OpenLLM-France/wikimedia huggingface dataset:
# Saltillo Rancho Seco

Saltillo Rancho Seco is a Mexican professional indoor soccer team based in Saltillo, the capital of the northern Mexican state of Coahuila. Since 2011, Saltillo has been a member of the Liga Mexicana de Futbol Rápido Profesional (LMFR) and in November 2013 began play in the Central Division of the Professional Arena Soccer League (PASL). With the PASL's absorption of 6 former MISL teams, the league changed its name to the Major Arena Soccer League and the team moved to the new Southern division.
After three successful seasons in the Liga Mexicana de Futbol Rápido Profesional, Saltillo became the third team from Mexico to join the PASL. The team remains a member of both leagues. The team plays home games at the purpose-built Deportivo Rancho-Seco Saltillo but began league play on the campus of the Autonomous University of Coahuila while construction was underway.
The team is owned by Marco Antonio Davila De Leon.

## History

Under the direction of head coach Elizandro Campos and assistant coach Jesus Monroy, the Central Division team struggled from the start with a loss to the Monterrey Flash then split their next eight games, losing to teams with winning records and beating teams with losing records. Saltillo won only one game in 2014, faced steadily declining attendance at home, and earned a 6–10 record on the season, missing the Professional Arena Soccer League post-season.
Moving to the new Southern Division of the re-branded Major Arena Soccer League, Saltillo will face the Missouri Comets and Las Vegas Legends on the road while their other 18 games will be against opponents based in Texas and Mexico.

## Year-by-year

| League champions | Runners-up | Division champions | Playoff berth |
| Year | League | Reg. season | GF | GA | Finish | Playoffs | Avg. attendance |
| 2013–14 | PASL | 6–10 | 91 | 132 | 5th, Central | Did not qualify | 397 |
| 2014–15 | MASL | 2–17 | 121 | 201 | 5th, Southern | Did not qualify | 503 |
| 2015–16 | MASL | 7–13 | 150 | 170 | 4th, Southwest | Did not qualify | 183 |
# Sam Meikle

Sam Meikle (born 1971) is an Australian writer and director best known for his work in television. He has won several Australian Writers' Guild Awards. He is the son of actor Richard Meikle.

## Filmography
### Television

* Home and Away as James Fraser (1997, 1 episode)

## Writer
### Film

* Sunday (2000, short film)
* Variety Show at the End of the World (2000, TV special)
* Bound (2000, short film)
* The Money Shot (2001, short film) - also director
* Melancholly (2001, short film) - also director
* The Easter Tide (2003, short film)
* Fatbelly: Chopper Unchopped (2009, documentary film)

### Television

* All Saints (2003, S6E2: "Heroic Measures", S6E37: "Look Before You Leap")
* All Saints (2003-08, 11 episodes)
* Home and Away (2004-19, 228 episodes)
* Out of the Blue (2009, 12 episodes)
* Neighbours (2009-19, 83 episodes)
* Rescue: Special Ops (2010-11, 5 episodes)
* Crownies (2011, S1E19)
* Wild Boys (2011, S1E11)
* Vic the Viking (2013-14, 4 episodes)
* Tashi (2014, 2 episodes)
* Heidi (2015, S1E5: "The Treehouse Oath")
* Vikings: Athelstan's Journal (2015, web series, 13 episodes)
* Here Come the Habibs (2015, 3 episodes including: "Party Habibs Style")
* Texas Rising: The Lost Soldier (2015, miniseries, 9 episodes)
* House Husbands (2017, 1 episode)
* The Wild Adventures of Blinky Bill (2016-17)
* The Secret Daughter (2016-17, 12 episodes) - also creator
* Nate Is Late (2018-19, S1E20: "The Candy Factory", S1E27: "The Gremlins")
* Wakefield (2021, miniseries, 2 episodes)
* 100 Wolf: Legend of the Moonstone (2021, 2 episodes, S1E11: "Cherry, S1E24: "Swiss")
* MaveriX (2022-23, 10 episodes) - also creator

## Awards and nominations

| Year | Award | Category | Work | Result |
| 2009 | AWGIE Awards | Television Serial | Out of the Blue (episode 4) | Nominated |
| 2021 | 11th AACTA Awards | AACTA Award for Best Television Drama Series | Wakefield | Nominated |
| 2022 | 12th AACTA Awards | AACTA Award for Best Children's Television Series | MaveriX | Nominated |
# Wright's stain

