Search Publications

Cosmic evolution of low-excitation radio galaxies in the LOFAR two-metre sky survey deep fields
DOI: 10.1093/mnras/stac1128 Bibcode: 2022MNRAS.513.3742K

Calistro Rivera, Gabriela; Małek, Katarzyna; Wang, Lingyu +16 more

Feedback from low-excitation radio galaxies (LERGs) plays a key role in the lifecycle of massive galaxies in the local Universe; their evolution, and the impact of these active galactic nuclei on early galaxy evolution, however, remain poorly understood. We use a sample of 10 481 LERGs from the first data release of the LOFAR two-metre Sky Survey …

2022 Monthly Notices of the Royal Astronomical Society
Herschel 40
The Pristine survey - XVI. The metallicity of 26 stellar streams around the Milky Way detected with the STREAMFINDER in Gaia EDR3
DOI: 10.1093/mnras/stac2426 Bibcode: 2022MNRAS.516.5331M

Sestito, Federico; McConnachie, Alan W.; Malhan, Khyati +21 more

We use the photometric metallicities provided by the panoramic Pristine survey to study the veracity and derive the metallicities of the numerous stellar streams found by the application of the STREAMFINDER algorithm to the Gaia Early Data Release 3 data. All 26 streams present in Pristine show a clear metallicity distribution function, which prov…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 40
First discoveries and localizations of Fast Radio Bursts with MeerTRAP: real-time, commensal MeerKAT survey
DOI: 10.1093/mnras/stac1450 Bibcode: 2022MNRAS.514.1961R

Prochaska, J. Xavier; Kramer, M.; Tejos, N. +24 more

We report on the discovery and localization of fast radio bursts (FRBs) from the MeerTRAP project, a commensal fast radio transient-detection programme at MeerKAT in South Africa. Our hybrid approach combines a coherent search with an average field-of-view (FoV) of 0.4 $\rm deg^{2}$ with an incoherent search utilizing a FoV of ~1.27 $\rm deg^{2}$ …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 39
Comprehensive catalogue of the overall best distances and properties of 402 galactic novae
DOI: 10.1093/mnras/stac2900 Bibcode: 2022MNRAS.517.6150S

Schaefer, Bradley E.

I derive the overall best distances for all 402 known Galactic novae, and I collect their many properties. The centrepiece is the 74 novae with accurate parallaxes from the new Gaia data release. For the needed priors, I have collected 171 distances based on old methods (including expansion parallaxes and extinction distances). Further, I have col…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 39
WISDOM Project - X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure
DOI: 10.1093/mnras/stac600 Bibcode: 2022MNRAS.512.1522D

Kruijssen, J. M. Diederik; Schruba, Andreas; Williams, Thomas G. +12 more

We use high-resolution maps of the molecular interstellar medium (ISM) in the centres of 86 nearby galaxies from the millimetre-Wave Interferometric Survey of Dark Object Masses (WISDOM) and Physics at High Angular Resolution in Nearby GalaxieS (PHANGS) surveys to investigate the physical mechanisms setting the morphology of the ISM at molecular c…

2022 Monthly Notices of the Royal Astronomical Society
eHST 39
Polycyclic aromatic hydrocarbons in Seyfert and star-forming galaxies
DOI: 10.1093/mnras/stab3127 Bibcode: 2022MNRAS.509.4256G

Rigopoulou, D.; Pereira-Santaella, M.; Alonso-Herrero, A. +3 more

Polycyclic Aromatic Hydrocarbons (PAHs) are carbon-based molecules resulting from the union of aromatic rings and related species, which are likely responsible for strong infrared emission features. In this work, using a sample of 50 Seyfert galaxies (DL < 100 Mpc) we compare the circumnuclear (inner kpc) PAH emission of AGN to that …

2022 Monthly Notices of the Royal Astronomical Society
AKARI ISO 39
Mysterious odd radio circle near the large magellanic cloud - an intergalactic supernova remnant?
DOI: 10.1093/mnras/stac210 Bibcode: 2022MNRAS.512..265F

Haberl, F.; Umana, G.; Hill, T. +48 more

We report the discovery of J0624-6948, a low-surface brightness radio ring, lying between the Galactic Plane and the large magellanic cloud (LMC). It was first detected at 888 MHz with the Australian Square Kilometre Array Pathfinder (ASKAP), and with a diameter of ~196 arcsec. This source has phenomenological similarities to odd radio circles (OR…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 39
MIGHTEE: the nature of the radio-loud AGN population
DOI: 10.1093/mnras/stac2140 Bibcode: 2022MNRAS.516..245W

Prandoni, I.; Bowler, R. A. A.; Marchetti, L. +24 more

We study the nature of the faint radio source population detected in the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Early Science data in the COSMOS field, focusing on the properties of the radio-loud active galactic nuclei (AGNs). Using the extensive multiwavelength data available in the field, we are able to classify 88…

2022 Monthly Notices of the Royal Astronomical Society
Herschel eHST 38
Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey II: measurements in Fourier space with optimal weights
DOI: 10.1093/mnras/stac812 Bibcode: 2022MNRAS.514.3396M

Brownstein, Joel R.; Palanque-Delabrouille, Nathalie; Schneider, Donald P. +12 more

We present measurements of the local primordial non-Gaussianity parameter $f_{\mathrm{NL}}^\mathrm{local} $from the clustering of 343 708 quasars with redshifts 0.8 < z < 2.2 distributed over 4808 deg2 from the final data release (DR16) of the extended Baryon Acoustic Oscillation Spectroscopic Survey (eBOSS), the largest volume sp…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 38
The GALAH Survey: dependence of elemental abundances on age and metallicity for stars in the Galactic disc
DOI: 10.1093/mnras/stab3341 Bibcode: 2022MNRAS.510..734S

Lewis, Geraint F.; Buder, Sven; Lind, Karin +25 more

Using data from the GALAH survey, we explore the dependence of elemental abundances on stellar age and metallicity among Galactic disc stars. We find that the abundance of most elements can be predicted from age and [Fe/H] with an intrinsic scatter of about 0.03 dex. We discuss the possible causes for the existence of the abundance-age-metallicity…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 37