OpenLLM-France/wikimedia huggingface dataset:
# Gábor Török (political scientist)

Gábor Török (born 11 August 1971) is a Hungarian political scientist and historian, associate professor at the Institute of Political Science of the Corvinus University of Budapest.

## Biography

Gábor Török was born in Szombathely on 11 August 1971. He graduated from Nagy Lajos Secondary School, located in Szombathely, in 1989. He received his diplomas from the Eötvös Loránd University in history and political theory, both with distinction. In 1997, he placed first in the National Academic Student Conference. He received the Pro Scientia gold-medal in 1998 for excellence in studies and preeminent academic achievement. He earned his PhD summa cum laude from the Faculty of Law and Political Sciences in 2005.
He teaches at the Corvinus University of Budapest since 1997. Currently, he is the head of the Center for Political Analysis at the universities Institute of Political Science. He is an associate professor since 2009. He was awarded a certificate of merit by the rector of the university in 2005 in appreciation of his teaching and research work. He received the „ Teacher of the year” award in 2008. He is a visiting lecturer at the Zsigmond Király College, the Delta Political School, Századvég Political School as well as the Academy of Drama and Film.
Török was elected to the local representative body in Aszófő during the Hungarian local elections in 2010. He planned to run as an independent candidate in the parliamentary by-election at Veszprém in early 2015, however, following the outbreak of the so-called "Orbán–Simicska media war", stepped down.

## Works

He specializes in the analysis of the political system following the regime change, as well as in political and strategic analysis; wrote his doctoral dissertation on the topic of political agendas. He was a writer, co-writer or editor of eight books, of which two are widely used university text-books in Hungary. He was elected the secretary-general of the Hungarian Political Association for three years respectively in the years 2000 and 2003. Member of the presidium of the association since 2006.

### Main publications

* András Körösényi - Csaba Tóth - Gábor Török (2009): The Hungarian Political System. Hungarian Democracy Series. Volume 1. Budapest, Hungarian Center for Democracy Studies Foundation
* Török, Gábor (2005): A politikai napirend (Political Agenda). Budapest, Akadémiai Kiadó.
* Török Gábor (2012): The Political System in Hungary. In Wojciech Gizicki (ed): Political Systems of Visegrad Group Countries. Trnava-Lublin, 43–70.
* Török, Gábor (2017): A lakott sziget (Inhabited Island). Budapest, Atheneum Kiadó.
# Güneyçayırı, Elâzığ

Güneyçayırı is a village in the Elazığ District of Elazığ Province in Turkey. Its population is 3,757 (2021).
# Güler Ökten

Servet Güler Kıpçak Ökten (born 14 November 1941) is a Turkish actress. She is best known for her roles in Bizimkiler as Türkan and in Yaprak Dökümü as Cevriye.
A graduate of conservatory, she was among the students trained by Yıldız Kenter. Her father, Kani Kıpçak, was an actor and director as well. Ökten started her acting career in 1947 with a small role in a movie. She started appearing on stage in 1960 and appeared in many movies and TV series afterwards.

