id string | question string | answer string | documents list |
|---|---|---|---|
102.5_Radio_Pembrokeshire_24658517 | Based on the article about '102.5 Radio Pembrokeshire', describe the 'History' section. | further groups, More FM and Real Radio, also applied for the licence. In November 2001, Haven FM was awarded an eight-year licence. The station was renamed Radio Pembrokeshire following a pre-launch competition to find a new station name. Originally intended to broadcasts from studios in Haverfordwest, a lack of suitab... | [
"102.5 Radio Pembrokeshire — History\n\nstations in Fishguard and Tenby, broadcasting on 107.5 FM. Nearly two years after the launch of Radio Pembrokeshire, the station's Narberth studios became home to a second local station, Radio Carmarthenshire, followed in March 2010 by Radio Ceredigion. In August 2006, the st... |
102.6_&_106.8_Durham_FM_3551030 | Based on the article about '102.6 & 106.8 Durham FM', describe the 'Ex-presenters' section. | Peter Grant ; Craig Andrews ; Steve Phillips ; Vic Ribbands ; Chris Hakin ; Dicky Ord Dave 'Ceefax' Fenwick ; Geoff Longstaff ; Mike Jinx ; Marie Gardiner ; Mike Nicholson ; Kyle Wilkinson Les Gunn ; Mike Patterson ; Pete Clough ; Mat Page ; Tim West ; Sarah Knapper ; Lisa Dawson | [
"102.6 & 106.8 Durham FM — Ex-presenters\n\nPeter Grant ; Craig Andrews ; Steve Phillips ; Vic Ribbands ; Chris Hakin ; Dicky Ord Dave 'Ceefax' Fenwick ; Geoff Longstaff ; Mike Jinx ; Marie Gardiner ; Mike Nicholson ; Kyle Wilkinson Les Gunn ; Mike Patterson ; Pete Clough ; Mat Page ; Tim West ; Sarah Knapper ;... |
102.6_&_106.8_Durham_FM_3551029 | Summarize the 'History' part of '102.6 & 106.8 Durham FM'. | Since its launch in 2005, Durham FM was owned and operated by TLRC. In December 2008, Durham FM submitted an application to OFCOM to co-locate with sister station, Sun FM in Sunderland. Following a consultation, the majority of responses were against the idea. In July 2009, OFCOM give permission to rename Durham FM to ... | [
"102.6 & 106.8 Durham FM — Ex-presenters\n\nPeter Grant ; Craig Andrews ; Steve Phillips ; Vic Ribbands ; Chris Hakin ; Dicky Ord Dave 'Ceefax' Fenwick ; Geoff Longstaff ; Mike Jinx ; Marie Gardiner ; Mike Nicholson ; Kyle Wilkinson Les Gunn ; Mike Patterson ; Pete Clough ; Mat Page ; Tim West ; Sarah Knapper ;... |
102.6_FM_17744696 | Describe the 'Ireland' section of the article about '102.6 FM'. | Beat 102 103 in Gorey ; C103 in Cork City and East Cork ; Highland Radio in West Donegal ; Midlands 103 in Stradbally and Boris-in-Ossory | [
"102.6 FM — Fiji\n\nBula FM in Suva, Nadi, Lautoka and Labasa",
"102.6 FM — Ireland\n\nBeat 102 103 in Gorey ; C103 in Cork City and East Cork ; Highland Radio in West Donegal ; Midlands 103 in Stradbally and Boris-in-Ossory",
"102.6 FM — Bosnia\n\nRadio Prača in Goražde",
"102.6 FM — India\n\nAIR FM Rainbow ... |
102.6_FM_17744701 | From the article on '102.6 FM', restate the 'United Kingdom' content. | Heart Essex in Chelmsford, Braintree, Witham, Maldon and South Woodham Ferrers ; Heart West in Somerset ; in Oxford ; Metro Radio in Alnwick ; Signal 1 in North Staffordshire and South Cheshire ; Sine FM in Doncaster, South Yorkshire | [
"102.6 FM — Fiji\n\nBula FM in Suva, Nadi, Lautoka and Labasa",
"102.6 FM — Ireland\n\nBeat 102 103 in Gorey ; C103 in Cork City and East Cork ; Highland Radio in West Donegal ; Midlands 103 in Stradbally and Boris-in-Ossory",
"102.6 FM — Bosnia\n\nRadio Prača in Goražde",
"102.6 FM — India\n\nAIR FM Rainbow ... |
102.7_FM_29598083 | What does the article about '102.7 FM' say regarding 'United States (Channel 274)'? | WDKL in Mount Clemens, Michigan ; WEBN in Cincinnati, Ohio ; WEGR in Arlington, Tennessee ; WEKX in Jellico, Tennessee ; in Manchester, Vermont ; WGNI in Wilmington, North Carolina ; in New Ellenton, South Carolina ; in Mannington, West Virginia ; in Rockledge, Florida ; WICX-LP in Concord, New Hampshire ; WIEC-LP in E... | [
"102.7 FM — United States (Channel 274)\n\nWDKL in Mount Clemens, Michigan ; WEBN in Cincinnati, Ohio ; WEGR in Arlington, Tennessee ; WEKX in Jellico, Tennessee ; in Manchester, Vermont ; WGNI in Wilmington, North Carolina ; in New Ellenton, South Carolina ; in Mannington, West Virginia ; in Rockledge, Florida ; W... |
102.7_FM_29598081 | From the article on '102.7 FM', restate the 'United States (Channel 274)' content. | in Van Buren, Arkansas ; in Manitou Springs, Colorado ; KBLZ in Winona, Texas ; KBYH-LP in Midland, Texas ; KCHW in Chewelah, Washington ; KCNA in Cave Junction, Oregon ; KCYE in Boulder City, Nevada ; KDDB in Waipahu, Hawaii ; KGQD-LP in Kermit, Texas ; in Fresno, California ; KHXS in Merkel, Texas ; KHYX in Winnemucc... | [
"102.7 FM — United States (Channel 274)\n\nWDKL in Mount Clemens, Michigan ; WEBN in Cincinnati, Ohio ; WEGR in Arlington, Tennessee ; WEKX in Jellico, Tennessee ; in Manchester, Vermont ; WGNI in Wilmington, North Carolina ; in New Ellenton, South Carolina ; in Mannington, West Virginia ; in Rockledge, Florida ; W... |
102.7_FM_29598072 | What does the article about '102.7 FM' say regarding 'Australia'? | Sky Sports Radio in Jindabyne, New South Wales ; 3RRR in Melbourne, Victoria ; 4CCA in Cairns, Queensland ; 4DDB in Toowoomba, Queensland ; ABC Classic FM in Mildura, Victoria ; ABC North and West SA in Roxby Downs, South Australia ; 2RVR in Wagga Wagga, New South Wales ; Triple J in Rosebery, Tasmania | [
"102.7 FM — United States (Channel 274)\n\nWDKL in Mount Clemens, Michigan ; WEBN in Cincinnati, Ohio ; WEGR in Arlington, Tennessee ; WEKX in Jellico, Tennessee ; in Manchester, Vermont ; WGNI in Wilmington, North Carolina ; in New Ellenton, South Carolina ; in Mannington, West Virginia ; in Rockledge, Florida ; W... |
102.7_FM_29598077 | Describe the 'Mexico' section of the article about '102.7 FM'. | XEHL-FM in Guadalajara, Jalisco ; XHAC-FM in Campeche, Campeche ; XHCANQ-FM in Cancún (Santa Martha), Quintana Roo ; XHCHG-FM in Chilpancingo, Guerrero ; XHDM-FM in Hermosillo, Sonora ; XHGAS-FM in Cuatro Ciénegas, Coahuila ; XHHW-FM in Las Garzas, El Rosario, Sonora ; XHIRG-FM in Irapuato, Guanajuato ; XHJBT-FM in San... | [
"102.7 FM — United States (Channel 274)\n\nWDKL in Mount Clemens, Michigan ; WEBN in Cincinnati, Ohio ; WEGR in Arlington, Tennessee ; WEKX in Jellico, Tennessee ; in Manchester, Vermont ; WGNI in Wilmington, North Carolina ; in New Ellenton, South Carolina ; in Mannington, West Virginia ; in Rockledge, Florida ; W... |
102.7_FM_29598082 | Based on the article about '102.7 FM', describe the 'United States (Channel 274)' section. | KQHM in Zapata, Texas ; in Lake Ozark, Missouri ; in Juneau, Alaska ; in Midvale, Utah ; KTBH-FM in Kurtistown, Hawaii ; in Pequot Lakes, Minnesota ; KTXJ-FM in Jasper, Texas ; KVSS (FM) in Papillion, Nebraska ; in North Crossett, Arkansas ; KWVF in Guerneville, California ; in Box Elder, South Dakota ; KYBB in Canton,... | [
"102.7 FM — United States (Channel 274)\n\nWDKL in Mount Clemens, Michigan ; WEBN in Cincinnati, Ohio ; WEGR in Arlington, Tennessee ; WEKX in Jellico, Tennessee ; in Manchester, Vermont ; WGNI in Wilmington, North Carolina ; in New Ellenton, South Carolina ; in Mannington, West Virginia ; in Rockledge, Florida ; W... |
102.7_FM_29598084 | Explain what '102.7 FM' covers in the 'United States (Channel 274)' section. | in Pentwater, Michigan ; in Pompano Beach, Florida ; WMYW-LP in Paulding, Ohio ; WNEW-FM in New York, New York ; WNPE in Narragansett Pier, Rhode Island ; WOKH in Springfield, Kentucky ; WOPA-LP in Clio, South Carolina ; in Blountstown, Florida ; in Buckhead, Georgia ; in Camden, South Carolina ; in Baltimore, Maryland... | [
"102.7 FM — United States (Channel 274)\n\nWDKL in Mount Clemens, Michigan ; WEBN in Cincinnati, Ohio ; WEGR in Arlington, Tennessee ; WEKX in Jellico, Tennessee ; in Manchester, Vermont ; WGNI in Wilmington, North Carolina ; in New Ellenton, South Carolina ; in Mannington, West Virginia ; in Rockledge, Florida ; W... |
102.7_FM_29598075 | Based on the article about '102.7 FM', describe the 'Canada (Channel 274)' section. | CBH-FM in Halifax, Nova Scotia ; CBJE-FM in Chicoutimi, Quebec ; CBMS-FM in Blanc-Sablon, Quebec ; CBTF-FM in Falkland, British Columbia ; CFGI-FM in Georgina Island, Ontario ; CJFB-FM in Caledon, Ontario ; CFOA-FM in Algonquin Park, Ontario ; CFOA-FM-1 in Algonquin Park, Ontario ; CKPK-FM in Vancouver, British Columbi... | [
