[vsnet-outburst 16150] EI Psc: early superhumps?

[Ohshima]

VSNET campaign target list (2013 Oct 26)

  *** VSNET campaign selected current target list 2013 Oct 26 ***

Object     Class   Position     Type       State       Mag     Data   Remark
Added Date
============================================================================
EI Psc              23:29:54.2     UG     SU UMa     13.3        1
             1       +06:28:12           stage A superhump expected!!

MASTER OT J061335.30+395714.7    UG        WZ Sge     14.6         1
Oct 20 added    1                           early superhumps

MASTER OT J074940.48+071557.1    UG        WZ Sge      15.4        1
Oct 20 added   1                            ?

MASTER OT J015016.17+375620.5    UG      peculiar UG?   14.9        1
Oct 24 added1

TCP J23382254-2049518            UG        WZ Sge           16.0      1
Sep 30 added   1                           stage B ordinary superhumps

PB9151             02 42 42.86   UGSU:+E   SU UMa     16.9       1
Oct 23 added      -11 46 45.5              candidate

SY Cap       1     20:29:47.5    UGSU     SU UMa       13.2       1
Oct 24 added      -15:54:37              superoutburst

CP Eri 	      1    03:10:32.8     NLAC     SU UMa      <18     1
Oct 4 added       -9:45:04                 declined

V369 Peg      1    23:03:41.7    UGSU     SU UMa       15.4       1
Oct 24 added      +17:17:54              probable superoutburst

PU Per       1     02:42:16.1    UGSU     SU UMa       16.2:      1
                   +35:40:47              superoutburst? 

OT J210016.0-024258              UGSU     WZ Sge       17.7      1
             1                            decline from rebrightening?

CSS J163120.9+103134             UGSU      SU UMa      15.7:       1
Oct 11 added  1  

ASASSN-13dh        02:05:37.7     UG                   ?       1 
Oct 4 added   1      +26:43:5.2              faded?

ASASSN-13da        19:59:18       UGSU       SU UMa     <18?      1
Oct 3 added   1    -18:33:31                 faded?

AY For             02:19:28        UGSU+E      SU UMa   15.8      1
             1     -30:45:45.6                 superoutburst

ASASSN-13ck  1      0:11:33.7     UGSU     SU UMa       19.0     1
                   +04:51:23                WZ Sge   decline from rebrightening

MASTER OT J004527.52+503213.8    UGSU?     SU UMa      19.0       1
             1                             WZ Sge, decline from rebrightening

AW Sge              19:58:37.0     UGSU      SU UMa     <16.5:       1
Oct 7 added 2       +16:41:27                probably declined

V496 Aur            07:27:52.3     UGSU      SU UMa     <16.5?       1
Sep 30 added 2        +40:46:54.3             probably declined

======================================================================
other dwarf novae in superoutburst

======================================================================
other objects of current interest

V1323 Her (VY Scl?, deep fading), OR And (VY Scl, deep fading),
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), AY For(eclipsing novalike outburst)
======================================================================

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):