In this task, you are given a set of context paragraph and some supporting facts to answer a question. Your task is to generate answer for given question based on set of context paragraphs and supporting facts.

[EX Q]: Context_1 : In astrophysics, an extreme mass ratio inspiral (EMRI) is the orbit of a relatively light object around a much heavier (by a factor 10,000 or more) object, that gradually decays due the emission of gravitational waves. Such systems are likely to be found in the centers of galaxies, where stellar mass compact objects, such as stellar black holes and neutron stars, may be found orbiting a supermassive black hole. In the case of a black hole in orbit around another black hole this is an extreme mass ratio binary black hole. The term EMRI is sometimes used as a shorthand to denote the emitted gravitational waveform as well as the orbit itself. Context_2 : The Penrose process (also called Penrose mechanism) is a process theorised by Roger Penrose wherein energy can be extracted from a rotating black hole. That extraction is made possible because the rotational energy of the black hole is located not inside the event horizon of the black hole, but on the outside of it in a region of the Kerr spacetime called the ergosphere, a region in which a particle is necessarily propelled in locomotive concurrence with the rotating spacetime. All objects in the ergosphere become dragged by a rotating spacetime. In the process, a lump of matter enters into the ergosphere of the black hole, and once it enters the ergosphere, it is forcibly split into two parts. For example, the matter might be made of two parts that separate by firing an explosive or rocket which pushes its halves apart. The momentum of the two pieces of matter when they separate can be arranged so that one piece escapes from the black hole (it "escapes to infinity"), whilst the other falls past the event horizon into the black hole. With careful arrangement, the escaping piece of matter can be made to have greater mass-energy than the original piece of matter, and the infalling piece has negative mass-energy. Although momentum is conserved the effect is that more energy can be extracted than was originally provided, the difference being provided by the black hole itself. In summary, the process results in a slight decrease in the angular momentum of the black hole, which corresponds to a transference of energy to the matter. The momentum lost is converted to energy extracted. Context_3 : The ergosphere is a region located outside a rotating black hole's outer event horizon. Its name was proposed by Remo Ruffini and John Archibald Wheeler during the Les Houches lectures in 1971 and is derived from the Greek word "ergon", which means "work". It received this name because it is theoretically possible to extract energy and mass from this region. The ergosphere touches the event horizon at the poles of a rotating black hole and extends to a greater radius at the equator. With a low spin of the central mass the shape of the ergosphere can be approximated by an oblated spheroid, while with higher spins it resembles a pumpkin-shape. The equatorial (maximum) radius of an ergosphere corresponds to the Schwarzschild radius of a non-rotating black hole; the polar (minimum) radius can be as little as half the Schwarzschild radius (the radius of a non-rotating black hole) in the case that the black hole is rotating maximally (at higher rotation rates the black hole could not have formed). Context_4 : In general relativity, the deSitterSchwarzschild solution describes a black hole in a causal patch of de Sitter space. Unlike a flat-space black hole, there is a largest possible de Sitter black hole, which is the Nariai spacetime. The Nariai limit has no singularities, the cosmological and black hole horizons have the same area, and they can be mapped to each other by a discrete reflection symmetry in any causal patch. Context_5 : In black hole theory, the black hole membrane paradigm is a simplified model, useful for visualising and calculating the effects predicted by quantum mechanics for the exterior physics of black holes, without using quantum-mechanical principles or calculations. It models a black hole as a thin, classically radiating surface (or membrane) at or vanishingly close to the black hole's event horizon. This approach to the theory of black holes was created by Kip S. Thorne, R. H. Price and D. A. Macdonald. Context_6 : "The Wonderful Thing About Tiggers" is the theme song and personal anthem of Tigger, a fictional tiger from the children's book series Winnie-the-Pooh. Although Tigger's birthday is believed to be in October 1928, the year that "The House at Pooh Corner" was first published, on Tigger-related merchandise, Disney often indicates Tigger's birth year as 1968, a reference to the first year that Tigger appeared in a Disney production, "Winnie the Pooh and the Blustery Day". That was also the same instance when Tigger first