Observing Campaign to Monitor AR UMa
for Spitzer Space Telescope Observations
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| Spitzer Space Telescope (Courtesy: NASA) | |
From AAVSO Alert Notice 348:
Dr. Steve Howell (National Optical Astronomy Observatory) and Dr. Donald
Hoard (Spitzer Science Center) have requested time-series observations
of the AM Herculis-type cataclysmic variable AR UMa (11:15:44.68
+42:58:22.5 (J2000)) to coincide with upcoming Spitzer Space Telescope
observations.
Both B- and V-band CCD time-series observations are requested leading up
to and during the Spitzer observations scheduled for 2007 May 9-10, and
continuing through May 13-14. Time-series observations during the May
9-10 observing window are most critically needed, while time-series
observations before and after will help to establish the range of
behavior of this object. The star varies between V=14.5 and V=16.5;
please use exposure times that yield a signal-to-noise ratio of 50 per
measurement.
Charts: AR UMa charts and
Henden sequence file
Observing Window:
Now through the end of May, and beyond if possible
Intensive Observing Window:
Spitzer Space Telescope observations will be performed on May 9 - May 10,
and V-band time series observations are most urgently requested during
that time.
Both visual and CCD observations are useful, but V-band time-series
observations are most urgently requested. Please use exposure times such
that you can obtain a signal-to-noise of 50 per observation.
Light Curves
Light curve as of 070502: