OG-6

OGAE Video Contest 2010

OGAS

The OGC Reference Model describes a framework for the ongoing work of the Open Geospatial Consortium (OGC) and their specifications and implementing interoperable solutions and applications for geospatial services, data, and applications.

OGLE-TR-122B

OGDL (Ordered Graph Data Language), is a "structured textual format that represents information in the form of graphs, where the nodes are strings and the arcs or edges are spaces or indentation."Like XML, but unlike JSON and YAML, OGDL includes a schema notation and path traversal notation. There is also a binary representation.

Bond et al.

OGLE-2005-BLG-390L is a star thought to be a spectral type M (a red dwarf; 95% probability, 4% probability it is a white dwarf, <1% probability it is a neutron star or black hole). This dim magnitude 16 galactic bulge star is located in the Scorpius constellation at a far distance of about 21,500 light years.

Stanislav V. Neveynitsyn

OGLE-TR-56

OGLE-05-071L b

OFZ, a.s., Istebné

OFT v Abbey National plc

OGD

Opioid growth factor receptor repeat

OGAE Second Chance Contest 2004

OGAS (Russian: Общегосударственная автоматизированная система учёта и обработки информации, All-State Automated System) was a Soviet project to create a nationwide information network. The project began in 1962 but was denied necessary funding in 1970. It was one of a series of attempts to create a nationwide network analogous to what became the Internet, all of which failed.The primary architect of OGAS was Viktor Glushkov.

Published

OFSAA

yes

approx. 3,900

OGLE-TR-113 is a dim, distant magnitude 16 binary star in the star fields of the constellation Carina. Because of its distance of about 1170 light years, and location in a crowded field it was not notable in any way. Spectral type of the star is type K dwarf star, slightly cooler and less luminous than the Sun.

Red

OGLE-2005-BLG-169Lb is an extrasolar planet located approximately 2700 parsecs away in the constellation of Sagittarius, orbiting the star OGLE-2005-BLG-169L. This planet was discovered by the OGLE project using the gravitational microlensing method. Based on a most likely mass for the host star of 0.49 solar mass (M☉), the planet has a mass of 13 times that of Earth (M⊕). Its mass and estimated temperature are close to those of Uranus.

OGLE-TR-132

OFT-1

OG44

OF Muller

OFS (Optical Fiber Solutions)

OGAE Second Chance 2009

OGAE Video Contest 2011

OGLE-TR-111 is a yellow dwarf star approximately 5,000 light-years away in the constellation of Carina (the Keel). Having an apparent magnitude of about 17, this distant and dim star has not yet been cataloged.

OGAE Second Chance Contest 2003

Merged with OGK-2

OGHS

OGLE-2005-BLG-169L is a dim and distant magnitude 20 galactic bulge star located about 2,700 parsecs away in the constellation Sagittarius. If it is a main sequence star, then it is most likely a red dwarf with about half of the mass of the Sun. Other possibilities are a white dwarf star, or (less likely) a neutron star or black hole.

Udalski et al.

OGHS (disambiguation)

JSC The Third Generation Company of Wholesale Electric Market – (JSC WGC-3)

OGLE-2003-BLG-235Lb/MOA-2003-BLG-53Lb is an extrasolar planet discovered in April 2004 by the OGLE and MOA collaborations. Its high mass indicates that it is most probably a gas giant planet similar to Jupiter. It is located around 4.3 AU away from its parent star.

Pont et al.

OGAE Video Contest 2012

OAO Оптовая генерирующая компания № 1

Radial velocity

Confirmed

transit

G or K

ОАО «ОГК-6»

The OGAE Video Contest is a video event which, much like the OGAE Song Contest, is organised between branches of OGAE, the international fan club of the Eurovision Song Contest.All OGAE national clubs can enter with an original song and video released in the previous 12 months in their countries. There is no obligation on the entry for the OGAE Video Contest to be sung in one of the country's official languages.

OFWG

Udalski, Pont et al.

OFSS

OGL

OGLE-TR-182 b

OF Neas Ionias

OGLE-05-390L b

This article lists results for French association football team OGC Nice in European competition.

