Search Publications

Catalogues of active galactic nuclei from Gaia and unWISE data
DOI: 10.1093/mnras/stz2487 Bibcode: 2019MNRAS.489.4741S

McMahon, Richard G.; Belokurov, Vasily; Auger, Matthew W. +4 more

We present two catalogues of active galactic nucleus (AGN) candidates selected from the latest data of two all-sky surveys - Data Release 2 of the Gaia mission and the unWISE catalogue of the Wide-field Infrared Survey Explorer (WISE). We train a random forest classifier to predict the probability of each source in the Gaia-unWISE joint sample bei…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 56
Automated distant galaxy merger classifications from Space Telescope images using the Illustris simulation
DOI: 10.1093/mnras/stz1059 Bibcode: 2019MNRAS.486.3702S

Torrey, Paul; Rodriguez-Gomez, Vicente; Vogelsberger, Mark +5 more

We present image-based evolution of galaxy mergers from the Illustris cosmological simulation at 12 time-steps over 0.5 < z < 5. To do so, we created approximately one million synthetic deep Hubble Space Telescope and James Webb Space Telescope images and measured common morphological indicators. Using the merger tree, we assess methods to o…

2019 Monthly Notices of the Royal Astronomical Society
eHST 56
Gaia Data Release 2 catalogue of extremely low-mass white dwarf candidates
DOI: 10.1093/mnras/stz1876 Bibcode: 2019MNRAS.488.2892P

Pelisoli, Ingrid; Vos, Joris

Extremely low-mass white dwarf stars (ELMs) are M < 0.3 M helium-core white dwarfs born either as a result of a common-envelope phase or after a stable Roche lobe overflow episode in a multiple system. The Universe is not old enough for ELMs to have formed through single-star evolution channels. As remnants of binary evolution, ELMs…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 56
The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5
DOI: 10.1093/mnras/stz2693 Bibcode: 2019MNRAS.490.1451F

Smail, I.; Cristiani, S.; D'Odorico, V. +12 more

We present the goals, design, and first results of the MUSE Ultra Deep Field (MUDF) survey, a large programme using the Multi Unit Spectroscopic Explorer (MUSE) instrument at the ESO Very Large Telescope. The MUDF survey is collecting ≈150 h on-source of integral field optical spectroscopy in a 1.5 × 1.2 arcmin2 region which hosts sever…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 56
The AGN fuelling/feedback cycle in nearby radio galaxies I. ALMA observations and early results
DOI: 10.1093/mnras/stz255 Bibcode: 2019MNRAS.484.4239R

Davis, Timothy A.; Bureau, Martin; Mignano, Arturo +7 more

This is the first paper of a series exploring the multifrequency properties of a sample of 11 nearby low-excitation radio galaxies (LERGs) in the southern sky. We are conducting an extensive study of different galaxy components (stars, warm and cold gas, radio jets) with the aim of improving our understanding of the active galactic nucleus (AGN) f…

2019 Monthly Notices of the Royal Astronomical Society
eHST 56
Standard Galactic field RR Lyrae II: a Gaia DR2 calibration of the period-Wesenheit-metallicity relation
DOI: 10.1093/mnras/stz2814 Bibcode: 2019MNRAS.490.4254N

Madore, Barry F.; Freedman, Wendy L.; Sarajedini, Ata +9 more

RR Lyrae stars have long been popular standard candles, but significant advances in methodology and technology have been made in recent years to increase their precision as distance indicators. We present multiwavelength (optical UBVRcIc and Gaia G, BP, RP; near-infrared JHKs; mid-infrared [3.6], [4.5]) period-lumi…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 55
Evident black hole-bulge coevolution in the distant universe
DOI: 10.1093/mnras/stz611 Bibcode: 2019MNRAS.485.3721Y

Alexander, D. M.; Brandt, W. N.; Yang, G. +4 more

Observations in the local universe show a tight correlation between the masses of supermassive black holes (SMBHs; MBH) and host-galaxy bulges (Mbulge), suggesting a strong connection between SMBH and bulge growth. However, direct evidence for such a connection in the distant universe remains elusive. We have studied sample-a…

2019 Monthly Notices of the Royal Astronomical Society
eHST 55
Binary asteroseismic modelling: isochrone-cloud methodology and application to Kepler gravity mode pulsators
DOI: 10.1093/mnras/sty2671 Bibcode: 2019MNRAS.482.1231J

Aerts, C.; Pápics, P. I.; Bowman, D. M. +5 more

The simultaneous presence of variability due to both pulsations and binarity is no rare phenomenon. Unfortunately, the complexities of dealing with even one of these sources of variability individually means that the other signal is often treated as a nuisance and discarded. However, both types of variability offer means to probe fundamental stell…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 55
H α morphologies of star clusters: a LEGUS study of H II region evolution time-scales and stochasticity in low-mass clusters
DOI: 10.1093/mnras/stz2820 Bibcode: 2019MNRAS.490.4648H

Herrero, A.; Cignoni, M.; Calzetti, D. +25 more

The morphology of H II regions around young star clusters provides insight into the time-scales and physical processes that clear a cluster's natal gas. We study ∼700 young clusters (≤10 Myr) in three nearby spiral galaxies (NGC 7793, NGC 4395, and NGC 1313) using Hubble Space Telescope (HST) imaging from LEGUS (Legacy ExtraGalactic Ultraviolet Su…

2019 Monthly Notices of the Royal Astronomical Society
eHST 55
Quasar and galaxy classification in Gaia Data Release 2
DOI: 10.1093/mnras/stz2947 Bibcode: 2019MNRAS.490.5615B

Fouesneau, Morgan; Bailer-Jones, Coryn A. L.; Andrae, Rene

We construct a supervised classifier based on Gaussian Mixture Models to probabilistically classify objects in Gaia data release 2 (GDR2) using only photometric and astrometric data in that release. The model is trained empirically to classify objects into three classes - star, quasar, galaxy - for G ≥ 14.5 mag down to the Gaia magnitude limit of …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 54