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20002025
most citedBlackCAT: A catalogue of stellar-mass black holes in X-ray transients

424 citations · 1.3k across the 23 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2025★ 4 cited

Characterising the short-orbital period X-ray transient Swift J1910.2-0546

J. M. Corral-Santana, P. Rodriguez-Gil, M. A. P. Torres +13

SwiftJ1910.2-0546 is a Galactic X-ray transient discovered during a bright outburst in 2012. We use time-series optical photometry and spectroscopy to estimate the orbital period,…

astro-ph.HE2015★ 424 cited

BlackCAT: A catalogue of stellar-mass black holes in X-ray transients

Jesus M. Corral-Santana, Jorge Casares, Teo Munoz-Darias +3

During the last ~50 years, the population of black hole candidates in X-ray binaries has increased considerably with 59 Galactic objects detected in transient low-mass X-ray binari…

astro-ph.SR2015

Dynamical masses of a nova-like variable on the edge of the period gap

P. Rodríguez-Gil, T. Shahbaz, T. R. Marsh +12

We present the first dynamical determination of the binary parameters of an eclipsing SW Sextantis star in the 3-4 hour orbital period range during a low state. We obtained time-re…

astro-ph.SR2009★ 16 cited

The magnetic SW Sextantis star RX J1643.7+3402

P. Rodriguez-Gil, I. G. Martinez-Pais, J. de la Cruz Rodriguez

We present time-resolved spectroscopy and circular spectropolarimetry of the SW Sex star RX J1643.7+3402. We find significant polarisation levels exhibiting a variability at a peri…

astro-ph.HE2009★ 28 cited

Dynamical constraints on the neutron star mass in EXO 0748-676

T. Muñoz-Darias, J. Casares, K. O'Brien +4

We present VLT intermediate resolution spectroscopy of UY Vol, the optical counterpart of the LMXB X-ray burster EXO 0748-676. By using Doppler tomography we detect narrow componen…

astro-ph2008★ 124 cited

On the masses and evolutionary status of the black hole binary GX 339-4. A twin system of XTE J1550-564?

T. Muñoz-Darias, J. Casares, I. G. Martinez-Pais

We apply the K-correction to the black hole LMXB GX 339-4 which implies Mx > 6 Msun by only assuming that the companion is more massive than ~0.17 Msun, the lower limit allowed by…