Search Publications

Cosmological constraints from DES Y1 cluster abundances and SPT multiwavelength data
DOI: 10.1103/PhysRevD.103.043522 Bibcode: 2021PhRvD.103d3522C

Bacon, D.; Smith, M.; Abbott, T. M. C. +89 more

We perform a joint analysis of the counts of redMaPPer clusters selected from the Dark Energy Survey (DES) year 1 data and multiwavelength follow-up data collected within the 2500 deg2 South Pole Telescope (SPT) Sunyaev-Zel'dovich (SZ) survey. The SPT follow-up data, calibrating the richness-mass relation of the optically selected redMa…

2021 Physical Review D
eHST 89
Stellar chromospheric activity of 1674 FGK stars from the AMBRE-HARPS sample. I. A catalogue of homogeneous chromospheric activity
DOI: 10.1051/0004-6361/202039765 Bibcode: 2021A&A...646A..77G

Recio-Blanco, A.; de Laverny, P.; Monteiro, M. J. P. F. G. +9 more


Aims: The main objective of this project is to characterise chromospheric activity of FGK stars from the HARPS archive. We start, in this first paper, by presenting a catalogue of homogeneously determined chromospheric emission (CE), stellar atmospheric parameters, and ages for 1674 FGK main sequence (MS), subgiant, and giant stars. The analy…

2021 Astronomy and Astrophysics
Gaia 88
Evidence of a population of dark subhaloes from Gaia and Pan-STARRS observations of the GD-1 stream
DOI: 10.1093/mnras/stab210 Bibcode: 2021MNRAS.502.2364B

Bovy, Jo; Erkal, Denis; Bertone, Gianfranco +2 more

New data from the Gaia satellite, when combined with accurate photometry from the Pan-STARRS survey, allow us to accurately estimate the properties of the GD-1 stream. Here, we analyse the stellar density variations in the GD-1 stream and show that they cannot be due to known baryonic structures such as giant molecular clouds, globular clusters, o…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 88
Stars with Photometrically Young Gaia Luminosities Around the Solar System (SPYGLASS). I. Mapping Young Stellar Structures and Their Star Formation Histories
DOI: 10.3847/1538-4357/ac0251 Bibcode: 2021ApJ...917...23K

Rizzuto, Aaron C.; Kraus, Adam L.; Offner, Stella S. R. +1 more

Young stellar associations hold a star formation record that can persist for millions of years, revealing the progression of star formation long after the dispersal of the natal cloud. To identify nearby young stellar populations that trace this progression, we have designed a comprehensive framework for the identification of young stars and use i…

2021 The Astrophysical Journal
Gaia 88
Evidence for GN-z11 as a luminous galaxy at redshift 10.957
DOI: 10.1038/s41550-020-01275-y Bibcode: 2021NatAs...5..256J

Ho, Luis C.; Fan, Xiaohui; Jiang, Linhua +9 more

GN-z11 was photometrically selected as a luminous star-forming galaxy candidate at redshift z > 10 on the basis of Hubble Space Telescope imaging data1. Follow-up Hubble Space Telescope near-infrared grism observations detected a continuum break that was explained as the Lyα break corresponding to z =11.0 9−0.12+0.08<…

2021 Nature Astronomy
eHST 87
Internal calibration of Gaia BP/RP low-resolution spectra
DOI: 10.1051/0004-6361/202141249 Bibcode: 2021A&A...652A..86C

Jordi, C.; Evans, D. W.; van Leeuwen, F. +6 more

Context. The full third Gaia data release will provide, for the first time, the calibrated spectra obtained with the blue and red Gaia slitless spectrophotometers (BP and RP, respectively). Gaia is a very complex mission and cannot be considered as a single instrument, but rather as many instruments. The two lines of sight with wide fields of view…

2021 Astronomy and Astrophysics
Gaia 87
Detection of the LMC-induced sloshing of the Galactic halo
DOI: 10.1093/mnras/stab1828 Bibcode: 2021MNRAS.506.2677E

Bird, Sarah A.; Zhao, Gang; Erkal, Denis +8 more

A wealth of recent studies have shown that the LMC is likely massive, with a halo mass >1011 M. One consequence of having such a nearby and massive neighbour is that the inner Milky Way is expected to be accelerated with respect to our Galaxy's outskirts (beyond ~30 kpc). In this work, we compile a sample of ~500 stars wi…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 87
A High-resolution View of Fast Radio Burst Host Environments
DOI: 10.3847/1538-4357/abff56 Bibcode: 2021ApJ...917...75M

Kilpatrick, Charles D.; Simha, Sunil; Prochaska, J. Xavier +12 more

We present Hubble Space Telescope ultraviolet and infrared observations of eight fast radio burst (FRB) host galaxies with subarcsecond localizations, including the hosts of three known repeating FRBs. We quantify their spatial distributions and locations with respect to their host galaxy light distributions, finding that they occur at moderate ho…

2021 The Astrophysical Journal
eHST 87
FINK, a new generation of broker for the LSST community
DOI: 10.1093/mnras/staa3602 Bibcode: 2021MNRAS.501.3272M

Karpov, Sergey; Savchenko, Volodymyr; Coleiro, Alexis +33 more

FINK is a broker designed to enable science with large time-domain alert streams such as the one from the upcoming Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST). It exhibits traditional astronomy broker features such as automatized ingestion, annotation, selection, and redistribution of promising alerts for transient science. It…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 86
Statistics of 700 Individually Studied W UMa Stars
DOI: 10.3847/1538-4365/abeb23 Bibcode: 2021ApJS..254...10L

Lazarević, Sanja; Latković, Olivera; Čeki, Atila

We present a statistical study of the largest bibliographic compilation of stellar and orbital parameters of W UMa stars derived by light-curve synthesis with Roche models. The compilation includes nearly 700 individually investigated objects from over 450 distinct publications. Almost 70% of this sample is comprised of stars observed in the past …

2021 The Astrophysical Journal Supplement Series
Gaia 86