AAVSO Alert Notice 426
Rescheduled request for observations of V455 AND in support of HST observations
October 5, 2010

Rescheduled request for observations of V455 AND in support of HST observations
October 5, 2010

As originally announced in AAVSO Alert Notice 423, Dr. Paula Szkody (U. Washington) has requested the help of AAVSO observers in monitoring the WZ Sge-type cataclysmic variable V455 And in support of Hubble Space Telescope ultraviolet spectroscopic observations.

These observations, originally scheduled for September and postponed due to satellite troubles, have been rescheduled for 12:10-20:24 October 14 2010 UT (the night of Wednesday, October 13/14) (JD 2455483.00694-2455484.35000). Observations are requested beginning immediately and continuing through October 23. This monitoring is crucial to these HST observations.

The primary purpose of the monitoring is to know whether V455 And is in quiescence; if it is in outburst it will be too bright for the HST instrumentation. The decision whether to go forward with the HST observations will be made the evening of Tuesday, October 12/13, so the nights of October 11/12, 12/13, and 13/14 are the most critical for observations to be reported. Positive visual or V observations are preferred if at all possible, but fainter-than observations below V=14 are useful (<14.0 or fainter). Therefore, nightly observations are sufficient for now; 2-3 observations per night (reported as soon as they are made) are requested during the nights of October 11/12 through 15/16, after which nightly observations may be resumed. For CCD observers, Dr. Szkody writes, "[We] will also be summing the spectra to obtain UV light curves. Simultaneous photometry [shortly before, during, and after the HST observations] would be great for CCD observers. B filter would be best for a light curve, although for the magnitude estimates, a V measurement would be best. An uninterrupted light curve would be better than cycling between filters." During quiescence V455 And is around magnitude V=16. According to observations in the AAVSO International Database, the last outburst of V455 And occurred September 5, 2007, when it reached visual magnitude 8.0 and was brighter than about magnitude 15 until November 2007. V455 And (AUID 000-BDC-667) is located at the following (J2000) coordinates: RA: 23:34:01.45 Dec. +39:21:40.9 Charts for V455 And may be plotted using AAVSO VSP: http://www.aavso.org/vsp Please submit all observations of V455 And to the AAVSO International Datbase as V455 AND. Thank you for your observing efforts and valuable observations! This AAVSO Alert Notice was prepared by Elizabeth O. Waagen. Please use the following links: Data submission: http://www.aavso.org/webobs
Alert Notice archive: http://www.aavso.org/alert-notice-archive
Subscription information: http://www.aavso.org/observation-notification#alertnotice

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