in the nucleus of the galaxy NGC 7479. It was discovered July 27, 1990 by the Berkeley Automated Supernova Search after reaching magnitude 7001160000000000000♠16±0.5. Initially this was classified as a Type Ib supernova, but the weakness of the neutral helium absorption lines led to a reclassification.

*Owner operated except:-
*Mark Whitwill & Son Ltd, Bristol

*Four
*ten
*fourteen
*four torpedo tubes

Al-Razi, Bandura, Chopin, Da Vinci, Einstein, Frost, Galileo

This gene encodes a member of the sorting nexin family. Members of this family contain a phox domain, which is a phosphoinositide binding domain, and are involved in intracellular trafficking. This protein associated with the long isoform of the leptin receptor and with receptor tyrosine kinases for platelet-derived growth factor, insulin, and epidermal growth factor in cell cultures, but its function is unknown. This protein may form oligomeric complexes with family members.

SLNS-R or SLNS-II ?

SNÉTA

SN Brussels Airlines (SNBA) was a national airline of Belgium, which mainly operated from Brussels Airport. SNBA was the trading name of the Belgian airline Delta Air Transport. SNBA was a full-service airline, connecting Brussels with the rest of Europe. It also flew to Africa, continuing Sabena's extensive network there.

Tun Fuad Stephens

SMS Wien

Building 117

SN 2002bj was the explosion of a star in the galaxy NGC 1821, located in the constellation Lepus. The explosion was discovered by Jack Newton in scans of images produced by Tim Puckett. (It was independently discovered by the Lick/Tenagra Observatory as part of their combined supernova search program.) Initially it had an apparent magnitude of about 14.7 and was categorized as a Type IIn supernova. However, in 2008 Dovi Poznanski discovered that the spectrum more closely resembled a Type Ia supernova. Further, the energy output was much lower than a typical supernova and the luminosity dropped at a dramatic pace.A team consisting of Poznanski, Joshua Bloom, Alex Filippenko and others concluded that it was a new category of exploding star. This system is believed to consist of a binary pair of white dwarf stars, with helium being transferred from one dwarf to the other. The accreted helium exploded in a thermonuclear reaction on the surface of the more massive white dwarf, resulting in the observed outburst. In this sense, it was akin to a nova explosion, although the magnitude of the explosion was a thousand times greater. In 2007 Lars Bildsten et al. had predicted this category of explosion would occur in AM Canum Venaticorum-type binary systems.NGC 1821 is an irregular galaxy categorized as type IB(s)m. It is apparent magnitude 14.5 and has a redshift of 0.012029. This galaxy is located about 48 megaparsecs from the Earth.

SN 1994I is a Type Ic supernova discovered on April 2, 1994 in the Whirlpool Galaxy by amateur astronomers Tim Puckett and Jerry Armstrong of the Atlanta Astronomy Club. Type Ic supernova are a rare type of supernova that result from the explosion of a very massive star that has shed its outer layers of hydrogen and helium. The explosion results in a highly luminous burst of radiation that then dims over the course of weeks or months.

SN 2008D

SNX 111

SN 2005B, the second supernova discovered in 2005, was discovered by amateur astronomer Paul Gray, of Fredericton, New Brunswick, Canada, upon reviewing film shot by fellow amateur astronomer David J. Lane, at his backyard observatory in Stillwater Lake, Nova Scotia, Canada. It was located in the galaxy UGC 11066 in Draco.

SN 2003H was a supernova that appeared halfway between the colliding NGC 2207 and IC 2163 galaxies. It was discovered January 8, 2003, by the Lick Observatory and Tenagra Supernova Searches (LOTOSS).

SO(10) grand unification

The SN postcode area, also known as the Swindon postcode area, is a group of eighteen postcode districts in England, which are subdivisions of ten post towns. These postcode districts cover north Wiltshire, including Swindon, Chippenham, Calne, Corsham, Devizes, Malmesbury, Marlborough, Melksham and Pewsey, plus a small part of south-west Oxfordshire, including Faringdon, and a very small part of Gloucestershire.

SASILA

Pilin, 73000

SNCASE SE.535

N/A

SNi substitution

SN 1992bd

Hj. Zaini Zair

Budi Usaha Bakti

SN Brussels destinations

SO(1,N)

IIn

SN 2003gd

SN 2004GT was a type Ic supernova that happened in the interacting galaxy NGC 4038 on December 12, 2004. The event occurred in a region of condensed matter in the western spiral arm. The progenitor was not identified from older images of the galaxy, and is either a type WC Wolf-Rayet star with a mass over 40 times that of the Sun, or a star 20 to 40 times as massive as the Sun in a binary star system.

SNIC

SN Lakshmi

Countess Kielmannsegg

SN Brussels Airlines

SN 2006X

SMS Tiger

SMS V25

as built
SMS Siegfried was the lead ship of the six-member Siegfried class of coastal defense ships (Küstenpanzerschiffe) built for the German Imperial Navy. Her sister ships were Beowulf, Frithjof, Heimdall, Hildebrand, and Hagen. Siegfried was built by the Germaniawerft shipyard between 1888 and 1890, and was armed with a main battery of three 24-centimeter (9.4 in) guns. She served in the German fleet throughout the 1890s and was rebuilt in 1903 - 1904.

SN 2005B

S-TAIL

SN Trust

SN 2006gy was an extremely energetic supernova, sometimes referred to as a hypernova or quark-nova, that was discovered on September 18, 2006. It was first observed by Robert Quimby and P. Mondol, and then studied by several teams of astronomers using facilities that included the Chandra, Lick, and Keck Observatories. In May 2007 NASA and several of the astronomers announced the first detailed analyses of the supernova, describing it as the "brightest stellar explosion ever recorded". In October 2007 Quimby announced that SN 2005ap had broken SN 2006gy's record as the brightest ever recorded supernova, and several subsequent discoveries are brighter still. Time magazine listed the discovery of SN 2006gy as third in its Top 10 Scientific Discoveries for 2007.

SN 2003B was a type II supernova that happened in NGC 1097 on January 5, 2003.

Tun Ahmad Raffae

Shell

*1940: Empire Airman

SMS Szent Istvan

unknown

SN UDS10Wil

SN 1998bw

SN 2010lt

Business Centre

SN 2006gy was an extremely energetic supernova, sometimes referred to as a hypernova or quark-nova, that was discovered on September 18, 2006. It was first observed by Robert Quimby and P. Mondol, and then studied by several teams of astronomers using facilities that included the Chandra, Lick, and Keck Observatories. In May 2007 NASA and several of the astronomers announced the first detailed analyses of the supernova, describing it as the "brightest stellar explosion ever recorded".

to be included end 2014

Boarding school, Sekolah Berasrama Penuh, Mixed-gender education

SN 2011by

SMS Roon was the lead ship of her class of armored cruisers of the Imperial German Navy. The ship was authorized under the second Naval Law in 1902, and built at the Imperial Dockyard in Kiel at the cost of 15.3 million marks. The ship was named after Albrecht von Roon, a Prussian general and politician. She displaced up to 9,875 metric tons (9,719 long tons; 10,885 short tons) and was armed with a main battery of four 21 cm (8.3 in) guns.

SO(N)

HC 4039

SM Delgado is a department store owned by SM Land Inc. and operated by Metro Manila Shopping Mecca Corporation, the same arm of the SM Group that operate the branches at SM City Manila and SM City Santa Rosa. It is located within Iloilo City's commercial district along Delgado and Valeria Streets. It opened in May 1979 and was relaunched in the year 2004. It is the 4th SM Department Store built by Henry Sy Sr. and the first branch opened outside Metro Manila. SM Supermarket was conceptualized and opened its store at SM Delgado in 1985. The mall was relaunched in 2004.

SN 393

SN Power AS

SMS Rembau

SN 2005g1

SN 2005E

SNe Ia

Stuttgart

SN 2005gl was a supernova in the barred-spiral galaxy NGC 266. It was discovered using CCD frames taken October 5, 2005, from the 60 cm automated telescope at the Puckett Observatory in Georgia, US, and reported by Tim Puckett in collaboration with Peter Ceravolo. It was independently identified by Yasuo Sano in Japan. The supernova was located 29.8″ east and 16.7″ north of the galactic core. Based upon its spectrum, this was classified as a Type IIn core-collapse supernova.

