Search Publications

Chemo-kinematics of the Gaia RR Lyrae: the halo and the disc
DOI: 10.1093/mnras/stab005 Bibcode: 2021MNRAS.502.5686I

Belokurov, Vasily; Iorio, Giuliano

We present the results of a multicomponent kinematic model of a large sample of RR Lyrae detected by Gaia. By imposing a fourfold symmetry and employing Gaia proper motions, we are able to infer the behaviour of the velocity ellipsoid between ≈3 and ≈30 kpc from the centre of the Galaxy. We detect the presence of two distinct components: a dominan…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 85
The GALAH survey: effective temperature calibration from the InfraRed Flux Method in the Gaia system
DOI: 10.1093/mnras/stab2304 Bibcode: 2021MNRAS.507.2684C

Lewis, Geraint F.; Ting, Yuan-Sen; Casey, Andrew R. +23 more

In order to accurately determine stellar properties, knowledge of the effective temperature of stars is vital. We implement Gaia and 2MASS photometry in the InfraRed Flux Method and apply it to over 360 000 stars across different evolutionary stages in the GALAH DR3 survey. We derive colour-effective temperature relations that take into account th…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 81
HELP: the Herschel Extragalactic Legacy Project
DOI: 10.1093/mnras/stab1526 Bibcode: 2021MNRAS.507..129S

Aussel, H.; Shirley, R.; Buat, V. +29 more

We present the Herschel Extragalactic Legacy Project (HELP). This project collates, curates, homogenizes, and creates derived data products for most of the premium multiwavelength extragalactic data sets. The sky boundaries for the first data release cover 1270 deg2 defined by the Herschel SPIRE extragalactic survey fields; notably the …

2021 Monthly Notices of the Royal Astronomical Society
Herschel XMM-Newton eHST 81
Probing cosmic dawn: Ages and star formation histories of candidate z ≥ 9 galaxies
DOI: 10.1093/mnras/stab1239 Bibcode: 2021MNRAS.505.3336L

Chisholm, J.; Laporte, N.; Ellis, R. S. +3 more

We discuss the spectral energy distributions and physical properties of six galaxies whose photometric redshifts suggest they lie beyond a redshift z ≃ 9. Each was selected on account of a prominent excess seen in the Spitzer/IRAC 4.5 $\mu$m band which, for a redshift above z = 9.0, likely indicates the presence of a rest-frame Balmer break and a …

2021 Monthly Notices of the Royal Astronomical Society
eHST 80
The Global Meteor Network - Methodology and first results
DOI: 10.1093/mnras/stab2008 Bibcode: 2021MNRAS.506.5046V

Vida, Denis; Brown, Peter G.; Mazur, Michael J. +10 more

The Global Meteor Network (GMN) utilizes highly sensitive low-cost CMOS video cameras which run open-source meteor detection software on Raspberry Pi computers. Currently, over 450 GMN cameras in 30 countries are deployed. The main goal of the network is to provide long-term characterization of the radiants, flux, and size distribution of annual m…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 80
On the duration of the embedded phase of star formation
DOI: 10.1093/mnras/stab878 Bibcode: 2021MNRAS.504..487K

Kruijssen, J. M. Diederik; Leroy, Adam K.; Chevance, Mélanie +23 more

Feedback from massive stars plays a key role in molecular cloud evolution. After the onset of star formation, the young stellar population is exposed by photoionization, winds, supernovae, and radiation pressure from massive stars. Recent observations of nearby galaxies have provided the evolutionary timeline between molecular clouds and exposed y…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 77
Selecting accreted populations: metallicity, elemental abundances, and ages of the Gaia-Sausage-Enceladus and Sequoia populations
DOI: 10.1093/mnras/stab2614 Bibcode: 2021MNRAS.508.1489F

Feuillet, Diane K.; Casagrande, Luca; Feltzing, Sofia +1 more

Identifying stars found in the Milky Way as having formed in situ or accreted can be a complex and uncertain undertaking. We use Gaia kinematics and APOGEE elemental abundances to select stars belonging to the Gaia-Sausage-Enceladus (GSE) and Sequoia accretion events. These samples are used to characterize the GSE and Sequoia population metallicit…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 77
Dark Energy Survey year 3 results: point spread function modelling
DOI: 10.1093/mnras/staa3679 Bibcode: 2021MNRAS.501.1282J

Bechtol, K.; Smith, M.; Abbott, T. M. C. +79 more

We introduce a new software package for modelling the point spread function (PSF) of astronomical images, called PIFF (PSFs In the Full FOV), which we apply to the first three years (known as Y3) of the Dark Energy Survey (DES) data. We describe the relevant details about the algorithms used by PIFF to model the PSF, including how the PSF model va…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 76
A cool and inflated progenitor candidate for the Type Ib supernova 2019yvr at 2.6 yr before explosion
DOI: 10.1093/mnras/stab838 Bibcode: 2021MNRAS.504.2073K

Kilpatrick, Charles D.; Drout, Maria R.; Foley, Ryan J. +13 more

We present Hubble Space Telescope imaging of a pre-explosion counterpart to SN 2019yvr obtained 2.6 yr before its explosion as a type Ib supernova (SN Ib). Aligning to a post-explosion Gemini-S/GSAOI image, we demonstrate that there is a single source consistent with being the SN 2019yvr progenitor system, the second SN Ib progenitor candidate aft…

2021 Monthly Notices of the Royal Astronomical Society
eHST 76
Investigating the young AU Mic system with SPIRou: large-scale stellar magnetic field and close-in planet mass
DOI: 10.1093/mnras/staa3702 Bibcode: 2021MNRAS.502..188K

Gaidos, Eric; Doyon, René; Donati, Jean-François +12 more

We present a velocimetric and spectropolarimetric analysis of 27 observations of the 22-Myr M1 star AU Microscopii (AU Mic) collected with the high-resolution YJHK (0.98-2.35 µm) spectropolarimeter SPIRou from 2019 September 18 to November 14. Our radial velocity (RV) time-series exhibits activity-induced fluctuations of 45 m s-1

2021 Monthly Notices of the Royal Astronomical Society
Gaia 76