XMM-Newton observation of V5116 Sgr

Details XMM-Newton observation of V5116 Sgr XMM-Newton observation of V5116 Sgr

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1184....1s&link_type=abstract

The Astronomer's Telegram, #1184

Astronomy and Astrophysics

Astronomy

4

X-Ray, Cataclysmic Variables, Novae

Scientific paper

V5116 Sgr (=Nova Sgr 2005b), recently detected as a super-soft source with Swift (Ness et al. CBET #1030), was observed on 5 March 2007 by XMM-Newton, with a total exposure of 13 ks in the EPIC-MOS cameras and 9 ks in the EPIC-pn. The source count-rates in the EPIC cameras were 2-4 cts/s (MOS1 and MOS2) and 10-15 cts/s (pn) during most of the observation, increasing to 11-15 cts/s (MOS1 and MOS2) and 50-60 cts/s (pn) during 3.5 ks.

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