NIR observations of S5 0716+71 from MIRO

Details NIR observations of S5 0716+71 from MIRO NIR observations of S5 0716+71 from MIRO

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3704....1c&link_type=abstract

The Astronomer's Telegram, #3704

Astronomy and Astrophysics

Astronomy

Infra-Red, Agn, Blazar

Scientific paper

Blazar S5 0716+714 (PKS 0716+71) is highly variable at short and long term timescales in all energy regimes. Recently (ATel # 3700), it is reported to be in flaring state in optical and gamma-rays by Blinov et al (2011). Source is shown to have brightened by one magnitude during three nights with R~ 12.5 on 2011.10.21UT23. Following ATel#3700, we observed S5 0716+71 in J and H near IR bands with NICS (1kx1k) mounted on the 1.2m telescope of MIRO (Mt Abu InfraRed Observatory) operated by the Physical Research Laboratory, Ahmedabad.

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