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data/retrieval_individual-f62bcad9-19c4-430b-a7ba-aa2bfeba99dc.jsonl CHANGED
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  {"tstamp": 1722435270.6035, "task_type": "retrieval", "type": "chat", "model": "text-embedding-3-large", "gen_params": {}, "start": 1722435269.4399, "finish": 1722435270.6035, "ip": "", "conv_id": "8d888791d2974cfa870d136ae7fc249a", "model_name": "text-embedding-3-large", "prompt": "What is the speed of light?", "output": [["What is the speed of light?", "Speed of light\n\nThe speed of light in vacuum, commonly denoted , is a universal physical constant that is exactly equal to ). According to the special theory of relativity, is the upper limit for the speed at which conventional matter or energy (and thus any signal carrying information) can travel through space.\nAll forms of electromagnetic radiation, including visible light, travel at the speed of light. For many practical purposes, light and other electromagnetic waves will appear to propagate instantaneously, but for long distances and very sensitive measurements, their finite speed has noticeable effects. Any starlight viewed on Earth is from the distant past, allowing humans to study the history of the universe by viewing distant objects. When communicating with distant space probes, it can take minutes to hours for signals to travel. In computing, the speed of light fixes the ultimate minimum communication delay. The speed of light can be used in time of flight measurements to measure large distances to extremely high precision."]], "corpus": "wikipedia"}
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  {"tstamp": 1722435292.9616, "task_type": "retrieval", "type": "chat", "model": "jinaai/jina-embeddings-v2-base-en", "gen_params": {}, "start": 1722435292.4862, "finish": 1722435292.9616, "ip": "", "conv_id": "bc280a403a1f4f21aa4d6dd923fdaede", "model_name": "jinaai/jina-embeddings-v2-base-en", "prompt": "What is the speed of light?", "output": [["What is the speed of light?", "Speed of light\n\nBecause of this experiment Hendrik Lorentz proposed that the motion of the apparatus through the aether may cause the apparatus to contract along its length in the direction of motion, and he further assumed that the time variable for moving systems must also be changed accordingly (\"local time\"), which led to the formulation of the Lorentz transformation. Based on Lorentz's aether theory, Henri Poincaré (1900) showed that this local time (to first order in v/c) is indicated by clocks moving in the aether, which are synchronized under the assumption of constant light speed. In 1904, he speculated that the speed of light could be a limiting velocity in dynamics, provided that the assumptions of Lorentz's theory are all confirmed. In 1905, Poincaré brought Lorentz's aether theory into full observational agreement with the principle of relativity.\nSpecial relativity\nIn 1905 Einstein postulated from the outset that the speed of light in vacuum, measured by a non-accelerating observer, is independent of the motion of the source or observer. Using this and the principle of relativity as a basis he derived the special theory of relativity, in which the speed of light in vacuum c featured as a fundamental constant, also appearing in contexts unrelated to light. This made the concept of the stationary aether (to which Lorentz and Poincaré still adhered) useless and revolutionized the concepts of space and time.\nIncreased accuracy of c and redefinition of the metre and second"]], "corpus": "wikipedia"}
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  {"tstamp": 1722435292.9616, "task_type": "retrieval", "type": "chat", "model": "voyage-multilingual-2", "gen_params": {}, "start": 1722435292.4862, "finish": 1722435292.9616, "ip": "", "conv_id": "b1cfd58aed294f2882e246c2bc48e6c8", "model_name": "voyage-multilingual-2", "prompt": "What is the speed of light?", "output": [["What is the speed of light?", "Speed of light\n\nThe speed of light in vacuum, commonly denoted , is a universal physical constant that is exactly equal to ). According to the special theory of relativity, is the upper limit for the speed at which conventional matter or energy (and thus any signal carrying information) can travel through space.\nAll forms of electromagnetic radiation, including visible light, travel at the speed of light. For many practical purposes, light and other electromagnetic waves will appear to propagate instantaneously, but for long distances and very sensitive measurements, their finite speed has noticeable effects. Any starlight viewed on Earth is from the distant past, allowing humans to study the history of the universe by viewing distant objects. When communicating with distant space probes, it can take minutes to hours for signals to travel. In computing, the speed of light fixes the ultimate minimum communication delay. The speed of light can be used in time of flight measurements to measure large distances to extremely high precision."]], "corpus": "wikipedia"}
 
 
 
 
 
 
 