"102.7 FM — United States (Channel 274)\n\nWDKL in Mount Clemens, Michigan ; WEBN in Cincinnati, Ohio ; WEGR in Arlington, Tennessee ; WEKX in Jellico, Tennessee ; in Manchester, Vermont ; WGNI in Wilmington, North Carolina ; in New Ellenton, South Carolina ; in Mannington, West Virginia ; in Rockledge, Florida ; W... |
102.7FM_(Toowoomba)_29844680 | Summarize the following section from the article on '102.7FM (Toowoomba)'. | 102.7FM (ACMA callsign: 4DDB) is a community radio station operating in Toowoomba, Queensland. Established in the 1970s, it broadcasts from studios in the city's CBD, and is transmitted from the University of Southern Queensland in Darling Heights. It is a member of the Community Broadcasting Association of Association... | [
"102.7FM (Toowoomba)\n\n102.7FM (ACMA callsign: 4DDB) is a community radio station operating in Toowoomba, Queensland. Established in the 1970s, it broadcasts from studios in the city's CBD, and is transmitted from the University of Southern Queensland in Darling Heights. It is a member of the Community Broadcastin... |
102.7FM_(Toowoomba)_29844682 | From the article on '102.7FM (Toowoomba)', restate the 'Programming' content. | As a "generalist" style community broadcaster, 102.7FM seeks simply to connect with its audience within the geographic coverage provided by its transmitter. 102.7FM caters for special- interest groups by programming with dedicated, Dutch, Filipino, and Christian, multi-faith programs which air on a weekly basis. Likewi... | [
"102.7FM (Toowoomba)\n\n102.7FM (ACMA callsign: 4DDB) is a community radio station operating in Toowoomba, Queensland. Established in the 1970s, it broadcasts from studios in the city's CBD, and is transmitted from the University of Southern Queensland in Darling Heights. It is a member of the Community Broadcastin... |
102.7FM_(Toowoomba)_29844684 | Describe the 'Licence breaches' section of the article about '102.7FM (Toowoomba)'. | In May 2008, the Australian Communications and Media Authority found that 4DDB was in breach of its licence conditions by failing to appropriately disclose financial support during live interviews with commercial sponsors. No penalty was issued as this was the first such breach. In September 2008, the Australian Commun... | [
"102.7FM (Toowoomba)\n\n102.7FM (ACMA callsign: 4DDB) is a community radio station operating in Toowoomba, Queensland. Established in the 1970s, it broadcasts from studios in the city's CBD, and is transmitted from the University of Southern Queensland in Darling Heights. It is a member of the Community Broadcastin... |
102.7FM_(Toowoomba)_29844681 | Based on the article about '102.7FM (Toowoomba)', describe the 'Audience' section. | 102.7FM's signal propagates throughout Toowoomba, the Darling Downs and Lockyer Valley and listeners report acceptable signals from as far away as North Brisbane, the Lockyer Valley, Dalby, over the NSW border and to the South Burnett. | [
"102.7FM (Toowoomba)\n\n102.7FM (ACMA callsign: 4DDB) is a community radio station operating in Toowoomba, Queensland. Established in the 1970s, it broadcasts from studios in the city's CBD, and is transmitted from the University of Southern Queensland in Darling Heights. It is a member of the Community Broadcastin... |
102.8_FM_6202840 | Describe the 'United Kingdom' section of the article about '102.8 FM'. | Hot Radio in Dorset ; Capital Midlands in Derbyshire ; Sun FM in County Durham ; Heart South in Kent ; Moray Firth Radio in Moray ; Pirate FM 102 in Cornwall ; Canalside in Cheshire ; Tay FM in Dundee ; Free Herefordshire & Worcestershire in Worcestershire ; Capital Manchester in Lancashire | [
"102.8 FM\n\nThis is a list of radio stations that broadcast on FM frequency 102.8 MHz:",
"102.8 FM — India\n\nVividh Bharati in Hyderabad",
"102.8 FM — Malaysia\n\nEra in Kuala Terengganu, Terengganu",
"102.8 FM — United Kingdom\n\nHot Radio in Dorset ; Capital Midlands in Derbyshire ; Sun FM in County Durha... |
102/35_su_Fiat_634N_5635775 | Describe the content of the article about '102/35 su Fiat 634N'. | The 102/35 on Fiat 634N was an anti aircraft truck used by the Regia Marina during the Second World War. | [
"102/35 su Fiat 634N\n\nThe 102/35 on Fiat 634N was an anti aircraft truck used by the Regia Marina during the Second World War.",
"102/35 su Fiat 634N — Technology\n\nThe cannon 102/35 Mod. 1914 was installed on the truck bed using two different types of mounts: the OTO Mod. 33 on the first two specimens and the... |
102/35_su_Fiat_634N_5635778 | Describe the 'Technology' section of the article about '102/35 su Fiat 634N'. | The cannon 102/35 Mod. 1914 was installed on the truck bed using two different types of mounts: the OTO Mod. 33 on the first two specimens and the Vickers-Terni Mod. 25 mount on the others. The modifications of the vehicle, on the other hand, consisted in the "cutting" of the closed cabin, replaced by a canvas cover, a... | [
"102/35 su Fiat 634N\n\nThe 102/35 on Fiat 634N was an anti aircraft truck used by the Regia Marina during the Second World War.",
"102/35 su Fiat 634N — Technology\n\nThe cannon 102/35 Mod. 1914 was installed on the truck bed using two different types of mounts: the OTO Mod. 33 on the first two specimens and the... |
102/35_su_Fiat_634N_5635776 | Summarize the 'History' part of '102/35 su Fiat 634N'. | The 102/35 on SPA 9000, produced since 1914 and used during the Great War, was the first Italian gun truck, obtained from the installation on a truck of an anti-aircraft naval gun, designed for cruisers. After the end of the First World War, the trucks were disassembled and the guns were returned to Regia Marina. In 19... | [
"102/35 su Fiat 634N\n\nThe 102/35 on Fiat 634N was an anti aircraft truck used by the Regia Marina during the Second World War.",
"102/35 su Fiat 634N — Technology\n\nThe cannon 102/35 Mod. 1914 was installed on the truck bed using two different types of mounts: the OTO Mod. 33 on the first two specimens and the... |
102/35_su_Fiat_634N_5635777 | What information does the article about '102/35 su Fiat 634N' provide on 'History'? | 132nd Armoured Division Ariete, while section B of the 6th was subordinated to the 102nd Motorised Division Trento. In the last months of 1941 they participated in several battles; on November 19 it was used during the first battle of Bir el Gobi, destroying at least 15 British tanks from a long distance. All 102/35 tr... | [
"102/35 su Fiat 634N\n\nThe 102/35 on Fiat 634N was an anti aircraft truck used by the Regia Marina during the Second World War.",
"102/35 su Fiat 634N — Technology\n\nThe cannon 102/35 Mod. 1914 was installed on the truck bed using two different types of mounts: the OTO Mod. 33 on the first two specimens and the... |
1020_26474797 | Reconstruct the content from the article about '1020'. | Year 1020 (MXX) was a leap year starting on Friday (link will display the full calendar) of the Julian calendar. | [
"1020\n\nYear 1020 (MXX) was a leap year starting on Friday (link will display the full calendar) of the Julian calendar.",
"1020 — By place\n\nSummer – Emperor Henry II conducts his third Italian military campaign. He makes plans to invade the south, but remains non-commital. ; June 15 – Byzantine tr... |
1020_26474798 | Explain what '1020' covers in the 'By place' section. | Summer – Emperor Henry II conducts his third Italian military campaign. He makes plans to invade the south, but remains non-commital. ; June 15 – Byzantine troops under Catepan Basil Boioannes (supported by his ally Prince Pandulf IV) capture the fortress of Troia. ; The French city of Saint-Germain-en-Laye... | [
"1020\n\nYear 1020 (MXX) was a leap year starting on Friday (link will display the full calendar) of the Julian calendar.",
"1020 — By place\n\nSummer – Emperor Henry II conducts his third Italian military campaign. He makes plans to invade the south, but remains non-commital. ; June 15 – Byzantine tr... |
1020_26474800 | Explain what '1020' covers in the 'Births' section. | nobleman (approximate date) ; Otto of Nordheim, duke of Bavaria (approximate date) ; Stephen IX, pope of the Catholic Church (approximate date) ; Su Song, Chinese statesman and scientist (d. 1101) ; Sweyn Godwinson, English nobleman (approximate date) ; Vladimir Yaroslavich, Grand Prince of Kiev (d. 1052) ; William I (... | [
"1020\n\nYear 1020 (MXX) was a leap year starting on Friday (link will display the full calendar) of the Julian calendar.",
"1020 — By place\n\nSummer – Emperor Henry II conducts his third Italian military campaign. He makes plans to invade the south, but remains non-commital. ; June 15 – Byzantine tr... |
