activity
20152026
most citedSearching for Electromagnetic Counterparts to Gravitational-wave Merger Events with the Prototype Gravitational-wave Optical Transient Observer (GOTO-4)

108 citations · 494 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2026

Superorbital variability in the quiescent black hole X-ray transient A0620-00

Enzo A. Saavedra, Roi Alonso, Teo Muñoz-Darias +10

Quiescent black hole low-mass X-ray binaries provide a key setting for probing accretion physics at low luminosities. A0620-00, the archetypal system in this class, has remained in…

astro-ph.HE2022★ 13 cited

Panning for gold, but finding helium: discovery of the ultra-stripped supernova SN2019wxt from gravitational-wave follow-up observations

I. Agudo, L. Amati, T. An +96

We present the results from multi-wavelength observations of a transient discovered during the follow-up of S191213g, a gravitational wave (GW) event reported by the LIGO-Virgo Col…

astro-ph.IM2021★ 40 cited

Transient-optimised real-bogus classification with Bayesian Convolutional Neural Networks -- sifting the GOTO candidate stream

T. L. Killestein, J. Lyman, D. Steeghs +45

Large-scale sky surveys have played a transformative role in our understanding of astrophysical transients, only made possible by increasingly powerful machine learning-based filte…

astro-ph.HE2020★ 61 cited

Einstein@Home Discovery of the Gamma-ray Millisecond Pulsar PSR J2039-5617 Confirms Its Predicted Redback Nature

C. J. Clark, L. Nieder, G. Voisin +19

The Fermi Large Area Telescope gamma-ray source 3FGL J2039.65618 contains a periodic optical and X-ray source that was predicted to be a "redback" millisecond pulsar (MSP) binar…

astro-ph.HE2020★ 108 cited

Searching for Electromagnetic Counterparts to Gravitational-wave Merger Events with the Prototype Gravitational-wave Optical Transient Observer (GOTO-4)

B. P. Gompertz, R. Cutter, D. Steeghs +49

We report the results of optical follow-up observations of 29 gravitational-wave triggers during the first half of the LIGO-Virgo Collaboration (LVC) O3 run with the Gravitational-…

astro-ph.HE2020★ 29 cited

The Changing-look Optical Wind of the Flaring X-ray Transient Swift J1858.6-0814

T. Muñoz-Darias, M. Armas Padilla, F. Jiménez-Ibarra +15

We present the discovery of an optical accretion disk wind in the X-ray transient Swift J1858.6-0814. Our 90-spectrum data set, taken with the 10.4m GTC telescope over 8 different…

astro-ph.HE2019★ 85 cited

Hard-state accretion disk winds from black holes: the revealing case of MAXI J1820+070

T. Muñoz-Darias, F. Jiménez-Ibarra, G. Panizo-Espinar +16

We report on a detailed optical spectroscopic follow-up of the black hole transient MAXI J1820+070 (ASASSN-18ey). The observations cover the main part of the X-ray binary outburst,…

astro-ph.HE2018★ 12 cited

The long-term optical evolution of the black hole candidate MAXI J1659-152

Jesus M. Corral-Santana, Manuel A. P. Torres, Tariq Shahbaz +13

We present 5 years of optical and infrared data of the black hole candidate MAXI J1659-152 covering its 2010 outburst, decay and quiescence. Combining optical data taken during the…

astro-ph.HE2017★ 12 cited

Swift and SALT observations of the Multiple Outbursts of MAXI J1957+032

D. Mata Sánchez, P. A. Charles, M. Armas Padilla +4

The new recurrent X-ray transient MAXI J1957+032 has had four X-ray outbursts within 16 months, all very briefly detected (lasting <5 days). During the most recent event (Sep/Oct 2…

astro-ph.HE2016★ 48 cited

The donor of Aquila X-1 revealed by high angular resolution near-infrared spectroscopy

D. Mata Sánchez, T. Muñoz-Darias, J. Casares +1

The low mass X-ray binary Aquila X-1 is one of the most active neutron star X-ray transients. Despite it has a relatively bright quiescent optical counterpart, the detection of its…

astro-ph.HE2015★ 57 cited

Swift J1357.2-0933: a massive black hole in the Galactic thick disc

Daniel Mata Sánchez, Teo Munoz-Darias, Jorge Casares +2

Swift J1357.2-0933 is one of the shortest orbital period black hole X-ray transients (BHTs). It exhibited deep optical dips together with an extremely broad H line during outbur…

astro-ph.HE2015★ 29 cited

Mass constraints to Sco X-1 from Bowen flourescence and deep near-infrared spectroscopy

D. Mata Sánchez, T. Muñoz-Darias, J. Casares +3

More than 50 years after the dawn of X-ray astronomy, the dynamical parameters of the prototypical X-ray binary Sco X-1 are still unknown. We combine a Monte Carlo analysis, which…