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KIC11911480: the second ZZ Ceti in the field
S. Greiss, B. T. Gaensicke, J. J. Hermes +5
We report the discovery of the second pulsating hydrogen-rich (DA) white dwarf in the field, KIC11911480. It was selected from the -INT Survey (KIS) on the basis o…
The Galactic Bulge Survey: completion of the X-ray survey observations
Peter G. Jonker, Manuel A. P. Torres, Robert I. Hynes +8
We provide the Chandra source list for the last ~quarter of the area covered by the Galactic Bulge Survey (GBS). The GBS targets two strips of 6\degr x 1\degr (12 square degrees in…
Near-infrared counterparts to the Galactic Bulge Survey X-ray source population
S. Greiss, D. Steeghs, P. G. Jonker +6
We report on the near-infrared matches, drawn from three surveys, to the 1640 unique X-ray sources detected by Chandra in the Galactic Bulge Survey (GBS). This survey targets faint…
Two new AM Canum Venaticorum binaries from the Sloan Digital Sky Survey III
P. J. Carter, B. T. Gänsicke, D. Steeghs +6
The AM Canum Venaticorum (AM CVn) binaries are a rare group of ultra-short period, mass-transferring white dwarf binaries, some of which may be Type Ia supernova progenitors. More…
Precision ephemerides for gravitational-wave searches: I. Sco X-1
Duncan Galloway, Sammanani Premachandra, Danny Steeghs +3
Rapidly-rotating neutron stars are the only candidates for persistent high-frequency gravitational wave emission, for which a targeted search can be performed based on the spin per…
The AM CVn binary SDSS J173047.59+554518.5
P. J. Carter, D. Steeghs, T. R. Marsh +4
The AM Canum Venaticorum (AM CVn) binaries are a rare group of hydrogen-deficient, ultra-short period, mass-transferring white dwarf binaries, and are possible progenitors of type…