NGC 1097 for 21st century

Z of 0.024

SN 2007bi

*3× water-tube boilers
*2× steam turbines
*

SN 2003fg, sometimes called the "Champagne Supernova", was an unusual Type Ia supernova. It was discovered in 2003 with the Canada-France-Hawaii Telescope and the Keck Telescope, both on Mauna Kea in Hawaii, and announced by researchers at the University of Toronto. The supernova occurred in a galaxy some 4 billion light-years from Earth. It was nicknamed after the 1996 song "Champagne Supernova" by English rock band Oasis.It was unusual because of the mass of its progenitor.

*1921: Italian Government, Ministry of Transport
*1924: Ministry of Marine, Italy
*1926: Società Anonima di Navigazione Garibaldi, Genoa
*1940: Ministry of War Transport

Approximate location of the sinking of Empire Airman.

SMSS

SN Srivastava

SN 393 is the modern designation for a probable supernova that was reported by the Chinese in the year 393 CE.

First observed between August 4 and August 6, 1181, Chinese and Japanese astronomers recorded the supernova now known as SN 1181 in eight separate texts. One of only eight supernovae in the Milky Way observable with the naked eye in recorded history, it appeared in the constellation Cassiopeia and was visible in the night sky for about 185 days.The radio and X-ray pulsar J0205+6449 (also known as 3C 58), which rotates about 15 times per second, is possibly the remnant from this event.

SO(10) (physics)

SM Unterseeboot U31

Sekolah Menengah Sains Rembau (English: Rembau Science Secondary School) or SEMESRA is a co-educational secondary school situated in the district of Rembau and among fully residential schools (Sekolah Berasrama Penuh) in the state of Negeri Sembilan, Malaysia. Established in 2009, the school is widely known as SEMESRA.In the recent PMR examination (2013), the school managed to produce 108 straight A's students with GPS 1.0535 to become the third best school in Negeri Sembilan.On 30 October 2014, SEMESRA was awarded with the Sekolah Berprestasi Tinggi or High Performance School title, a title awarded to schools in Malaysia that have met stringent criteria including academic achievement, strength of alumni, international recognition, network and linkages.

April/May 386

SN 1994I is a Type Ic supernova discovered on April 2, 1994 in the Whirlpool Galaxy by amateur astronomers Tim Puckett and Jerry Armstrong of the Atlanta Astronomy Club. Type Ic supernova are a rare type of supernova that result from the explosion of a very massive star that has shed its outer layers of hydrogen and helium. The explosion results in a highly luminous burst of radiation that then dims over the course of weeks or months. SN 1994I was a relatively nearby supernova, and provided an important addition to the then small collection of known Type Ic supernova. Very early images were captured of SN 1994I, as two high school students in Oil City, Pennsylvania serendipitously took images of the Whirlpool Galaxy using the 30-inch telescope at Leuschner Observatory on March 31, 1994, which included SN 1994I just after it began to brighten.

Form 1 - Form 5
Tekun Bersatu Berjaya Terbilang

SN 1994I

Animation of light echoes from SN1987A

SN 1986G was a supernova that was observed on May 3, 1986 by Robert Evans. Its host galaxy, Centaurus A, is about 15 million light-years away in the constellation Centaurus. Since Centaurus A is about 15 million light-years away from us, this supernova happened 15 million years ago.SN 1986G was a bright blue-green star in the middle of the left part of the dust belt of Centaurus A.

Lela Maharaja

SMS Siegfried

SN survey

SNY (TV network)

SN 2004gt

Gerhard von Scharnhorst

SO(3)

The Wěi asterism appears in the lower half of the Scorpius constellation

SMS Teodo

SMS Tegetthoff was an Austro-Hungarian dreadnought battleship of the Tegetthoff class named after Wilhelm von Tegetthoff, a 19th-century Austrian admiral most notable for defeating the Italian Navy in the Battle of Lissa.Tegetthoff was built at the Stabilimento Tecnico Triestino yard in Trieste as part of the first and only class of dreadnought battleships in the Austro-Hungarian Navy.

White dwarf

SN 1993J is a supernova observed in the galaxy M81. It was discovered on 28 March 1993 by F. Garcia in Spain. At the time, it was the second brightest type II supernova observed in the twentieth century behind SN 1987A.The spectral characteristics of the supernova changed over time. Initially, it looked more like a type II supernova (a supernova formed by the explosion of a giant star) with strong hydrogen spectral line emission, but later the hydrogen lines faded and strong helium spectral lines appeared, making the supernova look more like a type Ib. Moreover, the variations in SN 1993J's luminosity over time were not like the variations observed in other type II supernovae but did resemble the variations observed in type Ib supernovae. Hence, the supernova has been classified as a type IIb, an intermediate class between type II and type Ib. The scientific results from this supernova suggested that type Ib and Ic supernovae were actually formed through the explosions of giant stars through processes similar to what takes place in type II supernovae. The supernova was also used to estimate a distance of 8.5 ± 1.3 Mly (2.6 ± 0.4 Mpc) to Messier 81.Light echoes from the explosion have subsequently been detected. The progenitor of SN 1993J was identified in pre-explosion ground-based images. The progenitor was observed to be a K-supergiant star, with an excess in the ultraviolet possibly due to surrounding hot stars or a hot binary companion. While the supernova is located in a region populated by young massive stars, late-time photometry with the Hubble Space Telescope and spectroscopy with the Keck 10m-telescope presented by Maund and collaborators revealed the presence of the long suspected B-supergiant companion star.

SN machine gun

* in belt
* in turret faces
* – in deck

Hulked, 1916

SN 1

SN 2003fg

Scrapped, 1923

*1926: Barbana G

SN 2004GT

Unknown

Surrendered to Britain, 1920, scrapped

SN UDS10Wil (SN Wilson) is a type Ia supernova, and as of April 2013, the farthest known. It has a redshift of 1.914, which strongly implies that it exploded when the universe was about a third of its current size. It was discovered with the Hubble Space Telescope's Wide Field Camera 3.

SN 2007UY

SM Unterseeboot U3

SN Brussels Airlines (SNBA) was a national airline of Belgium, which mainly operated from Brussels Airport. SNBA was the trading name of the Belgian airline Delta Air Transport. SNBA was a full-service airline, connecting Brussels with the rest of Europe. It also flew to Africa, continuing Sabena's extensive network there. The airline merged with Virgin Express into Brussels Airlines which started operations on 25 March 2007 The airline had its head office in Airport Building 117 in Brussels Airport, Zaventem, near Brussels.

SM Delgado

*Interned at Scapa Flow 22 November 1918

Sekolah Menengah Sains Sabah or (SMESH), is a prominent cluster boarding school in East Malaysia established since 1978 but fully operational on 1 January 1984. Previously known as Sekolah Berasrama Penuh Sabah (SBPS), it was the pioneer of boarding school project in Sabah and Sarawak and was built on 16-acre (65,000 m2) land near Sabah Golf and Country Club. The school is graded as A -- cluster type school and ranked as No.1 School in Sabah by the Ministry of Education, while school's administrator benefits number of autonomy powers from the status.In May 2011, Deputy Prime Minister cum Minister of Education announced SM Sains Sabah is enlisted as Nation's High Performance School (Sekolah Berprestasi Tinggi) status. SBT status allocates additional autonomy powers to pursue innovation in school management and raise the productivity of students. The benefits include fixing the minimum periods for subject, extending schooling hours and allowing students to complete their studies a year earlier. A lump sum grant would be channelled to the schools at the beginning of each year and that they would have the full flexibility to spend as needed and were exempted from the ministry’s centralised procurement system. In the recent PMR examination (2013), the school managed to produce 70 straight A's student out of 130 students with GPS 1.12 to become the second best school in Sabah. In 2014, the school ranked No.2 in the country and No.1 in Sabah based on SPM 2013 results.
Sekolah Menengah Sains Sabah or (SMESH), is a prominent cluster boarding school in East Malaysia established since 1978 but fully operational on 1 January 1984. Previously known as Sekolah Berasrama Penuh Sabah (SBPS), it was the pioneer of boarding school project in Sabah and Sarawak and was built on 16-acre (65,000 m2) land near Sabah Golf and Country Club.