1020_26474801 | Describe the 'Deaths' section of the article about '1020'. | June 12 – Lyfing, archbishop of Canterbury ; June 15 – Dattus (or Datto), Lombard rebel leader ; August 16 – Zhou Huaizheng, Chinese eunuch ; Al-Mu'ayyad Ahmad, Muslim imam (b. 944) ; Al-Sijzi, Persian mathematician (approximate date) ; Bernard I (Taillefer), Spanish nobleman ; Bouchard II (the Bearde... | [
"1020\n\nYear 1020 (MXX) was a leap year starting on Friday (link will display the full calendar) of the Julian calendar.",
"1020 — By place\n\nSummer – Emperor Henry II conducts his third Italian military campaign. He makes plans to invade the south, but remains non-commital. ; June 15 – Byzantine tr... |
1020_AM_26241402 | What information does the article about '1020 AM' provide? | The following radio stations broadcast on AM frequency 1020 kHz: 1020 AM is a clear-channel U.S. frequency. KDKA Pittsburgh and KVNT Eagle River, Alaska, share Class A status of 1020 AM. | [
"1020 AM — In Argentina\n\nLRA58 in Rio Mayo, Chubut ; LRJ214 in San Juan ; LT10 in Santa Fe",
"1020 AM — In the United States\n\nStations in bold are clear-channel stations.",
"1020 AM\n\nThe following radio stations broadcast on AM frequency 1020 kHz: 1020 AM is a clear-channel U.S. frequency. KDKA Pittsburgh... |
1020_Arcadia_19452923 | What does the article about '1020 Arcadia' say regarding 'Orbit and classification'? | Arcadia is a member of the Agnia family (514), a very large family of stony asteroids with more than 2000 known members. They most likely formed from the breakup of a basalt object, which in turn was spawned from a larger parent body that underwent igneous differentiation. The family's parent body and namesake is the a... | [
"1020 Arcadia — Orbit and classification\n\nArcadia is a member of the Agnia family (514), a very large family of stony asteroids with more than 2000 known members. They most likely formed from the breakup of a basalt object, which in turn was spawned from a larger parent body that underwent igneous differentiation... |
1020_Arcadia_19452924 | What does the article about '1020 Arcadia' say regarding 'Physical characteristics'? | In the SMASS classification, Arcadia is a common, stony S-type asteroid. It has been characterized as an S-type by Pan-STARRS photometric survey, as well as by SDSS-MFB (Masi Foglia Bus). | [
"1020 Arcadia — Orbit and classification\n\nArcadia is a member of the Agnia family (514), a very large family of stony asteroids with more than 2000 known members. They most likely formed from the breakup of a basalt object, which in turn was spawned from a larger parent body that underwent igneous differentiation... |
1020_Arcadia_19452926 | Reconstruct the content about 'Diameter and albedo' from the article on '1020 Arcadia'. | According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Arcadia measures between 10.067 and 13.02 kilometers in diameter and its surface has an albedo between 0.150 and 0.2364. The Collaborative Asteroid Lightcurve Link assumes an albedo 0.057, i.e. an albedo for a carb... | [
"1020 Arcadia — Orbit and classification\n\nArcadia is a member of the Agnia family (514), a very large family of stony asteroids with more than 2000 known members. They most likely formed from the breakup of a basalt object, which in turn was spawned from a larger parent body that underwent igneous differentiation... |
1020_Arcadia_19452925 | Summarize the 'Rotation period' part of '1020 Arcadia'. | In November 2011, a fragmentary rotational lightcurve of Arcadia was obtained from photometric observations by Gordon Gartrelle at the University of North Dakota. Lightcurve analysis gave a rotation period of 17.02 hours with a brightness amplitude of 0.05 magnitude (U=1). As of 2018, no secure period has been obtained... | [
"1020 Arcadia — Orbit and classification\n\nArcadia is a member of the Agnia family (514), a very large family of stony asteroids with more than 2000 known members. They most likely formed from the breakup of a basalt object, which in turn was spawned from a larger parent body that underwent igneous differentiation... |
1020_Arcadia_19452927 | Describe the 'Naming' section of the article about '1020 Arcadia'. | This minor planet was named after the Greek region of Arcadia in central Peloponnese. It is also a celebrated mythological region, where the shepherd god Pan lived. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 97). | [
"1020 Arcadia — Orbit and classification\n\nArcadia is a member of the Agnia family (514), a very large family of stony asteroids with more than 2000 known members. They most likely formed from the breakup of a basalt object, which in turn was spawned from a larger parent body that underwent igneous differentiation... |
1020_Arcadia_19452922 | Reconstruct the content from the article about '1020 Arcadia'. | 1020 Arcadia, provisional designation, is a stony Agnia asteroid from the central regions of the asteroid belt, approximately 11 km in diameter. It was discovered on 7 March 1924, by German astronomer Karl Reinmuth at the Heidelberg Observatory in Heidelberg, Germany. The asteroid was named after the Greek region of Ar... | [
"1020 Arcadia — Orbit and classification\n\nArcadia is a member of the Agnia family (514), a very large family of stony asteroids with more than 2000 known members. They most likely formed from the breakup of a basalt object, which in turn was spawned from a larger parent body that underwent igneous differentiation... |
10208_Germanicus_32926361 | Describe the content of the article about '10208 Germanicus'. | 10208 Germanicus, provisional designation, is a stony Florian asteroid and binary system from the inner regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 30 August 1997, by Italian amateur astronomer Antonio Vagnozzi at the Santa Lucia Stroncone Astronomical Observatory in Str... | [
"10208 Germanicus\n\n10208 Germanicus, provisional designation, is a stony Florian asteroid and binary system from the inner regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 30 August 1997, by Italian amateur astronomer Antonio Vagnozzi at the Santa Lucia Stroncone Astron... |
10208_Germanicus_32926365 | What does the article about '10208 Germanicus' say regarding 'Naming'? | This minor planet was named for the ancient Roman general and poet Germanicus (15 BC – AD 19), who led several successful campaigns into Germania. Germanicus was also the nephew and designated heir of the Roman Emperor Tiberius. As a poet, he wrote "Aratea", an astronomical treatise, which illustrated copy is known as ... | [
"10208 Germanicus\n\n10208 Germanicus, provisional designation, is a stony Florian asteroid and binary system from the inner regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 30 August 1997, by Italian amateur astronomer Antonio Vagnozzi at the Santa Lucia Stroncone Astron... |
10208_Germanicus_32926362 | Explain what '10208 Germanicus' covers in the 'Orbit and classification' section. | Germanicus is a member of the Flora family, one of the largest families of stony asteroids. It orbits the Sun in the inner main-belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,221 days). Its orbit has an eccentricity of 0.20 and an inclination of 5° with respect to the ecliptic. It was first observe... | [
"10208 Germanicus\n\n10208 Germanicus, provisional designation, is a stony Florian asteroid and binary system from the inner regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 30 August 1997, by Italian amateur astronomer Antonio Vagnozzi at the Santa Lucia Stroncone Astron... |
10208_Germanicus_32926364 | What does the article about '10208 Germanicus' say regarding 'Lightcurve and satellite'? | In August 2007, a rotational lightcurve of Germanicus was obtained from photometric observations by an international group of astronomers. Lightcurve analysis gave a rotation period of 3.1291 hours with a brightness variation of 0.13 magnitude (U=n.a.). It was also revealed that Germanicus is orbited by a minor-planet ... | [
"10208 Germanicus\n\n10208 Germanicus, provisional designation, is a stony Florian asteroid and binary system from the inner regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 30 August 1997, by Italian amateur astronomer Antonio Vagnozzi at the Santa Lucia Stroncone Astron... |
10208_Germanicus_32926363 | Reconstruct the content about 'Diameter and albedo' from the article on '10208 Germanicus'. | According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Germanicus measures 2.87 and 3.552 kilometers in diameter and its surface has an albedo of 0.36 and 0.267, respectively. The Collaborative Asteroid Lightcurve Link adopts Petr Pravec's revised WISE-dat... | [
