[vsnet-alert 16048] Re: stage A superhump paper and project (prioritytarget list)
Josch Hambsch
hambsch at telenet.be
Thu Jul 25 04:00:44 JST 2013
I will start observing BW Scl, which anyway was on my to do list.
If there are high priority Southern targets among this large list, I am
definitely interested.
Regards,
Groeten,
Grüße,
Josch
www.astronomie.be/hambsch
-----Original Message-----
From: Taichi Kato
Sent: Wednesday, July 24, 2013 4:19 AM
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Subject: [vsnet-alert 16046] stage A superhump paper and project
(prioritytarget list)
*** List of SU UMa-type dwarf novae with known orbital periods ***
RKCat name Porb
TU Men 0.1172
V1239 Her 0.100082e
V1006 Cyg 0.09904 (no SH yet)
NY Ser 0.0978
J2147+2445 0.09273
J0846+3115 0.09138
J1625+1203 0.0911
V1258 Cen 0.088941e
GZ Cnc 0.0881
V344 Lyr 0.087904 (Kepler target)
IR Com 0.087039e (no SH yet)
YZ Cnc 0.0868
V713 Cep 0.085418e (no SH yet)
J1639+1224 0.085
KK Tel 0.0845
BF Ara 0.08418
TY PsA 0.0841
V516 Lyr 0.08400 (Kepler target)
QU Aqr 0.083304
QZ Ser 0.083161
BG Ari 0.08242
TU Crt 0.08209
KP Cas 0.0814
V1032 Oph 0.081056e
CP Dra 0.0808
AR Pic 0.08022
V493 Ser 0.08001
BR Lup 0.0795
J0334-0710 0.079
CU Vel 0.0785
V660 Her 0.07826
V359 Cen 0.0779
PU UMa 0.077881e
V503 Cyg 0.07777
HS Vir 0.0769
J1730+6247 0.07654
SU UMa 0.07635
RZ Leo 0.076038
V893 Sco 0.075961 (no SH yet)
EG Aqr 0.07596
V342 Cam 0.07531
J0839+2828 0.0753
BK Lyn 0.07498 (ER)
J0814-0050 0.07485
WX Hyi 0.074813
LY Hya 0.0748
J0501+2038 0.0748
QT Aqr 0.0747
AY For 0.0746
QW Ser 0.07457
Z Cha 0.074499e
VW Hyi 0.074271
V1316 Cyg 0.0740
IY UMa 0.073909e
HT Cas 0.073647e
CC Cnc 0.07352
VZ Pyx 0.07332
OU Vir 0.07273e
QV Aqr 0.07196
NN Cam 0.0717
J1842+4837 0.07168
FO And 0.07161
GD 552 0.07134 (no outburst yet)
J0803+2516 0.071
J0221-2619 0.07049
J1443-1755 0.0702
J0345-0152 0.07018
V2779 Oph 0.070037
CY UMa 0.06957
V1504 Cyg 0.06951 (Kepler target)
V368 Peg 0.0686
IR Gem 0.0684
TY Psc 0.06833
J1509+4650 0.0683
J1715+6856 0.0683
RZ Sge 0.06828
V1212 Tau 0.0682
J1658+1847 0.068064
KS UMa 0.0680
BZ UMa 0.06799
SS UMi 0.0678
NSV 4838 0.0678
J1152+4049 0.0676e
V2690 Oph 0.06739
J2154+1557 0.067294
SX LMi 0.0672
J2206+3014 0.067
IX Dra 0.06646?