UB-125

Kampus Lama IPG Kent, Jalan Bolong

SMS Wien ("His Majesty's Ship Vienna") was one of three Monarch-class coastal defense ships built for the Austro-Hungarian Navy in the 1890s. After her commissioning, the ship participated in an international blockade of Crete during the Greco-Turkish War of 1897. Wien and the two other Monarch-class ships made several training cruises in the Mediterranean Sea in the early 1900s. They formed the 1st Capital Ship Division of the Austro-Hungarian Navy until they were replaced by the newly commissioned Habsburg-class predreadnought battleships at the turn of the century. In 1906 the three Monarchs were placed in reserve and only recommissioned for annual summer training exercises. After the start of World War I, Wien was recommissioned and assigned to 5th Division together with her sisters.The division was sent to Cattaro in August 1914 to attack Montenegrin and French artillery that was bombarding the port and they remained there until mid-1917. Wien and her sister Budapest were sent to Trieste in August 1917 and bombarded Italian fortifications in the Gulf of Trieste. On the night of 9–10 December, while Wien and Budapest were at anchor in Trieste, two Italian torpedo boats managed to penetrate the harbor defenses undetected and fired several torpedoes at the two ships. Budapest was not hit, but Wien was struck by two torpedoes and sank in less than five minutes with the loss of 46 of her crew. The wreck was salvaged sometime during the 1920s by the Italians.

SMS Siegfried was the lead ship of the six-member Siegfried class of coastal defense ships (Küstenpanzerschiffe) built for the German Imperial Navy. Her sister ships were Beowulf, Frithjof, Heimdall, Hildebrand, and Hagen. Siegfried was built by the Germaniawerft shipyard between 1888 and 1890, and was armed with a main battery of three 24-centimeter (9.4 in) guns. She served in the German fleet throughout the 1890s and was rebuilt in 1903 - 1904. She served in the VI Battle Squadron after the outbreak of World War I in August 1914, but saw no action. Siegfried was demobilized in 1915 and used as a barracks ship thereafter. She was ultimately broken up for scrap in 1920.

SN 2008ha

Roon

*2 shafts
*2 Melms-Pfenniger steam turbines
*16 Yarrow water-tube boilers

SN 2008ax

SN Ic

SNX26

SN 2008D is a supernova detected with NASA's Swift X-ray telescope. The explosion of the supernova precursor star, in the spiral galaxy NGC 2770 (88 million light years away (27 Mpc), was detected on January 9, 2008, by Carnegie-Princeton fellows Alicia Soderberg and Edo Berger, and Albert Kong and Tom Maccarone independently using Swift. They alerted eight other orbiting and ground-based observatories to record the event. This was the first time that astronomers have ever observed a supernova as it occurred.The supernova was determined to be of Type Ibc. The velocities measured from SN2008D indicated expansion rates of more than 10,000 kilometers per second. The explosion was off-center, with gas on one side of the explosion moving outward faster than on the other. This was the first time the X-ray emission pattern of a supernova (which only lasted about five minutes) was captured at the moment of its birth. Now that it is known what X-ray pattern to look for, the next generation of X-ray satellites is expected to find hundreds of supernovae every year exactly when they explode, which will allow searches for neutrino and gravitational wave bursts that are predicted to accompany the collapse of stellar cores and the birth of neutron stars.

Sunk, 10 December 1917, salvaged and scrapped 1920s

SNY

* 8 × guns
* 6 × guns
* 18 × guns
* 4 × torpedo tubes

SN 1000+0216 was an extremely remote superluminous supernova (SLSN), which occurred in between June and November 2006. Its peak far-ultraviolet absolute magnitude reached −21.5, which exceeded the total absolute magnitude of its host galaxy. The distance (redshift) to this supernova z=3.8993 ± 0.0074 makes it the most distant supernova observed as of 2012. The luminosity of SN 1000+0216 evolved slowly over several years as it was still detectable in November 2008. Both the high luminosity and slow decay indicate that the supernova's progenitor was a very massive star. The supernova explosion itself was likely either a pair-instability supernova or a pulsational pair-instability supernova similar to the SN 2007bi or event. It also had some similarities to the low redshift SN 2006gy supernova. Overall classification of SN 1000+0216 remains uncertain.

Scharnhorst

SM Delgado is a department store owned by SM Land Inc. and operated by Metro Manila Shopping Mecca Corporation, the same arm of the SM Group that operate the branches at SM City Manila and SM City Santa Rosa. It is located within Iloilo City's commercial district along Delgado and Valeria Streets. It opened in May 1979 and was relaunched in the year 2004. It is the 4th SM Department Store built by Henry Sy Sr. and the first branch opened outside Metro Manila.

Super Chandrasekhar

Lacroma, 1906

* 18 water-tube boilers
*

SN 1940B was a supernova discovered on 5 May 1940 in the galaxy NGC 4725 in Coma Berenices. It had a magnitude of 12.8 and became the first observed type II supernova.SN 1940B is one of the five supernovae discovered in 1940, the other being SN 1940A, SN 1940C, SN 1940D and SN 1940E.

SNePS is a knowledge representation, reasoning, and acting (KRRA) system developed and maintained by Stuart C. Shapiro and colleagues at the State University of New York at Buffalo.SNePS is simultaneously a logic-based, frame-based, and network-based KRRA system. It uses an assertional model of knowledge, in that a SNePS knowledge base (KB) consists of a set of assertions (propositions) about various entities.

SO(1,n)

SN 1979C

Sorting Nexin 6 also known as SNX6 is a well-conserved membrane-associated protein belonging to the sorting nexin family that is a component of the retromer complex. The protein contains a coiled-coil domain at its C terminus and a PX domain at its N terminus. Binding to PIM1 causes translocation to the nucleus. SNX6 has been shown to associate with TRAF4.

Image from Richie Jarvis http://nebul.ae/astro-imaging/galaxies/ngc3972/2011-05-03-ngc3972-supernova-sn2011by1-301

broken up in Kure.

In particle physics, one of the grand unified theories (GUT) is based on the SO(10) Lie group. (The Lie group involved is not really the special orthogonal group SO(10), but rather its double cover Spin(10); but calling it SO(10) is the standard convention.)Before the SU(5) theory behind the Georgi–Glashow model, Harald Fritzsch and Peter Minkowski and independently Howard Georgi found that all the matter contents are incorporated into a single representation, spinorial 16 of SO(10).

*52 officers
*788 enlisted

Tuaran

SO(32)

SN 2006gy

SMS V46 was a Großes Torpedoboot 1913 class torpedo boat of the Imperial German Navy during World War I, and the 22nd ship of her class.

SN 2005cs

+15° 48′ 31.2″

Open

SN II-P

SN 1999EC is a type Ib supernova that was discovered in the interacting galaxy NGC 2207 in October 1999. It was found on images taken with the Katzman Automatic Imaging Telescope at the Lick Observatory. The progenitor is estimated to have had 38 times the mass of the Sun and was 5.34 million years old at the time of the outburst.

UB-122

*Waterline belt:
*Deck:
*Gun turrets:
*Casemate:
*Conning tower:

SMS Victoria Louise

SN 2005ap was an extremely energetic type Ic supernova in the galaxy SDSS J130115.12+274327.5. With a peak absolute magnitude of around −22.7, it is the brightest supernova yet recorded, twice as bright as the previous record holder, SN 2006gy. It was initially classified as type II-L, but later revised to type Ic.

Mall Logo

Norway, Africa south of Sahara, Southeast Asia, Central America

*Design:
*Full load:

*2 × propeller shaft
*2 × Körting four-stroke 6-cylinder diesel engines,
*2 × Siemens-Schuckert electric motors,

Ia/IIn "hybrid"

Picture of Supernova 1987A

SN 1998S was a type IIn supernova that was observed in NGC 3877 in March 1998. SN 1998S was the brightest type IIn event observed .It was discovered on 1998 March 2.68 UT in NGC 3877 by Z. Wan at a broadband (unfiltered) optical magnitude of +15.2.Its spectrum showed prominent H and He emission lines with narrow peaks and broad wings, superimposed on a blue continuum. These narrow lines indicate the presence of a dense circumstellar medium (CSM) in the vicinity of the supernova. The high luminosity of SN1998S is due to the interaction of fast material (ejecta) with previously-expelled slowly-expanding material (CSM), which can more effectively convert kinetic energy of ejecta into radiation energy.

SN Airholding

SN 2005cs was a supernova in the Whirlpool Galaxy. It was a type II supernova, discovered in 2005 by Wolfgang Kloehr, a German amateur astronomer.

SN College, Kollam

SN 2011by was a supernova in NGC 3972. It was a type Ia supernova, discovered by Zhangwei Jin and Xing Gao (China). SN 2011by is about 5.3" east and 19.1" north of the center of NGC 3972.

