Spectroscopy of New and Poorly Known Cataclysmic Variables in the Kepler Field
arXiv:1302.3975 · doi:10.1088/0004-6256/145/4/109
Abstract
The NASA {\it Kepler} mission has been in science operation since May 2009 and is providing high precision, high cadence light curves of over 150,000 targets. Prior to launch, nine cataclysmic variables were known to lie within {\it Kepler's} field of view. We present spectroscopy for seven systems, four of which were newly discovered since launch. All of the stars presented herein have been observed by, or are currently being observed by, the {\it Kepler} space telescope. Three historic systems and one new candidate could not be detected at their sky position and two candidates are called into question as to their true identity.
Accepted to AJ
References in corpus (1)
Cited by in corpus (16)
- Study of Superoutbursts and Superhumps in SU UMa Stars by the Kepler Light Curves of V344 Lyrae and V1504 Cygni
- A Pan-STARRS1 study of the relationship between wide binarity and planet occurrence in the Kepler field
- RATS-Kepler -- a deep high cadence survey of the Kepler field
- The rms-flux relation in accreting white dwarfs: another nova-like variable and the first dwarf nova
- KIC 9406652: An Unusual Cataclysmic Variable in the Kepler Field of View
- Analysis of Three SU UMa-Type Dwarf Novae in the Kepler Field
- The Variable Sky of Deep Synoptic Surveys
- Spectroscopic properties of the dwarf nova-type cataclysmic variables observed by LAMOST
- Cataclysmic Variables observed during K2 Campaigns 0 and 1
- Continuous `stunted' outbursts detected from the Cataclysmic Variable KIC 9202990 using Kepler data
- Measuring White Dwarf Variability from Sparsely Sampled Gaia DR3 Multi-Epoch Photometry
- Spectroscopic Studies of 30 Short-period Cataclysmic Variable Stars, and Remarks on the Evolution and Population of Similar Objects
- BOKS 45906: a CV with an orbital period of 56.6 min in the Kepler field?
- The Kepler and Hale observations of V523 Lyr
- Investigation of superhumps in SU UMa-type dwarf novae based on the observations of TESS
- Census of blue stars in SDSS DR8