Search Publications

PSFGAN: a generative adversarial network system for separating quasar point sources and host galaxy light
DOI: 10.1093/mnras/sty764 Bibcode: 2018MNRAS.477.2513S

Stark, Dominic; Launet, Barthelemy; Schawinski, Kevin +7 more

The study of unobscured active galactic nuclei (AGN) and quasars depends on the reliable decomposition of the light from the AGN point source and the extended host galaxy light. The problem is typically approached using parametric fitting routines using separate models for the host galaxy and the point spread function (PSF). We present a new appro…

2018 Monthly Notices of the Royal Astronomical Society
eHST 15
Jets, arcs, and shocks: NGC 5195 at radio wavelengths
DOI: 10.1093/mnras/sty390 Bibcode: 2018MNRAS.476.2876R

Muxlow, T. W. B.; Argo, M. K.; Williams, D. R. A. +10 more

We studied the nearby, interacting galaxy NGC 5195 (M 51b) in the radio, optical and X-ray bands. We mapped the extended, low-surface-brightness features of its radio-continuum emission; determined the energy content of its complex structure of shock-ionized gas; constrained the current activity level of its supermassive nuclear black hole. In par…

2018 Monthly Notices of the Royal Astronomical Society
eHST 15
The origin of the LMC stellar bar: clues from the SFH of the bar and inner disc
DOI: 10.1093/mnrasl/slx158 Bibcode: 2018MNRAS.473L..16M

Stetson, P. B.; Monelli, M.; Gallart, C. +2 more

We discuss the origin of the Large Magellanic Cloud (LMC) stellar bar by comparing the star formation histories (SFHs) obtained from deep colour-magnitude diagrams (CMDs) in the bar and in a number of fields in different directions within the inner disc. The CMDs, reaching the oldest main-sequence turn-offs in these very crowded fields, have been …

2018 Monthly Notices of the Royal Astronomical Society
Gaia eHST 15
Polarization of seven MBM clouds at high Galactic latitude
DOI: 10.1093/mnras/sty485 Bibcode: 2018MNRAS.476.4442N

Neha, S.; Soam, A.; Maheswar, G. +1 more

We made R-band polarization measurements of 234 stars towards the direction of the MBM 33-39 cloud complex. The distance of the MBM 33-39 complex was determined as 120 ± 10 pc using polarization results and near-infrared photometry from the 2MASS survey. The magnetic field geometry of the individual clouds inferred from our polarimetric results re…

2018 Monthly Notices of the Royal Astronomical Society
AKARI Planck 15
Gaian bottlenecks and planetary habitability maintained by evolving model biospheres: the ExoGaia model
DOI: 10.1093/mnras/sty658 Bibcode: 2018MNRAS.477..727N

Nicholson, Arwen E.; Wilkinson, David M.; Williams, Hywel T. P. +1 more

The search for habitable exoplanets inspires the question - how do habitable planets form? Planet habitability models traditionally focus on abiotic processes and neglect a biotic response to changing conditions on an inhabited planet. The Gaia hypothesis postulates that life influences the Earth's feedback mechanisms to form a self-regulating sys…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 15
Polarization light curve modelling of corotating interaction regions in the wind of the Wolf-Rayet star WR 6
DOI: 10.1093/mnras/stx2813 Bibcode: 2018MNRAS.474.1886S

Ignace, Richard; St-Louis, N.; Tremblay, Patrick

The intriguing WN4b star WR 6 has been known to display epoch-dependent spectroscopic, photometric and polarimetric variability for several decades. In this paper, we set out to verify if a simplified analytical model in which corotating interaction regions (CIRs) threading an otherwise spherical wind is able to reproduce the many broad-band conti…

2018 Monthly Notices of the Royal Astronomical Society
IUE 15
A chemical study of M67 candidate blue stragglers and evolved blue stragglers observed with APOGEE DR14
DOI: 10.1093/mnras/sty2147 Bibcode: 2018MNRAS.480.4314B

Grebel, Eva K.; Pasquali, Anna; Caffau, Elisabetta +1 more

Within the variety of objects populating stellar clusters, blue straggler stars (BSSs) are among the most puzzling ones. BSSs are commonly found in globular clusters, but they are also known to populate open clusters of the Milky Way. Two main theoretical scenarios (collisions and mass transfer) have been suggested to explain their formation, alth…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 15
A census of radio-selected AGNs on the COSMOS field and of their FIR properties
DOI: 10.1093/mnras/stx2424 Bibcode: 2018MNRAS.473.2493M

Popesso, P.; Salvato, M.; Brusa, M. +1 more

We use the new catalogue by Laigle et al. to provide a full census of VLA-COSMOS radio sources. We identify 90 per cent of such sources and sub-divide them into active galactic nuclei (AGNs) and star-forming galaxies on the basis of their radio luminosity. The AGN sample is complete with respect to radio selection at all z ≲ 3.5. Out of 704 AGNs, …

2018 Monthly Notices of the Royal Astronomical Society
Herschel 15
Mid-UV studies of the transitional millisecond pulsars XSS J12270-4859 and PSR J1023+0038 during their radio pulsar states
DOI: 10.1093/mnras/sty291 Bibcode: 2018MNRAS.476.1086R

Altamirano, D.; Degenaar, N.; Wijnands, R. +7 more

We report mid-UV (MUV) observations taken with Hubble Space Telescope (HST)/WFC3, Swift/UVOT, and GALEX/NUV of the transitional millisecond pulsars XSS J12270-4859 and PSR J1023+0038 during their radio pulsar states. Both systems were detected in our images and showed MUV variability. At similar orbital phases, the MUV luminosities of both pulsars…

2018 Monthly Notices of the Royal Astronomical Society
eHST 15
HATS-39b, HATS-40b, HATS-41b, and HATS-42b: three inflated hot Jupiters and a super-Jupiter transiting F stars
DOI: 10.1093/mnras/sty726 Bibcode: 2018MNRAS.477.3406B

Henning, T.; Mancini, L.; Rabus, M. +22 more

We report the discovery of four transiting hot Jupiters from the HATSouth survey: HATS-39b, HATS-40b, HATS-41b, and HATS-42b. These discoveries add to the growing number of transiting planets orbiting moderately bright (12.5 ≲ V ≲ 13.7) F dwarf stars on short (2-5 d) periods. The planets have similar radii, ranging from 1.33^{+0.29}_{-0.20} R

2018 Monthly Notices of the Royal Astronomical Society
Gaia 15