sang this song. The song is repeated in Disney's 1974 release "Winnie the Pooh and Tigger Too!", The Many Adventures of Winnie the Pooh ride and then again in the 1977 release "The Many Adventures of Winnie the Pooh". "The Wonderful Thing About Tiggers" opens up the 2000 release of "The Tigger Movie". In 1974, Paul Winchell earned a Grammy for his rendition of the song. Context_7 : The Black Hole is a 1979 American science fiction film directed by Gary Nelson and produced by Walt Disney Productions. The film stars Maximilian Schell, Robert Forster, Joseph Bottoms, Yvette Mimieux, Anthony Perkins, and Ernest Borgnine, while the voices of the main robot characters are provided by Roddy McDowall and Slim Pickens (both unbilled). The music for the film was composed by John Barry. It was the first film from Walt Disney Productions to receive a PG rating. The film was released on December 18, 1979 in the United Kingdom and on December 21, 1979 in the United States. Context_8 : M33 X-7 is a black hole binary system in the galaxy M33. The system is made up of a stellar mass black hole and a companion star. M33 X-7 is the largest known stellar black hole with an estimated mass of 15.65 times that of the Sun (M ). The total mass of the system is estimated to be around 85.7M , which would make it the most massive black hole binary system. Context_9 : The Tigger Movie is a 2000 American animated musical comedy-drama film written and directed by Jun Falkenstein from a story by Eddie Guzelian. Part of the "Winnie-the-Pooh" series, this film features Pooh's friend Tigger searching for his family tree and other Tiggers like himself. Context_10 : V404 Cygni is a microquasar and a binary system consisting of a black hole with a mass of about and an early K companion star of mass slightly smaller than the Sun in the constellation of Cygnus. The star and the black hole orbit each other every at fairly close range. Due to their proximity and the intense gravity of the black hole, the companion star loses mass to an accretion disk around the black hole and ultimately to the black hole itself. fact_1 : The Black Hole is a 1979 American science fiction film directed by Gary Nelson and produced by Walt Disney Productions. fact_2 : The Tigger Movie is a 2000 American animated musical comedy-drama film written and directed by Jun Falkenstein from a story by Eddie Guzelian. Question: The Black Hole and The Tigger Movie are both what type of media?
[EX A]: film

[EX Q]: Context_1 : Ginza ( ) is a district of Chuo, Tokyo, located south of Yaesu and Kyobashi, west of Tsukiji, east of Yurakucho and Uchisaiwaicho, and north of Shinbashi. Context_2 : Nihonbashi ( , "Japan Bridge") is a business district of Chuo, Tokyo, Japan which grew up around the bridge of the same name which has linked two sides of the Nihonbashi River at this site since the 17th century. The first wooden bridge was completed in 1603. The current bridge designed by Tsumaki Yorinaka was constructed of stone on a steel frame dates from 1911. The district covers a large area to the north and east of the bridge, reaching Akihabara to the north and the Sumida River to the east. Otemachi is to the west and Yaesu and Ginza to the south. Context_3 : Toshima ( , Toshima-ku ) is a special ward in Tokyo, Japan. It is one of the eight central wards of the Tokyo Metropolitan area, including Chiyoda, Minato, Shibuya, Chuo, Shinjuku, Taito, and Bunkyo surrounding the Imperial Palace. Located in the northern area of Tokyo, Toshima is bordered by the wards of Nerima, Itabashi, and Kita wards, in the north, and Nakano, Shinjuku and Bunkyo in the south. Context_4 : The Imperial Hotel ( , teikoku hoteru ) is a hotel in Tokyo that was created in the late 1880s at the request of the Japanese aristocracy to cater to the increasing number of Western visitors to Japan. The hotel site is located just south of the Imperial Palace grounds, next to the previous location of the Palace moat. The modern hotel overlooks the Palace, the 40 acre Western-style Hibiya Park, and the Ginza neighborhood. Context_5 : Hibiya ( ) is a geographic name covering a part of Chiyoda Ward in Tokyo. The area along Hibiya Street (National Route 1) from Yurakucho to Uchisaiwaicho is Hibiya district. Hibiya is used in some local place names such as Hibiya Park and Hibiya Station. Hibiya was a ward named Kojimachi before Tokyo City was restructured. The outskirts of this district are reclaimed from the ocean, so the name of "hibi" of Hibiya is derived from the facility for the laver of nori made of bamboo whose name is also "hibi". Context_6 : 61st was a station on the Chicago Transit Authority's Green Line. The station was located at 316 E. 61st Street in the Washington Park neighborhood of Chicago. 61st was located south of 58th, which opened and closed at the same time as 61st, and north of King Drive. 