"10208 Germanicus\n\n10208 Germanicus, provisional designation, is a stony Florian asteroid and binary system from the inner regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered on 30 August 1997, by Italian amateur astronomer Antonio Vagnozzi at the Santa Lucia Stroncone Astron... |
1020s_in_England_22121428 | Based on the article about '1020s in England', describe the 'Deaths' section. | 1020 ; 12 June – Lyfing, Archbishop of Canterbury ; 1023 ; 28 May – Wulfstan II, Archbishop of York | [
"1020s in England — Incumbents\n\nMonarch – Canute",
"1020s in England\n\nEvents from the 1020s in England.",
"1020s in England — Deaths\n\n1020 ; 12 June – Lyfing, Archbishop of Canterbury ; 1023 ; 28 May – Wulfstan II, Archbishop of York",
"1020s in England — Events\n\n1020 ; Rotunda of Bury St Edmunds Abbe... |
1020s_in_England_22121426 | Based on the article about '1020s in England', describe the 'Events' section. | 1020 ; Rotunda of Bury St Edmunds Abbey constructed. ; Aethelnoth enthroned as Archbishop of Canterbury. ; 1021 ; 1022 ; 1023 ; Siward, a Dane, appointed Earl of Northumbria. ; Archbishop Wulfstan II of York writes Homilies. ; 1024 ; 1025 ; King Cnut forms an alliance with Byzantine emperor Constantine VIII. ; 1026 ; T... | [
"1020s in England — Incumbents\n\nMonarch – Canute",
"1020s in England\n\nEvents from the 1020s in England.",
"1020s in England — Deaths\n\n1020 ; 12 June – Lyfing, Archbishop of Canterbury ; 1023 ; 28 May – Wulfstan II, Archbishop of York",
"1020s in England — Events\n\n1020 ; Rotunda of Bury St Edmunds Abbe... |
1020s_in_art_19601389 | What information does the article about '1020s in art' provide on 'Deaths'? | 1028: Lin Bu - Chinese poet and calligrapher (born 967) ; 1027: Fujiwara no Yukinari - Japanese calligrapher (shodoka) during the Heian period (born 972) ; 1022: Ibn al-Bawwab – Arabic calligrapher and illuminator (b. unknown) | [
"1020s in art — Deaths\n\n1028: Lin Bu - Chinese poet and calligrapher (born 967) ; 1027: Fujiwara no Yukinari - Japanese calligrapher (shodoka) during the Heian period (born 972) ; 1022: Ibn al-Bawwab – Arabic calligrapher and illuminator (b. unknown)",
"1020s in art\n\nThe decade of the 1020s in art involved so... |
1020s_in_poetry_14038027 | Summarize the 'Births' part of '1020s in poetry'. | Solomon ibn Gabirol (died 1058), Hebrew poet in Al-Andalus ; Wang Anshi (died 1086), Song poet Death years link to the corresponding "[year] in poetry" article. There are conflicting or unreliable sources for the birth years of many people born in this period; where sources conflict, the poet is listed again and the co... | [
"1020s in poetry\n\nNationality words link to articles with information on the nation's poetry or literature (for instance, Irish or France).",
"1020s in poetry — Births\n\nSolomon ibn Gabirol (died 1058), Hebrew poet in Al-Andalus ; Wang Anshi (died 1086), Song poet Death years link to the corresponding \"[year]... |
1021_26474796 | Summarize the 'Deaths' part of '1021'. | February 13 – Al-Hakim bi-Amr Allah, Fatimid caliph (b. 985) ; March 5 – Arnulf, French archbishop and illegitimate son of Lothair III ; March 16 – Heribert, archbishop of Cologne (b. c. 970) ; July 7 – Fujiwara no Akimitsu, Japanese bureaucrat (b. 944) ; August 17 – Erkanbald, German abbo... | [
"1021 — Africa\n\nThe last evidence of indigenous Christian and non-Arabophone culture in Tripolitania (modern Libya) is seen.",
"1021 — Japan\n\nDaughter of Michinaga, Fujiwara no Kishi is married to Crown Prince Atsunaga (to be next empress)",
"1021 — Deaths\n\nFebruary 13 – Al-Hakim bi-Amr Allah, Fatim... |
1021_26474793 | Reconstruct the content about 'Asia' from the article on '1021'. | Senekerim-Hovhannes Artsruni, king of Vaspurakan (Greater Armenia), surrenders his kingdom to the Byzantine Empire. He receives in return Sebasteia and becomes governor of Cappadocia. ; Battle of Shirimni, the Byzantine Empire under Basil II defeats the Kingdom of Georgia under Giorgi I at Shirimni, at the Lake Palaka... | [
"1021 — Africa\n\nThe last evidence of indigenous Christian and non-Arabophone culture in Tripolitania (modern Libya) is seen.",
"1021 — Japan\n\nDaughter of Michinaga, Fujiwara no Kishi is married to Crown Prince Atsunaga (to be next empress)",
"1021 — Deaths\n\nFebruary 13 – Al-Hakim bi-Amr Allah, Fatim... |
1021_26474794 | Describe the 'North America' section of the article about '1021'. | Using a new dating technique analysing tree rings has provided evidence that Vikings occupied L'Anse aux Meadows in Newfoundland, Canada, in this year. Although It has long been known that Europeans reached the Americas before Columbus's arrival in the New World in 1492 - Using an atmospheric radiocarbon signal produce... | [
"1021 — Africa\n\nThe last evidence of indigenous Christian and non-Arabophone culture in Tripolitania (modern Libya) is seen.",
"1021 — Japan\n\nDaughter of Michinaga, Fujiwara no Kishi is married to Crown Prince Atsunaga (to be next empress)",
"1021 — Deaths\n\nFebruary 13 – Al-Hakim bi-Amr Allah, Fatim... |
1021_26474789 | Describe the content of the article about '1021'. | Year 1021 (MXXI) was a common year starting on Sunday (link will display the full calendar) of the Julian calendar. | [
"1021 — Africa\n\nThe last evidence of indigenous Christian and non-Arabophone culture in Tripolitania (modern Libya) is seen.",
"1021 — Japan\n\nDaughter of Michinaga, Fujiwara no Kishi is married to Crown Prince Atsunaga (to be next empress)",
"1021 — Deaths\n\nFebruary 13 – Al-Hakim bi-Amr Allah, Fatim... |
1021_26474795 | Explain what '1021' covers in the 'Births' section. | December 8 – Wang Anshi, Chinese chancellor (d. 1086) ; Eudokia Makrembolitissa, Byzantine empress (d. 1096) ; Fujiwara no Kanshi, Japanese empress consort (d. 1102) ; Wugunai, Chinese chieftain of the Wanyan tribe (d. 1074) | [
"1021 — Africa\n\nThe last evidence of indigenous Christian and non-Arabophone culture in Tripolitania (modern Libya) is seen.",
"1021 — Japan\n\nDaughter of Michinaga, Fujiwara no Kishi is married to Crown Prince Atsunaga (to be next empress)",
"1021 — Deaths\n\nFebruary 13 – Al-Hakim bi-Amr Allah, Fatim... |
1021_Flammario_20258246 | Summarize the 'Rotation period' part of '1021 Flammario'. | Several rotational lightcurves of Flammario have been obtained from photometric observations since the 1990s (U=2/2/2). Analysis of the best-rated lightcurve obtained by French amateur astronomer Laurent Bernasconi in January 2005 gave a rotation period of 12.160 hours with a consolidated brightness amplitude between 0... | [
"1021 Flammario — Rotation period\n\nSeveral rotational lightcurves of Flammario have been obtained from photometric observations since the 1990s (U=2/2/2). Analysis of the best-rated lightcurve obtained by French amateur astronomer Laurent Bernasconi in January 2005 gave a rotation period of 12.160 hours with a co... |
1021_Flammario_20258245 | Summarize the 'Physical characteristics' part of '1021 Flammario'. | In the SMASS classification, Flammario is a "bright" carbonaceous B-type, while it is an uncommon F-type asteroid in the Tholen taxonomy. (The SMASS taxonomic scheme classifies all F-types as B-type asteroids). More recent polarimetric observations also characterized the asteroid as a dark F-type. | [
"1021 Flammario — Rotation period\n\nSeveral rotational lightcurves of Flammario have been obtained from photometric observations since the 1990s (U=2/2/2). Analysis of the best-rated lightcurve obtained by French amateur astronomer Laurent Bernasconi in January 2005 gave a rotation period of 12.160 hours with a co... |
1021_Flammario_20258243 | What information does the article about '1021 Flammario' provide? | 1021 Flammario, provisional designation, is a dark background asteroid from the central regions of the asteroid belt, approximately 100 km in diameter. It was discovered on 11 March 1924, by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory in Heidelberg, Germany. The asteroid was named after Fr... | [
"1021 Flammario — Rotation period\n\nSeveral rotational lightcurves of Flammario have been obtained from photometric observations since the 1990s (U=2/2/2). Analysis of the best-rated lightcurve obtained by French amateur astronomer Laurent Bernasconi in January 2005 gave a rotation period of 12.160 hours with a co... |
