[vsnet-alert 17084] OT J060009.9+142615 : rapid fading
Ohshima
ohshima at kusastro.kyoto-u.ac.jp
Wed Mar 26 06:36:04 JST 2014
VSNET campaign target list (2014 Mar 25)
*** VSNET campaign selected current target list 2014 Mar 25 ***
Object Class Position Type State Mag Data Remark
Added Date
============================================================================
PTF1 J071912.13+485834.0 NLAC+UGSU SU UMa with HeWD? 16.1 1
probable superoutburst
2QZ J130441.7+010330 UGSU? SU UMa 16.0 1
candidate
SDSS J090221.35+381941.9 NLAC+UGSU SU UMa with HeWD 14.2 1
stage A superhumps
OT J060009.9+142615 UG? unusual SU UMa 14.0 1
stage C superhump, fading?
ASASSN-14ag 08:13:18.5 UGSU+E SU UMa 15.2 1
-01:03:27.7 superhumps and eclipses
V4641 Sgr 18:19:21.5 XN outburst 12.6(I) 1
-25:24:25
======================================================================
other dwarf novae in superoutburst
======================================================================
other objects of current interest
V1323 Her (VY Scl?, deep fading),
CSS J220031.2+033429 (Z Cam candidate)
AG Peg (bright ZAND. active state),
HS2133+0513(VY Scl? fading)
V3804 Sgr (Z And type outburst),
HS0220+0603 (VY Scl type, recovering from a deep fading),
MASTER OT J015016.17+375620.5 (unusual dwarf nova?)
======================================================================
Remarks:
* Class: 1 = primary target for time-resolved photometry
2 = secondary target for time-resolved photometry
3 = optional target. Daily monitoring is enough in
most cases.
* Data: data request, 1 = VSNET core team, data will be received by
campaign report list
(vsnet-campaign-report at ooruri.kusastro.kyoto-u.ac.jp).
Please closely watch vsnet-alert and vsnet-outburst for other new
outbursts.
*** Notice ***
This list is "read-only", i.e. it is used only for announcement
of the target lists. Other information, as well as reports and
discussions on particular targets, should be directed to the
appropriate VSNET campaign sub-lists (e.g. vsnet-campaign-dn for
dwarf novae).
Nightly time-series observations should be now directed to
(cc: to Ohshima-san ohshima at kusastro.kyoto-u.ac.jp may quicken
the analysis):
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