SN Brussels

Kelana Petra ,

SNX28

standard

Houses

MUSD 996,8

Sekolah Menengah Sains Selangor or SM Sains Selangor (SMSS) (English: Selangor Science Secondary School) is one of three fully residential schools (Sekolah Berasrama Penuh) in Kuala Lumpur, Malaysia. Established in 1973 under the Second Malaysia Plan to comply with Malaysian New Economic Policy,the school is located about a small hill in Bandar Tun Razak,overlooking the scenic Permaisuri lake.

SNaN

* Belt: 15 cm
* Turrets:
* Deck:

SN 1987A

Zealous Unite Success Distinguished

SN 2005bc was a Type Ia supernova occurring in the Barred spiral galaxy NGC 5698 in the constellation of Boötes. SN 2005bc was discovered on 2 April 2005 by LOSS and independently by Tim Puckett and L. Cox.

armored cruiser

SN 1999eu was a type IIP supernova that happened in NGC 1097 in the constellation Fornax. It was discovered 5 November 1999, possibly three months after its initial brightening, and is unusually under-luminous for a type II supernova.

Supernova SN 393

SMS Seeadler (1878)

SN 2007sr

Red, Blue and Yellow

May 1892

SN 2002bj

SN (disambiguation)

SN 386 is a probable transient astronomical event in the constellation Sagittarius, which appeared as a "guest star" that was reported by Chinese astronomers in 386 CE.

SNewtons

SMS Stuttgart was a Königsberg-class light cruiser of the Kaiserliche Marine, named after the city of Stuttgart. She had three sister ships: Königsberg, Nürnberg, and Stettin. Stuttgart was laid down at the Imperial Dockyard in Danzig in 1905, launched in September 1906, and commissioned in February 1908. Like her sisters, Stettin was armed with a main battery of ten 10.5 cm (4.1 in) guns and a pair of 45 cm (18 in) torpedo tubes, and was capable of a top speed in excess of 25 knots (46 km/h; 29 mph).Stuttgart was used as a gunnery training ship from her commissioning to the outbreak of World War I in August 1914, when she was mobilized into the reconnaissance forces of the High Seas Fleet. There, she saw action at the Battle of Jutland, where she engaged the British cruiser HMS Dublin. Stuttgart was not damaged during the battle. She was converted into a seaplane tender in 1918, and after the end of the war, was surrendered to Britain as a war prize in 1920 and subsequently broken up for scrap.

A guest star appeared within the asterism Wěi during the second lunar month of the 18th year of the Tai-Yuan reign period, and disappeared during the ninth lunar month.

SN 2010cr

SMS S-36

Sorting nexin-4 is a protein that in humans is encoded by the SNX4 gene.This gene encodes a member of the sorting nexin family. Members of this family contain a phox (PX) domain, which is a phosphoinositide binding domain, and are involved in intracellular trafficking. This protein associated with the long isoform of the leptin receptor and with receptor tyrosine kinases for platelet-derived growth factor, insulin, and epidermal growth factor in cell cultures, but its function is unknown.

SN Brussels (airline)

Neil Burrows ; Étienne Davignon, chairman

SMS Stuttgart was a Königsberg-class light cruiser of the Kaiserliche Marine, named after the city of Stuttgart. She had three sister ships: Königsberg, Nürnberg, and Stettin. Stuttgart was laid down at the Imperial Dockyard in Danzig in 1905, launched in September 1906, and commissioned in February 1908.

*1 merchant ship sunk
*1 merchant ship damaged
*3 merchant ships captured as prizes

SN 2003B

by Nearby Supernova Factory

SO(4)

Main Building: 2

SNX9

Austria-Hungary

SN 2005bc

SM UB-123 was a German Type UB III submarine or U-boat in the German Imperial Navy (German: Kaiserliche Marine) during World War I. She was commissioned into the German Imperial Navy on 6 April 1918 as SM UB-123.She torpedoed and sunk Leinster a vessel operated by the City of Dublin Steam Packet Company on 10 October 1918, shortly after the new German Government had asked President Wilson to negotiate an armistice. Leinster went down just outside Dublin Bay. Over 500 people perished in the sinking — the greatest single loss of life in the Irish Sea.UB-123 struck a mine at the North Sea Mine Barrage on 19 October 1918, all 36 crew members died in the event.

SN 2005gj

SN 1997D

Sorting nexin-9 is a protein that in humans is encoded by the SNX9 gene.This gene encodes a member of the sorting nexin family. Members of this family contain a phox (PX) domain, which is a phosphoinositide binding domain, and are involved in intracellular trafficking. This protein does not contain a coiled coil region, like some family members, but does contain an SH3 domain near its N-terminus. This protein interacts with the cytoplasmic domains of the precursor but not the processed forms of a disintegrin and metalloprotease domain 9 and 15. This protein binds the beta-appendage domain of adaptor protein 2 and may function to assist adaptor protein 2 in its role at the plasma membrane. This protein interacts with activated Cdc42-associated kinase-2 to regulate the degradation of epidermal growth factor receptor protein.

SN 1000+0216 was an extremely remote superluminous supernova (SLSN), which occurred in between June and November 2006. Its peak far-ultraviolet absolute magnitude reached −21.5, which exceeded the total absolute magnitude of its host galaxy. The distance (redshift) to this supernova z=3.8993 ± 0.0074 makes it the most distant supernova observed as of 2012. The luminosity of SN 1000+0216 evolved slowly over several years as it was still detectable in November 2008.

SN Roy

SMS Stosch (1877)

Teguh Setia Budi

Delgado corner Valeria Sts., Iloilo City, Iloilo

O 6

Sekolah Menengah Sains Rembau (English: Rembau Science Secondary School) or SEMESRA is a co-educational secondary school situated in the district of Rembau and among fully residential schools (Sekolah Berasrama Penuh) in the state of Negeri Sembilan, Malaysia.

SMS Voting

SN 2007sr was a Type Ia supernova event that happened in the galaxy NGC 4038. It was announced on December 18, 2007, but was visible on images beginning December 7. It peaked at magnitude 12.7 on December 14.

SM UB-125 was a German Type UB III submarine or U-boat in the German Imperial Navy (German: Kaiserliche Marine) during World War I. She was commissioned into the German Imperial Navy on 18 May 1918 as SM UB-125.UB-125 was surrendered 20 November 1918 in accordance with the requirements of the Armistice with Germany. Handed over to Japan, she served as O 6 in the Imperial Japanese Navy until 1921 when she was broken up in Kure.

SNX3 (gene)

SN 1986G

UB-124

SN 2213-1745 was an extremely remote superluminous supernova (SLSN), which occurred in between November 2004 and June 2005. Its peak far-ultraviolet absolute magnitude reached −21.2, which was comparable to the total absolute magnitude of its host galaxy. The distance (redshift) to this supernova z=2.0458 ± 0.0005 makes it one of the most remote supernova observed as of 2012. The luminosity of SN 2213-1745 evolved slowly over several years as it was still detectable in November 2006.

In particle physics, one of the grand unified theories (GUT) is based on the SO(10) Lie group. (The Lie group involved is not really the special orthogonal group SO(10), but rather its double cover Spin(10); but calling it SO(10) is the standard convention.)Before the SU(5) theory behind the Georgi–Glashow model, Harald Fritzsch and Peter Minkowski and independently Howard Georgi found that all the matter contents are incorporated into a single representation, spinorial 16 of SO(10). (Historical note: the before in the previous sentence is misleading: Georgi found the SO(10) theory a few hours before finding SU(5) at the end of 1973.)