OGI School of Science and Engineering

OGLE-TR-123A

OGLE-TR-113

France
Logistics

Unsure

OGLE-TR-182b is a transiting extrasolar planet. It is a hot Jupiter with a similar mass to Jupiter but a larger radius.

Opioid growth factor receptor conserved region

OGLE-TR-182

OGLE-TR-122A

G2V
OGLE-TR-10 is a distant, magnitude 16 star in the constellation of Sagittarius. It is located near the Galactic Center. This star is listed as an eclipsing type variable star with the eclipse due to the passage of the planet as noted in the discovery papers.

La Rochelle

OFS (disambiguation)

OFZ

OGDL

Merged into Inter RAO

– present

OFW Diaries at Mga Kwentong Pinoy Overseas

OGLE-TR-56 is a dim, distant, magnitude 17 Sun-like star located approximately 1500 parsecs away in the constellation of Sagittarius. This star is listed as an eclipsing type variable star with the eclipse due to the passage of the planet as noted in the discovery papers.

oFono

OGFr

OGLE-2006-BLG-109L b

The Oregon Golf Association (OGA) Golf Course is a public golf course located in Woodburn, Oregon. The course was rated by Golf Digest in 1996 as a "One of the Top Ten Affordable Courses in the US." It is located at 45.1606164°N 122.8477049°W﻿ / 45.1606164; -122.8477049.

OGC Nice Côte d'Azur Handball

Boris Kovalchuck,

Private university

OGAE Video Contest 2005

OGCM

OG: Optimized Gaia

OGAE Second Chance Contest 2010

OF Nea Ionia

OGLE-TR-10

OGLE-2005-BLG-071Lb is a planet discovered by the Optical Gravitational Lensing Experiment (OGLE) and others in 2005, using gravitational microlensing. According to the best fit model, it has about 3.5 times the mass of Jupiter and a projected separation of 3.6 astronomical units from the star. This would result in an effective temperature around 50 K, similar to that of Neptune. However, an alternative model which gives a slightly lower mass of 3.3 times that of Jupiter and a projected separation of 2.1 AU is only slightly less likely. It may be the most massive planet currently known around a red dwarf star (though only lower limits are known for those planets detected by the radial velocity method).

OGLE-2007-BLG-349(AB)b is a circumbinary extrasolar planet about 8,000 light-years away in the constellation of Sagittarius. It is the first circumbinary exoplanet to be discovered using the microlensing method of detecting exoplanets.

OFP La Rochelle-Maritime Rail Services

OGAE Second Chance Contest 2001

OGAS (Russian: Общегосударственная автоматизированная система учёта и обработки информации, All-State Automated System) was a Soviet project to create a nationwide information network. The project began in 1962 but was denied necessary funding in 1970. It was one of a series of attempts to create a nationwide network analogous to what became the Internet, all of which failed.The primary architect of OGAS was Viktor Glushkov. A previous proposal for a national computer network to improve central planning, Anatolii Kitov's Economic Automated Management System, had been rejected in 1959 because of concerns in the military that they would be required to share information with civilian planners. Glushkov proposed OGAS in 1962 as a three-tier network with a computer centre in Moscow, up to 200 midlevel centres in other major cities, and up to 20,000 local terminals in economically significant locations, communicating in real time using the existing telephone infrastructure. The structure would also permit any terminal to communicate with any other. Glushkov further proposed using the system to move the Soviet Union towards a moneyless economy, using the system for electronic payments. The project failed because Glushkov's request for funding on 1 October 1970 was turned down. The 24th Communist Party Congress in 1971 was to have authorised implementation of the plan, but ultimately endorsed only expansion of local information management systems. Glushkov subsequently pursued another network plan, EGSVT, which was also underfunded and not carried out. Soviet network plans failed while the American ARPANET succeeded.The OGAS proposal was resented by some liberals as excessive central control, but failed primarily because of bureaucratic infighting: it was under the auspices of the Central Statistical Administration and as such fell afoul of Vasily Garbuzov, who saw a threat to his Ministry of Finance. When EGSVT failed, the next attempt (SOFE) was done in 1964 by Nikolay Fedorenko, who attempted to build an information network that could be used in economic planning in Soviet Union's planned economy. The project was successful at a micro-level but did not spread into wide use.

