X-ray detection of the supernova candidate MASTER OT 082752.77+704606.0
ATel #3367; K. V. Sokolovsky (MPIfR/ASC Lebedev/SAI MSU)
on 20 May 2011; 15:22 UT
Credential Certification: Frank Schinzel (schinzel@mpifr-bonn.mpg.de)
Subjects: Optical, Ultra-Violet, X-ray, Request for Observations, Supernovae, Transient
The optical transient MASTER OT 082752.77+704606.0 (ATel #3255, #3265) was
observed by Swift on 2011 May 14 for the total exposure time of 4ks.
A weak X-ray source has been detected by Swift/XRT at the position
08:27:53.31 +70:46:10.07 (+/-6.2", J2000) only 3.4" from the optical
transient (ATel #3265). The source is detected at the 3.5 sigma level
with the XRT count rate of 0.005 +/-0.001 counts/sec. Good positional
coincidence together with the absence of other detections of comparable
significance in the field (apart from the brighter source
GALEX 2682502750548263862 reported in ATel #3265) indicate that
the X-ray detection of MASTER OT 082752.77+704606.0 is real.
No X-ray source was seen at this position during the previous Swift/XRT
observations on 2011 April 06 (2.1ks) and 14 (0.6ks).
Simultaneous Swift/UVOT data show only marginal changes in
the ultraviolet brightness of the transient compared to previous
observations:
JD filter mag. err.
2455696.31 W2 18.26 0.05
2455696.31 M2 18.16 0.07
2455696.30 W1 18.06 0.06
2455696.30 U 18.41 0.08
2455696.30 B 19.58 0.14
2455696.31 V 19.40 0.16
2455665.82 W2 17.94 0.14
2455665.76 W1 18.11 0.13
2455665.89 U >19.0
2455665.82 B >19.0
2455657.57 W2 18.24 0.13 (ATel #3265)
The optical spectrum of the transient reported in ATel #3255, its
ultraviolet brightness and the initial lack of X-ray detection resemble
the
properties of ROTSE3 J115649.1+542726 = SN 2008es
(Miller et al. 2009, ApJ, 690, 1303; Gezari et al. 2009, ApJ, 690, 1313)
which was initially classified as an AGN flare (ATel #1515) or
possible tidal disruption event (ATel #1524), but has later developed
spectral features indicating that it was in fact an extremely luminous
Type II supernova at z=0.21 (ATel #1644).
The emission feature in the optical spectrum of MASTER OT 082752.77+704606.0
(ATel #3255) may be attributed to the HeII 4686 emission in analogy to
SN 2008es (Adam Miller, private communication). MASTER OT 082752.77+704606.0
is likely a luminous Type II supernova at z=0.135. New spectroscopic
observations which could trace the expected evolution of the optical
spectrum are necessary to confirm this interpretation.