NIR Brightening of SBS1150+497

Details NIR Brightening of SBS1150+497 NIR Brightening of SBS1150+497

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3317....1c&link_type=abstract

The Astronomer's Telegram, #3317

Mathematics

Probability

Radio, Infra-Red, Optical, Gamma Ray, Tev, Request For Observations, Agn, Blazar, Quasar

Scientific paper

Following the report of the Fermi/Lat detection of a Gamma Ray flare (Hays and Donato, etal. Atel #3313) in the general direction of the quasar SBS1150+497 (z=0.334). The instrumental beam also included with smaller probability the quasar SBS1149+499 (z=1.093). We observed both objects in the NIR. We found that on JD 2455680.827569, SBS1150+497 had a flux H = 13.515 ± 0.09, 1.4 magnitudes brighter than the value reported in the 2mass survey.

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