White Dwarf WD 1929+012 Photometric
Monitoring Observations by Amateurs
B. L. Gary, Last updated 2015.11.03
This web page is devoted to a photometric monitoring of white
dwarf WD 1929+012 for the purpose of
identifying transit features produced by an asteroid dust cloud.
Links on this web page
Summary of results
Observing session LCs
Summary of Results
No transit events have been observed.
Feasibility of monitoring using a 14" telescope has been
demonstrated.
Observing Sessions
2015 Nov 03
This 3.2-hr observing session demonstrates the feasibility of
monitoring WD1929 with a 14" telescope.
Light curve with fit using a large value for "air mass
curvature" that is required, apparently, because the target WD
is much bluer than the reference stars.
Return to Croll observing list main
page.
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WebMaster: B. Gary. Nothing on this web page is copyrighted. This
site opened: Nov 03, 2015