OpenLLM-France/wikimedia huggingface dataset:
# Momoko 120%

Momoko 120% (モモコ120%, Momoko Hyakunijū Pāsento) is a 1986 arcade game by Jaleco released in Japan. The game was originally intended to be an Urusei Yatsura game, but for an unknown reason the license was not obtained for the arcade version—while the characters were changed, "Lum's Love Song" — the first opening theme of the first anime adaptation, still loops throughout the game, but the Family Computer port retained the license and was titled Urusei Yatsura: Lum's Wedding Bell. The game was re-released for mobile phones in Japan on February 28, 2006. Three mobile phone sequels, Momoko 1200%, Momoko 1200% in Machigai Sagashi and Momoko no Kasei Bowling ~La Mars Cup~, were released in Japan only in 2006.

## Gameplay

This platform game features Momoko, a young Japanese girl who ages by several years each time the player reaches the next level. The goal for each level is to quickly climb several floors by escalator, ladder, or trampoline in the building she is in before the fire that is below her reaches her. These level settings start out from grade school settings to office type buildings. While jumping over obstacles, she must shoot various alien-like enemies that come after her on each floor. She can upgrade her weapon by destroying certain enemies as well as entering special hidden doorways which feature minigames which require you to jump obstacles. These doorways can also be used as a short-cut, and sometimes they are mandatory to be used in order to climb to the next floor. When Momoko reaches the top floor of a level, she must jump onto a small blimp flying above her to beat the level. Momoko begins as a four-year-old and ages through five levels. The final level is a bonus chance in which she is a twenty-year-old bride collecting items – the game concludes with her getting married, thus giving birth to a new Momoko and starting the cycle anew.

## Urusei Yatsura: Lum's Wedding Bell

In Urusei Yatsura: Lum's Wedding Bell (うる星やつら ラムのウェディングベル, Urusei Yatsura: Ramu no Uedingu Beru), the player controls Lum as she grows up and has to avoid alien invaders while trying to reach her rescue UFO. The game's storyline involves a severe earthquake striking in Tomobiki-cho (the town where the Urusei Yatsura series takes place) and tearing the space-time continuum, forcing Lum to have to travel forward through time in order to be reunited with her "darling" Ataru Moroboshi.
The player starts out at infant school, then works her way to elementary school, junior high school, high school, college, and finally the player marries a bridegroom (Ataru) in a white tie outfit. After that, the game starts over again. The game has never been released outside Japan.

## Reception

In Japan, Game Machine listed Momoko 120% on their October 15, 1986 issue as being the tenth most-successful table arcade unit of the month.
# Kyōgoku Maria

Kyōgoku Maria (京極マリア) or Yōfuku-in (養福院) (1543 – August 20, 1618) was a Japanese noble lady and religious leader from the Sengoku period to the early Edo period. She was the second daughter of Azai Hisamasa as well as Azai Nagamasa's elder sister and the mother of Kyōgoku Takatsugu and Kyōgoku Takatomo. She was the mostly successful woman catechist with her own assistants as well as Naitō Julia and her women catechists. She faced the rules of samurai governments, staying true to her missionary campaigns even when Christianity was banned in Japan.

## Life

Her birth name is unknown, but she was given the name "Maria" after her conversion to Christianity. She was baptized with her husband Kyōgoku Takayoshi in the Jesuits church in Kyoto in 1581, though Takayoshi died soon after being baptized. After becoming a widow, she began preaching her new religion to people around her, and Jesuits named her one of the best female catechists of the Kyoto-Osaka area.
Sometime in 1606 or 1607, Maria moved to Wakasa Province under Takatsugu's protection, and in 1609 she moved again to a remote place in Tango Province to avoid the persecution of Christians. She died peacefully in a small hut belonging to a Buddhist nunnery Sengen-ji (泉源寺) in 1618.
One of her daughters, Kyōgoku Tatsuko, is notable for being one of Toyotomi Hideyoshi's favorite concubines.