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  {"tstamp": 1722435270.6035, "task_type": "retrieval", "type": "chat", "model": "text-embedding-3-large", "gen_params": {}, "start": 1722435269.4399, "finish": 1722435270.6035, "ip": "", "conv_id": "8d888791d2974cfa870d136ae7fc249a", "model_name": "text-embedding-3-large", "prompt": "What is the speed of light?", "output": [["What is the speed of light?", "Speed of light\n\nThe speed of light in vacuum, commonly denoted , is a universal physical constant that is exactly equal to ). According to the special theory of relativity, is the upper limit for the speed at which conventional matter or energy (and thus any signal carrying information) can travel through space.\nAll forms of electromagnetic radiation, including visible light, travel at the speed of light. For many practical purposes, light and other electromagnetic waves will appear to propagate instantaneously, but for long distances and very sensitive measurements, their finite speed has noticeable effects. Any starlight viewed on Earth is from the distant past, allowing humans to study the history of the universe by viewing distant objects. When communicating with distant space probes, it can take minutes to hours for signals to travel. In computing, the speed of light fixes the ultimate minimum communication delay. The speed of light can be used in time of flight measurements to measure large distances to extremely high precision."]], "corpus": "wikipedia"}
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  {"tstamp": 1722435292.9616, "task_type": "retrieval", "type": "chat", "model": "jinaai/jina-embeddings-v2-base-en", "gen_params": {}, "start": 1722435292.4862, "finish": 1722435292.9616, "ip": "", "conv_id": "bc280a403a1f4f21aa4d6dd923fdaede", "model_name": "jinaai/jina-embeddings-v2-base-en", "prompt": "What is the speed of light?", "output": [["What is the speed of light?", "Speed of light\n\nBecause of this experiment Hendrik Lorentz proposed that the motion of the apparatus through the aether may cause the apparatus to contract along its length in the direction of motion, and he further assumed that the time variable for moving systems must also be changed accordingly (\"local time\"), which led to the formulation of the Lorentz transformation. Based on Lorentz's aether theory, Henri Poincaré (1900) showed that this local time (to first order in v/c) is indicated by clocks moving in the aether, which are synchronized under the assumption of constant light speed. In 1904, he speculated that the speed of light could be a limiting velocity in dynamics, provided that the assumptions of Lorentz's theory are all confirmed. In 1905, Poincaré brought Lorentz's aether theory into full observational agreement with the principle of relativity.\nSpecial relativity\nIn 1905 Einstein postulated from the outset that the speed of light in vacuum, measured by a non-accelerating observer, is independent of the motion of the source or observer. Using this and the principle of relativity as a basis he derived the special theory of relativity, in which the speed of light in vacuum c featured as a fundamental constant, also appearing in contexts unrelated to light. This made the concept of the stationary aether (to which Lorentz and Poincaré still adhered) useless and revolutionized the concepts of space and time.\nIncreased accuracy of c and redefinition of the metre and second"]], "corpus": "wikipedia"}
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  {"tstamp": 1722435292.9616, "task_type": "retrieval", "type": "chat", "model": "voyage-multilingual-2", "gen_params": {}, "start": 1722435292.4862, "finish": 1722435292.9616, "ip": "", "conv_id": "b1cfd58aed294f2882e246c2bc48e6c8", "model_name": "voyage-multilingual-2", "prompt": "What is the speed of light?", "output": [["What is the speed of light?", "Speed of light\n\nThe speed of light in vacuum, commonly denoted , is a universal physical constant that is exactly equal to ). According to the special theory of relativity, is the upper limit for the speed at which conventional matter or energy (and thus any signal carrying information) can travel through space.\nAll forms of electromagnetic radiation, including visible light, travel at the speed of light. For many practical purposes, light and other electromagnetic waves will appear to propagate instantaneously, but for long distances and very sensitive measurements, their finite speed has noticeable effects. Any starlight viewed on Earth is from the distant past, allowing humans to study the history of the universe by viewing distant objects. When communicating with distant space probes, it can take minutes to hours for signals to travel. In computing, the speed of light fixes the ultimate minimum communication delay. The speed of light can be used in time of flight measurements to measure large distances to extremely high precision."]], "corpus": "wikipedia"}
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+ {"tstamp": 1722435310.9782, "task_type": "retrieval", "type": "chat", "model": "jinaai/jina-embeddings-v2-base-en", "gen_params": {}, "start": 1722435310.8086, "finish": 1722435310.9782, "ip": "", "conv_id": "babf562a686149cea3962c0693cb5669", "model_name": "jinaai/jina-embeddings-v2-base-en", "prompt": "What is the main ingredient in sushi?", "output": [["What is the main ingredient in sushi?", "The Main Ingredient\n\nThe Main Ingredient was an American soul and R&B group which had a run of hits in the 1970s, including their 1972 million-selling song \"Everybody Plays the Fool\"."]], "corpus": "wikipedia"}