SN Sportsman of the Year

Puan Hajah Norzila Idris

SN 2008ha was a type Ia supernova which was first observed around November 7, 2008 in the galaxy UGC 12682, which lies in the constellation Pegasus at a distance of about 21.3 megaparsecs (69 Mly) from Earth.SN 2008ha was unusual in several ways: with an absolute V band magnitude of −14.2 it is one of the faintest supernovae ever observed; its host galaxy type very rarely produces supernovae. Another unusual feature of SN 2008ha was its low expansion velocity of only ~2000 km/s at maximum brightness, which indicates a very small kinetic energy released in the explosion. For comparison, SN 2002cx expanded at a velocity of ~5000 km/s whereas typical SN Ia expand at around ~10,000 km/s. The low expansion velocity of SN2008ha resulted in relatively small Doppler broadening of spectral emission lines and this led to higher quality data.The supernova was studied with ultraviolet, optical, and near-infrared photometry as well as optical spectra, using the Magellan telescopes in Chile, the MMT telescope in Arizona, the Gemini and Keck telescopes in Hawaii, and NASA's Swift satellite. Spectroscopically, SN 2008ha was identified as a SN 2002cx-type, a peculiar sub-class of SN Ia. SN 2008ha had a brightness period of only 10 days, which is significantly shorter than that of other SN 2002cx-like objects (~15 days) or normal Ia supernovas (~20 days). From the peak luminosity and the brightness time it was estimated that SN 2008ha generated (3.0 ± 0.9) × 10−3 M⊙ of 56Ni, had a kinetic energy of 2 × 1048 ergs, and ejected 0.15 M⊙ of material.SN 2008ha was co-discovered by Caroline Moore, Jack Newton and Tim Puckett, members of the Puckett Observatory World Supernova Search. The 14-year-old Moore received considerable attention for her role in the discovery because at the time, she was the youngest person to have discovered a supernova. Moore is currently majoring in Political Science at Georgetown University. She was born and raised in Warwick, NY. To make the discovery she spent almost 7 months sifting through Puckett Observatory Supernova Search (POSS) images. Incredibly, she made her discovery using a relatively small, low-powered telescope.In July of 2009, she discovered her second supernova named SN2009he.From young, Moore had practiced amateur astronomy with the assistance of her father. Early on she was very familiar with telescopes because of her scientific upbringing. She even converted her tree house into an observatory. Following her discovery, Moore was awarded $384,000 in grants from the University of California-Berkeley.Moore has since traveled across the US to promote the field of astronomy to children and discuss her discovery at astronomy events. She also used fundraising to construct an observatory in her former elementary school.Moore's discovery has allowed scientists to better understand the nature of the death of stars. It challenged the assumptions of the then current model for the explosive nature of supernovas. This is because 2008ha’s low energy and low luminosity during the death of the star could not be explained with the current scientific model at the time due to it not being able to be distinctly classified as either a type Ia or type II Supernova.Despite being one of the weakest observed supernova on record, it was up to 1000 times brighter than the sun at one point and is approximately 70 million light years away from earth.[1] Some scientists suggested that the supernova may have failed in exploding completely which is why the light emitted from it is so weak compared to other supernovas.In reference to Moore, one astrophysicist remarked that "the youngest person to ever discover a supernova found one of the most peculiar and interesting supernovae ever." President of the United States Barack Obama and First Lady Michelle Obama met with Moore after her discovery.

SN 1987a

* 2 × Shafts
* 2 × Vertical triple-expansion steam engines

SMS Tegetthoff

SMS Selangor

IAUC 8633

Supernova 2008ax was a type Ib supernova in Peculiar Galaxy NGC 4490. As the name indicates, it was discovered in 2008 on 3 March by LOSS and Koichi Itagaki. It was the third-brightest supernova of 2008.

SNY (disambiguation)

+15° 47′ 52.7″

Scrapped 1921

SO(10)

SN 2005gj was a supernova located approximately 864 million light years (265 million parsecs) away from Earth. It was discovered on September 29, 2005, by the Sloan Digital Sky Survey and the Nearby Supernova Factory. 2005gj was noted because it had qualities of both type Ia and type IIn supernovae, and because hydrogen emission lines were found in its spectrum (see hydrogen spectral series). These hydrogen lines, which were found on the spectrum at redshift z=0.0613, are thought to be indicative of interactions with a circumstellar medium (CSM; a donut-shaped, nebula-like ring of matter around a star) by the supernova's ejected matter or white dwarf progenitor. Such emission lines are extremely rare in Type Ia supernovae – only one other Type Ia, SN 2002ic, has been observed to exhibit the same properties. However, 2005jg's CSM interaction was much stronger and more clearly observed than 2002ic's. The mass-loss history 2005gj's hydrogen lines suggest has been cited as evidence that Luminous Blue Variable (LBV) hypergiants can be progenitors of thermonuclear supernovae.2005gj was also noted for its overluminosity. With a light curve that maximised 14–47 days after the initial observation, it was three times more luminous than SN 1991T (which was, at the time of its 1991 discovery, the brightest Ia supernova on record), 1.5 times more luminous than SN 2002ic, and close to 100 times more luminous than previously thought possible. Scientists Denis Leahy and Rachid Ouyed from the University of Calgary contend that the incidence of a quark nova, a very luminous process involving the degeneration of neutrons into their constituent quarks, could explain the unusual magnitude of the luminosity.

NGC266 LBV 1

Sunk in action,Battle of the Falkland Islands, 8 December 1914

Cik Rosnah Binti Osman

SDSS J130114+2743

None

SM Department Store Delgado

SN 2213-1745 was an extremely remote superluminous supernova (SLSN), which occurred in between November 2004 and June 2005. Its peak far-ultraviolet absolute magnitude reached −21.2, which was comparable to the total absolute magnitude of its host galaxy. The distance (redshift) to this supernova z=2.0458 ± 0.0005 makes it one of the most remote supernova observed as of 2012. The luminosity of SN 2213-1745 evolved slowly over several years as it was still detectable in November 2006. Both the high luminosity and slow decay indicate that the supernova's progenitor was a star with an initial mass as high as 250 solar masses. The supernova explosion itself was likely a pair-instability supernova similar to the SN 2007bi event, with which it shares many similarities.

SN 2005ap was an extremely energetic type Ic supernova in the galaxy SDSS J130115.12+274327.5. With a peak absolute magnitude of around −22.7, it is the brightest supernova yet recorded, twice as bright as the previous record holder, SN 2006gy. It was initially classified as type II-L, but later revised to type Ic. It was discovered on 3 March 2005 on unfiltered optical images taken with the 0.45 m ROTSE-IIIb (Robotic Optical Transient Search Experiment) telescope, which is located at the McDonald observatory in West Texas, by Robert Quimby as part of the Texas Supernova Search that also discovered SN 2006gy. Although it was discovered before SN 2006gy it was not recognised as being brighter until October 2007. As it occurred 4.7 billion light years from Earth it was not visible to the naked eye.Although SN 2005ap was twice as bright at its peak than SN 2006gy it was not as energetic overall as the former brightened and dimmed in a typical period of a few days whereas the latter remained very bright for many months. SN 2005ap was about 300 times brighter than normal for a type II supernova. It has been speculated that this supernova involved the formation of a quark star. Quimby has suggested that the supernova is of a new type distinct from the standard type II supernova and his research group have identified five other supernovae similar to SN 2005ap and SCP 06F6, all of which were extremely bright and lacking in hydrogen.

SN 2002cx is a peculiar type Ia supernova. It was discovered in May 2002 by a team of researchers from LBL. It behaved differently from normal type Ia supernovae, and differently from several other previously observed peculiar type Ia supernovae including SN 1991T and SN 1991bg.

Type Ic

SO(2)

IAUC 7902

*3 shafts
*3 × triple-expansion steam engines

Siegfried

sorting nexin 6

Akhirul Zaman ,

SMS Tiger (1887)

Supernova 2008ax - Image Courtesy Hunter Wilson

protected cruiser

Excellent Principal

Only SN in NGC 5128

Victoria Louise

SN 1939C

SN 2005gl

SMS Teodo was a 6,561 ton collier built in 1915 for the Austro-Hungarian Navy. She was ceded to Italy in 1921 as a war reparation. She was renamed Barbana in 1924 and Barbana G in 1926. In 1940, she was seized by the United Kingdom and renamed Empire Airman. On 21 September 1940, Empire Airman was torpedoed and sunk by German submarine U-100.

Sorting nexin-9 is a protein that in humans is encoded by the SNX9 gene.This gene encodes a member of the sorting nexin family. Members of this family contain a phox (PX) domain, which is a phosphoinositide binding domain, and are involved in intracellular trafficking. This protein does not contain a coiled coil region, like some family members, but does contain an SH3 domain near its N-terminus.

SO(N,1)

SN 2005gj was a supernova located approximately 864 million light years (265 million parsecs) away from Earth. It was discovered on September 29, 2005, by the Sloan Digital Sky Survey and the Nearby Supernova Factory. 2005gj was noted because it had qualities of both type Ia and type IIn supernovae, and because hydrogen emission lines were found in its spectrum (see hydrogen spectral series).

SEMESRA

~ 250 star

*20 officers
*256 enlisted men

maybe Red supergiant

Type IIn

SM UB-122 was a German Type UB III submarine or U-boat in the German Imperial Navy (German: Kaiserliche Marine) during World War I. She was commissioned into the German Imperial Navy on 4 March 1918 as SM UB-122.UB-122 was surrendered to the British on 24 November 1918 in accordance with the requirements of the Armistice with Germany.