## Family

* Father: Azai Hisamasa (1526–1573)
* Brother: Azai Nagamasa (1545–1573)
* Husband: Kyōgoku Takayoshi (1504–1581)
* Son: Kyōgoku Takatsugu (1563–1609), Kyōgoku Takatomo (1572–1622)
* Daughter: Kyōgoku Tatsuko (d. 1634), Kyōgoku Magdalena
* Niece: Ohatsu, (1570–1633)
# Juliusz Madecki

Juliusz Madecki (born 17 June 1979) is an Austrian rower. He competed in the men's lightweight coxless four event at the 2004 Summer Olympics.
# Lu Laysreng

Lu Laysreng (born 1938) is one of Cambodia's deputy prime ministers as well as the country's minister of rural development. He belongs to Funcinpec and was elected to represent Kampong Speu province in the National Assembly of Cambodia in 2003.
Lu was born in Phnom Penh, Cambodia, to Chinese immigrants from Jieyang but stayed in Swatow between the ages of six and fifteen for his primary and secondary education before returning to Cambodia. Lu pursued his university studies at California State University, Long Beach, also acquiring American citizenship before returning to Cambodia to serve in politics. After the 2003 elections, he was subsequently appointed as the Cambodian information minister, and is one of the key personalities instrumental in fostering the kingdom's closer ties with China.
In one interview, Lu mentioned that his Chinese name is "杨来盛", but that he was frequently addressed as "呂来盛", a transliteration of his Khmer name "Lu Lay Sreng". Lu is fluent in Khmer, Teochew and English.
# Ernie Myers

Ernie Myers is an American former basketball player. Myers is originally from East Harlem, New York. Myers went to high school in New York at Tolentine High School. He was recruited by Jim Valvano as a sophomore in high school, while he was playing against Rice High School (Manhattan, New York).

## North Carolina State

Myers was the ACC freethrow champion. During this time he also played at Riverside Church. For a time, he led North Carolina State in scoring. In 1983, he was a true Freshman. He was part of the team that went 26-10. He teamed with Cozell McQueen, Terry Gannon, Alvin Battle, Lorenzo Charles, Thurl Bailey, Dereck Whittenburg and Sidney Lowe to lead North Carolina State to the National Championships in 1983.
# (471240) 2011 BT15

(471240) 2011 BT$_{15}$, provisional designation 2011 BT$_{15}$, is a stony, sub-kilometer sized asteroid and fast rotator, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group. It had been one of the objects with the highest impact threat on the Palermo Technical Impact Hazard Scale.

## Discovery

It was discovered on 24 January 2011, by a team of astronomers at Pan-STARRS, the Panoramic Survey Telescope and Rapid Response System at Haleakala Observatory on Hawaii, United States. The discovery was made using a 1.8-meter Ritchey–Chrétien telescope. At the time of discovery, the object had an apparent magnitude of 22.

## Orbit

Before the 2013 recovery it had an observation arc of 41 days with an uncertainty parameter of 7. Due to precovery images from 2007 it now has an observation arc of more than 5 years. It makes close approaches to Earth and Mars.
On 28 December 2013, it passed 0.03222 AU (4,820,000 km) from Earth. The December 2013 passage was studied by the Goldstone Deep Space Network and further refined the orbit.

### Impact risk

While listed on the Sentry Risk Table, virtual clones of the asteroid that fit the uncertainty region in the known trajectory showed a 1 in 71,000 chance that the asteroid could impact Earth on 5 January 2080.
In 2013 it had the 5th highest impact threat on the Palermo Technical Impact Hazard Scale. It was removed from the Sentry Risk Table on 17 June 2013.
With a 2080 Palermo Technical Scale of −3.58, the odds of impact by 2011 BT$_{15}$ in 2080 were about 3800 times less than the background hazard level of Earth impacts which is defined as the average risk posed by objects of the same size or larger over the years until the date of the potential impact. JPL Horizons shows that the nominal pass will be on 17 January 2080 at a distance of 0.125 AU (18,700,000 km; 11,600,000 mi) from Earth.

