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- W2891591431 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." @default.
- W2891591431 created "2018-09-27" @default.
- W2891591431 creator A5070078630 @default.
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- W2891591431 date "2018-09-20" @default.
- W2891591431 modified "2023-10-13" @default.
- W2891591431 title "A feasibility study on the photometric detection of quiescent black hole X-ray binaries" @default.
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- W2891591431 doi "https://doi.org/10.1093/mnras/sty2570" @default.
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