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marion.json

@@ -172,5 +172,11 @@
         "query":"Where are the peaks of the VHE blazars ?",
         "target_page":1,
         "target_passage":" VHE blazars have double-humped spectral energy  distributions (SEDs), with one peak at UV\/X-ray energies and another at GeV\/TeV energies."
+    },
+    {
+        "source_file":"1001.0770.pdf",
+        "query":"What are the blazars observed in the discovery program ?",
+        "target_page":2,
+        "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."
     }
 ]