SN Sanyal

SN 1895B was a supernova in the galaxy NGC 5253. It reached a maximum brightness of apparent magintude 8.0 before fading.

Luminous blue variable

Rembau

SNX5 (gene)

SN 2014J was a type-Ia supernova in Messier 82 (the 'Cigar Galaxy', M82) discovered in mid-January 2014. It was the closest type-Ia supernova discovered for 42 years, and none have been closer as of 2016. The supernova was discovered by chance during an undergraduate teaching session at University of London Observatory. It peaked on 31 January 2014, reaching an apparent magnitude of 10.5. SN 2014J was the subject of an intense observing campaign by professional astronomers, and was bright enough to be seen by amateur astronomers.

about 200,000,000 light-years

SN 1961v

SN Brussels Destinations

SN 1961i

SN 1999ec

SN 1992bd was a type II supernova event in NGC 1097, positioned some 1.5″ east and 9″ south of the galactic nucleus. It was discovered by astronomers Chris Smith and Lisa Wells on October 12, 1992. Spectra of the object collected October 17 showed it to have an expansion velocity of 7,500 km/s.

Privilege

SN 1992bd was a type II supernova event in NGC 1097, positioned some 1.5″ east and 9″ south of the galactic nucleus. It was discovered by astronomers Chris Smith and Lisa Wells on October 12, 1992. Spectra of the object collected October 17 showed it to have an expansion velocity of 7,500 km/s. Subsequent examination of archival images from the Hubble Space Telescope showed an image of the supernova had been captured on September 20, 1992, 12 days prior to its discovery with ground-based telescopes. The eruption occurred in the circumnuclear star-forming region of the galaxy.

*1921: Genoa
*1940: Newcastle upon Tyne

SN 1181

SN Hanumantha Rao

M100 before and after the supernova explosion

is located near the apparent host galaxy Anon J131920+0855

UB-123

SNX4 (gene)

SMS Saida

SM Unterseeboot U30

SNYSB

Passionate about you

Sekolah Menengah Sains Selangor or SM Sains Selangor (SMSS) (English: Selangor Science Secondary School) is one of three fully residential schools (Sekolah Berasrama Penuh) in Kuala Lumpur, Malaysia. Established in 1973 under the Second Malaysia Plan to comply with Malaysian New Economic Policy,the school is located about a small hill in Bandar Tun Razak,overlooking the scenic Permaisuri lake. In 2011,the school was awarded with the Sekolah Berprestasi Tinggi or High Performance School title, a title awarded to schools in Malaysia that have met stringent criteria including academic achievement, strength of alumni, international recognition, network and linkages.In the recent PMR examination (2013), the school managed to produce 84 straight A's students out of 120 with GPS 1.06 to be the best schools in Kuala Lumpur.

*31 officers
*446 enlisted men

SNYA Radio

SNe

SN 2006gy and the core of its home galaxy, NGC 1260, viewed in x-ray light from the Chandra X-ray Observatory. The NGC 1260 galactic core is on the lower left and SN 2006gy is on the upper right.

*1921: Teodo

SN Ib
SN 1999EC

SMS Roon was the lead ship of her class of armored cruisers of the Imperial German Navy. The ship was authorized under the second Naval Law in 1902, and built at the Imperial Dockyard in Kiel at the cost of 15.3 million marks. The ship was named after Albrecht von Roon, a Prussian general and politician. She displaced up to 9,875 metric tons (9,719 long tons; 10,885 short tons) and was armed with a main battery of four 21 cm (8.3 in) guns. Her top speed was 20.4 knots (37.8 km/h; 23.5 mph).The ship participated in several actions during the First World War, including the raid on Scarborough, Hartlepool and Whitby, where she acted as a scout for the High Seas Fleet. Roon also saw duty in the Baltic Sea, including a battle in July 1915 against Russian cruisers and shore bombardment missions. After 1916, Roon was used as a training and barracks ship in Kiel until the end of the war. It was intended to convert the ship into a seaplane tender, but the plan was eventually abandoned. The ship was struck from the naval register in 1920 and scrapped thereafter.

X-ray and visible light images of SN 2008D , and SN 2007uy .

Venezia

Jalan Yaacob Latif,

SNX9 (gene)

SMS Scharnhorst

This gene encodes a member of the sorting nexin family. Members of this family contain a phox domain, which is a phosphoinositide binding domain, and are involved in intracellular trafficking. The specific function of this protein has not been elucidated. Alternative splice variants have been described but their full length nature has not been determined.

Annex Building: 1

SN 1979C was a supernova about 50 million light-years away in Messier 100, a spiral galaxy in the constellation Coma Berenices. The Type II supernova was discovered April 19, 1979 by Gus Johnson, a school teacher and amateur astronomer. This type of supernova is known as a core collapse and is the result of the internal collapse and violent explosion of a large star. A star must have at least 9 times the mass of the Sun in order to undergo this type of collapse. The star that resulted in this supernova was estimated to be in the range of 20 solar masses.On November 15, 2010 NASA announced that evidence of a black hole had been detected as a remnant of the supernova explosion. Scientists led by Dr. Dan Patnaude from the Harvard–Smithsonian Center for Astrophysics in Cambridge, MA evaluated data gathered between 1995 and 2007 from several space based observatories. NASA's Chandra X-ray Observatory, the Swift Gamma-Ray Burst Mission, as well as the European Space Agency's XMM-Newton, and Germany's ROSAT all participated in the examination.The researchers observed a steady source of X-rays and determined that it was likely that this was material being fed into the object either from the supernova or a binary companion. However, an alternative explanation would be that the X-ray emissions could be from the pulsar wind nebula from a rapidly spinning pulsar, similar to the one in the center of the Crab Nebula. These two ideas account for several types of known X-ray sources. In the case of black holes the material that falls into the black hole emits the X-rays and not the black hole itself. Gas is heated by the fall into the strong gravitational field.SN 1979C has also been studied in the radio frequency spectrum. A light curve study was performed between 1985 and 1990 using the Very Large Array radio telescope in New Mexico.

SN Ia

SO(n)

SN 2007bi was an extremely energetic supernova discovered early in 2007 by the international Nearby Supernova Factory based at the U.S. Department of Energy's Lawrence Berkeley National Laboratory. The precursor star is estimated to have had 200 solar masses at the time of its formation and around 100 solar masses in its core when it went supernova. The explosion ejected more than 22 solar masses of silicon and other heavy elements into space during this supernova including more than 6 solar masses of radioactive nickel which caused the expanding gases to glow very brightly for many months.The supernova has been described as an unambiguous fit for the pair-instability supernova model.

SMS Tiger was a so-called "torpedo ram cruiser" (Torpedo-Rammkreuzer) of the Austro-Hungarian Navy. An enlarged and improved version of Panther and Leopard she was part of a program to build up Austria-Hungary's fleet of torpedo craft in the 1880s. In 1906 she was converted to an admiralty yacht and renamed SMS Lacroma.

SNX27 (gene)

SN Behrman

SNX6

SN 2003fg, sometimes called the "Champagne Supernova", was an unusual Type Ia supernova. It was discovered in 2003 with the Canada-France-Hawaii Telescope and the Keck Telescope, both on Mauna Kea in Hawaii, and announced by researchers at the University of Toronto. The supernova occurred in a galaxy some 4 billion light-years from Earth. It was nicknamed after the 1996 song "Champagne Supernova" by English rock band Oasis.It was unusual because of the mass of its progenitor. According to the current understanding, white dwarf stars explode as Type Ia supernovas when their mass approaches 1.4 solar masses, termed the Chandrasekhar limit. The mass added to the star is believed to be donated by a companion star, either from the companion's stellar wind or the overflow of its Roche lobe as it evolves.However, the progenitor of SN 2003fg reached two solar masses before exploding. The primary mechanism invoked to explain how a white dwarf can exceed the Chandrasekhar mass is unusually rapid rotation; the added support effectively increases the critical mass. An alternative explanation is that the explosion resulted from the merger of two white dwarfs. The evidence indicating a higher than normal mass comes from the light curve and spectra of the supernova—while it was particularly overluminous, the kinetic energies measured from the spectra appeared smaller than usual. One proposed explanation is that more of the total kinetic energy budget was expended climbing out of the deeper than usual potential well.This is important because the brightness of type Ia supernovae was thought to be essentially uniform, making them useful "standard candles" in measuring distances in the universe. Such an aberrant type Ia supernova could throw distances and other scientific work into doubt; however, the light curve characteristics of SN 2003fg were such that it would never have been mistaken for an ordinary high-redshift Type Ia supernova.

