activity
20182022
most citedDiscovery and characterization of five new eclipsing AM CVn systems

48 citations · 98 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.SR202218 cited

The OmegaWhite Survey for Short-Period Variable Stars VII: High amplitude, short period blue variables

G. Ramsay, P. A. Woudt, T. Kupfer +11

Blue Large Amplitude Pulsators (BLAPs) are a relatively new class of blue variable stars showing periodic variations in their light curves with periods shorter than a few tens of m…

astro-ph.SR202148 cited

Discovery and characterization of five new eclipsing AM CVn systems

J. van Roestel, T. Kupfer, M. J. Green +19

AM CVn systems are ultra-compact, helium-rich, accreting binaries with degenerate or semi-degenerate donors. We report the discovery of five new eclipsing AM CVn systems with orbit…

astro-ph.IM2020

IGAPS: the merged IPHAS and UVEX optical surveys of theNorthern Galactic Plane

M. Monguió, R. Greimel, J. E. Drew +47

The INT Galactic Plane Survey (IGAPS) is the merger of the optical photometric surveys, IPHAS and UVEX, based on data from the Isaac Newton Telescope (INT) obtained between 2003 an…

astro-ph.HE201916 cited

The Palomar Transient Factory Sky2Night programme

J. van Roestel, P. J. Groot, T. Kupfer +9

We present results of the Sky2Night project: a systematic, unbiased search for fast optical transients with the Palomar Transient Factory. We have observed 407 deg in -band…

astro-ph.SR201916 cited

Phase-Resolved Spectroscopy of Gaia14aae: Line Emission From Near the White Dwarf Surface

M. J. Green, T. R. Marsh, D. Steeghs +8

AM CVn binaries are a class of ultracompact, hydrogen-deficient binaries, each consisting of a white dwarf accreting helium-dominated material from a degenerate or semi-degenerate…

astro-ph.SR2018

The physical properties of AM CVn stars: new insights from Gaia DR2

G. Ramsay, M. J. Green, T. R. Marsh +9

AM CVn binaries are hydrogen deficient compact binaries with an orbital period in the 5-65 min range and are predicted to be strong sources of persistent gravitational wave radiati…