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+ {"tstamp": 1722435310.9782, "task_type": "retrieval", "type": "chat", "model": "BAAI/bge-large-en-v1.5", "gen_params": {}, "start": 1722435310.8086, "finish": 1722435310.9782, "ip": "", "conv_id": "135ce3388f7a4e75be4c5139e102d9c8", "model_name": "BAAI/bge-large-en-v1.5", "prompt": "What is the main ingredient in sushi?", "output": [["What is the main ingredient in sushi?", "Sushi\n\nThe ingredients used inside sushi are called and are, typically, varieties of fish. For culinary, sanitary, and aesthetic reasons, the minimum quality and freshness of fish to be eaten raw must be superior to that of fish that is to be cooked. Sushi chefs are trained to recognize important attributes, including smell, color, firmness, and freedom from parasites that may go undetected in a commercial inspection. Commonly used fish are tuna (), Japanese amberjack, yellowtail (), snapper (), mackerel (), and salmon (). The most valued sushi ingredient is , the fatty cut of the fish. This comes in a variety of (often from the bluefin species of tuna) and , meaning \"middle toro\", implying that it is halfway into the fattiness between and the regular cut. style refers to nigiri sushi, where the fish is partially grilled (topside) and partially raw. Most nigiri sushi will have completely raw toppings, called .\nOther seafoods such as squid (), eel ( and ), pike conger (), octopus (), shrimp ( and ), clam (, and ), fish roe (, , and ), sea urchin (), crab (), and various kinds of shellfish (abalone, prawn, scallop) are the most popular seafoods in sushi. Oysters are less common, as the taste is thought to not go well with the rice. , or imitation crab stick, is commonly substituted for real crab, most notably in California rolls.\nPickled daikon radish () in , pickled vegetables (), fermented soybeans () in , avocado, cucumber in , asparagus, yam, pickled (), gourd (), burdock (), and sweet corn (sometimes mixed with mayonnaise) are plant products used in sushi.\nTofu, eggs (in the form of slightly sweet, layered omelette called ), and raw quail eggs (as a topping) are also common."]], "corpus": "wikipedia"}
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+ {"tstamp": 1722435342.8347, "task_type": "retrieval", "type": "chat", "model": "jinaai/jina-embeddings-v2-base-en", "gen_params": {}, "start": 1722435342.71, "finish": 1722435342.8347, "ip": "", "conv_id": "6d12ed28ca1249f994a0ef06a4f67a46", "model_name": "jinaai/jina-embeddings-v2-base-en", "prompt": "What is the boiling point of water in Celsius?", "output": [["What is the boiling point of water in Celsius?", "Boiling point\n\nIn general, compounds with ionic bonds have high normal boiling points, if they do not decompose before reaching such high temperatures. Many metals have high boiling points, but not all. Very generally—with other factors being equal—in compounds with covalently bonded molecules, as the size of the molecule (or molecular mass) increases, the normal boiling point increases. When the molecular size becomes that of a macromolecule, polymer, or otherwise very large, the compound often decomposes at high temperature before the boiling point is reached. Another factor that affects the normal boiling point of a compound is the polarity of its molecules. As the polarity of a compound's molecules increases, its normal boiling point increases, other factors being equal. Closely related is the ability of a molecule to form hydrogen bonds (in the liquid state), which makes it harder for molecules to leave the liquid state and thus increases the normal boiling point of the compound. Simple carboxylic acids dimerize by forming hydrogen bonds between molecules. A minor factor affecting boiling points is the shape of a molecule. Making the shape of a molecule more compact tends to lower the normal boiling point slightly compared to an equivalent molecule with more surface area.\nMost volatile compounds (anywhere near ambient temperatures) go through an intermediate liquid phase while warming up from a solid phase to eventually transform to a vapor phase. By comparison to boiling, a sublimation is a physical transformation in which a solid turns directly into vapor, which happens in a few select cases such as with carbon dioxide at atmospheric pressure. For such compounds, a sublimation point is a temperature at which a solid turning directly into vapor has a vapor pressure equal to the external pressure."]], "corpus": "wikipedia"}