## Physical characteristics

This near-Earth object is characterized as a common, stony S-type asteroid by the Collaborative Asteroid Lightcurve Link (CALL).

### Fast rotator

In January 2014, a rotational lightcurve of 2011 BT$_{15}$ was obtained from photometric observations by American astronomer Brian Warner at the CS3-Palmer Divide Station (U82) in California. Lightcurve analysis gave a well-defined rotation period of 0.109138 hours (393 seconds) with a brightness amplitude of 0.61 magnitude (U=3).

### Diameter and albedo

According to the CALL and JPL's impact-risk table, this near-Earth object measures 136 and 150 meters, respectively. For its size estimate, CALL uses a standard for stony asteroids of 0.20 with an absolute magnitude of 21.7.

## Naming

As of 2017, this minor planet remains unnamed.
# Greigia berteroi

Greigia berteroi is a species of flowering plant in the family Bromeliaceae. This species is endemic to the Juan Fernández Islands in the South Pacific, off the coast of Chile.
The species is listed as critically endangered.
# 1580 Betulia

1580 Betulia, provisional designation 1950 KA, is an eccentric, carbonaceous asteroid, classified as near-Earth object of the Amor group, approximately 4.2 kilometers in diameter. It was discovered on 22 May 1950, by South African astronomer Ernest Johnson at the Union Observatory in Johannesburg. The asteroid was named for Betulia Toro, wife of astronomer Samuel Herrick.

## Orbit and classification

Betulia orbits the Sun at a distance of 1.1–3.3 AU once every 3 years and 3 months (1,190 days). Its orbit has an eccentricity of 0.49 and an inclination of 52° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Johannesburg in 1950.

### Close approaches

Betulia is a near-Earth asteroid with an Earth minimum orbital intersection distance of 0.1365 AU (20,400,000 km), which corresponds to 53.2 lunar distances. As an Amor asteroid, and contrary to the Apollo and Aten asteroids, it approaches Earth's orbit from beyond but does not cross it. Betulia is also a Mars-crosser due to its eccentric orbit.

## Physical characteristics

In the Tholen classification, Betulia is an unusual C-type asteroid, as near-Earth objects are typically of stony rather than carbonaceous composition. Based on images taken by the Sloan Digital Sky Survey, the asteroid has also been characterized as a carbonaceous but "brighter" B-type asteroid.

### Rotation period

Several rotational lightcurves of Betulia were obtained from photometric observations since the 1970s. Analysis of the best-rated lightcurve gave a rotation period of 6.1324 hours with a brightness variation of 0.70 magnitude (U=3), indicating that the body has a non-spheroidal shape. Other observations gave a period between 6.130 and 6.48 hours.

### Poles

Photometric and radiometric observations of Betulia were also used to model the asteroid's lightcurve. It gave a concurring period of 6.13836 hours as well as a spin axis of (133.0°, 22.0°) and (136.0°, 22.0°) in ecliptic coordinates (λ, β), respectively. The results supersede previously determined rotational poles (also see LCDB summary).

### Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Radar observations at the Arecibo Observatory in Puerto Rico, Tom Gehrels estimate from the Hazards due to Comets and Asteroids, and observations by Alan W. Harris using the NASA Infrared Telescope Facility on Mauna Kea, Hawaii, Betulia measures between 3.82 and 8.55 kilometers in diameter and its surface has an albedo between 0.04 and 0.17.
The Collaborative Asteroid Lightcurve Link takes an albedo of 0.09 and a diameter of 4.2 kilometers as best estimates and adopts an absolute magnitude of 15.1.

## Naming

This minor planet was named after Betulia Toro Herrick, wife of Samuel Herrick (1911–1974), an American astronomer who specialized in celestial mechanics. Herrick had studied the asteroid's orbit, and requested the name, along with that of 1685 Toro. The official naming citation was published by the Minor Planet Center in May 1952 (M.P.C. 768).
# 1943 Anteros

1943 Anteros /ˈæntərɒs/, provisional designation 1973 EC, is a spheroidal, rare-type asteroid and near-Earth object of the Amor group, approximately 2 kilometers in diameter.
It was discovered on 13 March 1973, by American astronomer James Gibson at the Leoncito Astronomical Complex in Argentina, and named for the Greek god Anteros.