1021_Flammario_20258247 | Describe the 'Poles' section of the article about '1021 Flammario'. | In 2016, a modeled lightcurve using photometric data from various sources, rendered a similar sidereal period of 12.15186 hours and two spin axes of (32.0°, 22.0°) and (216.0°, 55.0°) in ecliptic coordinates. | [
"1021 Flammario — Rotation period\n\nSeveral rotational lightcurves of Flammario have been obtained from photometric observations since the 1990s (U=2/2/2). Analysis of the best-rated lightcurve obtained by French amateur astronomer Laurent Bernasconi in January 2005 gave a rotation period of 12.160 hours with a co... |
1021_Flammario_20258248 | Explain what '1021 Flammario' covers in the 'Diameter and albedo' section. | According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Flammario measures between 84.78 and 105 kilometers in diameter and its surface has a low albedo between 0.04 and 0.05. The Collaborative ... | [
"1021 Flammario — Rotation period\n\nSeveral rotational lightcurves of Flammario have been obtained from photometric observations since the 1990s (U=2/2/2). Analysis of the best-rated lightcurve obtained by French amateur astronomer Laurent Bernasconi in January 2005 gave a rotation period of 12.160 hours with a co... |
1021_Flammario_20258244 | Based on the article about '1021 Flammario', describe the 'Orbit and classification' section. | Flammario is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 2.0–3.5 AU once every 4 years and 6 months (1,654 days; semi-major axis of 2.74 AU). Its orbit has an eccentricity of 0.29 and an inclination of 16° with respect to the ecliptic... | [
"1021 Flammario — Rotation period\n\nSeveral rotational lightcurves of Flammario have been obtained from photometric observations since the 1990s (U=2/2/2). Analysis of the best-rated lightcurve obtained by French amateur astronomer Laurent Bernasconi in January 2005 gave a rotation period of 12.160 hours with a co... |
1022_26474782 | Describe the 'Byzantine Empire' section of the article about '1022'. | Spring – Battle of Svindax: The Byzantine army under Emperor Basil II defeats the Georgians at Svindax (modern Turkey). King George I is forced to negotiate a peace treaty, ending the Byzantine–Georgian wars. ; Summer – Nikephoros Phokas (Barytrachelos) conspires with the Byzantine general Nikephoros Xiphia... | [
"1022 — Byzantine Empire\n\nSpring – Battle of Svindax: The Byzantine army under Emperor Basil II defeats the Georgians at Svindax (modern Turkey). King George I is forced to negotiate a peace treaty, ending the Byzantine–Georgian wars. ; Summer – Nikephoros Phokas (Barytrachelos) conspires with the Byz... |
1022_26474784 | What does the article about '1022' say regarding 'Africa'? | The 14-year-old Al-Mu'izz ibn Badis takes over, with support of the Zirid nobles, the government and ascends (as a minor) to the throne in Ifriqiya (modern Tunisia). | [
"1022 — Byzantine Empire\n\nSpring – Battle of Svindax: The Byzantine army under Emperor Basil II defeats the Georgians at Svindax (modern Turkey). King George I is forced to negotiate a peace treaty, ending the Byzantine–Georgian wars. ; Summer – Nikephoros Phokas (Barytrachelos) conspires with the Byz... |
1022_26474786 | Describe the 'Religion' section of the article about '1022'. | After the Council of Orléans, King Robert II (the Pious) burns thirteen heretics at Orléans. These are the first burning victims for heresy in Medieval Europe. ; Pope Benedict VIII convenes a synod at Pavia. He issues decrees to restrain simony and incontinence of the clergy. ; Æthelnoth, archbishop of Canterbury, trav... | [
"1022 — Byzantine Empire\n\nSpring – Battle of Svindax: The Byzantine army under Emperor Basil II defeats the Georgians at Svindax (modern Turkey). King George I is forced to negotiate a peace treaty, ending the Byzantine–Georgian wars. ; Summer – Nikephoros Phokas (Barytrachelos) conspires with the Byz... |
1022_26474788 | What does the article about '1022' say regarding 'Deaths'? | March 12 – Symeon (the New Theologian), Byzantine monk (b. 949) ; March 23 – Zhen Zong, emperor of the Song Dynasty (b. 968) ; March 30 – Atenulf, Italian nobleman and Benedictine abbot ; June 28 – Notker III, German Benedictine monk and writer ; July 23 – Lei Yungong, Chinese palace eunuc... | [
"1022 — Byzantine Empire\n\nSpring – Battle of Svindax: The Byzantine army under Emperor Basil II defeats the Georgians at Svindax (modern Turkey). King George I is forced to negotiate a peace treaty, ending the Byzantine–Georgian wars. ; Summer – Nikephoros Phokas (Barytrachelos) conspires with the Byz... |
1022_26474785 | What does the article about '1022' say regarding 'Asia'? | The Chinese military has one million registered soldiers during the Song Dynasty, an increase since the turn of the 11th century (approximate date). | [
"1022 — Byzantine Empire\n\nSpring – Battle of Svindax: The Byzantine army under Emperor Basil II defeats the Georgians at Svindax (modern Turkey). King George I is forced to negotiate a peace treaty, ending the Byzantine–Georgian wars. ; Summer – Nikephoros Phokas (Barytrachelos) conspires with the Byz... |
1022_26474787 | What information does the article about '1022' provide on 'Births'? | Fujiwara no Nobunaga, Japanese nobleman (d. 1094) ; Harold II, king of England (approximate date) ; Manasses III, French nobleman (d. 1065) ; Michael Attaleiates, Byzantine historian (d. 1080) ; Ordulf, duke of Saxony (approximate date) ; Rajaraja Narendra, Indian ruler (d. 1061) | [
"1022 — Byzantine Empire\n\nSpring – Battle of Svindax: The Byzantine army under Emperor Basil II defeats the Georgians at Svindax (modern Turkey). King George I is forced to negotiate a peace treaty, ending the Byzantine–Georgian wars. ; Summer – Nikephoros Phokas (Barytrachelos) conspires with the Byz... |
1022_26474783 | Reconstruct the content about 'Europe' from the article on '1022'. | Spring – Emperor Henry II divides his army into three columns and descends through Rome onto Capua. The bulk of the expeditionary force (20,000 men) led by Henry, makes its way down the Adriatic coast. ; Pilgrim, archbishop of Cologne, marches with his army down the Tyrrhenian coast to lay siege to Capua. The cit... | [
"1022 — Byzantine Empire\n\nSpring – Battle of Svindax: The Byzantine army under Emperor Basil II defeats the Georgians at Svindax (modern Turkey). King George I is forced to negotiate a peace treaty, ending the Byzantine–Georgian wars. ; Summer – Nikephoros Phokas (Barytrachelos) conspires with the Byz... |
1022_Olympiada_20258273 | What information does the article about '1022 Olympiada' provide on 'Rotation period'? | Several rotational lightcurves of Olympiada have been obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Analysis of the best-rated lightcurve from April 2008 gave a rotation period of 3.833 hours with a consolidated brightness variation between 0.27... | [
"1022 Olympiada — Rotation period\n\nSeveral rotational lightcurves of Olympiada have been obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Analysis of the best-rated lightcurve from April 2008 gave a rotation period of 3.833 hours with a conso... |
1022_Olympiada_20258275 | What information does the article about '1022 Olympiada' provide on 'Diameter and albedo'? | According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Olympiada measures between 26.39 and 34.30 kilometers in diameter and its surface has an albedo between 0.105 and 0.1600. The Collaborativ... | [
"1022 Olympiada — Rotation period\n\nSeveral rotational lightcurves of Olympiada have been obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Analysis of the best-rated lightcurve from April 2008 gave a rotation period of 3.833 hours with a conso... |
1022_Olympiada_20258270 | What does the article about '1022 Olympiada' say regarding 'Orbit and classification'? | Olympiada is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 2.3–3.3 AU once every 4 years and 8 months (1,716 days; semi-major axis of 2.81 AU). Its orbit has an eccentricity of 0.17 and an inclination of 21° with respect to the ecliptic... | [
"1022 Olympiada — Rotation period\n\nSeveral rotational lightcurves of Olympiada have been obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Analysis of the best-rated lightcurve from April 2008 gave a rotation period of 3.833 hours with a conso... |
1022_Olympiada_20258269 | What information does the article about '1022 Olympiada' provide? | 1022 Olympiada, provisional designation, is a background asteroid from the central regions of the asteroid belt, approximately 30 km in diameter. It was discovered at the Simeiz Observatory on the Crimean peninsula on 23 June 1924, by Soviet astronomer Vladimir Albitsky, who named it after his mother, Olimpiada Albitsk... | [
