Dr. Steve Howell (NOAO) requests monitoring of a subset of the known and
suspected tremendous outburst amplitude dwarf novae (TOADs) in support of
Spitzer Space Telescope observations of these objects. Observers are asked
to increase their monitoring of the objects in the table below in support
of this campaign. We note that several of these objects -- notably the
WZ Sge stars WZ Sge, GW Lib, and V455 And -- are not expected to
superoutburst during the next year, but observations are still encouraged
in case they exhibit unexpected behavior.
The following table lists the observed magnitude range and an outburst
threshold for each star. Any observation above the threshold should be
considered in outburst, and any observation at or near the maximum is
likely a superoutburst. If the object is in outburst or near maximum,
please contact the AAVSO immediately. Spitzer observations will not
be triggered immediately, however, an Alert Notice will be issued
requesting concentrated coverage of the star.
Name RA(J2000) Dec(J2000) thrshld. maximum minimum type period(m)
------------------------------------------------------------------------------
WX Cet 01:17:04.20 -17:56:23.0 13.5 9.5 18.5 ugwz 83.9
UV Per 02:10:08.00 +57:11:20.0 15.0 11.0 17.5 ugsu 93.3
UW Per 02:12:29.59 +57:05:19.7 15.5 13.5 18.0 ug unknown
PQ And 02:29:29.54 +40:02:40.2 15.0 10.1 19.0 ugwz unknown
SW UMa 08:36:42.70 +53:28:38.0 15.0 9.7 16.5 su/dq 81.8
EG Cnc 08:43:04.00 +27:51:50.0 15.0 11.9 17.0 ugwz 84.6
BZ UMa 08:53:44.20 +57:48:41.0 14.5 10.2 15.9 ugsu 97.9
RZ Leo 11:37:22.2 +01:48:58.0 14.5 11.5 19.2 ugwz 109.5
QZ Vir 11:38:26.80 +03:22:07.0 13.5 10.0 15.7 ugsu 86.4
BC UMa 11:52:15.90 +49:14:42.0 15.0 10.9 18.3 ugsu 91.2
HV Vir 13:21:03.10 +01:53:30.0 15.0 11.5 19.0 ugwz 83.5
UZ Boo 14:44:01.21 +22:00:54.8 15.0 11.5 20.4 ugwz unknown
EK TrA 15:14:00.40 -65:05:36.0 14.0 10.4 16.6 ugsu 90.5
GW Lib 15:19:55.40 -25:00:25.0 14.0 9.0 18.5 ugwz 76.8
V544 Her 16:38:05.40 +08:37:59.0 16.0 14.5 20.0 ug unknown
DH Aql 19:26:10.8 -10:15:29.0 15.0 12.5 18.3 ugsu unknown
KX Aql 19:33:53.70 +14:17:48.0 15.5 12.5 18.4 ug 86.9
WZ Sge 20:07:36.50 +17:42:15.0 14.0 7.0 15.5 ugwz 81.6
VY Aqr 21:12:09.2 -08:49:37.0 15.0 8.4 17.5 ugwz 91
V455 And 23:34:01.45 +39:21:41.0 14.0 8.5 16.5 ugwz 81.1
Both visual and CCD observations are useful, and multicolor photometry
would be greatly appreciated. Visual observers are asked to observe these
objects as normal; if they are already in your list of objects, please
continue, and if not, please add them to your nightly observing program.
CCD observers are asked to use exposure times such that you can obtain a
signal-to-noise of 50 per observation. CCD observers are asked to
obtain filtered photometry, in at least two filters if you are capable of
doing so; single-filtered or unfiltered observations are also appreciated.
Time-series observations are not required except for cases where superhumps
have not yet been observed or the orbital period is unknown, and then are
only requested when the star is in outburst. For both visual and CCD
observations, "fainter-than" observations are also important, particularly
for objects with faint minima, so please report them as promptly as
positive detections.
This campaign begins now (May 16, 2008) and continues through May 2009.
Once an object has been verified in superoutburst, Spitzer observations
will be scheduled within 2-4 weeks of maximum, and will be repeated twice
-- 4-6 weeks and 6-10 weeks later. Observers are asked to provide nightly
monitoring of these stars, and to begin intensive observations if and when
any of them go into outburst to determine whether the star is in
superoutburst.
For more detailed information on this campaign, visit the following URL:
http://www.aavso.org/news/toads_campaign.shtml
This campaign is being organized for Dr. Howell at AAVSO Headquarters by
Dr. Matthew Templeton.
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