Search Publications

X-ray properties of z > 4 blazars
DOI: 10.1093/mnras/stz2340 Bibcode: 2019MNRAS.489.2732I

Moretti, A.; Ballo, L.; Dallacasa, D. +4 more

We present the X-ray analysis of the largest flux-limited complete sample of blazar candidates at z > 4 selected from the Cosmic Lens All Sky Survey (CLASS). After obtaining a nearly complete (24/25) X-ray coverage of the sample (from Swift-XRT, XMM-Newton, and Chandra), we analysed the spectra in order to identify the bona fide blazars. We cla…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 34
Accounting for multiplicity in calculating eta Earth
DOI: 10.1093/mnras/stz1246 Bibcode: 2019MNRAS.487..246Z

Zink, Jon K.; Hansen, Bradley M. S.

Using the updated exoplanet population parameters of our previous study, which includes the planetary radius updates from Gaia DR2 and an inferred multiplicity distribution, we provide a revised η calculation. This is achieved by sampling planets from our derived population model and determining which planets meet our criterion for hab…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 34
The stellar initial mass function of the solar neighbourhood revealed by Gaia
DOI: 10.1093/mnras/stz2093 Bibcode: 2019MNRAS.489.2377S

Sollima, A.

I use a sample of more than 120 000 stars in the solar neighbourhood, with parallaxes, magnitudes and colours estimated with unprecedented accuracy by the second data release of the Gaia mission, to derive the initial mass function of the Galactic disc. A full-forward technique is used to take into account, for the population of unresolved binarie…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 34
Expected intermediate-mass black holes in the Virgo cluster - II. Late-type galaxies
DOI: 10.1093/mnras/sty3068 Bibcode: 2019MNRAS.484..814G

Soria, Roberto; Graham, Alister W.; Davis, Benjamin L.

The Chandra X-ray Observatory's Cycle 18 Large Program titled `Spiral galaxies of the Virgo Cluster' will image 52 galaxies with the ACIS-S detector. Combined with archival data for an additional 22 galaxies, this will represent the complete sample of 74 spiral galaxies in the Virgo cluster with star formation rates ≳0.3 M yr-1

2019 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton eHST 34
The AGN fuelling/feedback cycle in nearby radio galaxies - II. Kinematics of the molecular gas
DOI: 10.1093/mnras/stz2368 Bibcode: 2019MNRAS.489.3739R

Davis, Timothy A.; Bureau, Martin; Casasola, Viviana +7 more

This is the second paper of a series exploring the multicomponent (stars, warm and cold gas, and radio jets) properties of a sample of 11 nearby low-excitation radio galaxies, with the aim of better understanding the active galactic nuclei (AGN) fuelling/feedback cycle in these objects. Here, we present a study of the molecular gas kinematics of s…

2019 Monthly Notices of the Royal Astronomical Society
eHST 34
An observational test for star formation prescriptions in cosmological hydrodynamical simulations
DOI: 10.1093/mnras/stz969 Bibcode: 2019MNRAS.486.1481B

Buck, Tobias; Dutton, Aaron A.; Macciò, Andrea V.

State-of-the-art cosmological hydrodynamical simulations of galaxy formation have reached the point at which their outcomes result in galaxies with ever more realism. Still, the employed sub-grid models include several free parameters such as the density threshold, n, to localize the star-forming gas. In this work, we investigate the possibilities…

2019 Monthly Notices of the Royal Astronomical Society
eHST 33
An extreme amplitude, massive heartbeat system in the LMC characterized using ASAS-SN and TESS
DOI: 10.1093/mnras/stz2460 Bibcode: 2019MNRAS.489.4705J

Kochanek, C. S.; Stanek, K. Z.; Thompson, Todd A. +3 more

Using ASAS-SN data, we find that the bright (V∼ 13.5 mag) variable star MACHO 80.7443.1718 (ASASSN-V J052624.38-684705.6) is the most extreme heartbeat star yet discovered. This massive binary, consisting of at least one early B-type star, has an orbital period of P_ASAS-SN=32.83627± 0.00846 d, and is located towards the LH58 OB complex in the LMC…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 33
New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South
DOI: 10.1093/mnras/sty2741 Bibcode: 2019MNRAS.482.1379H

Bouchy, F.; Queloz, D.; Hellier, Coel +16 more

We report the discovery of eight hot-Jupiter exoplanets from the WASP-South transit survey. WASP-144b has a mass of 0.44 MJup, a radius of 0.85 RJup, and is in a 2.27-d orbit around a V = 12.9, K2 star which shows a 21-d rotational modulation. WASP-145Ab is a 0.89 MJup planet in a 1.77-d orbit with a grazing transi…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 33
Deep multi-survey classification of variable stars
DOI: 10.1093/mnras/sty2836 Bibcode: 2019MNRAS.482.5078A

Becker, I.; Pichara, K.; Aguirre, C.

During the last decade, a considerable amount of effort has been made to classify variable stars using different machine-learning techniques. Typically, light curves are represented as vectors of statistical descriptors or features that are used to train various algorithms. These features demand high computational power and can last from hours to …

2019 Monthly Notices of the Royal Astronomical Society
CoRoT 33
A search for red giant solar-like oscillations in all Kepler data
DOI: 10.1093/mnras/stz622 Bibcode: 2019MNRAS.485.5616H

García, Rafael A.; Sharma, Sanjib; Stello, Dennis +4 more

The recently published Kepler mission Data Release 25 (DR25) reported on ∼197 000 targets observed during the mission. Despite this, no wide search for red giants showing solar-like oscillations have been made across all stars observed in Kepler's long-cadence mode. In this work, we perform this task using custom apertures on the Kepler pixel file…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 33