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+ {"tstamp": 1722435342.8347, "task_type": "retrieval", "type": "chat", "model": "BAAI/bge-large-en-v1.5", "gen_params": {}, "start": 1722435342.71, "finish": 1722435342.8347, "ip": "", "conv_id": "af2f8752a33e4ce5aab95975ad9e84fb", "model_name": "BAAI/bge-large-en-v1.5", "prompt": "What is the boiling point of water in Celsius?", "output": [["What is the boiling point of water in Celsius?", "Fahrenheit\n\nThough the United Kingdom changed from Fahrenheit to Celsius in metrology, Fahrenheit is sometimes still used in newspaper headlines to sensationalise heatwaves.\nDefinition and conversion\nHistorically, on the Fahrenheit scale the freezing point of water was 32 °F, and the boiling point was 212 °F (at standard atmospheric pressure). This put the boiling and freezing points of water 180 degrees apart. Therefore, a degree on the Fahrenheit scale was of the interval between the freezing point and the boiling point. On the Celsius scale, the freezing and boiling points of water were originally defined to be 100 degrees apart. A temperature interval of 1 °F was equal to an interval of  degrees Celsius. With the Fahrenheit and Celsius scales now both defined by the kelvin, this relationship was preserved, a temperature interval of 1 °F being equal to an interval of  K and of  °C. The Fahrenheit and Celsius scales intersect numerically at −40 in the respective unit (i.e, −40 °F ≘ −40 °C).\nAbsolute zero is 0 K, −273.15 °C, or −459.67 °F. The Rankine temperature scale uses degree intervals of the same size as those of the Fahrenheit scale, except that absolute zero is 0 °R the same way that the Kelvin temperature scale matches the Celsius scale, except that absolute zero is 0 K."]], "corpus": "wikipedia"}
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+ {"tstamp": 1722435382.2086, "task_type": "retrieval", "type": "chat", "model": "jinaai/jina-embeddings-v2-base-en", "gen_params": {}, "start": 1722435382.0223, "finish": 1722435382.2086, "ip": "", "conv_id": "891f518100f244f88c090ec059a543dc", "model_name": "jinaai/jina-embeddings-v2-base-en", "prompt": "Who developed the theory of relativity?", "output": [["Who developed the theory of relativity?", "Theory of relativity\n\nThe Michelson–Morley experiment was designed to detect second-order effects of the \"aether wind\"—the motion of the aether relative to the Earth. Michelson designed an instrument called the Michelson interferometer to accomplish this. The apparatus was sufficiently accurate to detect the expected effects, but he obtained a null result when the first experiment was conducted in 1881, and again in 1887. Although the failure to detect an aether wind was a disappointment, the results were accepted by the scientific community. In an attempt to salvage the aether paradigm, FitzGerald and Lorentz independently created an ad hoc hypothesis in which the length of material bodies changes according to their motion through the aether. This was the origin of FitzGerald–Lorentz contraction, and their hypothesis had no theoretical basis. The interpretation of the null result of the Michelson–Morley experiment is that the round-trip travel time for light is isotropic (independent of direction), but the result alone is not enough to discount the theory of the aether or validate the predictions of special relativity.\nWhile the Michelson–Morley experiment showed that the velocity of light is isotropic, it said nothing about how the magnitude of the velocity changed (if at all) in different inertial frames. The Kennedy–Thorndike experiment was designed to do that, and was first performed in 1932 by Roy Kennedy and Edward Thorndike. They obtained a null result, and concluded that \"there is no effect ... unless the velocity of the solar system in space is no more than about half that of the earth in its orbit\". That possibility was thought to be too coincidental to provide an acceptable explanation, so from the null result of their experiment it was concluded that the round-trip time for light is the same in all inertial reference frames."]], "corpus": "wikipedia"}
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+ {"tstamp": 1722435382.2086, "task_type": "retrieval", "type": "chat", "model": "BAAI/bge-large-en-v1.5", "gen_params": {}, "start": 1722435382.0223, "finish": 1722435382.2086, "ip": "", "conv_id": "afaede0c88b04fce85064bfd7039c2ab", "model_name": "BAAI/bge-large-en-v1.5", "prompt": "Who developed the theory of relativity?", "output": [["Who developed the theory of relativity?", "Theory of relativity\n\nThe theory transformed theoretical physics and astronomy during the 20th century, superseding a 200-year-old theory of mechanics created primarily by Isaac Newton. It introduced concepts including 4-dimensional spacetime as a unified entity of space and time, relativity of simultaneity, kinematic and gravitational time dilation, and length contraction. In the field of physics, relativity improved the science of elementary particles and their fundamental interactions, along with ushering in the nuclear age. With relativity, cosmology and astrophysics predicted extraordinary astronomical phenomena such as neutron stars, black holes, and gravitational waves.\nDevelopment and acceptance\nAlbert Einstein published the theory of special relativity in 1905, building on many theoretical results and empirical findings obtained by Albert A. Michelson, Hendrik Lorentz, Henri Poincaré and others. Max Planck, Hermann Minkowski and others did subsequent work.\nEinstein developed general relativity between 1907 and 1915, with contributions by many others after 1915. The final form of general relativity was published in 1916.\nThe term \"theory of relativity\" was based on the expression \"relative theory\" () used in 1906 by Planck, who emphasized how the theory uses the principle of relativity. In the discussion section of the same paper, Alfred Bucherer used for the first time the expression \"theory of relativity\" ()."]], "corpus": "wikipedia"}