activity
20052026
most citedOverlapping abundance gradients and azimuthal gradients related to the spiral structure of the Galaxy

119 citations · 545 across the 21 of their papers we have counts for

collaborators

22 papers

astro-ph.SR2026

Identification of unresolved binaries in the VVV b294 tile: A Pro-Am collaboration using the Virtual Observatory

M. Cortés-Contreras, P. Cruz, E. Solano +22

Stellar binaries and multiples are common objects. Their identification and characterization are primarily limited by the angular resolution of current instrumentation, survey dept…

astro-ph.SR2023★ 24 cited

White dwarf spectral type-temperature distribution from Gaia-DR3 and the Virtual Observatory

S. Torres, P. Cruz, R. Murillo-Ojeda +6

The characterization of white dwarf atmospheres is crucial for accurately deriving stellar parameters such as effective temperature, mass, and age. We aim to classify the populatio…

astro-ph.SR2023★ 2 cited

Searching for the nature of stars with debris disks and planets

R. de la Reza, C. Chavero, S. Roca-Fàbrega +3

The nature of the few known solar-mass stars simultaneously containing debris disks and planets remains an open question. A number of works have shown that this property appears to…

astro-ph.SR2023★ 2 cited

M-dwarf stars in the b294 field from the VISTA Variables in the Vía Láctea (VVV)

Patricia Cruz, Miriam Cortés-Contreras, Enrique Solano +4

M-dwarf stars are the dominant stellar population in the MilkyWay and they are important for a wide variety of astrophysical topics. The Gaia mission has delivered a superb collect…

astro-ph.SR2022★ 63 cited

Spectral classification of the 100 pc white dwarf population from Gaia-DR3 and the Virtual Observatory

F. M. Jiménez-Esteban, S. Torres, A. Rebassa-Mansergas +5

The third data release of Gaia has provided low resolution spectra for ~100,000 white dwarfs (WDs) that, together with the excellent photometry and astrometry, represent an unrival…

astro-ph.SR2022★ 4 cited

The miniJPAS survey: stellar atmospheric parameters from 56 optical filters

H. -B. Yuan, L. Yang, P. Cruz +29

With a unique set of 54 overlapping narrow-band and two broader filters covering the entire optical range, the incoming Javalambre-Physics of the Accelerating Universe Astrophysica…

astro-ph.SR2022★ 6 cited

J-PLUS: Discovery and characterisation of ultracool dwarfs using Virtual Observatory tools II. Second data release and machine learning methodology

P. Mas-Buitrago, E. Solano, A. González-Marcos +20

Ultracool dwarfs (UCDs) comprise the lowest mass members of the stellar population and brown dwarfs, from M7 V to cooler objects with L, T, and Y spectral types. Most of them have…

astro-ph.SR2022★ 11 cited

Detached eclipsing binaries from the Kepler field: radii and photometric masses of components in short-period systems

Patricia Cruz, John F. Aguilar, Hernán E. Garrido +2

The characterisation of detached eclipsing binaries with low mass components has become important when verifying the role of convection in stellar evolutionary models, which requir…

astro-ph.SR2022★ 9 cited

Gaia0007-1605: an old triple system with an inner brown dwarf-white dwarf binary and an outer white dwarf companion

Alberto Rebassa-Mansergas, Siyi Xu, Roberto Raddi +5

We identify Gaia0007-1605AC as the first inner brown dwarf-white dwarf binary of a hierarchical triple system in which the outer component is another white dwarf (Gaia0007-1605B).…

astro-ph.SR2018★ 13 cited

The radius inflation problem in short-period low-mass binaries: a large sample analysis

Hernan E. Garrido, Patricia Cruz, Marcos P. Diaz +1

Due to the recent increase in the availability of photometric time-series databases, the characterisation of low-mass eclipsing binaries for the study of their orbital and physical…

astro-ph.SR2018★ 19 cited

Low-mass eclipsing binaries in the WFCAM Transit Survey: the persistence of the M-dwarf radius inflation problem