"1022 Olympiada — Rotation period\n\nSeveral rotational lightcurves of Olympiada have been obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Analysis of the best-rated lightcurve from April 2008 gave a rotation period of 3.833 hours with a conso... |
1022_Olympiada_20258274 | What information does the article about '1022 Olympiada' provide on 'Poles'? | In 2011, a modeled lightcurve using data from the Uppsala Asteroid Photometric Catalogue and other sources gave a concurring sidereal period 3.83359 hours, as well as two poles at (46.0°, 10.0°) and (242.0°, 52.0°) in ecliptic coordinates (λ, β) (Q=2+). Brian Warner also determined two spin axes at (40.0°, 18.0°) and (... | [
"1022 Olympiada — Rotation period\n\nSeveral rotational lightcurves of Olympiada have been obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Analysis of the best-rated lightcurve from April 2008 gave a rotation period of 3.833 hours with a conso... |
1022_Olympiada_20258271 | Summarize the 'Naming' part of '1022 Olympiada'. | This minor planet was named after Olimpiada Albitskaya, mother of the discoverer Vladimir Albitsky (1891–1952). No accurate naming citation was given for this asteroid in The Names of the Minor Planets. The author of the Dictionary of Minor Planets, Lutz Schmadel, learned about the naming circumstances from Nikolai Che... | [
"1022 Olympiada — Rotation period\n\nSeveral rotational lightcurves of Olympiada have been obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Analysis of the best-rated lightcurve from April 2008 gave a rotation period of 3.833 hours with a conso... |
1023_26474775 | Based on the article about '1023', describe the 'Japan' section. | 60th Birthday and Longevity Ceremony of Minamoto no Rinshi (Female head of the Fujiwara clan, Wife of Fujiwara no Michinaga, mother of Grand Empress Dowager Shoshi, Empress Dowager Kenshi and Empress Ishi, grandmother of Emperor Go-Ichijo) April: An epidemic in Kyoto was so severe that there were corpses in the streets... | [
"1023 — Japan\n\n60th Birthday and Longevity Ceremony of Minamoto no Rinshi (Female head of the Fujiwara clan, Wife of Fujiwara no Michinaga, mother of Grand Empress Dowager Shoshi, Empress Dowager Kenshi and Empress Ishi, grandmother of Emperor Go-Ichijo) April: An epidemic in Kyoto was so severe that there were c... |
1023_26474778 | What does the article about '1023' say regarding 'Religion'? | The Dom Church at Utrecht (modern Netherlands) is severely damaged by fire. Bishop Adalbold II builds a new Romanesque style church. | [
"1023 — Japan\n\n60th Birthday and Longevity Ceremony of Minamoto no Rinshi (Female head of the Fujiwara clan, Wife of Fujiwara no Michinaga, mother of Grand Empress Dowager Shoshi, Empress Dowager Kenshi and Empress Ishi, grandmother of Emperor Go-Ichijo) April: An epidemic in Kyoto was so severe that there were c... |
1023_26474774 | What information does the article about '1023' provide? | Year 1023 (MXXIII) was a common year starting on Tuesday (link will display the full calendar) of the Julian calendar. | [
"1023 — Japan\n\n60th Birthday and Longevity Ceremony of Minamoto no Rinshi (Female head of the Fujiwara clan, Wife of Fujiwara no Michinaga, mother of Grand Empress Dowager Shoshi, Empress Dowager Kenshi and Empress Ishi, grandmother of Emperor Go-Ichijo) April: An epidemic in Kyoto was so severe that there were c... |
1023_26474780 | Summarize the 'Deaths' part of '1023'. | March 27 – Gebhard I, bishop of Regensburg ; May 28 – Wulfstan (or Lupus), archbishop of York ; October 18 – Zirid princess and regent ; October 21 – Gero, archbishop of Magdeburg ; October 24 – Kou Zhun, Chinese grand chancellor ; November 24 – Eilward, bishop of Dresden-Meissen ; D... | [
"1023 — Japan\n\n60th Birthday and Longevity Ceremony of Minamoto no Rinshi (Female head of the Fujiwara clan, Wife of Fujiwara no Michinaga, mother of Grand Empress Dowager Shoshi, Empress Dowager Kenshi and Empress Ishi, grandmother of Emperor Go-Ichijo) April: An epidemic in Kyoto was so severe that there were c... |
1023_26474779 | What information does the article about '1023' provide on 'Births'? | Lý Thánh Tông, Vietnamese emperor (d. 1072) ; Otto I (or Odon), count of Savoy (approximate date) ; Ramon Berenguer I, count of Barcelona (d. 1076) ; William VII (the Bold), duke of Aquitaine (d. 1058) | [
"1023 — Japan\n\n60th Birthday and Longevity Ceremony of Minamoto no Rinshi (Female head of the Fujiwara clan, Wife of Fujiwara no Michinaga, mother of Grand Empress Dowager Shoshi, Empress Dowager Kenshi and Empress Ishi, grandmother of Emperor Go-Ichijo) April: An epidemic in Kyoto was so severe that there were c... |
1023_26474776 | Reconstruct the content about 'Europe' from the article on '1023'. | The Judge-Governor of Seville in Al-Andalus (modern Spain) takes advantage of the disintegration of the Caliphate of Córdoba, and seizes power as Abbad I, founding the Abbadid Dynasty. ; December – Abbad I declares the Taifa of Seville independent from Córdoban rule. Abd ar-Rahman V is proclaimed Caliph at Córdob... | [
"1023 — Japan\n\n60th Birthday and Longevity Ceremony of Minamoto no Rinshi (Female head of the Fujiwara clan, Wife of Fujiwara no Michinaga, mother of Grand Empress Dowager Shoshi, Empress Dowager Kenshi and Empress Ishi, grandmother of Emperor Go-Ichijo) April: An epidemic in Kyoto was so severe that there were c... |
1023_Thomana_20699611 | Based on the article about '1023 Thomana', describe the 'Rotation period' section. | Between 2006 and 2009, three rotational lightcurves of Thomana were obtained from photometric observations by astronomers James W. Brinsfield, Pierre Antonini as well as René Roy and Laurent Bernasconi. Lightcurve analysis gave a concurring rotation period of 17.56 hours with a brightness variation between 0.27 and 0.3... | [
"1023 Thomana — Rotation period\n\nBetween 2006 and 2009, three rotational lightcurves of Thomana were obtained from photometric observations by astronomers James W. Brinsfield, Pierre Antonini as well as René Roy and Laurent Bernasconi. Lightcurve analysis gave a concurring rotation period of 17.56 hours with a br... |
1023_Thomana_20699614 | Reconstruct the content about 'Naming' from the article on '1023 Thomana'. | This minor planet was named by the discoverer after the St. Thomas Choir of Leipzig ("Thomanerchor"), a boys' choir at St. Thomas Church in Leipzig, Germany, where Johann Sebastian Bach used to work as music director. The official naming citation was published by Paul Herget in The Names of the Minor Planets in 1955 (H... | [
"1023 Thomana — Rotation period\n\nBetween 2006 and 2009, three rotational lightcurves of Thomana were obtained from photometric observations by astronomers James W. Brinsfield, Pierre Antonini as well as René Roy and Laurent Bernasconi. Lightcurve analysis gave a concurring rotation period of 17.56 hours with a br... |
1023_Thomana_20699613 | Explain what '1023 Thomana' covers in the 'Diameter and albedo' section. | According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Thomana measures between 53.28 and 61.34 kilometers in diameter and its surface has an albedo between 0.05 and 0.065. The Co... | [
"1023 Thomana — Rotation period\n\nBetween 2006 and 2009, three rotational lightcurves of Thomana were obtained from photometric observations by astronomers James W. Brinsfield, Pierre Antonini as well as René Roy and Laurent Bernasconi. Lightcurve analysis gave a concurring rotation period of 17.56 hours with a br... |
1023_Thomana_20699612 | Summarize the 'Spin axis' part of '1023 Thomana'. | In 2016, an international study modeled a lightcurve from various data sources with a period of 17.5611 hours and found two spin axis of (86.0°, −65.0°) and (272.0°, −42.0°), respectively, in ecliptic coordinates (λ, β) (Q=n.a.). | [
"1023 Thomana — Rotation period\n\nBetween 2006 and 2009, three rotational lightcurves of Thomana were obtained from photometric observations by astronomers James W. Brinsfield, Pierre Antonini as well as René Roy and Laurent Bernasconi. Lightcurve analysis gave a concurring rotation period of 17.56 hours with a br... |
1023_Thomana_20699608 | What information does the article about '1023 Thomana' provide? | 1023 Thomana, provisional designation, is a rare-type carbonaceous background asteroid from the outer regions of the asteroid belt, approximately 58 kilometers in diameter. It was discovered on 25 June 1924, by German astronomer Karl Reinmuth at Heidelberg Observatory in southwest Germany. The asteroid was named after ... | [
