KANATA confirmation of the optical flare of SDSS J123932.75+044305

Details KANATA confirmation of the optical flare of SDSS J123932.75+044305 KANATA confirmation of the optical flare of SDSS J123932.75+044305

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.1892....1i&link_type=abstract

The Astronomer's Telegram, #1892

Astronomy and Astrophysics

Astronomy

Optical, Agn, Quasars

Scientific paper

Following the Fermi/LAT detection of the gamma-ray flare from J123939+044409 (ATEL #1888), we performed optical photopolarimetric observations with the "KANATA" 1.5-m telescope at Higashi-Hiroshima Observatory. Our preliminary analysis shows that the V-band magnitude of SDSS J123932.75+044305 (a possible counterpart of the LAT source J123939+044409) was 15.7+/-0.1 and 16.1+/-0.1 on 2.8 and 3.8 (UT) Jan 2009, respectively.

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