## Filmography

* Bir Demet Menekşe – 1973
* Kapıcılar Kralı – 1976
* Şabanoğlu Şaban – 1977
* Seninle Son Defa – 1978
* Sürü – 1978
* İsyan – 1979
* Demiryolu – 1979
* At – 1981
* Kırık Bir Aşk Hikayesi – 1981
* Fidan – 1984
* Bir Kadın Bir Hayat – 1985
* Gülüşan – 1985
* Asiye Nasıl Kurtulur? – 1986
* Bekçi – 1986
* Asılacak Kadın – 1986
* Ses [tr] – 1986
* Dilan – 1986
* Afife Jale – 1987
* Biri ve Diğerleri – 1987
* Hüzün Çemberi – 1988
* Geçmiş Bahar Mimozaları – 1989
* Bizimkiler – 1989
* Cahide – 1989
* Hiçbir Gece – 1989
* Çiçekler Boy Verince – 1990
* Bir Milyara Bir Çocuk – 1990
* Yıldızlar Gece Büyür – 1991
* Acılar ve Arzular – 1991
* Yazlıkçılar – 1993
* Saygılar Bizden – 1993
* C Blok – 1993
* Ali / Sakın Arkana Bakma – 1996
* Baba Evi – 1997
* Mektup – 1997
* Kaçıklık Diploması – 1998
* Günaydın İstanbul Kardeş – 1999
* Güle Güle – 1999
* Beni Unutma – 2000
* Bana Şans Dile – 2001
* Canım Kocacığım – 2002
* Gülüm – 2002
* Bana Abi De – 2002
* Sultan Makamı – 2003
* Kalbin Zamanı – 2004
* Perili Ev – 2004
* Çemberimde Gül Oya – 2004 (guest appearance)
* Hırsız Polis – 2005–2006
* Erkek Tarafı – 2005
* Sen Ne Dilersen – 2005
* Kabuslar Evi: Tanıdık Yabancı – 2006
* Yaprak Dökümü – 2007–2010 – Cevriye
* Leyla ile Mecnun – 2011–2012
* Karanlıklar Çiçeği – 2012
* İntikam – 2013 (guest appearance)
* Kara Para Aşk – 2014
* İtirazım Var – 2014 – Ani Hanım
* Aşk ve Gurur – 2017 – Gülnaz Işıl
* Cennet'in Gözyaşları – 2017
* Yürek Çıkmazı – 2022
# Gurkovo, Dobrich Province

Gurkovo is a village in Balchik Municipality, Dobrich Province, northeastern Bulgaria. Between 1913 and 1940, during the Romanian rule, the village was called Rasoviceni.
# Gwalior trade fair

The Gwalior Trade Fair is the largest trade fair in India. It was started in 1905 by the King of Gwalior, Maharaj Madhav Rao Scindia.
Gwalior trade fair consists of large showrooms of several national and international brands such as Audi, Mercedes, BMW, Samsung, and LG along with food zones, amusement rides, shops of clothes, bags, electronics, mobiles, laptops, cars, bikes, buses, trucks etc.

## Location

Covering 104 acres (0.42 km$^2$) and divided into several 'blocks' and 'sectors', the Mela (Hindi for fair) Ground at Race Course Road is known as the Pragati Maidan of Madhya Pradesh, India. The Gwalior Trade Fair Authority, an autonomous body, is responsible for the administration of the Fair.

## Attractions

Major attractions of the fair include the "Haasya Kavi Sammelan" (the poet's gathering), the "Kavvali Dangals", the "Mushairas", Cultural Evenings, Music Nights, and several other activities integral to the Mela.
The cattle trade fair is an integral part of the Fair, with about 10,000 animals being sold or bought each year.
Shilp Bazaar is a beautiful attraction of Gwalior Trade Fair. In this bazaar, different types of handmade things are sold by people from all over India.
Many attractive and decorated rides, shops and circuses attract people in Gwalior Trade Fair.
# Gymnopilus karnalensis

Gymnopilus karnalensis is a species of mushroom in the family Hymenogastraceae.
# Gymnopilus konkinyerius

Gymnopilus konkinyerius is a species of mushroom in the family Hymenogastraceae.
# Gyraulus acronicus

Gyraulus acronicus is a small species of freshwater snail, an aquatic pulmonate gastropod mollusk in the family Planorbidae, the ram's horn snails.

## Distribution

The distribution of this species is Holarctic.
It is known to occur in islands and countries including:
* Czech Republic
* Slovakia
* Germany - critically endangered (vom Aussterben bedroht)
* Poland - endangered
* Great Britain

## Description

The shell is nearly planispiral in its coiling.