Wright's stain is a hematologic stain that facilitates the differentiation of blood cell types. It is classically a mixture of eosin (red) and methylene blue dyes. It is used primarily to stain peripheral blood smears, urine samples, and bone marrow aspirates, which are examined under a light microscope. In cytogenetics, it is used to stain chromosomes to facilitate diagnosis of syndromes and diseases.
It is named for James Homer Wright, who devised the stain, a modification of the Romanowsky stain, in 1902. Because it distinguishes easily between blood cells, it became widely used for performing differential white blood cell counts, which are routinely ordered when conditions such as infection or leukemia are suspected.
The related stains are known as the buffered Wright stain, the Wright-Giemsa stain (a combination of Wright and Giemsa stains), and the buffered Wright-Giemsa stain, and specific instructions depend on the solutions being used, which may include eosin Y, azure B, and methylene blue (some commercial preparations combine solutions to simplify staining). The May–Grünwald stain, which produces a more intense coloration, also takes a longer time to perform.
Urine samples stained with Wright's stain will identify eosinophils, which can indicate interstitial nephritis or urinary tract infection.
White blood cells stained with Wright's stain:
# HD 118203 b

HD 118203 b, formally named Staburags, is a jovian planet that takes only 6.13 days or 147 hours to orbit the parent star HD 118203 at a distance of 0.07 astronomical units. The exact mass was not known since inclination was not known until TESS detected the planet. This hot Jupiter is unusual since it has relatively high eccentricity of 0.31.
The planet HD 118203 b is named Staburags. The name was selected in the NameExoWorlds campaign by Latvia, during the 100th anniversary of the IAU. Staburags is the name of a character from the Latvian poem Staburags un Liesma, and denotes a rock with symbolic meaning in literature and history.
HD 118203 b was discovered in August 2005 in Haute-Provence Observatory in France by Da Silva who used the doppler spectroscopy to look for shifts in the star's spectrum caused by the planet's gravity as the planet orbits the star.
In 2019 the transits of the planet were detected with the Transiting Exoplanet Survey Satellite. The host star is one of the brightest stars for transiting planets and HD 118203 b is therefore a good target for follow-up observations.
# HD 117618

HD 117618, named Dofida by the IAU, is a single, yellow-hued star in the southern constellation of Centaurus. With an apparent visual magnitude of 7.17, it is too faint to be visible to the naked eyes of a typical observer. The distance to this star, as determined from its annual parallax shift of 26.34±0.60 mas as seen from Earth's orbit, is about 124 light years. It is moving further away with a heliocentric radial velocity of around +1.6 km/s.
This star is similar to the Sun, being a G-type main-sequence star with a stellar classification of G0 V. It is about 10% more massive and 17% larger than the Sun, with an estimated age of roughly four billion years and a projected rotational velocity of 3.67 km/s. The star is radiating 1.6 times the Sun's luminosity from its photosphere at an effective temperature of 6,019 K.

## Name

HD 117618, and its planet HD 117618b, were chosen as part of the 2019 NameExoWorlds campaign organised by the International Astronomical Union, which assigned each country a star and planet to be named. HD 117618 was assigned to Indonesia. The winning proposal named the star "Dofida" meaning our star in Nias language, and its planet "Noifasui" meaning revolve around in Nias language (derived from the word ifasui, meaning to revolve around, and no, indicating that the action occurred in the past and continued to the present time).

## Planetary system

In 2005, the Anglo-Australian Planet Search program announced the discovery of a low-mass planet in orbit around HD 117618. This object was found through measurements of radial velocity variation, which were larger than those produced by the intrinsic jitter of the host star. The best Keplerian fit to the data gave a periodicity of 25.8 days with an eccentricity of around 0.37 and a semimajor axis of 0.17 AU. The lower bound on the object's mass was estimated to be 0.16 M$_J$. These values were subsequently refined, as shown in the table below.
The HD 117618 planetary system :
| Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
| b / Noifasui | >0.178 ± 0.021 M$_J$ | 0.176 ± 0.010 | 25.827±0.019 | 0.42 ± 0.17 | — | — |
# HD 117939

HD 117939 is a Sun-like star in the southern constellation of Centaurus. With an apparent visual magnitude of 7.29 it is too faint to be viewed with the naked eye, but is within the range of binoculars or a small telescope. It is located at a distance of 98.5 light years from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +82 km/s. This is an intermediate disk star with a high proper motion, traversing the celestial sphere at an angular rate of 0.68 arcsec yr$^{−1}$.
An ordinary G-type main-sequence star with a stellar classification of G4V, this star is an "excellent photometric match for the Sun"; the atmospheric properties of the star make it a near solar twin. It is older than the sun at 6.1 billion years, but is more chromospherically active.
To date no exact solar twin (precisely matching all important properties of the Sun) has been found. However, there are some stars that come very close to being identical to the Sun, and as such are dubbed solar twins by astronomers. An exact solar twin would be a 4.6 billion years old G2V star with a 5,778K temperature, the correct metallicity, and a 0.1% solar luminosity variation. G2V stars with an age of 4.6 billion years or more have typically reached their most stable state. Proper metallicity and size are also important to low luminosity variation.