## Orbit and classification

Anteros is an Amor asteroid, which approach the orbit of Earth from beyond but do not cross it. It orbits the Sun at a distance of 1.1–1.8 AU once every 1 year and 9 months (625 days). Its orbit has an eccentricity of 0.26 and an inclination of 9° with respect to the ecliptic.
The near-Earth object has an Earth minimum orbit intersection distance of 0.0630 AU (9,420,000 km) or 24.5 lunar distances, which is slightly above the defined limit of 0.05 AU for potentially hazardous objects.
The body's observation arc begins 3 days prior to its official discovery observation in 1973, as a 1968-precovery from Palomar remained unused.

## Physical characteristics

In the Tholen classification, Anteros is a common S-type asteroid, while in the SMASS taxonomy, it is a relatively rare L-type asteroid, described as a reddish but otherwise featureless stony asteroid. It has also been characterized as a Sq subtype, which transitions to the Q-type asteroids.

### Rotation period

Several rotational lightcurves of Anteros were obtained from photometric observations by Brian Warner, Petr Pravec, the Palomar Transient Factory and others since the 1980s. One of the best-rated and most recent lightcurves was obtained at the Palmer Divide Station (716) in December 2013, and gave a rotation period of 2.867 hours with a brightness variation of 0.1 magnitude, which indicates that Anteros has a nearly spheroidal shape (U=3).

### Diameter and albedo

According to the EXPLORENEOs survey carried out by the Spitzer Space Telescope, Anteros measures between 2.38 and 2.43 kilometers in diameter, and its surface has an albedo of 0.138 to 0.170. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.18 and derives a diameter of 2.0 kilometers with an absolute magnitude of 15.89.

## Naming

This minor planet was named after the Greek god Anteros, avenger of unrequited love and punisher of those who scorn love and the advances of others. The asteroid's name may have been chosen because its orbit is similar to the asteroid 433 Eros, and in Greek mythology, Anteros was said to be the twin brother of Eros. The official naming citation was published by the Minor Planet Center on 15 October 1977 (M.P.C. 4237).
# 7336 Saunders

7336 Saunders, provisional designation 1989 RS$_1$, is a stony asteroid and near-Earth object of the Amor group, approximately 0.5 kilometers in diameter.
The asteroid was discovered on 6 September 1989, by American astronomer Eleanor Helin at Palomar Observatory in California, United States. It was named for JPL-project scientist R. Stephen Saunders.

## Orbit and classification

Saunders orbits the Sun at a distance of 1.2–3.4 AU once every 3 years and 6 months (1,278 days). Its orbit has an eccentricity of 0.48 and an inclination of 7° with respect to the ecliptic.
A first precovery was taken at the Australian Siding Spring Observatory in 1982, extending the body's observation arc by 7 years prior to its official discovery at Palomar. It has a minimum orbital intersection distance with Earth of 0.1908 AU (28,500,000 km), which corresponds to 74.3 lunar distances.

## Physical characteristics

In the SMASS classification, Saunders is a Sq-type, which transitions from the common S-type to the Q-type asteroids. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 467 meters, based on an absolute magnitude of 19.02.

### Lightcurve

In October 1989, the first photometric observations of Saunders were made with the ESO 1-metre telescope at La Silla in Chile. It gave a rotation period of 6 hours with a brightness variation of 0.3 magnitude (U=2). Another rotational lightcurve was obtained by Czech astronomer Petr Pravec at Ondřejov Observatory in August 2003, giving a period of 6.423±0.004 and an amplitude of 0.2 magnitude (U=n.a.).