## Habitat

This small snail lives on water plants in freshwater.
# Guzmania osyana

Guzmania osyana is a species of plant in the family Bromeliaceae. It is endemic to Ecuador. Its natural habitats are subtropical or tropical moist lowland forests and subtropical or tropical moist montane forests. It was last known to be threatened by habitat loss in 2003.
# Guzmania pseudospectabilis

Guzmania pseudospectabilis is a species of plant in the family Bromeliaceae. It is endemic to Ecuador. Its natural habitat is subtropical or tropical moist montane forests. It is threatened by habitat loss.
# Guzmania obtusiloba

Guzmania obtusiloba is a plant species in the genus Guzmania. This species is native to Costa Rica, Panama, and Colombia.
# H21

H21 or H-21 may refer to:
* British NVC community H21, a type of heath community in the British National Vegetation Classification
* Highway H21 (Ukraine)
* HMS H21, a Royal Navy H-class submarine
* HMS Scimitar (H21), a Royal Navy S-class destroyer
* Mata Hari (1876–1917), German spy code named H-21
* Piasecki H-21, an American helicopter
* Institute H21, a Czech think tank that created the website Prezident 21
# HD 141846

HD 141846 is a double star in the southern constellation of Apus. As of 1996, the pair have an angular separation of 0.7″ along a position angle of 332°.
# HD 142415

HD 142415 is a single star in the southern constellation of Norma, positioned next to the southern constellation border with Triangulum Australe and less than a degree to the west of NGC 6025. With an apparent visual magnitude of 7.33, it is too faint to be visible to the naked eye. The distance to this star is 116 light years from the Sun based on parallax, but it is drifting closer with a radial velocity of −12 km/s. It is a candidate member of the NGC 1901 open cluster of stars.
This is an ordinary G-type main-sequence star with a stellar classification of G1V. It has been identified as a solar twin by Datson et al. (2012), which means its physical properties are very similar to the Sun. It has 10% more mass than the Sun but only a 3% larger radius. The star is estimated to be 1.6 billion years old and is spinning with a projected rotational velocity of 4.2 km/s. It is radiating 1.16 times the luminosity of the Sun from its photosphere at an effective temperature of 5,869 K.
The star is currently known to have one planet, designated HD 142415 b. This was detected via the radial velocity method and announced in 2004. The orbital period is just over a year, which made a determination of the orbital eccentricity more difficult due to undersampling over part of the orbit, in combination with jitter. The authors chose to pin the eccentricity value to 0.5, although solutions in the range 0.2–0.8 would be equally plausible.
The HD 142415 planetary system :
| Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
| b | >1.62 M$_J$ | 1.05 | 386.3 ± 1.6 | 0.5(fixed) | — | — |
# HD 142

HD 142 is a wide binary star system in the southern constellation of Phoenix. The main component has a yellow-white hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.7. The system is located at a distance of 85.5 light years from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +6 km/s.
The primary component is an F-type main-sequence star with a stellar classification of F7V, which indicates it is undergoing core hydrogen fusion. It is an estimated 2.5 billion years old and is spinning with a projected rotational velocity of 10 km/s. The star has 1.25 times the mass of the Sun and 1.4 times the Sun's radius. It is radiating 2.9 times the luminosity of the Sun from its photosphere at an effective temperature of 6,338 K.
A magnitude 11.5 companion star was detected in 1894 making this a binary star system. The binary companion was confirmed to be gravitationally bound in 2007 and determined to be a red dwarf of spectral type K8.5-M1.5 with 54% of the Sun's mass. The pair have a projected separation of 120.6 AU.