OFV

OFW Diaries was a television show in the Philippines aired Friday evenings by GMA Network. The program was hosted by journalist Kara David, who previously hosted Case Unclosed.

OGAE Second Chance Contest 1989

OFTA

Black

Power and heat

Hubble Space Telescope

OFW Diaries

Ogags was a prime time variety/comedy show on the Philippines produced by TV5 (Philippines) The ''Kapatid'' Network. The show broadcasts from (formerly known as ABC 5) a major Filipino television network. Studios based in Mandaluyong City, Philippines. Aired weekly on Wednesday nights at 8:30 pm for 1 hour.The show Ogags was filled with comedy sketches, performance by the main host Ariana Barouk with her co-hosts and guests.

K5V?

OGLE-2005-BLG-071Lb is a planet discovered by the Optical Gravitational Lensing Experiment (OGLE) and others in 2005, using gravitational microlensing. According to the best fit model, it has about 3.5 times the mass of Jupiter and a projected separation of 3.6 astronomical units from the star. This would result in an effective temperature around 50 K, similar to that of Neptune.

OGLE-TR 122

OGAE Second Chance Contest 1990

OGLE-2014-BLG-0124Lb is one of the farthest planets that we know of today. It is approximately 13,000 light years away, located near the center of the galaxy. The planet was discovered using a technique called microlensing. In this case it took 150 days. Two telescopes are used to detect the planet and the time difference between identification by each telescope is used to calculate the distance to the planet. This also contributes to determining the mass of the planet which is about half of Jupiter's. The planet orbits a star with a mass of 0.7 solar masses and is 3.1 AUs from it.

OGLE-TR-056b

OF Mueller

OFS Studio Theatre

OGLE-TR-132 b

OGAE Second Chance 1989

Opioid growth factor receptor, also known as OGFr or the ζ-opioid receptor, is a protein which in humans is encoded by the OGFR gene. The protein encoded by this gene is a receptor for opioid growth factor (OGF), also known as [Met(5)]-enkephalin. The endogenous ligand is thus a known opioid peptide, and OGFr was originally discovered and named as a new opioid receptor zeta (ζ).

approx. 12,700

transit found in 2002,

OGC Nice in European football

OGLE-TR-113b is an extrasolar planet orbiting the star OGLE-TR-113.In 2002 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet, radial velocity measurements were necessary to calculate the mass of the body. In 2004, the object was proved to be a new transiting extrasolar planet.The planet has a mass 1.32 times that of Jupiter.

OFRB

OGAE Second Chance Contest 2009

OGLE-2006-BLG-109L (where 'L' stands for lens) is a dim magnitude 17 M0V galactic bulge star approximately 4,920 light-years away in the constellation of Scorpius.

OGK-3

OFWAT

Rolf Mahilom

OGA (disambiguation)

The OFSAA cross country championships are the Ontario high school cross country championships, held annually in varying locations around Ontario, usually on the first Saturday of November. Approximately 1600 runners compete in six races, making it the largest OFSAA meet of any sport.

The Sixth Wholesale Power Market Generating Company JSC (OGK-6) was a Russian power generation company formed by merger of six generation companies.

Public

OGLE-TR-113b is an extrasolar planet orbiting the star OGLE-TR-113.In 2002 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet, radial velocity measurements were necessary to calculate the mass of the body. In 2004, the object was proved to be a new transiting extrasolar planet.The planet has a mass 1.32 times that of Jupiter. Since the planet's inclination is known, the value is exact. It orbits the star (OGLE-TR-113) in an extremely close orbit, even closer than the famous planets 51 Pegasi b and HD 209458 b. The planet races around the star every 1.43 days. The radius of the planet is only 9% larger than Jupiter's, despite the heating effect by the star. Planets of its kind are sometimes called "super-hot Jupiters".