"1023 Thomana — Rotation period\n\nBetween 2006 and 2009, three rotational lightcurves of Thomana were obtained from photometric observations by astronomers James W. Brinsfield, Pierre Antonini as well as René Roy and Laurent Bernasconi. Lightcurve analysis gave a concurring rotation period of 17.56 hours with a br... |
1023_Thomana_20699609 | Reconstruct the content about 'Classification and orbit' from the article on '1023 Thomana'. | Thomana orbits the Sun in the outer main-belt at a distance of 2.8–3.5 AU once every 5 years and 8 months (2,058 days). Its orbit has an eccentricity of 0.10 and an inclination of 10° with respect to the ecliptic. The asteroid's observation arc begins at Heidelberg, one night after its official discovery observation. | [
"1023 Thomana — Rotation period\n\nBetween 2006 and 2009, three rotational lightcurves of Thomana were obtained from photometric observations by astronomers James W. Brinsfield, Pierre Antonini as well as René Roy and Laurent Bernasconi. Lightcurve analysis gave a concurring rotation period of 17.56 hours with a br... |
1024_26474771 | Based on the article about '1024', describe the 'Religion' section. | April 9 – Pope Benedict VIII dies after a 12-year pontificate at Rome. He is succeeded by his brother John XIX as the 144th pope of the Catholic Church. | [
"1024 — Religion\n\nApril 9 – Pope Benedict VIII dies after a 12-year pontificate at Rome. He is succeeded by his brother John XIX as the 144th pope of the Catholic Church.",
"1024 — Deaths\n\nApril 9 – Benedict VIII, pope of the Catholic Church ; July 13 – Henry II, Holy Roman Emperor (b. 973) ... |
1024_26474773 | Reconstruct the content about 'Deaths' from the article on '1024'. | April 9 – Benedict VIII, pope of the Catholic Church ; July 13 – Henry II, Holy Roman Emperor (b. 973) ; Abd ar-Rahman V, Umayyad caliph of Córdoba ; Alpert of Metz, French Benedictine chronicler ; Brihtwine, bishop of Wells (approximate date) ; Choe Hang, civil minister of Goryeo (Korea) ; Cúán úa Lothchái... | [
"1024 — Religion\n\nApril 9 – Pope Benedict VIII dies after a 12-year pontificate at Rome. He is succeeded by his brother John XIX as the 144th pope of the Catholic Church.",
"1024 — Deaths\n\nApril 9 – Benedict VIII, pope of the Catholic Church ; July 13 – Henry II, Holy Roman Emperor (b. 973) ... |
1024_26474767 | Reconstruct the content about 'Japan' from the article on '1024'. | Daini no Sanmi (waka poet, lady-in-waiting to Grand Empress Dowager Shoshi) is married to Kanetaka Sagami (waka poet) divorce and return to Kyoto - she become a lady-in-waiting to Imperial Princess Shushi Murder of the daughter of late Emperor Kazan - the girl was a lady-in-waiting to Grand Empress Dowager Shoshi who o... | [
"1024 — Religion\n\nApril 9 – Pope Benedict VIII dies after a 12-year pontificate at Rome. He is succeeded by his brother John XIX as the 144th pope of the Catholic Church.",
"1024 — Deaths\n\nApril 9 – Benedict VIII, pope of the Catholic Church ; July 13 – Henry II, Holy Roman Emperor (b. 973) ... |
1024_26474766 | Reconstruct the content from the article about '1024'. | Year 1024 (MXXIV) was a leap year starting on Wednesday (link will display the full calendar) of the Julian calendar. | [
"1024 — Religion\n\nApril 9 – Pope Benedict VIII dies after a 12-year pontificate at Rome. He is succeeded by his brother John XIX as the 144th pope of the Catholic Church.",
"1024 — Deaths\n\nApril 9 – Benedict VIII, pope of the Catholic Church ; July 13 – Henry II, Holy Roman Emperor (b. 973) ... |
1024_26474770 | Based on the article about '1024', describe the 'Asia' section. | The world's first paper-printed money, which later greatly benefits the economy of the Song Dynasty, originates in the Sichuan province of China. ; Sultan Mahmud of Ghazni sacks the Hindu religious center of Somnath, and takes away a booty of 20 million dinars (approximate date). ; In Japan, the Manju (万寿) era begins. | [
"1024 — Religion\n\nApril 9 – Pope Benedict VIII dies after a 12-year pontificate at Rome. He is succeeded by his brother John XIX as the 144th pope of the Catholic Church.",
"1024 — Deaths\n\nApril 9 – Benedict VIII, pope of the Catholic Church ; July 13 – Henry II, Holy Roman Emperor (b. 973) ... |
1024_26474768 | Describe the 'Byzantine Empire' section of the article about '1024'. | Emperor Basil II prepares a Byzantine expedition to invade Sicily. Governor Ahmed al-Akhal appeals to the Zirids of Ifriqiya for help. They dispatch a fleet, but these are caught up in a storm and destroyed near Pantelleria. ; Battle of Lemnos: Kievan Viking raiders (800 men) sail through the straits at Abydos to the A... | [
"1024 — Religion\n\nApril 9 – Pope Benedict VIII dies after a 12-year pontificate at Rome. He is succeeded by his brother John XIX as the 144th pope of the Catholic Church.",
"1024 — Deaths\n\nApril 9 – Benedict VIII, pope of the Catholic Church ; July 13 – Henry II, Holy Roman Emperor (b. 973) ... |
1024_26474772 | Summarize the 'Births' part of '1024'. | May 13 – Hugh the Great, abbot of Cluny (d. 1109) ; Al-Kunduri, vizier of the Seljuk Empire (d. 1064) ; Bruno II, margrave of Friesland (d. 1057) ; Fu Yaoyu, Chinese official and politician (d. 1091) ; Iziaslav I, Grand Prince of Kiev (d. 1078) ; Magnus the Good, king of Norway (d. 1047) | [
"1024 — Religion\n\nApril 9 – Pope Benedict VIII dies after a 12-year pontificate at Rome. He is succeeded by his brother John XIX as the 144th pope of the Catholic Church.",
"1024 — Deaths\n\nApril 9 – Benedict VIII, pope of the Catholic Church ; July 13 – Henry II, Holy Roman Emperor (b. 973) ... |
1024_26474769 | Reconstruct the content about 'Europe' from the article on '1024'. | July 13 – Emperor Henry II dies in his imperial palace at Göttingen (modern Germany). He leaves no heirs, thereby ending the Ottonian Dynasty. The Salian Dynasty of the Holy Roman Empire is founded by Conrad II. ; September – Conrad II (the Elder) is elected and crowned as King of Germany in Mainz, while bo... | [
"1024 — Religion\n\nApril 9 – Pope Benedict VIII dies after a 12-year pontificate at Rome. He is succeeded by his brother John XIX as the 144th pope of the Catholic Church.",
"1024 — Deaths\n\nApril 9 – Benedict VIII, pope of the Catholic Church ; July 13 – Henry II, Holy Roman Emperor (b. 973) ... |
1024_(number)_17774855 | Based on the article about '1024 (number)', describe the 'Approximation to 1000' section. | The neat coincidence that 210 is nearly equal to 103 provides the basis of a technique of estimating larger powers of 2 in decimal notation. Using 210a+b ≈ 2b103a is fairly accurate for exponents up to about 100. For exponents up to 300, 3a continues to be a good estimate of the number of digits. For example, 253 ≈ 8×1... | [
"1024 (number) — Approximation to 1000\n\nThe neat coincidence that 210 is nearly equal to 103 provides the basis of a technique of estimating larger powers of 2 in decimal notation. Using 210a+b ≈ 2b103a is fairly accurate for exponents up to about 100. For exponents up to 300, 3a continues to be a good estimate o... |
1024_(number)_17774854 | Reconstruct the content from the article about '1024 (number)'. | 1024 is the natural number following 1023 and preceding 1025. 1024 is a power of two: 210 (2 to the tenth power). It is the nearest power of two from decimal 1000 and senary 100006 (decimal 1296). 1024 is the smallest number with exactly 11 divisors (but note that there are smaller numbers with more than 11 divisors; e... | [
"1024 (number) — Approximation to 1000\n\nThe neat coincidence that 210 is nearly equal to 103 provides the basis of a technique of estimating larger powers of 2 in decimal notation. Using 210a+b ≈ 2b103a is fairly accurate for exponents up to about 100. For exponents up to 300, 3a continues to be a good estimate o... |
1024_(number)_17774856 | What information does the article about '1024 (number)' provide on 'Special use in computers'? | In binary notation, 1024 is represented as 10000000000, making it a simple round number occurring frequently in computer applications. 1024 is the maximum number of computer memory addresses that can be referenced with ten binary switches. This is the origin of the organization of computer memory into 1024-byte chunks ... | [