## Planetary system

In 2001, the Anglo-Australian Planet Search team led by Chris Tinney announced the discovery of an extrasolar planet orbiting the primary star. An additional linear trend in the radial velocity data was noticed in 2006 that could have been due to another planet or to the stellar companion. In 2012, additional measurements allowed the detection of a second planet. A third possible planet with a period of 108 days was seen in the data, but with a false alarm probability of five percent. Another paper by the same team updated the parameters for b and c but did not mention the possible planet d.
An astrometric measurement of HD 142 b's inclination and true mass was published in 2022 as part of Gaia DR3. Another 2022 study determined the inclination and true mass of planet c, and confirmed the existence of planet d.
The HD 142 A planetary system :
| Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
| d | ≥0.260+0.032 −0.036 M$_J$ | 0.474+0.021 −0.023 | 108.5±0.1 | 0.130+0.103 −0.085 | — | — |
| b | 7.1±1.0 M$_J$ | 1.039+0.046 −0.051 | 351.4±0.4 | 0.158+0.033 −0.030 | 59±7° | — |
| c | 10.901+1.278 −0.937 M$_J$ | 9.811+0.515 −0.520 | 10,159.6+384.8 −321.9 | 0.277+0.026 −0.027 | 90.374+10.495 −12.319° | — |
# Gümüştaş, Çınar

Gümüştaş is a neighbourhood in the municipality and district of Çınar, Diyarbakır Province in Turkey. Its population is 1,103 (2022).
# Gümüşyayla, Çubuk

Gümüşyayla is a neighbourhood in the municipality and district of Çubuk, Ankara Province, Turkey. Its population is 103 (2022).
# HD 92209

HD 92209 (HR 4170) is a probable spectroscopic binary in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude of 6.29, placing it near the max naked eye visibility. Parallax measurements place the system at a distance of 600 light years and is currently receding with a heliocentric radial velocity of almost 18 km/s.
The visible component has a stellar classification of K2 III, indicating that it is a red giant. As a consequence, it has expanded to 14.39 times the radius of the Sun. Nevertheless, it has 122% the mass of the Sun and shines with a luminosity of 81.3 L$_☉$, yielding an effective temperature of 4,460 K from its enlarged photosphere, which in turn gives an orange hue. HD 92209 has a metallicity 115% that of the Sun and spins leisurely with a projected rotational velocity lower than 1 km/s.
# HAT-P-24

HAT-P-24 is an F8 dwarf star about 413 parsecs away. A planet was discovered with the transit method by the HATNet Project in 2010. HAT-P-24b, is a typical hot Jupiter orbiting in only 3 days.

## Planetary system

In 2010 the HATNet Project announced the discovery of a hot jupiter type gas giant extrasolar planet in orbit around this star. Following the designation scheme used by the HATNet Project, the star is designated as HAT-P-24, and the planet itself HAT-P-24b.
The HAT-P-24 planetary system :
| Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
| b | 0.723+0.031 −0.030 M$_J$ | 0.04651+0.00055 −0.00056 | 3.3552479±0.0000062 | <0.038 | 88.217 $^{+0.716}$ $_{−0.693}$° | 1.364 ± 0.068 R$_J$ |
# HAT-P-20

HAT-P-20 is a K-type main-sequence star about 233 light-years away. The star has a strong starspot activity, and its equatorial plane is misaligned by 36$^{+10}$ $_{−12}$° with the planetary orbit. Although star with a giant planet on close orbit is expected to be spun-up by tidal forces, only weak indications of tidal spin-up were detected.

## Planetary system

In 2010 a transiting hot super-Jovian planet was detected. Its equilibrium temperature is 996±19 K.
The HAT-P-20 planetary system :
| Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
| b | 7.59±0.12 M$_J$ | 0.03671±0.00027 | 2.8753172±0.0000003 | 0.0172±0.0016 | 86.3±0.1° | 0.952±0.017 R$_J$ |
# HMS Black Prince

Five ships of the British Royal Navy have been named HMS Black Prince, after Edward, the Black Prince (1330–1376), the eldest son of King Edward III of England.
* The first Black Prince was a 10-gun vessel purchased by the Royalists in March 1650, and burnt by Parliamentarians on 4 November of the same year.
* The second HMS Black Prince (1816) was a 74-gun third rate launched in 1816, in use as a prison ship after 1848, and broken up 1855.
* The third HMS Black Prince (1861), launched in 1861, was the second Warrior-class battleship. Retired to the reserve fleet in 1878; became a training ship in 1896; renamed Emerald in 1903; renamed Impregnable III in 1910; scrapped in 1923.
* The fourth HMS Black Prince (1904), launched in 1904, was a Duke of Edinburgh-class cruiser sunk with all hands during the Battle of Jutland in 1916.
* The fifth HMS Black Prince (81), launched in 1942, was a Dido-class (Bellona subclass) cruiser that saw extensive action in World War II, following which she was transferred to the Royal New Zealand Navy in 1946. She was decommissioned in 1962 and scrapped.