OGAE Second Chance 1987

OGAE Second Chance Contest 1988

OFallon Township High School District 203

approx. 3900

OAO Optovaya Generiruyushchaya Kompaniya 3

OG04

OGAE Video Contest

OGLE-TR-123b

ΟΦ Νέας Ιωνίας

OG's Theme

OG107

OF Nea Ionia (Greek: Όμιλος Φιλάθλων Νέας Ιωνίας/ΟΦ Νέας Ιωνίας) is a Greek handball club, based in Nea Ionia, Athens. It was founded in 1926. The club dominates in women handball, winning the most of the last championships and cups. The team's colours are cyan and white.

OGK-2

OGLE-TR-111

Marjan Kolev

OGDCL Institute of Science and Technology

OGA Golf Course

رَبِّ زدْنيِ عِلْماً

OFT v Abbey

OGAE Second Chance 2005

OFR (disambiguation)

OGAE Video Contest 2007

OGLE-2003-BLG-235/MOA 2003-BLG-53 was a gravitational microlensing event which occurred in the constellation of Sagittarius during July 2003. The event was observed both as part of the Optical Gravitational Lensing Experiment (OGLE) and by the Microlensing Observations in Astrophysics group (MOA), hence the double designation. The source star in the gravitational lens is a main sequence star of spectral type G located around 8.8 kiloparsecs (29,000 light years) away in the galactic bulge. The lens star is an orange dwarf star of spectral type K, which is accompanied by a giant planet.

OGLE-2007-BLG-368Lb is an extrasolar planet located approximately 19,230 light-years away in the constellation of Scorpius, orbiting the star OGLE-2007-BLG-368L. This planet was detected on December 8, 2009 by the gravitational microlensing by Sumi. It has mass 6.94% of Jupiter (i.e. 22 times that of Earth) and is located 3.3 AU from the star when observed. Based on those properties it would classify as a Cold Neptune. It is the second Cold Neptune to be observed, the first being OGLE-2005-BLG-169Lb. This planet is most likely be similar to Uranus and Neptune in the solar system in terms of atmospheric and internal properties.

Arts at the Old Fire Station (OFS, formerly the Old Fire Station Theatre and Old Fire Station Arts Centre) is a social enterprise in Oxford (40 George Street or Gloucester Green, Oxford, OX1 2AQ) comprising a gallery, theatre and studio for dance, drama and music, workshops for artists as well as a shop selling original work by artists and designers.

OF ep

Philippe Guillard

OGG Theora

Maxim Kuznetsov

OFX (disambiguation)

OGAE Second Chance 2006

Perci M. Intalan

OFallon Missouri

Merged intoInter RAO

OGB

OGAE Second Chance Contest 2013

OFWGKTA

Anthony Pastorpide

OGLE-2007-BLG-368Lb is an extrasolar planet located approximately 19,230 light-years away in the constellation of Scorpius, orbiting the star OGLE-2007-BLG-368L. This planet was detected on December 8, 2009 by the gravitational microlensing by Sumi. It has mass 6.94% of Jupiter (i.e. 22 times that of Earth) and is located 3.3 AU from the star when observed. Based on those properties it would classify as a Cold Neptune.

OGDC

OFWGKTADGAF

Konacki et al.

OFallon, Missouri

OGC (disambiguation)

OFT

OGITW

Rose C Camina

OGLE-TR-111b is an extrasolar planet approximately 5,000 light-years away in the constellation of Carina (the Keel). The planet is currently the only confirmed planet orbiting the star OGLE-TR-111 (though a possible second planet is plausible).In 2002 the Optical Gravitational Lensing Experiment (OGLE) survey detected that the light from the star periodically dimmed very slightly every 4 days, indicating a planet-sized body transiting the star. But since the mass of the object had not been measured, it was not clear that it was a true planet, low-mass red dwarf or something else.. In 2004 radial velocity measurements showed unambiguously that the transiting body is indeed a planet.The planet is probably very similar to the other hot Jupiters orbiting nearby stars. Its mass is about half that of Jupiter and it orbits the star at a distance less than 1/20th that of Earth from the Sun.OGLE-TR-111b has similar mass and orbital distance as the first transiting planet, HD 209458 b (Osiris). But unlike it, the planet has a radius comparable to Jupiter which is typical to other transiting planets detected by OGLE. However, those other planets tend to be more massive and orbit even closer than typical hot Jupiters. Therefore this planet is an important "missing link" between the different types of transiting planets.

