A feasibility study on the photometric detection of quiescent black hole X-ray binaries
Abstract
We investigate the feasibility of detecting quiescent black hole X-ray binaries using optical photometric techniques. To test this we employ a combination of r-band and Halpha filters currently available at the Roque de los Muchachos Observatory. Photometric observations of four dynamical black holes (GRO J0422+320, A 0620-00, XTE J1118+480 and XTE J1859+226) at SNR>~35-50, supplemented with near simultaneous spectroscopic data, demonstrate that it is possible to recover the FWHM of the Halpha emission line to better than 10% for targets with a wide range of line EWs and down to magnitude r~22. We further explore the potential of our photometric system to disentangle other populations of compact stars and Halpha emitters. In particular, we show that HAWKs, a survey designed to unveil quiescent black holes, will also provide a detailed census of other Galactic populations, most notably short period (eclipsing) cataclysmic variables, neutron star X-ray binaries and ultra-compact binaries.
Cite
@article{arxiv.1809.07330,
title = {A feasibility study on the photometric detection of quiescent black hole X-ray binaries},
author = {Jorge Casares and Manuel A. P. Torres},
journal= {arXiv preprint arXiv:1809.07330},
year = {2018}
}
Comments
Accepted for publication in MNRAS, 11 pages, 5 figures, 3 Tables. v2 with updated references