## Naming

This minor planet was named in honor of JPL-project scientist R. Stephen Saunders (born 1940), director of the RPIF and head scientist of the Solar System Exploration Office. He worked on the Mars Surveyor 2001/03 program and on the Magellan spacecraft, that visited and mapped Venus in 1990. The official naming citation was published by the Minor Planet Center on 26 July 2000 (M.P.C. 41028).
# Binignit

Binignit is a Visayan dessert soup from the central Philippines. The dish is traditionally made with glutinous rice cooked in coconut milk with various slices of sabá bananas, taro, ube, and sweet potato, among other ingredients. It is comparable to various dessert guinataán (coconut milk-based) dishes found in other regions such as bilo-bilo. Among the Visayan people, the dish is traditionally served during Good Friday of Holy Week.

## Names

Binignit is also called giná-tan in Bikolano, tabirák in Mindanao Cebuano, alpahor in Chavacano, wit-wit in Hiligaynon, ginettaán, tambo-tambong, and paradusdos in Ilokano, ginat-an (or ginat-ang lugaw) in Waray and Hiligaynon/Ilonggo, kamlo in western Iloilo, scramble in Tuguegarao City, linugaw in Bacolod, and eangkuga by Akeanons in Aklan.
Binignit is considered a type of lugaw (rice gruel) and guinataán (dishes cooked in coconut milk).

## Preparation

The meat of a mature coconut is grated and the "thick" milk (coconut cream) is extracted. Two cups of water are then added to the grated coconut, and a second extraction is made. This becomes the "thin" milk. This "thin" coconut milk extract is added to cubed kamote (sweet potato), gabi (taro) and ube (purple yam), sliced ripe sabá bananas, langka (jack fruit), and tapioca pearls. Sometimes, young coconut meat strips are also added. This is simmered on low to medium heat, to prevent the coconut milk from curdling. Glutinous rice (pilit) is added once the root crops have sufficiently softened and the mixture is brought to a boil; being stirred occasionally until done. Just before removal from the flame, the "thick" coconut milk is added.
The people of the neighboring island of Leyte use ingredients such as landang (palm flour jelly balls), jackfruit, and anise, and thicken it with milled glutinous rice. The vegetables and the pearl sago are cooked in a mixture of water, coconut milk and landang, and sweetened by muscovado or brown sugar.
For the people of Panay, their version contains balls made of glutinous flour, as well as jackfruit. The balls are formed and boiled until they float, indicating that they are cooked. These are then added to the linugaw or eangkuga. This is similar to the preparation of bilo-bilo but the locals call it by eangkuga or linugaw.

## Cultural significance

A popular afternoon snack, it is best served when hot. Others serve it chilled or even frozen, eating the dessert much like ice cream. Among the Visayan people, the soup is also widely cooked and eaten for the Holy Week, especially during Good Friday when observant Catholics fast and avoid meat.
# Cheick Doucouré

Cheick Oumar Doucouré (born 8 January 2000) is a Malian professional footballer who plays as a defensive midfielder for Premier League club Crystal Palace and the Mali national team.

## Club career
### Lens

Doucouré developed as a youth player at JMG Academy Bamako. He then spent the 2016–17 season with Real Bamako before moving the following season to Lens. Doucouré quickly cemented his place at Lens in the 2018–19 Ligue 2 campaign with him playing a total of 34 games across all competitions that season.

### Crystal Palace

On 11 July 2022, Doucouré was signed by English club Crystal Palace on a five-year contract. In his first season, he was named the club's Player of the Year.
On 25 November 2023, Doucouré sustained an Achilles injury in a 2–1 loss to Luton Town, likely ruling him out for the rest of the 2023–24 season. On 28 February 2024, he extended his contract with Palace until 2029.

## International career

In October 2018, Doucouré received his first call-up to the Mali national team. He made his debut for Mali in a 1–0 2019 Africa Cup of Nations qualification win over Gabon on 17 November 2018.