OGLE-TR-122

proved to be a planet

OFS Studio

Electricity

OGK-3 (meaning: The Third Generation Company of the Wholesale Electricity Market – WGC-3) was a Russian power company. The stock was traded on the MICEX-RTS stock exchange.

OGLE-TR-122 is a binary stellar system containing one of the smallest main-sequence stars whose radius has been measured. It was discovered when the Optical Gravitational Lensing Experiment (OGLE) survey observed the smaller star eclipsing the larger primary. The orbital period is approximately 7.3 days.

OGDH (gene)

OGDCL Institute of Science and Technology also referred to as OIST is postgraduate institute affiliated with Quaid-i-Azam University located in Islamabad. OIST commenced classes in May, 2013 with an intake of 30 students, in affiliation with Quaid-i-Azam University.

OGAE Video Contest 2003

OGIZ

OFallon, IL

The First Generation Company of the Wholesale Electricity Market (OGK-1) was a large Russian company formed by the merger of six electricity generation companies.

OGG Airport

OGDB

Bennett et al.

OGF (disambiguation)

OJSC OGK-1

OGLE-TR-211

OGLE-TR-113b

OGLE-2005-BLG-169Lb is an extrasolar planet located approximately 2700 parsecs away in the constellation of Sagittarius, orbiting the star OGLE-2005-BLG-169L. This planet was discovered by the OGLE project using the gravitational microlensing method. Based on a most likely mass for the host star of 0.49 solar mass (M☉), the planet has a mass of 13 times that of Earth (M⊕). Its mass and estimated temperature are close to those of Uranus. It is speculated that this planet may either be an ice giant like Uranus, or a "naked super-Earth" with a solid icy or rocky surface.

OG56

OG47

> 0.7 billion

Russia

OGAE Second Chance 2008

OFP La Rochelle

JSC The Third Generation Company of Wholesale Electric Market –

OGLE-TR-111c

OGE (disambiguation)

OFUNAM

OGK-6

OGAE Second Chance Contest 2006

OGAE Second Chance Contest 1997

OGLE-TR-111b is an extrasolar planet approximately 5,000 light-years away in the constellation of Carina (the Keel). The planet is currently the only confirmed planet orbiting the star OGLE-TR-111 (though a possible second planet is plausible).In 2002 the Optical Gravitational Lensing Experiment (OGLE) survey detected that the light from the star periodically dimmed very slightly every 4 days, indicating a planet-sized body transiting the star.

Gaudi and

OGK-5

OGFC

The OGC Reference Model describes a framework for the ongoing work of the Open Geospatial Consortium (OGC) and their specifications and implementing interoperable solutions and applications for geospatial services, data, and applications. It is not an OGC standard.It has the following purposes:Provides a foundation for coordination and understanding (both internal and external to OGC) of ongoing OGC activities and the Technical Baseline;Update/Replacement of parts of the 1998 OpenGIS Guide;Describes the OGC requirements baseline for geospatial interoperability;Describes the OGC architecture framework through a series of non-overlapping viewpoints: including existing and future elements;Regularize the development of domain-specific interoperability architectures by providing examples.

OGFr_N

t approach

OGAE Video Contest 2006

F /M

OG45

OGCBuying.Solutions

OGC

OGLE-TR+113

Intel and Nokia

Various cities

OGLE-2005-BLG-071L b

OGAE Second Chance Contest 1996

OGFR (gene)

joint stock

Aki Niemi, Marcel Holtmann, Denis Kenzior, Claudio Takahasi, etc.

OGAE Video Contest 2014

OGAE Second Chance Contest 1987

OGAE Second Chance Contest 1998

NAME+OGLE-TR+56b

OFSAA cross country

OGLE-2006-BLG-109Lc is an extrasolar planet approximately 4,920 light-years away in the constellation of Sagittarius. The planet was detected orbiting the star OGLE-2006-BLG-109L in 2008 by a research team using Microlensing. The host star is about 50% the mass of the Sun and the planet is about 90% the mass of Saturn.

