Search Publications

Transit timing variations, radial velocities, and long-term dynamical stability of the system Kepler-410
DOI: 10.1093/mnras/stz305 Bibcode: 2019MNRAS.484.4352G

Kabáth, Petr; Skarka, Marek; Šubjak, Ján +6 more

Transit timing variations (TTVs) of Kepler-410Ab were already reported in a few papers. Their semi-amplitude is about 14.5 min. In our previous paper, we found that the TTVs could be caused by the presence of a stellar companion in this system. Our main motivation for this paper was to investigate variation in a radial-velocity (RV) curve generate…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
Astroinformatics-based search for globular clusters in the Fornax Deep Survey
DOI: 10.1093/mnras/stz2801 Bibcode: 2019MNRAS.490.4080A

Paolillo, M.; Peletier, R.; Hilker, M. +15 more

In the last years, Astroinformatics has become a well-defined paradigm for many fields of Astronomy. In this work, we demonstrate the potential of a multidisciplinary approach to identify globular clusters (GCs) in the Fornax cluster of galaxies taking advantage of multiband photometry produced by the VLT Survey Telescope using automatic self-adap…

2019 Monthly Notices of the Royal Astronomical Society
eHST 4
Selection of M-dwarfs using Gaia, WISE, and 2MASS
DOI: 10.1093/mnras/stz2823 Bibcode: 2019MNRAS.490.4107B

Tinney, C. G.; Sharma, S.; Wright, D. +1 more

We present criteria for the selection of M-dwarfs down to G < 14.5 using all-sky survey data, with a view to identifying potential M-dwarfs, to be confirmed spectroscopically by the FunnelWeb survey. Two sets of criteria were developed. The first, based on absolute magnitude in the Gaia G passband, with MG > 7.7, selects 76,392 st…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
The loud and the quiet: searching for radio counterparts of two radio-weak BL Lac candidates with VLBI
DOI: 10.1093/mnrasl/sly184 Bibcode: 2019MNRAS.482L..34C

Frey, Sándor; Yang, Jun; An, Tao +4 more

BL Lac objects are known to have compact jets inclined to our line of sight at a small angle, showing prominent radio emission. Two radio-weak BL Lac candidates with no counterparts in current radio surveys were recently reported by Massaro et al. Both sources were selected as candidate low-energy counterparts of unassociated Fermi γ-ray sources. …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
HD 42659: the only known roAp star in a spectroscopic binary observed with B photometry, TESS, and SALT
DOI: 10.1093/mnras/stz2419 Bibcode: 2019MNRAS.489.4063H

Holdsworth, Daniel L.; Saio, Hideyuki; Kurtz, Donald W.

We present a multi-instrument analysis of the rapidly oscillating Ap (roAp) star HD 42659. We have obtained B photometric data for this star and use these data, in conjunction with the Transiting Exoplanet Survey Satellite (TESS) observations, to analyse the high-frequency pulsation in detail. We find a triplet that is split by the rotation freque…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
Post-rendezvous radar properties of comet 67P/CG from the Rosetta Mission: understanding future Earth-based radar observations and the dynamical evolution of comets
DOI: 10.1093/mnras/stz2174 Bibcode: 2019MNRAS.489.1667H

Kofman, Wlodek; Heggy, Essam; Palmer, Elizabeth M. +2 more

Radar observations provide crucial insights into the formation and dynamical evolution of comets. This ability is constrained by our knowledge of the dielectric and textural properties of these small-bodies. Using several observations by Rosetta as well as results from the Earth-based Arecibo radio telescope, we provide an updated and comprehensiv…

2019 Monthly Notices of the Royal Astronomical Society
Rosetta 4
2MASS J10274572+0629104: the very short period young M6 dwarf binary system identified in K2 data
DOI: 10.1093/mnras/stz1067 Bibcode: 2019MNRAS.486.4144P

Burgasser, A. J.; Gizis, J. E.; Paudel, R. R. +1 more

We report the identification of a very low mass new binary system 2MASS J10274572+0629104, based on Kepler K2 photometry and Gaia DR2 astrometry. It is located at a distance of 90.0 ± 2.9 pc. The K2 light curve is consistent with a beat pattern of two periodic signals, and using Lomb-Scargle periodogram, we find two rotation periods of 0.2114 ± 0.…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
Data-driven stellar parameters for southern TESS FGK targets
DOI: 10.1093/mnras/stz722 Bibcode: 2019MNRAS.486..251D

Henning, Th; Deacon, N. R.; Kossakowski, D. E.

We present stellar parameter estimates for 939 457 southern FGK stars that are candidate targets for the Transiting Exoplanet Survey Satellite (TESS) mission. Using a data-driven method similar to the CANNON, we build a model of stellar colours as a function of stellar parameters. We then use these in combination with stellar evolution models to e…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
A study of full space motions of outer Galactic disc A and F stars in two deep pencil beams
DOI: 10.1093/mnras/stz442 Bibcode: 2019MNRAS.485.2312H

Monguió, M.; Harris, A.; Drew, J. E.

A and F stars can be used as probes of outer Galactic disc kinematics: here we extend the work of Harris et al. by cross-matching their A/F sample with Gaia DR2 to bring in proper motions. These are combined with the already measured radial velocities and spectrophotometric distances to obtain full space motions. We use this sample of 1173 stars, …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
A revisit to the enigmatic variable star 21 Comae
DOI: 10.1093/mnras/stz413 Bibcode: 2019MNRAS.485.4247P

Kallinger, Thomas; Pribulla, Theodor; Walczak, Przemysław +12 more

The magnetic chemically peculiar (Ap/CP2) star 21 Com has been extensively studied in the past, albeit with widely differing and sometimes contradictory results, in particular concerning the occurrence of short-term variability between about 5 to 90 min. We have performed a new investigation of 21 Com using Microvariability and Oscillations of Sta…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4