SN 2011dh is a supernova in the Whirlpool Galaxy (M51). On 31 May 2011 an apparent magnitude 13.5 type II supernova (the explosion of a single massive star) was detected in M51 at coordinates 13:30:05.08 +47:10:11.2. It was discovered by Tom Reiland; Thomas Griga; Amédée Riou; and Stephane Lamotte Bailey and confirmed by several sources, including the Palomar Transient Factory. A candidate progenitor has been detected in Hubble Space Telescope images at coordinates 13:30:05.119 +47:10:11.55. The progenitor may have been a highly luminous yellow supergiant with an initial mass of 18-24 solar masses. The supernova appears to have peaked near apparent magnitude 12.1 on 19 June 2011.Emission spectra from W. M. Keck Observatory, obtained by Palomar Transient Factory indicate that this is a type II supernova with a relatively blue continuum with P Cygni profiles in the Balmer series. This is a unique event, because it occurs in a galaxy that is imaged almost constantly. It is expected to be observable for northern hemisphere observers for several months.This is the third supernova to be recorded in the Whirlpool galaxy in 17 years (following SN 1994I and SN 2005cs) which is a lot for a single galaxy. The galactic supernova frequency is estimated to be around one event every 40 years.

Venice, Italy

Supernova SN 386

*2 shafts
*2 Triple-expansion steam engines
*4 locomotive boilers

SN 1604

"Strength, Loyalty, Morality"

Sorting nexin-4 is a protein that in humans is encoded by the SNX4 gene.This gene encodes a member of the sorting nexin family. Members of this family contain a phox (PX) domain, which is a phosphoinositide binding domain, and are involved in intracellular trafficking. This protein associated with the long isoform of the leptin receptor and with receptor tyrosine kinases for platelet-derived growth factor, insulin, and epidermal growth factor in cell cultures, but its function is unknown. This protein may form oligomeric complexes with family members.

SM UB-123

Texas Supernova Search

SN 1999eu

SN 386

SMS V46

SN 1954J

*Deck:
*Conning tower:

SN 1998S was a type IIn supernova that was observed in NGC 3877 in March 1998. SN 1998S was the brightest type IIn event observed .It was discovered on 1998 March 2.68 UT in NGC 3877 by Z. Wan at a broadband (unfiltered) optical magnitude of +15.2.Its spectrum showed prominent H and He emission lines with narrow peaks and broad wings, superimposed on a blue continuum. These narrow lines indicate the presence of a dense circumstellar medium (CSM) in the vicinity of the supernova.

Full load:

Q9UNH7

~ 0.2 mag

* 3 × water tube boilers
* 2 × AEG Vulcan Steam Turbines

SN 1997D, discovered on January 1997 in galaxy NGC 1536 in Reticulum constellation is a first clearly identified example of atypical Type II supernova with a very low luminosity and expansion velocity.

SNCASE SE.5003

Broken up in Italy, 1924

Tun Said Keruak

SMS Tegetthoff (1912)

SN 2002bj was the explosion of a star in the galaxy NGC 1821, located in the constellation Lepus. The explosion was discovered by Jack Newton in scans of images produced by Tim Puckett. (It was independently discovered by the Lick/Tenagra Observatory as part of their combined supernova search program.) Initially it had an apparent magnitude of about 14.7 and was categorized as a Type IIn supernova.

SN 2008D is a supernova detected with NASA's Swift X-ray telescope. The explosion of the supernova precursor star, in the spiral galaxy NGC 2770 (88 million light years away (27 Mpc), was detected on January 9, 2008, by Carnegie-Princeton fellows Alicia Soderberg and Edo Berger, and Albert Kong and Tom Maccarone independently using Swift. They alerted eight other orbiting and ground-based observatories to record the event.

SM UB-124 was a German Type UB III submarine or U-boat in the German Imperial Navy (German: Kaiserliche Marine) during World War I. She was commissioned into the German Imperial Navy on 22 April 1918 as SM UB-124.UB-124 was sunk on 20 July 1918 by HMS Marne, HMS Milbrook, HMS Pigeon, and more than 30 patrol craft at 55°43′N 7°51′W.

*1924: Barbana

SO(5)

SN 2011dh

*
*5 × cylindrical boilers

SNi reaction

*2 × guns
*8 × guns
*10× guns
*3 × torpedo tubes

SN fleet

SN 1993J

SN 1986G was a supernova that was observed on May 3, 1986 by Robert Evans. Its host galaxy, Centaurus A, is about 15 million light-years away in the constellation Centaurus. Since Centaurus A is about 15 million light-years away from us, this supernova happened 15 million years ago.SN 1986G was a bright blue-green star in the middle of the left part of the dust belt of Centaurus A. The blue-green color occurs because David Malin could take the red plate used in this composite image only one year after the supernova occurred, and it had faded away at that time.

*Waterline belt:
*Deck:

scrapped, 1920

SM UB-123 was a German Type UB III submarine or U-boat in the German Imperial Navy (German: Kaiserliche Marine) during World War I. She was commissioned into the German Imperial Navy on 6 April 1918 as SM UB-123.She torpedoed and sunk Leinster a vessel operated by the City of Dublin Steam Packet Company on 10 October 1918, shortly after the new German Government had asked President Wilson to negotiate an armistice. Leinster went down just outside Dublin Bay.

SN 1998S, AAVSO 1140+48

SMS Victoria Louise was the lead ship of her class of protected cruisers, built for the German Imperial Navy (Kaiserliche Marine) in the late 1890s. She was laid down at the AG Weser shipyard in 1895, launched in March 1897, and commissioned into the German fleet in February 1899. She was named after Princess Victoria Louise, the daughter of Kaiser Wilhelm II. The ship was armed with a battery of two 21 cm guns and eight 15 cm guns and had a top speed of 19.2 knots (35.6 km/h; 22.1 mph).Victoria Louise served with the fleet for the first seven years of her career. During this time, she represented Germany during the funeral of Queen Victoria in 1901. In 1906, she was modernized and after 1908, used as a training ship for naval cadets. In 1909, she visited the United States, and at the outbreak of World War I, was mobilized into the 5th Scouting Group. She was attacked unsuccessfully by the British submarine HMS E1 in October 1914, and at the end of the year she was withdrawn from service. She was used as a minelayer and barracks ship based in Danzig for the rest of the war. Victoria Louise was sold in 1919 and converted into a freighter the following year, though she served in this capacity until 1923, when she was broken up for scrap.

SNX4

SMS UB-48

SN Power Invest

General knowledge and science

NGC 266

, three shafts

SN Power

Broken up in Italy, 1920

TC10/CDC42 GTPase-activating protein is an enzyme that in humans is encoded by the SNX26 gene.This gene encodes a member of the sorting nexin family. Members of this family contain a phox (PX) domain, which is a phosphoinositide binding domain, and are involved in intracellular trafficking. The specific function of this protein has not been elucidated. Alternative splice variants have been described but their full length nature has not been determined.

SN UDS10Wil, SN Wilson

56000Bandar Tun Razak

SN postcode area

SNCASO-ONDERA Deltaviex

IIP

SNiP technique

*Italian official number 1496
*UK Official Number 165788
*Code letters NFVG
*
*Code letters GLZT
*

SNX2 (gene)

SN 1940B

SN 1998S

initially a 140–250 star

SN 2014J

SN 2005gl was a supernova in the barred-spiral galaxy NGC 266. It was discovered using CCD frames taken October 5, 2005, from the 60 cm automated telescope at the Puckett Observatory in Georgia, US, and reported by Tim Puckett in collaboration with Peter Ceravolo. It was independently identified by Yasuo Sano in Japan. The supernova was located 29.8″ east and 16.7″ north of the galactic core. Based upon its spectrum, this was classified as a Type IIn core-collapse supernova. It has a redshift of z = 0.016, which is the same as the host galaxy.Using archived images from the Hubble Space Telescope, a candidate progenitor star was identified. This is believed to be a luminous blue variable (LBV), similar to Eta Carinae, with an absolute magnitude of −10.3 and a surface temperature of about 13,000 K. However, there is a small probability that the source was instead located in a compact cluster of stars.

Ceded to Italy as war reparation, 1921

Twin triple expansion engines,

SM UB-122

SN Power AS (formerly called Statkraft Norfund Power Invest AS) invests in clean, renewable energy on a commercial basis in emerging markets. The company focuses on investments in hydroelectricity and has several running plants in the Philippines, Zambia and Panama. The company operates in Southeast Asia, Africa and Central America and has established offices in Netherlands, Singapore, Philippines, Zambia, Mozambique, and Panama.