Patricia Cruz, Marcos Diaz, Jayne Birkby +3

We present the characterization of 5 new short-period low-mass eclipsing binaries from the WFCAM Transit Survey. The analysis was performed by using the photometric WFCAM J-mag dat…

astro-ph.EP2016★ 12 cited

Detection of the secondary eclipse of Qatar-1b in the Ks band

Patricia Cruz, David Barrado, Jorge Lillo-Box +4

Qatar-1b is a close-orbiting hot Jupiter ( , ) around a metal-rich K-dwarf, with orbital separation and period of 0.023 AU and 1.42 days.…

astro-ph.EP2014★ 20 cited

Detection of the secondary eclipse of WASP-10b in the Ks-band

Patricia Cruz, David Barrado, Jorge Lillo-Box +5

WASP-10b, a non-inflated hot Jupiter, was discovered around a K-dwarf in a near circular orbit (). Since its discovery in 2009, different published parameters for this…

astro-ph.EP2014

The first planet detected in the WTS: an inflated hot-Jupiter in a 3.35 day orbit around a late F-star [ERRATUM]

M. Cappetta, R. P. Saglia, J. L. Birkby +35

We report the discovery of WTS-1b, the first extrasolar planet found by the WFCAM Transit Survey, which began observations at the 3.8-m United Kingdom Infrared Telescope (UKIRT) in…

astro-ph.EP2014★ 59 cited

WTS-2 b: a hot Jupiter orbiting near its tidal destruction radius around a K-dwarf

J. L. Birkby, M. Cappetta, P. Cruz +34

We report the discovery of WTS-2 b, an unusually close-in 1.02-day hot Jupiter (Mp=1.12MJ, Rp=1.363RJ) orbiting a K2V star, which has a possible gravitationally-bound M-dwarf compa…

astro-ph.EP2013★ 15 cited

A sensitivity analysis of the WFCAM Transit Survey for short-period giant planets around M dwarfs

Gábor Kovács, S. Hodgkin, B. Sipőcz +11

The WFCAM Transit Survey (WTS) is a near-infrared transit survey running on the United Kingdom Infrared Telescope (UKIRT), designed to discover planets around M dwarfs. The WTS act…

astro-ph.IM2012★ 13 cited

Properties of ultra-cool dwarfs with Gaia. An assessment of the accuracy for the temperature determination

Luis M. Sarro, Angel Berihuete, Cesar Carrion +3

We aimed to assess the accuracy of the Gaia teff and logg estimates as derived with current models and observations. We assessed the validity of several inference techniques for de…

astro-ph.SR2012★ 36 cited

First T dwarfs in the VISTA Hemisphere Survey

N. Lodieu, B. Burningham, A. Day-Jones +21

The aim of the project is to improve our current knowledge of the density of T dwarfs and the shape of the substellar initial mass function by identifying a magnitude-limited sampl…

astro-ph.EP2012★ 26 cited

The first planet detected in the WTS: an inflated hot-Jupiter in a 3.35 day orbit around a late F-star

M. Cappetta, R. P. Saglia, J. L. Birkby +36

We report the discovery of WTS-1b, the first extrasolar planet found by the WFCAM Transit Survey, which began observations at the 3.8-m United Kingdom Infrared Telescope. Light cur…

astro-ph.SR2012★ 60 cited

Four ultra-short period eclipsing M-dwarf binaries in the WFCAM Transit Survey

S. V. Nefs, J. L. Birkby, I. A. G. Snellen +16

We report on the discovery of four ultra-short period (P<0.18 days) eclipsing M-dwarf binaries in the WFCAM Transit Survey. Their orbital periods are significantly shorter than of…

astro-ph.GA2011★ 119 cited

Overlapping abundance gradients and azimuthal gradients related to the spiral structure of the Galaxy

J. R. D. Lepine, P. Cruz, S. Scarano +6

The connection between some features of the metallicity gradient in the Galactic disk, best revealed by Open Clusters and Cepheids, and the spiral structure, is explored. The step-…

astro-ph2005★ 32 cited

Search for Planetary Candidates within the OGLE Stars

Adriana V. R. Silva, Patricia C. Cruz

We propose a method to distinguish between planetary and stellar companions to stars which present a periodic decrease in brightness, interpreted as a transit. Light curves from a…