Transit

OGLE-TR-111 b

OGAE Second Chance Contest 1994

OGK-1

Electrical power and heat

Power generation

O my Lord! Advance me in Knowledge

alpha

OGEL

OGE Energy Corp.

OGLE-TR-111b

OGAE Second Chance Contest 2000

OGLE-TR-56 b

OFWGKTΔ

OGLE-2014-BLG-0124Lb is one of the farthest planets that we know of today. It is approximately 13,000 light years away, located near the center of the galaxy. The planet was discovered using a technique called microlensing. In this case it took 150 days. Two telescopes are used to detect the planet and the time difference between identification by each telescope is used to calculate the distance to the planet.

Merged withOGK-2

NAME+OGLE-TR-111b

OGAWA Seiyo

OGAE Second Chance Contest 2005

OGAGS

? /M

OGA

OFris

NAME+OGLE-TR+211b

Ange Ferracci

OAO Оптовая генерирующая компания № 2

OGLE-TR-211 b

OGLE-TR-56b is an extrasolar planet located approximately 1500 parsecs away in the constellation of Sagittarius, orbiting the star OGLE-TR-56. This planet was discovered on November 3, 2002 by the OGLE project using the transit method and confirmed on January 4, 2003 by the Doppler technique. The period of this confirmed planet was the shortest until the confirmed discovery of WASP-12b on April 1, 2008.

OGE Energy Corp

OGLE-TR-10 b

OGAE Video Contest 2008

OGLE-TR-122 is a binary stellar system containing one of the smallest main-sequence stars whose radius has been measured. It was discovered when the Optical Gravitational Lensing Experiment (OGLE) survey observed the smaller star eclipsing the larger primary. The orbital period is approximately 7.3 days. The system's primary is thought to resemble the Sun.The smaller star, OGLE-TR-122B, is estimated to have a radius around 0.12 solar radii, or around 20% larger than Jupiter's, and a mass of around 0.1 solar masses, or approximately 100 times Jupiter's. This makes its average density approximately 50 times the Sun's or over 80 times the density of water. OGLE-TR-122b's mass is close to the lowest possible mass for a hydrogen-fusing star, estimated to be around 0.07 or 0.08 solar masses. The observed transit provides the first direct evidence for a star with a radius comparable to Jupiter's.

ferroalloys, wires, construction materials

OGLE-TR-113 b

Portland, and Hillsboro

Arts at the Old Fire Station (OFS, formerly the Old Fire Station Theatre and Old Fire Station Arts Centre) is a social enterprise in Oxford (40 George Street or Gloucester Green, Oxford, OX1 2AQ) comprising a gallery, theatre and studio for dance, drama and music, workshops for artists as well as a shop selling original work by artists and designers. There are studios available to hire for classes, rehearsals and meetings.Arts at the Old Fire Station was redeveloped in 2011 for use as a Crisis Skylight Centre. Crisis Skylight Oxford is a training centre providing creative and formal learning opportunities to homeless and vulnerably housed people and a dedicated employment service which helps them find and keep jobs. The Crisis Skylight Cafe provides on-the-job training as well as food and drink to the wider public.

OG53

cyan, white

OGLE-TR-211b is a transiting planet in Carina constellation. Its radius is about 36% more than Jupiter and has mass 3% more than Jupiter, which is considered an “inflated Hot Jupiter”. The planet takes 3.7 days at about the same distance as 51 Pegasi b orbits around 51 Pegasi.

OFWs

OF Ouragan

Robert Quebral

OGBL

M / M

OGLE-TR-56b

OGLE-TR-182 is a dim magnitude 17 star far off in the constellation Carina at a distance of approximately 12,700 light years.