## Sun comparison

Chart compares the sun to HD 117939.
| Identifier | Stellar Class | Temperature (K) | Metallicity (dex) | Age (Gyr) | Notes |
| Sun | G2V | 5,778 | +0.00 | 4.6 | |
| HD 117939 | G4V | 5,765 | −0.22 | 6.1 | |
# HD 117566

HD 117566, also known as HR 5091, is a solitary yellow-hued star located in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.74, making it faintly visible to the naked eye. This object is relatively close at a distance of 291 light years based on Gaia DR3 parallax measurements but is receding with a heliocentric radial velocity of 14 km/s. At its current distance, HD 117566's brightness is diminished by 0.12 magnitudes due to interstellar dust.
HD 117566 has a stellar classification of G3 IIIb Fe−1 CH1, indicating that it is a G-type giant with an under-abundance of iron and an overabundance of the CH radical in its spectrum. Its evolutionary stage is unclear. A 1994 paper places it in the Hertzsprung gap, indicating it has ceased hydrogen core fusion and is now evolving toward the red giant branch (RGB). However, Mishenina et al. (2006) said that HD 117566 is already past the RGB and is on the horizontal branch, fusing helium at its core. Nevertheless, it has 2.29 times the mass of the Sun and, at the age of 760 million years, it has expanded to 7.2 times the Sun's radius. It radiates 38.2 times the luminosity of the Sun from its photosphere at an effective temperature of 5,420 K. HD 117566 has a solar metallicity and spins modestly with a projected rotational velocity of 9 km/s.
# XII Brigade, Royal Horse Artillery

XII Brigade, Royal Horse Artillery was a brigade of the Royal Horse Artillery which existed in the early part of the 20th century. It was dissolved during World War I as its constituent batteries were posted to other formations.

## History
### Background

Royal Horse Artillery brigades did not exist as an organizational or operational grouping of batteries until 1 July 1859 when the Horse Brigade, Royal Artillery was formed. The brigade system was extended to five (later six) brigades when the horse artillery of the Honourable East India Company had been transferred to the British Army in 1861. These brigades were reduced to five in 1871, then to three (of 10 batteries each) in 1877 and to two (of 13 batteries each) in 1882. The brigade system was finally abolished in 1889.
As battery designations were tied to the brigade that the battery was assigned to, batteries were redesignated in a bewildering sequence as they were transferred between brigades. For example, E Battery of C Brigade (E/C Bty) might become N Battery of A Brigade (N/A Bty) upon transfer. Henceforth, batteries were designated in a single alphabetical sequence in order of seniority from date of formation.
The brigade system was revived in 1901. Each brigade now commanded just two batteries and a small staff (a Lieutenant-Colonel in command, an adjutant and a brigade sergeant major). Initially, batteries were not assigned to brigades in any particular order, but in 1906, at the insistence of Edward VII, brigades were redesignated so that batteries were roughly in order of seniority (hence I Brigade commanded A Battery and B Battery).

### Formation

XII Brigade, RHA was formed on 1 March 1901 as the II Brigade-Division, RHA with V Battery and W Battery. In 1903 it was redesignated as II Brigade, RHA and was stationed at Woolwich. On 1 October 1906, it was redesignated as XII Brigade, RHA.
By the time World War I broke out, the brigade was in Meerut, India assigned to 7th (Meerut) Division. On mobilization, V Battery was assigned to the newly formed II Indian Brigade, RHA with 2nd Indian Cavalry Division (attached to 7th (Meerut) Cavalry Brigade) and sailed for the Western Front in November 1914. W Battery moved to Sialkot and joined the 2nd (Rawalpindi) Division in October 1914. It returned to the 7th (Meerut) Divisional Area where it joined 4th (Meerut) Cavalry Brigade in February 1915. In November 1917 it departed for Mesopotamia where it joined the 11th Indian Cavalry Brigade. With the departure of its batteries, the brigade HQ was dissolved.
# HD 18970