J0932+4725 0.066303
J2158+2419 0.06607
J0431-0314 0.06605
FL Lyn 0.066
GO Com 0.0658
J0945-1944 0.065769
J0426+3541 0.06551
DM Lyr 0.065409
AO Oct 0.06535
J1524+2209 0.065319e
J0912-0349 0.0653:
AK Cnc 0.0651
UV Per 0.0649
J1538+5123 0.06466
V1227 Her 0.06442e
HW Boo 0.06435
V632 Cyg 0.06377
ER UMa 0.06366 (ER)
J0039+0054 0.063469
V453 Nor 0.06338
CG CMa 0.063275
J1440+4947 0.0632
OY Car 0.063121
J1125-0016 0.0631
V1229 Her 0.0631
VY Aqr 0.06309
J1227+5139 0.062950e
TV Crv 0.0629
V5662 Sgr 0.06289:
EK TrA 0.06288
HO Del 0.0627
J1300+1151 0.06267
BC UMa 0.06261
V436 Cen 0.062501
V2051 Oph 0.062428e
V1159 Ori 0.062178 (ER)
V1141 Aql 0.06202:
DT Pyx 0.06165
V4140 Sgr 0.061430e
J1025-1542 0.06136
J0332+0204 0.06121
XZ Eri 0.061159e
J1537-2440 0.061
AQ Eri 0.06094
J2048-0610 0.060597
KX Aql 0.06035
V1040 Cen 0.060296
CI UMa 0.060
J1051+6725 0.060
J1405-1902 0.060:
V521 Peg 0.0599
J2112+2421 0.0598
J0826-0007 0.05976
J0904+0355 0.059723
HT Cam 0.059712 (IP, no superoutburst?)
FS Aur 0.059581 (no superoutburst?)
J1404-1027 0.059579
EN Cet 0.05933
J0903+3300 0.059074e
EZ Lyn 0.059005e
NZ Boo 0.058910e
J0755+1435 0.05886
DV Dra 0.05883:
QZ Vir 0.05882
EG Cnc 0.05877
KV Dra 0.05876
OV Dra 0.058736e
J2109+1348 0.05865
J1112-3538 0.05847
J1735+1547 0.0583:
J2230-1458 0.0583:
WX Cet 0.058261
J1706+1434 0.0582
V386 Ser 0.0581
J0627+3952 0.0579
CC Scl 0.05763
MM Hya 0.057590
J2205+1155 0.05752
V355 UMa 0.05731
J0043-0037 0.057170
J0120+3255 0.057145
HV Vir 0.057069
J1035+0551 0.057007
V1108 Her 0.0570
J1610+0907 0.0569
J1501+5501 0.056841e
SW UMa 0.056815
J1605+2030 0.0567
PU CMa 0.056694:
WZ Sge 0.056688
AL Com 0.056668
GY Cet 0.05663
FL Psc 0.05654
J0902+0525 0.05652
J0947+0610 0.0564
V466 And 0.05635
V455 And 0.056309e
V391 Cam 0.05620
PQ And 0.0560:
LV Cnc 0.056
GS Cet 0.056
VV Equ 0.056
V406 Vir 0.0559
V1247 Her 0.05580
SS LMi 0.0557
V500 And 0.05550
GZ Cet 0.055351
LL And 0.055055
HO Cet 0.05490
V572 And 0.05487
V844 Her 0.054643
DI UMa 0.05457 (ER)
BW Scl 0.054323
J1433+1011 0.054241e
PR Her 0.0542
J1457+5148 0.054087
J2138+2619 0.0536:
UW Tri 0.05334
GW Lib 0.05332
PHL 1445 0.052985
CT Tri 0.05281
EQ Lyn 0.0528
OV Boo 0.046258e
J1122-1110 0.04530
V396 Hya 0.04519 (AM)
J1740+4147 0.0450
EI Psc 0.044567
V485 Cen 0.040995
1108+5728 0.038449
J1028-0819 0.0362?
J0450-0931 0.03283: (AM)
GP Com 0.032339 (AM, no outburst yet)
J0129+3842 0.026080 (AM)
V558 Vir 0.02539 (AM)
J0435+0029 0.024 (AM)
V406 Hya 0.023470 (AM)
J0943+1029 0.0210 (AM)
CP Eri 0.019692 (AM)
YZ LMi 0.019661 (AM)
J0719+4858 0.01859 (AM)
V803 Cen 0.01848 (AM)
KL Dra 0.017382 (AM)
CR Boo 0.017029 (AM)
(* Note that the quality of Porb is heterogeneous.
The list is still very incomplete and we will make updates.)
They are our primary targets. Exclude Kepler targets
(enough good data). ER UMa stars don't show stage A superhump
near their peak, they need to be monitored *before*
the superoutburst.
AM CVn stars are particularly good targets, because
their mass ratios are very difficult to determine in other ways.
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