OG03

approx. 11000

OGLE-TR-10b/version 2

OGLE-2005-BLG-390L b

OGLE-2006-BLG-109L c

OGLE-TR-123

approx. 12700

OGLE-2005-BLG-169L b

OGAE Second Chance Contest 2014

approx. 17300

OAO Optovaya Generiruyushchaya Kompaniya 1

OF (disambiguation)

OFT (disambiguation)

OAO Optovaya Generiruyushchaya Kompaniya 2

OGLE-TR-132 is a distant magnitude 15.72 star in the star fields of the constellation Carina. Because of its great distance, about 4900 light years, and location in the crowded field it was not notable in any way. Spectral type of the star is type F yellow-white very metal rich dwarf star, slightly hotter and more luminous than the Sun.

OFTC

OGDCL

OGAE Second Chance Contest 2008

OF star

OFP La Rochelle is a rail freight company; a joint venture between Euro Cargo Rail and the port of La Rochelle. The company's first operations began in October 2010.

Ogags was a prime time variety/comedy show on the Philippines produced by TV5 (Philippines) The ''Kapatid'' Network. The show broadcasts from (formerly known as ABC 5) a major Filipino television network. Studios based in Mandaluyong City, Philippines. Aired weekly on Wednesday nights at 8:30 pm for 1 hour.The show Ogags was filled with comedy sketches, performance by the main host Ariana Barouk with her co-hosts and guests. The concept of the show was a foreigner trying to speak Tagalog and mispronouncing the words. The script was never given to the foreign hosts, it was purposely read on camera, to make fun of the foreigner trying to pronounce each Tagalog word.The show had various addition segments that featured almost stunt-like acts from crazy groups like The Calamity Fun, The Ogagsters in "Silent Lamay" featuring RJ! also joined by Gomz, Mad Killah, Caloy Alde and other celebrities. And the Smurfets! OGAGS was taped throughout the many Islands of the Philippines. Upon the station being taken over by new management the network re-vamped and many shows were cancelled and replaced by new ones, as was Ogags in 2010.

OJSC OGK-2

OGG1

OGLE-2003-BLG-235/MOA 2003-BLG-53 was a gravitational microlensing event which occurred in the constellation of Sagittarius during July 2003. The event was observed both as part of the Optical Gravitational Lensing Experiment (OGLE) and by the Microlensing Observations in Astrophysics group (MOA), hence the double designation. The source star in the gravitational lens is a main sequence star of spectral type G located around 8.8 kiloparsecs (29,000 light years) away in the galactic bulge.

OGAE Second Chance Contest 2012

OFTP2

OGLE-TR-56b is an extrasolar planet located approximately 1500 parsecs away in the constellation of Sagittarius, orbiting the star OGLE-TR-56. This planet was discovered on November 3, 2002 by the OGLE project using the transit method and confirmed on January 4, 2003 by the Doppler technique. The period of this confirmed planet was the shortest until the confirmed discovery of WASP-12b on April 1, 2008. The short period and proximity of the OGLE-TR-56 b to its host mean it belongs to a class of objects known as hot Jupiters.The planet is theorized to have iron rain.

OGB-L

The Orquesta Filarmónica de la UNAM (National Autonomous University of Mexico's Philharmonic Orchestra, also known as OFUNAM) was founded in 1936 and is the oldest symphonic group in Mexico City. It is based at Sala Nezahuacóyotl at the University City of the National Autonomous University of Mexico, in Mexico City. It was the first orchestra in Mexico to present annual concert seasons. Also, it is already a tradition that the orchestra presents an annual program of Mexican symphonic music.Some consider OFUNAM was created in 1929 when, soon after the obtainment of UNAM's autonomy, a group of students and professors set an orchestra at the Faculty of Music. However, it was officially founded in 1936, with the official approval granted by Lázaro Cárdenas's government. The original name was Orquesta Sinfónica de la Universidad (University's Symphonic University) and was conducted by José F. Vásquez and José Rocabruna. The orchestra was based at Anfiteatro Simón Bolívar.In 1966, a new base was assigned: Auditorio Justo Sierra at the Faculty of Philosophy and Literature. In 1966, the assignment of a new art director, Eduardo Mata, established the start of a new period, when UNAM's Symphonic Orchestra became UNAM's Philharmonic Orchestra (OFUNAM). During this period the orchestra’s name was changed and became Orquesta Filamonica de la UNAM. Hector Quintanar was appointed artistic director in 1975. The following year, the orchestra moved to its actual home, the Sala Nezahualcóyotl. From 1981 until 1984, the artistic responsibilities were in the hands of a tandem of associate conductors: Enrique Diemecke and Eduardo Diazmuñoz. From 1985 until 1989, it was Jorge Velzaco’s turn to be artistic director. He was followed by Jesús Medina, from 1989 unntil 1993. In 1994, Ronald Zollmhan became the new artistic director, a post he held during eight years, until 2002. Zuohuang Chen was the conductor from 2002 to 2006. In 2006, OFUNAM celebrated its 70th anniversary, Sala Nezahualcóyotl's 30th anniversary, as well as Mozart's 250th birth anniversary and Shostakovich's 100th birth anniversary. The Welsh Alun Francis followed Chen in 2007, assisted by the Mexican Rodrigo Macias. Presently, Massimo Quarta is the OFUNAM's artistic conductor.