## Battle honours

Ships named Black Prince have earned the following battle honours:
* Jutland, 1916
* Arctic, 1944
* Normandy, 1944
* English Channel, 1944
* Aegean, 1944
* South France, 1944
* Okinawa, 1945
# H. Brandt Ayers

Harry Brandt Ayers, also known as Brandy Ayers (8 April 1935 - 3 May 2020) was a publisher and journalist based in Anniston, Alabama, part of the Ayers family of publishers.

## Early life

Ayers was born in Anniston, Alabama to Colonel Harry Mell Ayers and his wife. At that time Colonel Ayers was owner of the Anniston Star newspaper. Ayers attended Woodstock Elementary School, followed by The Wooster School in Danbury, Connecticut. He subsequently attended the University of Alabama, where he received his BA. Ayers served in the US Navy as an officer, following which he briefly worked for the Anniston Star before moving to work for a newspaper in Raleigh, North Carolina, where he met his wife Josephine.

## Publishing career

Ayers returned to Anniston in the 1960s to take over the family newspaper and succeed his father as publisher. During this time he moved the newspaper towards being more favourable towards the Civil rights movement that was active in Alabama during this time. Ayers also provided commentary for National Public Radio.
Under Ayers' leadership, the Star's critical stance towards the leadership of Alabama governor George Wallace, and generally left-wing position on the political issues of the day, led Wallace to label it The Red Star.
Ayers stood down as publisher of the Star in 2016, but remained in charge of the publishing company that owned it, Consolidated Publishing Co.

## Me Too controversy

In November 2017, during the Me Too movement, allegations that Ayers had physically assaulted female employees, in particular by spanking them, emerged. In January 2018 Ayers acknowledged that one of the incidents had occurred but claimed that this incident, which had occurred in his employee's home, had been on a doctor's advice to "calm her down". When confronted with a second incident that had occurred at the offices of the Star he stated that he would "Let the accusation stand". Subsequent research showed that allegations of spanking had been levelled against Ayers as early as 2007.
Ayers initially refused to resign as head of Consolidated Publishing in the wake of the allegations. However, as further incidents emerged he resigned from his post at Consolidated Publishing and was replaced by his wife. Ayers was listed amongst prominent media figures to have been the subject of sexual harassment, assault, or other misconduct allegations during the Me Too movement.
# HC Merano

HC Merano is a professional ice hockey team in Merano, Italy. They play in the Alps Hockey League

## History

Merano was founded in 1968. They won the Serie A twice, in 1986 and 1999. Since 2004 the club is playing in the 2nd highest league in Italy.

### Honours

* Serie A champion : 1986, 1999
* Serie A2 champion: 1971, 1978, 1991
* Serie B champion: 2016
* Serie C champion: 2009

## Notable players

* Rick Morocco
# HD 208741

HD 208741, also known as HR 8380, is a yellowish-white hued star located in the southern circumpolar constellation Octans. It has an apparent magnitude of 5.91, making it faintly visible to the naked eye. Parallax measurements place it at a distance of 211 light years, and it is currently receding with a heliocentric radial velocity of 8 km/s.
HD 208741 has a 10th magnitude K-type main-sequence companion separated by 34.8″. Together, they make up a wide binary system designated collectively as CPD−76°1542. Sir John Herschel, the discoverer of the pair, noted the primary to be a probable spectroscopic binary.
This object has a stellar classification of F3 III, indicating that it is a slightly evolved F-type star. Gaia Data Release 3 models it to be a dwarf that is 81.3% through its main sequence lifetime. At present it has 1.52 times the mass of the Sun and a slightly enlarged radius of 2.6 R$_☉$ due to its evolved state. It radiates at 12.9 times the luminosity of the Sun from its photosphere at an effective temperature of 6,937 K. HD 208741 has a metallicity twice the Sun's, making it metal enriched. It is estimated to be 1.1 billion years old, and is spinning with a projected rotational velocity of 36 km/s.
# HD 208177