HD 18970 is a class G9.5III (yellow giant) star in the constellation Perseus. Its apparent magnitude is 4.77 and it is approximately 211 light years away based on parallax.
# Wulingyuan

Wulingyuan (, Chinese: 武陵源) is a scenic and historical site in the Wulingyuan District of South Central China's Hunan Province. It was inscribed as a UNESCO World Heritage Site in 1992. It is noted for more than 3,000 quartzite sandstone pillars and peaks across most of the site, many over 200 metres (660 ft) in height, along with many ravines and gorges with picturesque streams, pools, lakes, rivers, and waterfalls. It features 40 caves, many with large calcite deposits and a natural bridge named Tianqiashengkong (meaning 'bridge across the sky'), which is one of the highest natural bridges in the world. The site also provides habitat for many vulnerable species, including the dhole, Asiatic black bear, and Chinese water deer.
The site is situated in Zhangjiajie City and lies about 270 kilometres (170 mi) to the northwest of Changsha, the capital of Hunan Province. The park covers an area of 690 square kilometers (266 square miles). Wulingyuan forms part of the Wuling Mountain Range. The scenic area consists of four national parks, which are the Zhangjiajie National Forest Park, Suoxi Valley Nature Reserve, Tianzi Mountain Nature Reserve, and the recently added Yangjiajie Scenic Area. Overall there are over 560 attraction sights to view.

## Geology

The quartzite sandstone pillars and the surrounding regions were formed during the Devonian period (400 to 350 million years ago) from a combination of tectonic uplift and water erosion. The highest area in the park is Huang Shi Zhai (黃石寨). It reaches a height of 3,450 feet (1,050 m) and is accessible via cable car or a set of stairs. Another cliff is accessed by the 326 m (1,070 ft) Bailong Elevator.

## Gallery

* Panorama of the Five Fingers Peak of Huangshizhai
* Zhangjiajie River
* Wulingyuan park entrance
# Sam-Woode Limited

Sam Woode Limited is a Ghanaian publishing company. The company is listed on the stock index of the Ghana Stock Exchange, the GSE All-Share Index. Sam Woode Limited was founded on 16 October 1984 and was listed on the Ghana Stock Exchange in 2002, having converted into a public company in 1998.

## Operations

Sam Woode Limited publishes educational textbooks, story books, as well as non-book materials for different levels. Sam Woode Limited's products portfolio includes pre-school and primary school levels, among others.
The company produces books in categories including agency books, agricultural science, basic design and technology, citizenship education, handwriting, information and communication technology, integrated science, social studies, mathematics and religious and moral education, among others. Products from the Sam Woode catalogue are also available for purchase online.
Sam Woode Limited holds exclusive distribution rights for the territory of West Africa for titles by foreign publishers listed on the company's Agency Lists.
# HP 7935

The HP 7935 is a business computer hard disc drive system manufactured by Hewlett Packard. It was produced by the Disc Memory Division in Boise, Idaho USA beginning in 1982 at a cost of about $27,000. Within the company the drive was known as the "BFD", ostensibly an acronym for "big fixed disc" but the development engineers had used that acronym for "big fucking disc", a term relative to the smaller 7920 series drives introduced earlier by the company.

## Size

The 7935 had four bottom mounted casters for moving and four lock-down feet for stability in the computer room.
The drive's linear motor was so powerful if the feet were not down, when in operation the drive could literally move about the computer room.
Height: 82.5 cm (32.5 inches), Width: 55.2 cm (21.7 inches), Depth: 83.4 cm (32.8 inches), 154 kg (339.5 lb.)

## Media

The HP7935 allowed the user to remove and install a 404 megabyte model 97935 Disc Pack.
The HP7933 was the same basic drive with a disc pack only removable by service personnel.
The 793x series provided a 300% increase in capacity of the HP 7925 at only a slightly increased cost. Performance-wise, the 7935 had a 15-20% performance decrease compared to the 7925. Apparently modifications were made by HP, in a program called the Performance Enhancement Project, raising 7935 performance 15% making it comparable to the older model.
The HP 7935/33 achieved a track density of 625 tracks per inch (considered high at the time), achieving capacity using 7 platters, 13 data surfaces and 14 heads (one head and surface were used for servo data). The disc pack spun at 2694 RPM.
Despite an extensive air purging spin-up sequence to prevent disc and head contamination, human users reportedly caused so many 7935 packs to have disc head crashes, many users simply purchased the 7933.

