The Impact of the Astro2010 Recommendations on Variable Star Science (2009)
Walkowicz, Lucianne M., Becker, Andrew C., Anderson, Scott F., Bloom, Joshua S., Georgiev, Leonid, Grindlay, Josh, ...
The next decade of survey astronomy has the potential to transform our knowledge of variable stars. Stellar variability underpins our knowledge of the cosmological distance ladder, and provides...
XMM-Newton and Optical Observations of Cataclysmic Variables from SDSS (2009)
Hilton, Eric J., Szkody, Paula, Mukadam, Anjum, Henden, Arne, Dillon, William, Schmidt, Gary D.
We report on XMM-Newton and optical results for 6 cataclysmic variables that were selected from Sloan Digital Sky Survey spectra because they showed strong HeII emission lines, indicative of being...
Two more candidate AM Canum Venaticorum (AM CVn) Binaries from the Sloan Digital Sky Survey (2008)
Anderson, Scott, Becker, Andrew, Haggard, Daryl, Prieto, Jose Luis, Knapp, Gillian, Sako, Masao, ...
Also archived in: arXiv:0802.2240 v1 Feb 15 2008
XMM-Newton Observations of the Cataclysmic Variable GW Lib (2007)
Hilton, Eric J., Szkody, Paula, Mukadam, Anjum, Mukai, Koji, Hellier, Coel, Van Zyl, Liza, ...
XMM-Newton observations of the accreting, pulsating white dwarf in the quiescent dwarf nova GW Librae were conducted to determine if the non-radial pulsations present in previous UV and optical data...
Szkody, Paula, Mukadam, Anjum, Gaensicke, Boris T., Woudt, Patrick A., Solheim, Jan-Erik, Nitta, Atsuko, ...
Ultraviolet observations using the Solar Blind Channel on the Hubble Space Telescope provide light curves and low resolution spectra of three pulsating white dwarfs in the cataclysmic variables...
Cataclysmic variables from sloan digital sky survey - V. The fifth year (2004) (2006)
Szkody, Paula, Henden, Arne, Agüeros, Marcel, Anderson, Scott F., Bochanski, John J., Knapp, Gillian R., ...
Evolutionary Timescale of the DAV G117-B15A: The Most Stable Optical Clock Known (2000)
Kepler, S. O., Mukadam, Anjum, Winget, D. E., Nather, R. E., Metcalfe, T. S., Reed, M. D., ...
We observe G117-B15A, the most precise optical clock known, to measure the rate of change of the main pulsation period of this blue-edge DAV white dwarf. Even though the obtained value is only within...