HD 208177 is a double star system in the equatorial constellation of Aquarius. They are faintly visible to the naked eye with an apparent magnitude of 6.20. The pair have an angular separation of 19.113″. The primary component is an evolved subgiant star with a stellar classification of F5IV. It has an estimated 163% of the Sun's mass and is about 1.7 billion years old
# HD 44594

HD 44594 is a star in the southern constellation Puppis. It has an apparent visual magnitude of 6.64, so it can be seen with the naked eye from the southern hemisphere under good viewing conditions. Based upon parallax measurements, it is located at a distance of 85 light-years (26 parsecs) from the Earth, giving it an absolute magnitude of 4.56.
Measurement of the star's spectrum show it to match a stellar classification of G1.5V, which is close to the Sun's spectral class of G2V. In the wavelength range 3,250–8,750 Â, the energy emission of this star is very similar to the Sun, and thus it is considered a solar analog. The luminosity class 'V' means this is a main sequence star that is generating energy through the thermonuclear fusion of hydrogen at its core. The effective temperature of the outer envelope of HD 44594 is 5,840 K, which is giving it the characteristic yellow hue of a G-type star.
This star has about 108% of the Sun's mass and is about the same radius as the Sun. It may be slightly younger than the Sun with an estimated age of 4.1 billion years. the abundance of elements other than hydrogen or helium, what astronomers term the star's metallicity, is 41% higher than in the Sun. The projected rotational velocity of the star is 4.4 km/s, which gives the minimum azimuthal velocity along the star's equator.
This star has been examined in the infrared using the Spitzer Space Telescope. However, no excess emission was discovered, which might otherwise have indicated the presence of a circumstellar debris disk of orbiting dust. Gaia Data Release 3 shows a faint companion about 7″ away. The companion is 9 magnitudes fainter than the G-type star with an almost-identical parallax and common proper motion.
# HD 45350 b

HD 45350 b is an extrasolar planet located approximately 160 light-years away in the constellation of Auriga. It has a minimum mass about 1.79 times that of Jupiter. The mean distance of the planet from the star is more than the distance between Mars and the Sun, but due to the planet's high orbital eccentricity, it is as close to the star as Mercury is from the Sun at periastron, while at apastron, it is eight times further.
The planet HD 45350 b is named Peitruss. The name was selected in the NameExoWorlds campaign by Luxembourg, during the 100th anniversary of the IAU. Peitruss is derived from the name of the Luxembourg river Pétrusse. The 2019–2020 class of 3B from the Luxembourgish Echternach high school won the contest to name both the star and its planet. The students who helped name both celestial objects were Lucien Nicolas Berger, Léna Boucq Kieffel, Ben de Boer, Cédric Dehlez, Nicolas Delhez, Sergio Manuel Dias Costa, Pierre Fusshoeller, Jil Menei, Philippe Schaack and Claire Zeien. The overseeing committee members who organized the contest and the vote of the respective celestial objects were Eric Buttini, Patrick Michaely, Nicolas Faber, Jeanny-Jungbluth-Schmidt and Yanna Di Ronco.
Dynamical simulations covering a period of 10$^7$ years show that a second, low-mass, planet could only orbit stably if it were no more than 0.2 AU away from the star; in the simulations, these planets show oscillations in eccentricity up to an eccentricity of 0.25. Radial velocity observations rule out any such planet whose mass is greater than 4 Neptune masses.