"1024 (number) — Approximation to 1000\n\nThe neat coincidence that 210 is nearly equal to 103 provides the basis of a technique of estimating larger powers of 2 in decimal notation. Using 210a+b ≈ 2b103a is fairly accurate for exponents up to about 100. For exponents up to 300, 3a continues to be a good estimate o... |
1024_Hale_20699625 | Describe the 'Naming' section of the article about '1024 Hale'. | This minor planet was named after George Ellery Hale (1868–1938), a prolific American astronomer and pioneer of a new generation of large aperture telescopes, namely the 60-inch Hale and the 100-inch Hooker telescope at Mount Wilson Observatory, as well as the 200-inch Hale telescope at Palomar Observatory. He founded ... | [
"1024 Hale — Naming\n\nThis minor planet was named after George Ellery Hale (1868–1938), a prolific American astronomer and pioneer of a new generation of large aperture telescopes, namely the 60-inch Hale and the 100-inch Hooker telescope at Mount Wilson Observatory, as well as the 200-inch Hale telescope at Palom... |
1024_Hale_20699621 | Explain what '1024 Hale' covers in the 'Orbit and classification' section. | Hale is a non-family asteroid from the main belt's background population. It orbits the Sun in the outer asteroid belt at a distance of 2.2–3.5 AU once every 4 years and 10 months (1,772 days; semi-major axis of 2.87 AU). Its orbit has an eccentricity of 0.22 and an inclination of 16° with respect to the ecliptic. The ... | [
"1024 Hale — Naming\n\nThis minor planet was named after George Ellery Hale (1868–1938), a prolific American astronomer and pioneer of a new generation of large aperture telescopes, namely the 60-inch Hale and the 100-inch Hooker telescope at Mount Wilson Observatory, as well as the 200-inch Hale telescope at Palom... |
1024_Hale_20699622 | What information does the article about '1024 Hale' provide on 'Physical characteristics'? | Hale has been characterized as a carbonaceous C-type asteroid by Pan-STARRS photometric survey and by the SDSS-MFB (Masi Foglia Binzel). In the SMASS classification it is a "hydrated" Ch-subtype. | [
"1024 Hale — Naming\n\nThis minor planet was named after George Ellery Hale (1868–1938), a prolific American astronomer and pioneer of a new generation of large aperture telescopes, namely the 60-inch Hale and the 100-inch Hooker telescope at Mount Wilson Observatory, as well as the 200-inch Hale telescope at Palom... |
1024_Hale_20699623 | Based on the article about '1024 Hale', describe the 'Rotation period' section. | In January 2013, a first rotational lightcurve of Hale was obtained from photometric observations by Michael S. Alkema at the Elephant Head Observatory in Arizona, United States. Analysis of the fragmentary lightcurve gave a rotation period of 16.0 hours with a brightness amplitude of 0.10 magnitude (U=1+). As of 2018,... | [
"1024 Hale — Naming\n\nThis minor planet was named after George Ellery Hale (1868–1938), a prolific American astronomer and pioneer of a new generation of large aperture telescopes, namely the 60-inch Hale and the 100-inch Hooker telescope at Mount Wilson Observatory, as well as the 200-inch Hale telescope at Palom... |
1024_Hale_20699624 | From the article on '1024 Hale', restate the 'Diameter and albedo' content. | According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Hale measures between 28.46 and 51.37 kilometers in diameter and its surface has an albedo between 0.0260 and 0.10. The Collaborative Asteroid Lightcurve Link derives an albedo of ... | [
"1024 Hale — Naming\n\nThis minor planet was named after George Ellery Hale (1868–1938), a prolific American astronomer and pioneer of a new generation of large aperture telescopes, namely the 60-inch Hale and the 100-inch Hooker telescope at Mount Wilson Observatory, as well as the 200-inch Hale telescope at Palom... |
1024_in_Norway_27638050 | From the article on '1024 in Norway', restate the 'Events' content. | After gaining control over Norway in 1016, Olaf II Haraldsson constructed a religious code which established the Church of Norway. It is considered to represent Norway's first national legislation | [
"1024 in Norway — Events\n\nAfter gaining control over Norway in 1016, Olaf II Haraldsson constructed a religious code which established the Church of Norway. It is considered to represent Norway's first national legislation",
"1024 in Norway\n\nEvents in the year 1024 in Norway.",
"1024 in Norway — Births\n\nM... |
10241_Miličević_27460637 | What information does the article about '10241 Miličević' provide on 'Naming'? | This minor planet was named after Don Nikola Miličević (1887-1963), Croatian amateur astronomer and last administrator of Blaca hermitage. The Hermitage is an UNESCO World Heritage Site located on the Brač island in Croatia. The official naming citation was published by the Minor Planet Center on 15 December 2005 (M.P.... | [
"10241 Miličević — Naming\n\nThis minor planet was named after Don Nikola Miličević (1887-1963), Croatian amateur astronomer and last administrator of Blaca hermitage. The Hermitage is an UNESCO World Heritage Site located on the Brač island in Croatia. The official naming citation was published by the Minor Planet... |
10241_Miličević_27460635 | Reconstruct the content about 'Rotation period' from the article on '10241 Miličević'. | In December 2014, a rotational lightcurve of Miličević was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a short rotation period of 3.87 hours with a brightness amplitude of 0.34 magnitude (U=2). | [
"10241 Miličević — Naming\n\nThis minor planet was named after Don Nikola Miličević (1887-1963), Croatian amateur astronomer and last administrator of Blaca hermitage. The Hermitage is an UNESCO World Heritage Site located on the Brač island in Croatia. The official naming citation was published by the Minor Planet... |
10241_Miličević_27460634 | Explain what '10241 Miličević' covers in the 'Physical characteristics' section. | Based on its classification to the Themis family and on observations conducted by the Pan-STARRS survey, Miličević is a carbonaceous C-type asteroid. | [
"10241 Miličević — Naming\n\nThis minor planet was named after Don Nikola Miličević (1887-1963), Croatian amateur astronomer and last administrator of Blaca hermitage. The Hermitage is an UNESCO World Heritage Site located on the Brač island in Croatia. The official naming citation was published by the Minor Planet... |
10241_Miličević_27460632 | What information does the article about '10241 Miličević' provide? | 10241 Miličević, provisional designation, is a carbonaceous Themistian asteroid from the outer regions of the asteroid belt, approximately 11 km in diameter. It was discovered on 9 January 1999, by Croatian astronomer Korado Korlević at the Višnjan Observatory in Croatia. The C-type asteroid has a short rotation period... | [
"10241 Miličević — Naming\n\nThis minor planet was named after Don Nikola Miličević (1887-1963), Croatian amateur astronomer and last administrator of Blaca hermitage. The Hermitage is an UNESCO World Heritage Site located on the Brač island in Croatia. The official naming citation was published by the Minor Planet... |
10241_Miličević_27460636 | From the article on '10241 Miličević', restate the 'Diameter and albedo' content. | According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Miličević measures 10.882 kilometers in diameter and its surface has an albedo of 0.065, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculate... | [
"10241 Miličević — Naming\n\nThis minor planet was named after Don Nikola Miličević (1887-1963), Croatian amateur astronomer and last administrator of Blaca hermitage. The Hermitage is an UNESCO World Heritage Site located on the Brač island in Croatia. The official naming citation was published by the Minor Planet... |
10241_Miličević_27460633 | What information does the article about '10241 Miličević' provide on 'Orbit and classification'? | Miličević is a Themistian asteroid that belongs to the Themis family (602), a very large family of carbonaceous asteroids, named after 24 Themis. It orbits the Sun in the outer main-belt at a distance of 2.6–3.5 AU once every 5 years and 4 months (1,944 days; semi-major axis of 3.05 AU). Its orbit has an eccentricity o... | [
"10241 Miličević — Naming\n\nThis minor planet was named after Don Nikola Miličević (1887-1963), Croatian amateur astronomer and last administrator of Blaca hermitage. The Hermitage is an UNESCO World Heritage Site located on the Brač island in Croatia. The official naming citation was published by the Minor Planet... |
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