61st opened on January 22, 1893; The station closed on January 9, 1994, when the entire Green Line closed for a renovation and rehabilitation project, and did not reopen with the rest of the Green Line on May 12, 1996, due to service cuts, The station was later demolished and was located south from the 61st Yard. Context_7 : Yurakucho ( ) is a district of Chiyoda, Tokyo, Japan, situated in between the Ginza and Hibiya Park, near the district of Shinbashi. Unlike its tonier neighbor Ginza, Yurakucho provides a glimpse of Japanese life from the early postwar period, with its many "izakaya" (Japanese-style bars, denoted by their red lanterns known as "akachochin") and outdoor "yakitori" restaurants, many of which are located under the train tracks serving Tokyo's JR Yamanote Line. Because of its many traditional Japanese-style eating establishments, as well as its location on the Yamanote Line with easy access to Tokyo Station, Yurakucho is a favorite drinking spot for businessmen on their way home from work. Context_8 : Hibiya Park ( , Hibiya Koen ) is a park in Chiyoda City, Tokyo, Japan. It covers an area of 161,636.66m between the east gardens of the Imperial Palace to the north, the Shinbashi district to the southeast and the Kasumigaseki government district to the west. Context_9 : Wakasu ( ) also "Wakasu Island", is an island located in Koto, Tokyo. It is located south of Shin-Kiba and is connected to a new unnamed island to the south by the Tokyo Gate Bridge. Context_10 : Imperial Hotel, Ltd. (; "Kabushiki Gaisha Teikoku Hoteru") is a company that operates hotels in Japan. Its flagship hotel is the Imperial Hotel, Tokyo (), and its headquarters are located in the Chiyoda Ward of Tokyo, near the Imperial Palace, Hibiya Park, and Ginza. fact_1 : Yurakucho ( ) is a district of Chiyoda, Tokyo, Japan, situated in between the Ginza and Hibiya Park, near the district of Shinbashi. fact_2 : Ginza ( ) is a district of Chuo, Tokyo, located south of Yaesu and Kyobashi, west of Tsukiji, east of Yurakucho and Uchisaiwaicho, and north of Shinbashi. Question: Yurakucho is situated in between Hibiya Park, and what district of Chuo, Tokyo, that is located south of Yaesu and Kyobashi?
[EX A]: Ginza

[EX Q]: Context_1 : Admiral of the Fleet Sir Michael Patrick Pollock, {'1': ", '2': ", '3': ", '4': "} (19 October 1916 27 September 2006) was a senior officer in the Royal Navy who rose to become First Sea Lord and Chief of the Naval Staff in the early 1970s. In the Second World War, he was an officer on ships tasked with protecting convoys in the Atlantic and the Mediterranean, and was gunnery officer on the cruiser HMS "Norfolk" when she fought the German battleship "Scharnhorst" during the Battle of North Cape. He later commanded the aircraft carrier HMS "Ark Royal" , and hosted Ian Smith on HMS "Tiger" . In retirement, he held the position of King of Arms of the Order of the Bath and Gloucester King of Arms, with responsibility for heraldry in Wales. Context_2 : SMS "Oldenburg" was an armored warship of the German Imperial Navy. Laid down at the AG Vulcan shipyard in Stettin in 1883, the ship was launched in December 1884 and commissioned into the Navy in April 1886. "Oldenburg" was intended to have been a fifth member of the "Sachsen"class of sortie corvettes, but budgetary limitations and dissatisfaction with the "Sachsen" class prompted a redesign that bore little resemblance to the earlier vessels. "Oldenburg" mounted her main battery of eight 24 cm guns amidships, six in a central casemate on the main deck and two directly above them on the broadside. She was the first German capital ship constructed entirely from German-made steel. Context_3 : Admiral of the Fleet Sir Varyl Cargill Begg {'1': ", '2': ", '3': ", '4': "} (1 October 1908 13 July 1995) was a Royal Navy officer. He fought in the Second World War as gunnery officer in a cruiser taking part in the North Atlantic convoys, the Norwegian campaign and the occupation of Iceland and then as gunnery officer in a battleship operating in the Mediterranean Fleet during the Battle of Cape Matapan. After that he commanded a destroyer during the Korean War and was Commander-in-Chief of Far East Command during the IndonesiaMalaysia confrontation. He was First Sea Lord and Chief of the Naval Staff in the late 1960s. In that role he vehemently opposed plans to introduce large new aircraft carriers and instead managed to persuade the British Government to develop the design for three small "through-deck cruisers". Context_4 : HMS "Resistance" was the second of two "Defence"-class ironclad s built for the Royal Navy in the 1860s. She was the first capital ship in the Royal Navy to be fitted with a ram and was given the nickname of "Old Rammo". "Resistance" was initially assigned to the Channel Fleet upon commissioning, but was transferred to the Mediterranean Fleet in 1864, the first ironclad to be assigned to that fleet. She was rearmed in 1867 and became a guardship when recommissioned in 1869. The ship was reassigned to the Channel Fleet in 1873 before reverting to her former duties in 1877. "Resistance" was