XCov 15 Observing Instructions for DQ Her
DQ Her is an eclipsing binary with an orbital period of 4h 39m, clear
evidence of mass transfer in the light curve, and the presence of a rapid
oscillation at 71.1 seconds. DQ Her in eclipse is very faint (~ 17 mag) so
if you can't find it, check the ephemeris. It is an old nova (Nova Her
1934) and hence may be changing as it cools down. We ask that all WET
observers follow the same procedures to assure uniformity; these are
outlined below.
- Timing: A leap second will be inserted into Universal Time
at midnight on 30 June 1997. Please be sure this has been properly
taken into account when you establish the start times of your runs, by
checking that the observatory clock you reference has been properly
updated.
- As usual, we ask that you use no filter in the light path (white light),
and an aperture size of 15 arcseconds if this is possible. There is a
faint nebula around the target star about this size, or a bit smaller
--- probably not visible to the eye even on large telescopes, but we
want to include most of its light. A slightly larger aperture is
probably OK but a smaller one is not.
- Set the integration time to 2 seconds. We recognize that
the data files will be large, but not impossibly so. Try to start each
run on an even second (0, 2, 4, 6 ...) rather than on an odd one, for
easier merging of the runs.
- Please use one of the guide stars, marked with a circle on the
finding charts, if you can. We have included two of them, at different
distances from the target star, to allow for differences in telescope
plate scale. Use whichever one you feel will be unvignetted for your
instrument.
- Please send the data to wet@bullwinkle.as.utexas.edu each night
when you finish observing, if you can. You can use email or, if you
prefer, annonymous FTP (put the runs into the "incoming" directory).
As before, we'll try to contact you by telephone at your observatory to
learn about your weather conditions, and to pass along any questions we may
have about your data or procedures. We had rather bad luck with the
weather last time, so we expect unusually good weather for this run :-).
ed