## Career statistics
### Club

    As of match played 4 January 2025
Appearances and goals by club, season and competition :
| Club | Season | League | League | League | National cup | National cup | League cup | League cup | Other | Other | Total | Total |
| Club | Season | Division | Apps | Goals | Apps | Goals | Apps | Goals | Apps | Goals | Apps | Goals |
| Lens II | 2017–18 | Championnat National 2 | 4 | 0 | — | — | — | — | — | — | 4 | 0 |
| Lens II | 2019–20 | Championnat National 2 | 1 | 0 | — | — | — | — | — | — | 1 | 0 |
| Lens II | Total | Total | 5 | 0 | — | — | — | — | — | — | 5 | 0 |
| Lens | 2018–19 | Ligue 2 | 27 | 2 | 2 | 0 | 2 | 0 | 4 | 0 | 35 | 2 |
| Lens | 2019–20 | Ligue 2 | 21 | 1 | 1 | 0 | 2 | 0 | — | — | 24 | 1 |
| Lens | 2020–21 | Ligue 1 | 33 | 2 | 2 | 2 | — | — | — | — | 35 | 4 |
| Lens | 2021–22 | Ligue 1 | 34 | 1 | 3 | 0 | — | — | — | — | 37 | 1 |
| Lens | Total | Total | 115 | 6 | 8 | 2 | 4 | 0 | 4 | 0 | 131 | 8 |
| Crystal Palace | 2022–23 | Premier League | 34 | 0 | 1 | 0 | 0 | 0 | — | — | 35 | 0 |
| Crystal Palace | 2023–24 | Premier League | 11 | 0 | 0 | 0 | 1 | 0 | — | — | 12 | 0 |
| Crystal Palace | 2024–25 | Premier League | 12 | 0 | 0 | 0 | 1 | 0 | — | — | 13 | 0 |
| Crystal Palace | Total | Total | 57 | 0 | 1 | 0 | 2 | 0 | — | — | 60 | 0 |
| Career total | Career total | Career total | 177 | 6 | 9 | 2 | 6 | 0 | 4 | 0 | 196 | 8 |
* ↑ Includes Coupe de France, FA Cup
* ↑ Includes Coupe de la Ligue, EFL Cup
* ↑ Appearances in Ligue 1 promotion play-offs

### International

    As of match played 18 June 2023
Appearances and goals by national team and year :
| National team | Year | Apps | Goals |
| Mali | 2018 | 1 | 0 |
| Mali | 2019 | 4 | 0 |
| Mali | 2020 | 2 | 0 |
| Mali | 2021 | 1 | 0 |
| Mali | 2022 | 2 | 0 |
| Mali | 2023 | 2 | 0 |
| Total | Total | 12 | 0 |

## Honours

Individual
* Crystal Palace Player of the Season: 2022–23
# Fatima Gate

Fatima Gate, also known as the Good Fence Crossing, is a former border crossing between Lebanon and Israel. On the Lebanese side, it is close to the village of Kfar Kila and on the Israeli side, it is west of Metula. The crossing has been closed since the Israeli withdrawal from Lebanon at the end of the 1982-2000 South Lebanon conflict, and since the summer of 2000 has been the site of many anti-Israeli demonstrations and cross-border stone throwing from Lebanon to Israel.
# Fathallah barracks

The Fathallah barracks were the early headquarters of the Hezbollah organisation, situated in the Basta neighbourhood of West Beirut.

## History

On 22 February 1987, following the defeat of the Amal Militia by a combination of Druze and Communist street fighters, 7,000 Syrian commandos moved into West Beirut for the first time since 1982. On 24 February the Basta HQ was taken over by the Syrians after an incident in which a Syrian soldier was wounded in the leg. At least 20 young Hizbollah supporters were taken prisoner and executed. Other sources put the number of victims as twenty seven, twenty three men and four women. Fifty thousand people attended their funeral. The killings put intense strain on the relationship between Iran and Syria and under pressure from Tehran the Syrian army stopped further activity in Beirut's Southern suburbs with its population of 800,000 Shiites. Hezbollah's headquarters were later moved to secret locations in Dahieh, a suburb of Beirut.