decommissioned in 1880 and was used for gunnery and torpedo trials beginning in 1885. The ship was sold for scrap in 1898 and foundered in 1899 en route to the breaker's yard. She was salvaged and later scrapped. Context_5 : The YMS-418 was a YMS-1 class minesweeper which saw service in World War II. The hull was laid down 16 September 1943 by Henry C. Grebe and Co., Chicago, IL. It was launched 22 February 1944 It was struck from the Navy Register 7 February 1947 and sold 17 December 1947. According to deck logs stored at the National Archives in College Park Maryland, the ship's commanding officer was Lt. Victor A. Lang, executive officer Ensign Toivo John Hamalainen, gunnery officer Ensign J. J. Dennehy, Jr., engineering officer Ensign Bruce F. Kingsbury. Its fate is unknown. Context_6 : Admiral of the Fleet Sir Arthur John Power (12 April 1889 28 January 1960) was a Royal Navy officer. He took part in the First World War as a gunnery officer and saw action in the Dardanelles Campaign. During the inter-war years he commanded the gunnery school at HMS"Excellent" and then the aircraft carrier HMS"Ark Royal" . During the Second World War he played a leading role in the planning for the Allied invasion of Sicily and for the Allied invasion of Italy and then commanded the naval forces for the actual landing of V Corps at Taranto in Italy in September 1943. He went on to be Commander-in-Chief of the East Indies Fleet in the closing stages of the war and conducted naval strikes on the Imperial Japanese Army in Borneo and Malaya. After the War he became Second Sea Lord and Chief of Naval Personnel, Commander-in-Chief, Mediterranean Fleet and then Commander-in-Chief, Portsmouth. Context_7 : Admiral of the Fleet Peter John Hill-Norton, Baron Hill-Norton, {'1': ", '2': ", '3': ", '4': "} (8 February 1915 16 May 2004) was a senior Royal Navy officer. He fought in the Second World War as gunnery officer in a cruiser operating on the Western Approaches and in the North Sea taking part in the Norwegian Campaign, then in a cruiser taking part in the Arctic convoys and finally in a battleship operating in the Eastern Fleet. After the War he commanded a destroyer and then an aircraft carrier. He served as First Sea Lord and Chief of the Naval Staff and then Chief of the Defence Staff in early 1970s. In the latter role he gave the final commitment to Project Chevaline, the Polaris missile improvement programme. He went on to be Chairman of the NATO Military Committee. Context_8 : Scharnhorst was a German capital ship, alternatively described as a battleship and battlecruiser, of Nazi Germany's "Kriegsmarine". She was the lead ship of her class, which included one other ship, "Gneisenau" . The ship was built at the "Kriegsmarinewerft" dockyard in Wilhelmshaven; she was laid down on 15 June 1935 and launched a year and four months later on 3 October 1936. Completed in January 1939, the ship was armed with a main battery of nine 28 cm (11 in) C/34 guns in three triple turrets. Plans to replace these weapons with six 38 cm (15 in) SK C/34 guns in twin turrets were never carried out. Context_9 : Gneisenau was a German capital ship, alternatively described as a battleship and battlecruiser, of Nazi Germany's "Kriegsmarine". She was the second vessel of her class, which included one other ship, "Scharnhorst" . The ship was built at the "Deutsche Werke" dockyard in Kiel; she was laid down on 6 May 1935 and launched on 8 December 1936. Completed in May 1938, the ship was armed with a main battery of nine 28cm (11in) C/34 guns in three triple turrets, though there were plans to replace these weapons with six 38cm (15in) SK C/34 guns in twin turrets. Context_10 : Admiral of the Fleet Sir Michael Le Fanu (2 August 1913 28 November 1970) was a Royal Navy officer. He fought in the Second World War as gunnery officer in a cruiser operating in the Home Fleet during the Norwegian Campaign and the Battle of the Mediterranean and then as gunnery officer in a battleship operating in the Eastern Fleet before becoming liaison officer between the British Pacific Fleet and the United States Third Fleet. After the War he commanded a frigate, a training establishment and an aircraft carrier. He served as First Sea Lord and Chief of the Naval Staff in the late 1960s. In that role, in the face of economic difficulties, he worked hard to reshape the Navy as an anti-submarine force operating primarily in the Atlantic Ocean. fact_1 : In the Second World War, he was an officer on ships tasked with protecting convoys in the Atlantic and the Mediterranean, and was gunnery officer on the cruiser HMS "Norfolk" when she fought the German battleship "Scharnhorst" during the Battle of North Cape. fact_2 : Scharnhorst was a German capital ship, alternatively described as a battleship and battlecruiser, of Nazi Germany's "Kriegsmarine". Question: Michael Pollock was a gunnery officer on the Norfolk when it fought which German capital ship?
[EX A]:
Scharnhorst