OGAE Video Contest 2004

OGG1 (gene)

OAO Оптовая генерирующая компания № 3

Europe

approx. 3300

oFono is a free software project for mobile telephony (GSM/UMTS) applications. It is built on 3GPP standards and uses a high-level D-Bus API for use by telephony applications. oFono is free software released under the terms of the GNU General Public License v2.

OGI

OGLE-TR-123 is a binary stellar system containing one of the smallest main-sequence stars whose radius has been measured. It was discovered when the Optical Gravitational Lensing Experiment (OGLE) survey observed the smaller star eclipsing the larger primary. The orbital period is approximately 1.80 days.The smaller star, OGLE-TR-123b, is estimated to have a radius around 0.13 solar radii, and a mass of around 0.085 solar masses (M☉), or approximately 90 times Jupiter's. OGLE-TR-123b's mass is close to the lowest possible mass, estimated to be around 0.07 or 0.08 M☉, for a hydrogen-fusing star. OGLE-TR-123b is the second star with mass less than 0.1 M☉ whose radius has been directly measured; the first such star was the similar OGLE-TR-122b.

OGDC (disambiguation)

OGG Vorbis

OGK-2 is a Russian power generation company. Majority of the company's stock is owned by Gazprom.

Opioid growth factor receptor, also known as OGFr or the ζ-opioid receptor, is a protein which in humans is encoded by the OGFR gene. The protein encoded by this gene is a receptor for opioid growth factor (OGF), also known as [Met(5)]-enkephalin. The endogenous ligand is thus a known opioid peptide, and OGFr was originally discovered and named as a new opioid receptor zeta (ζ). However it was subsequently found that it shares little sequence similarity with the other opioid receptors, and has quite different function.

OGAE Second Chance Contest 2002

OGFr_III

The Orquesta Filarmónica de la UNAM (National Autonomous University of Mexico's Philharmonic Orchestra, also known as OFUNAM) was founded in 1936 and is the oldest symphonic group in Mexico City. It is based at Sala Nezahuacóyotl at the University City of the National Autonomous University of Mexico, in Mexico City. It was the first orchestra in Mexico to present annual concert seasons.

OGEL Journal

approx. 5300

OGAE Second Chance Contest 1993

OJSC OGK-6

OGLE-TR-123 is a binary stellar system containing one of the smallest main-sequence stars whose radius has been measured. It was discovered when the Optical Gravitational Lensing Experiment (OGLE) survey observed the smaller star eclipsing the larger primary. The orbital period is approximately 1.80 days.The smaller star, OGLE-TR-123b, is estimated to have a radius around 0.13 solar radii, and a mass of around 0.085 solar masses (M☉), or approximately 90 times Jupiter's.

Transit and Doppler

Istebné, Slovakia

OFono

OGLE2-TR-L9 b

OFWGK†A

OFTA (disambiguation)

OFf-Line Text System

OGLE-390

OGAE Second Chance Contest 1992

Mobile

OGLE-TR-211b

Sumi et al.

OGLE-TR 122B

OGLE-tr-122b

OGD (disambiguation)

OGLE-TR-182b

Alexey Mityushov

NAME+OGLE-TR-113b

OGC Reference Model

OFT 1