SNePS is a knowledge representation, reasoning, and acting (KRRA) system developed and maintained by Stuart C. Shapiro and colleagues at the State University of New York at Buffalo.SNePS is simultaneously a logic-based, frame-based, and network-based KRRA system. It uses an assertional model of knowledge, in that a SNePS knowledge base (KB) consists of a set of assertions (propositions) about various entities. Its intended model is of an intensional domain of mental entities---the entities conceived of by some agent, and the propositions believed by it. The intensionality is primarily accomplished by the absence of a built-in equality operator, since any two syntactically different terms might have slightly different Fregean senses.SNePS has three styles of inference: formula-based, derived from its logic-based personality; slot-based, derived from its frame-based personality; and path-based, derived from its network-based personality. However, all three are integrated, operating together.SNePS may be used as a stand-alone KRR system. It has also been used, along with its integrated acting component, to implement the mind of intelligent agents (cognitive robots), in accord with the GLAIR agent architecture (a layered cognitive architecture). The SNePS Research Group often calls its agents Cassie.

*3 × guns
*6 × guns
*4 × torpedo tubes

SM UB-125

Tun Datu Mustapha

*4 × Krupp guns
*6 × guns
*4 × 47 mm revolver cannon
*4 × torpedo tubes

Maroon, Black and White

SN Balagangadhara

SN Reactions

normal; full load

Malay, English, Arabic, Japanese and French

SN 2006aj

SN 1990U

*3 × 8.8 cm guns
*6 × 500 mm torpedo tubes
*24 mines

at a speed of

F9/A0Ia

Supernova SN 1181

none

SMS V-45

Ibc-pec

* Belt, barbettes, turrets and conning tower:
* Deck: maximum

Form 1 to Form 5

Johan Pahlawan ,

Proposed "quark nova".

SNCASE SE.532

*6 merchant ships sunk
*1 merchant ship damaged

SNewton

SN 2008ha was a type Ia supernova which was first observed around November 7, 2008 in the galaxy UGC 12682, which lies in the constellation Pegasus at a distance of about 21.3 megaparsecs (69 Mly) from Earth.SN 2008ha was unusual in several ways: with an absolute V band magnitude of −14.2 it is one of the faintest supernovae ever observed; its host galaxy type very rarely produces supernovae.

about 15,000,000 light-years

Type Ia

SN 2007bi was an extremely energetic supernova discovered early in 2007 by the international Nearby Supernova Factory based at the U.S. Department of Energy's Lawrence Berkeley National Laboratory. The precursor star is estimated to have had 200 solar masses at the time of its formation and around 100 solar masses in its core when it went supernova.

JRP Design Inc.

SNCASE SE.3160

SN Brussels Airlines destinations

SMS Stuttgart

SN 2011dh is a supernova in the Whirlpool Galaxy (M51). On 31 May 2011 an apparent magnitude 13.5 type II supernova (the explosion of a single massive star) was detected in M51 at coordinates 13:30:05.08 +47:10:11.2. It was discovered by Tom Reiland; Thomas Griga; Amédée Riou; and Stephane Lamotte Bailey and confirmed by several sources, including the Palomar Transient Factory. A candidate progenitor has been detected in Hubble Space Telescope images at coordinates 13:30:05.119 +47:10:11.55.

light cruiser

*3 × L/45 guns
*6 × 500 mm torpedo tubes
*24 mines

< 12

SM Cyril

SN 2014J was a type-Ia supernova in Messier 82 (the 'Cigar Galaxy', M82) discovered in mid-January 2014. It was the closest type-Ia supernova discovered for 42 years, and none have been closer as of 2016. The supernova was discovered by chance during an undergraduate teaching session at University of London Observatory. It peaked on 31 January 2014, reaching an apparent magnitude of 10.5.

SMS Sabah
Malaysia

*Waterline belt:
*Deck:
*Conning tower:

SN Wilson

SN 2006X was a Type Ia supernova about 65 million light-years away in Messier 100, a spiral galaxy in the constellation Coma Berenices. The supernova was independently discovered in early February 2006 by Shoji Suzuki of Japan and Marco Migliardi of Italy.SN 2006X is particularly significant because it is a Type Ia supernova. These supernovae are used for measuring distances, so observations of these supernovae in nearby galaxies are needed for calibration. SN 2006X is located in a well-studied galaxy, and it was discovered two weeks before its peak brightness, so it may be extraordinarily useful for understanding supernovae and for calibrating supernovae for distance measurements. It may even be possible to identify the progenitor of this supernova.

SM UB-124

>8kpc

*10 × rapid fire guns
*2 × torpedo-tubes

SN 1939C was a supernova in the Fireworks Galaxy first discovered by Fritz Zwicky on 17 July 1939. With a right ascension of 20:34:23.0 and a declination of +60:09:37.3, it lies 215"W and 24"N from the center of the Fireworks Galaxy. It peaked at a magnitude of 13.0 mag.

March 1888

aberrant Ia

August 1902

SM Department Store

SN 1993J is a supernova observed in the galaxy M81. It was discovered on 28 March 1993 by F. Garcia in Spain. At the time, it was the second brightest type II supernova observed in the twentieth century behind SN 1987A.The spectral characteristics of the supernova changed over time.

Red supergiant

SO-152

DAT

*14 Officers
*308 Enlisted men

SNePS

SMS Wien ("His Majesty's Ship Vienna") was one of three Monarch-class coastal defense ships built for the Austro-Hungarian Navy in the 1890s. After her commissioning, the ship participated in an international blockade of Crete during the Greco-Turkish War of 1897. Wien and the two other Monarch-class ships made several training cruises in the Mediterranean Sea in the early 1900s.

SM UB-122 was a German Type UB III submarine or U-boat in the German Imperial Navy (German: Kaiserliche Marine) during World War I. She was commissioned into the German Imperial Navy on 4 March 1918 as SM UB-122.UB-122 was surrendered to the British on 24 November 1918 in accordance with the requirements of the Armistice with Germany. She may have been broken up in 1921, have been marooned on a sandbank at Hoo on the River Medway, or have foundered in the North Sea off the east coast of England in 1921.

Mutiara SEMESRA

SN Power AS (formerly called Statkraft Norfund Power Invest AS) invests in clean, renewable energy on a commercial basis in emerging markets. The company focuses on investments in hydroelectricity and has several running plants in the Philippines, Zambia and Panama. The company operates in Southeast Asia, Africa and Central America and has established offices in Netherlands, Singapore, Philippines, Zambia, Mozambique, and Panama. The company is a joint venture between Statkraft and Norfund, both owned by the Government of Norway.The company was established in 2002. Along with Norfund, the Norwegian Investment Fund for Developing Countries, Statkraft created the international power company Statkraft Norfund Power Invest (in short called SN Power) in 2002. The company was formed to promote economic growth and sustainable development in new and emerging markets. SN Power was a continuation of efforts that Statkraft began in the 1990s with projects in Laos and Nepal. In May 2003, SN Power made its first investment, with the acquisition of 30 per cent of Nividhu in Sri Lanka, a venture partner that operates the power plants Assupiniella and Belihuloya.SN Power AS was reestablished as a new company in 2013 after its parent company Statkraft and Norfund decided to make changes to their share portfolios. The company retained its short named 'SN Power AS', however it is no longer abbreviated to 'Statkraft Norfund Power Invest AS'. Through change of control the former company 'Statkraft Norfund Power Invest AS' remained with Statkraft as a holding company.

*Three triple expansion engines
*12 Dürr boilers

SO-2

SN Bandekar

Sabah

by Robert Quimby

SMS Tegetthoff was an Austro-Hungarian dreadnought battleship of the Tegetthoff class named after Wilhelm von Tegetthoff, a 19th-century Austrian admiral most notable for defeating the Italian Navy in the Battle of Lissa.Tegetthoff was built at the Stabilimento Tecnico Triestino yard in Trieste as part of the first and only class of dreadnought battleships in the Austro-Hungarian Navy. After her construction in 1912, an earlier armoured battleship named SMS Tegetthoff was renamed Mars.During World War I, Tegetthoff participated in the bombardment of the Italian city of Ancona. She remained in port in Pola for the rest of the war until she participated in an ill-fated raid on the Otranto Barrage in 1918 that resulted in the loss of her sister ship, SMS Szent István. Following the end of the war in late 1918, Tegetthoff was surrendered to Italy and later scrapped in 1924.