[vsnet-campaign-target 235] VSNET campaign target list (2013 Dec 27)
Ohshima
ohshima at kusastro.kyoto-u.ac.jp
Sat Dec 28 03:53:24 JST 2013
VSNET campaign target list (2013 Dec 27)
*** VSNET campaign selected current target list 2013 Dec 27 ***
Object Class Position Type State Mag Data Remark
Added Date
============================================================================
AL Com UGWZ SU UMa 15.2 1
12:32:25.8 ordinary superhumps
+14:20:43
1RXS J041924.8+653006 UG SU UMa 13.9 1
candidate
MASTER OT J162323.48+782603.3 UGWZ: WZ Sge? 18.5 1
post superoutburst stage
MASTER OT J005740.99+443101.5 UG WZ Sge 19.5 1
1 stage C superhumps
TY Psc 01:25:39.3 UGSU SU UMa 13.5? 1
+32:23:09 superhumps
======================================================================
other dwarf novae in superoutburst
======================================================================
other objects of current interest
V1323 Her (VY Scl?, deep fading), OR And (VY Scl,recovering from deep
fade),MASTER OT J204200.48+041839.9(ER UMa candidate?)
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, 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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