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marion.json
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@@ -178,5 +178,11 @@
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"query":"What are the blazars observed in the discovery program ?",
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"target_page":2,
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"target_passage":"The blazars observed in the discovery program are largely high-frequency-peaked BL Lac objects. How ever, the program also includes IBLs (intermediate peaked) and LBLs (low-peaked), as well as flat spec trum radio quasars (FSRQs), in an attempt to in crease the types of blazars known to emit VHE γ-rays."
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}
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]
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"query":"What are the blazars observed in the discovery program ?",
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"target_page":2,
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"target_passage":"The blazars observed in the discovery program are largely high-frequency-peaked BL Lac objects. How ever, the program also includes IBLs (intermediate peaked) and LBLs (low-peaked), as well as flat spec trum radio quasars (FSRQs), in an attempt to in crease the types of blazars known to emit VHE γ-rays."
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},
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{
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"source_file":"1001.0770.pdf",
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"query":"How many VHE blazar candidates were observed by VERITAS between September 2007 andJune 2009 ?",
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"target_page":3,
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"target_passage":"More than 50 VHE blazar candidates were observed by VERITAS betweenSeptember 2007 andJune 2009."
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}
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]
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