Search Publications

Identifying RR Lyrae Variable Stars in Six Years of the Dark Energy Survey
DOI: 10.3847/1538-4357/abe873 Bibcode: 2021ApJ...911..109S

Bacon, D.; Bechtol, K.; Smith, M. +67 more

We present a search for RR Lyrae stars using the full six-year data set from the Dark Energy Survey covering ∼5000 deg2 of the southern sky. Using a multistage multivariate classification and light-curve template-fitting scheme, we identify RR Lyrae candidates with a median of 35 observations per candidate. We detect 6971 RR Lyrae candi…

2021 The Astrophysical Journal
Gaia 30
White dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 16
DOI: 10.1093/mnras/stab2411 Bibcode: 2021MNRAS.507.4646K

Kepler, S. O.; Pelisoli, Ingrid; Romero, Alejandra D. +2 more

White dwarfs are the end state of the evolution of more than 97 per cent of all stars, and therefore carry information on the structure and evolution of the Galaxy through their luminosity function and initial-to-final mass relation. Examining the new spectra of all white or blue stars in the Sloan Digital Sky Survey Data Release 16, we report the…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 30
The pristine dwarf-galaxy survey - III. Revealing the nature of the Milky Way globular cluster Sagittarius II
DOI: 10.1093/mnras/stab604 Bibcode: 2021MNRAS.503.2754L

McConnachie, Alan W.; Navarro, Julio F.; Martin, Nicolas +13 more

We present a new spectroscopic study of the faint Milky Way satellite Sagittarius II. Using multiobject spectroscopy from the Fibre Large Array Multi-Element Spectrograph, we supplement the data set of Longeard et al. with 47 newly observed stars, 19 of which are identified as members of the satellite. These additional member stars are used to put…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 30
Modelling a multi-spacecraft coronal mass ejection encounter with EUHFORIA
DOI: 10.1051/0004-6361/202140315 Bibcode: 2021A&A...652A..27A

Palmerio, E.; Temmer, M.; Poedts, S. +6 more

Context. Coronal mass ejections (CMEs) are a manifestation of the Sun's eruptive nature. They can have a great impact on Earth, but also on human activity in space and on the ground. Therefore, modelling their evolution as they propagate through interplanetary space is essential.
Aims: EUropean Heliospheric FORecasting Information Asset (EUHF…

2021 Astronomy and Astrophysics
SOHO VenusExpress 30
Shock Induced Strong Substorms and Super Substorms: Preconditions and Associated Oxygen Ion Dynamics
DOI: 10.1007/s11214-021-00806-x Bibcode: 2021SSRv..217...33Z

Zong, Q. -G.; Fu, S. -Y.; Yue, C.

It is well known that the interaction between interplanetary (IP) shocks and the Earth's magnetosphere would generate/excite various types of geomagnetic phenomena. Progresses have been made on the Earth's magnetospheric response to solar wind forcing in recent years in the aspects associated with magnetospheric substorms. Strong substorms and sup…

2021 Space Science Reviews
Cluster DoubleStar 30
Connecting X-ray nuclear winds with galaxy-scale ionised outflows in two z ∼ 1.5 lensed quasars
DOI: 10.1051/0004-6361/202040190 Bibcode: 2021A&A...648A..99T

Marconi, A.; Vignali, C.; Comastri, A. +15 more


Aims: Outflows driven by active galactic nuclei (AGN) are expected to have a significant impact on host galaxy evolution, but the matter of how they are accelerated and propagated on galaxy-wide scales is still under debate. This work addresses these questions by studying the link between X-ray, nuclear ultra-fast outflows (UFOs), and extende…

2021 Astronomy and Astrophysics
eHST 30
Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS
DOI: 10.1093/mnras/staa3285 Bibcode: 2021MNRAS.500..942D

Scott, D.; Shirley, R.; Smail, Ian +16 more

We analyse the physical properties of 121 SNR ≥ 5 sub-millimetre galaxies (SMGs) from the STUDIES 450 µm survey. We model their UV-to-radio spectral energy distributions using MAGPHYS+photo-z and compare the results to similar modelling of 850 µm-selected SMG sample from AS2UDS, to understand the fundamental physical differences betwee…

2021 Monthly Notices of the Royal Astronomical Society
Herschel 30
Overdensities of submillimetre-bright sources around candidate protocluster cores selected from the South Pole Telescope survey
DOI: 10.1093/mnras/stab2800 Bibcode: 2021MNRAS.508.3754W

Greve, Thomas R.; Phadke, Kedar A.; Aravena, Manuel +21 more

We present APEX-LABOCA 870-µm observations of the fields surrounding the nine brightest high-redshift unlensed objects discovered in the South Pole Telescope's (SPT) 2500 deg2 survey. Initially seen as point sources by SPT's 1-arcmin beam, the 19-arcsec resolution of our new data enables us to deblend these objects and search for …

2021 Monthly Notices of the Royal Astronomical Society
Herschel 30
Abundances of neutron-capture elements in thin- and thick-disc stars in the solar neighbourhood
DOI: 10.1051/0004-6361/202039979 Bibcode: 2021A&A...649A.126T

Tautvaišienė, G.; Drazdauskas, A.; Mikolaitis, Š. +4 more


Aims: The aim of this work is to determine abundances of neutron-capture elements for thin- and thick-disc F, G, and K stars in several selected sky fields near the north ecliptic pole and to compare the results with the Galactic chemical evolution models, to explore elemental gradients according to stellar ages, mean galactocentric distances…

2021 Astronomy and Astrophysics
Gaia 30
The Astrophysical Distance Scale. III. Distance to the Local Group Galaxy WLM Using Multiwavelength Observations of the Tip of the Red Giant Branch, Cepheids, and JAGB Stars
DOI: 10.3847/1538-4357/abd253 Bibcode: 2021ApJ...907..112L

Madore, Barry F.; Freedman, Wendy L.; Lee, Abigail J. +3 more

The local determination of the Hubble constant sits at a crossroad. Current estimates of the local expansion rate of the universe differ by about 1.7σ, derived from the Cepheid- and TRGB-based calibrations, applied to Type Ia supernovae. To help elucidate possible sources of systematic error causing the tension, we show in this study the recently …

2021 The Astrophysical Journal
eHST 30