## Features

The 7935H had a HP-IB interface mounted in the rear. The drive's front panel had a key pad for running internal disc drive diagnostics, a LED character display, a load and unload button, and a lid opening button.
The 7935G was a bundled package of three 7935H units at a reduced cost of $74,000.

## Use

The 7933 and 7935 drives were often used with the HP 3000 series family of minicomputers and later in early versions of the HP 9000 series computers. Drives were connected via the HP-IB interface to the host computer and multiple drives could be connected in a daisy-chain. The HP-IB address of the drive was selectable via DIP switches next to the interface.
The robustness of the drive hardware was tested by the 7.1 1989 Loma Prieta earthquake. The HP campus in Cupertino had 1,682 HP 7935 drives operating at the time of the quake and 97.25 percent were still operational afterwards. Within an hour, only 2 percent were non-operational and only 1.5 percent were non-operational several days later.
Later with development and production of smaller, rack mountable, high-density, sealed HP disc drive units using Winchester mechanism designs (like the HP 7963), the demand for HP793x drive line declined.
# HP 7470

The HP 7470 was a small low-cost desktop pen plotter introduced by Hewlett-Packard's San Diego division in 1982. It was the first small-format plot that moved the paper, rather than the pens. It used a revolutionary "grit wheel" design which moved the paper held in place by a wheel with embedded grit and a pinch roller.
The HP 7470 had two pens, one on either side and plotted on ANSI A (8.5 x 11 inch) or A4-sized paper. It was much less expensive than the previous flatbed design. It was very heavy but had 4 pens. The HP 7475 used a rotating carousel with six pens. That plotter was used in greeting card kiosks. This design was also scaled up for very large pen plotters. These were driven by the HP-GL plotter language which used ASCII commands such as PA 300, 4500;PD;. The plotter had three electrical interfaces: HP-IB, RS-232, and HP-IL for HP handheld calculators.
Pen plotters became obsolete with the adoption of ink-jet printers, and processors fast enough to rasterize complex images. Houston Instrument and other manufacturers would follow with similar plotters.
# Hanneke Kappen

Hanneke Kappen (born 1954) is a Dutch singer and radio and TV presenter. Kappen started a musical career by singing in a rock band in the late 1970s during the zenith of the Groningen music scene, but became a radio presenter and from 1981 to 1982 had a weekly show that focused on heavy metal music, only the second such show on Dutch radio. She then moved on to television, presenting programs for a number of public broadcasters. She returned to radio in 1999, while continuing to play and record music.

## Biography

Hanneke Kappen was attending art school when she became a singer for the rock band White Honey from Groningen, with, among others, Erwin Java. This happened at the height of what was later called "the Groninger springtij" (the "Groningen spring tide"), a period when the music scene in Groningen was very lively, and many local acts were propelled to the national stage, including Herman Brood, who picked up Java, the band's guitarist. The group had a minor hit with "Nothing Going On In The City" but disbanded in 1980, just after releasing their first and only album. Kappen continued playing music, including jazz (with her brother, and with guitarist Winfred Buma).
Kappen moved into radio, and from 1981 to 1982 presented the radio program Stampij for the public broadcaster KRO, playing heavy metal and hard rock music. This was only the second Dutch radio program (after the VARA's Betonuur, with Alfred Lagarde, 1976–1982) oriented toward heavy metal. After Stampij she moved to television and presented a number of shows for the VARA, including Wereldwijs, Je ziet maar, and Vroege Vogels [nl]. In 1989 she presented the Kinderen voor Kinderen festival, and that same year presented a show, Avonduur met Kappen, that she herself had pitched to the VARA. For Teleac, an educational broadcaster, she presented Werken aan Werk, and the educational program Plein 1. In 1999 she returned to radio and took over presenting the Sunday morning show Dag Zondag for the NPS. By that time she was a mother of two and spent a lot of time travelling; besides her radio and TV work, she had started a study in communication, hosted conferences and symposiums, and was doing promotional work for the city of Groningen as well as the province. She also played music, in a duo called "Kappen & Klat" with Boelo Klat. She has continued to be active as a musician; in 2005 and 2006 she sang on a CD for the Eastgate project of composer Gerard Ammerlaan and performed with his band, and later formed a duo with guitarist Winfred Buma.

## Discography

Source: Poparchief Groninger
* Some Kinda Woman (White Honey, 1979)
* Human Electrics (with Gerry Arling, 1989)
* State of Soul (with Gerry Arling, 1991)
* Klatwerk (with Boelo Klat, 1994)
* Kappen & Klat (with Boelo Klat, 1997/2004)
* Alien Visitors (with Eastgate, 2005)