Search Publications

The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release
DOI: 10.1093/mnras/stab510 Bibcode: 2021MNRAS.503.1149Z

Kneib, Jean-Paul; Zhao, Gong-Bo; Rossi, Graziano +18 more

We produce 1000 realizations of synthetic clustering catalogues for each type of the tracers used for the baryon acoustic oscillation and redshift space distortion analysis of the Sloan Digital Sky Surveys-IV extended Baryon Oscillation Spectroscopic Survey final data release (eBOSS DR16), covering the redshift range from 0.6 to 2.2, to provide re…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 107
Revisiting the Integrated Star Formation Law. II. Starbursts and the Combined Global Schmidt Law
DOI: 10.3847/1538-4357/abd3a2 Bibcode: 2021ApJ...908...61K

Kennicutt, Robert C., Jr.; De Los Reyes, Mithi A. C.

We compile observations of molecular gas contents and infrared-based star formation rates (SFRs) for 112 circumnuclear star-forming regions, in order to reinvestigate the form of the disk-averaged Schmidt surface density star-formation law in starbursts. We then combine these results with total gas and SFR surface densities for 153 nearby nonstarb…

2021 The Astrophysical Journal
Herschel 107
The HETDEX Instrumentation: Hobby-Eberly Telescope Wide-field Upgrade and VIRUS
DOI: 10.3847/1538-3881/ac2c02 Bibcode: 2021AJ....162..298H

Schneider, Donald P.; Marshall, J. L.; Janowiecki, Steven +46 more

The Hobby-Eberly Telescope (HET) Dark Energy Experiment (HETDEX) is undertaking a blind wide-field low-resolution spectroscopic survey of 540 deg2 of sky to identify and derive redshifts for a million Lyα-emitting galaxies in the redshift range 1.9 < z < 3.5. The ultimate goal is to measure the expansion rate of the universe at th…

2021 The Astronomical Journal
Gaia 107
Cloud-cloud collisions and triggered star formation
DOI: 10.1093/pasj/psaa103 Bibcode: 2021PASJ...73S...1F

Inoue, Tsuyoshi; Tachihara, Kengo; Fukui, Yasuo +2 more

Star formation is a fundamental process for galactic evolution. One issue over the last several decades has been determining whether star formation is induced by external triggers or self-regulated in a closed system. The role of an external trigger, which can effectively collect mass in a small volume, has attracted particular attention in connec…

2021 Publications of the Astronomical Society of Japan
Herschel eHST 106
Galactic spiral structure revealed by Gaia EDR3
DOI: 10.1051/0004-6361/202140687 Bibcode: 2021A&A...651A.104P

Marshall, D. J.; Fouesneau, M.; Andrae, R. +14 more

Using the astrometry and integrated photometry from the Gaia Early Data Release 3, we map the density variations in the distribution of young upper main sequence (UMS) stars, open clusters, and classical Cepheids in the Galactic disc within several kiloparsecs of the Sun. We derive maps of relative over- and under-dense regions for UMS stars in th…

2021 Astronomy and Astrophysics
Gaia 106
All-sky dynamical response of the Galactic halo to the Large Magellanic Cloud
DOI: 10.1038/s41586-021-03385-7 Bibcode: 2021Natur.592..534C

Conroy, Charlie; Johnson, Benjamin D.; Naidu, Rohan P. +4 more

Gravitational interactions between the Large Magellanic Cloud (LMC) and the stellar and dark matter halo of the Milky Way are expected to give rise to disequilibrium phenomena in the outer Milky Way1-7. A local wake is predicted to trail the orbit of the LMC, and a large-scale overdensity is predicted to exist across a large area of the…

2021 Nature
Gaia 106
Deep Search for Decaying Dark Matter with XMM-Newton Blank-Sky Observations
DOI: 10.1103/PhysRevLett.127.051101 Bibcode: 2021PhRvL.127e1101F

Safdi, Benjamin R.; Foster, Joshua W.; Kongsore, Marius +4 more

Sterile neutrinos with masses in the keV range are well-motivated extensions to the Standard Model that could explain the observed neutrino masses while also making up the dark matter (DM) of the universe. If sterile neutrinos are DM then they may slowly decay into active neutrinos and photons, giving rise to the possibility of their detection thr…

2021 Physical Review Letters
XMM-Newton 106
Constraining velocity-dependent self-interacting dark matter with the Milky Way's dwarf spheroidal galaxies
DOI: 10.1093/mnras/stab506 Bibcode: 2021MNRAS.503..920C

Correa, Camila A.

The observed anticorrelation between the central dark matter (DM) densities of the bright Milky Way (MW) dwarf spheroidal galaxies (dSphs) and their orbital pericentre distances poses a potential signature of self-interacting dark matter (SIDM). In this work, we investigate this possibility by analysing the range of SIDM scattering cross-section p…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 106
Gaia Early Data Release 3. Gaia photometric science alerts
DOI: 10.1051/0004-6361/202140735 Bibcode: 2021A&A...652A..76H

Prusti, T.; Gilmore, G.; Smith, M. D. +108 more

Context. Since July 2014, the Gaia mission has been engaged in a high-spatial-resolution, time-resolved, precise, accurate astrometric, and photometric survey of the entire sky.
Aims: We present the Gaia Science Alerts project, which has been in operation since 1 June 2016. We describe the system which has been developed to enable the discove…

2021 Astronomy and Astrophysics
Gaia 105
ASASSN-14ko is a Periodic Nuclear Transient in ESO 253-G003
DOI: 10.3847/1538-4357/abe38d Bibcode: 2021ApJ...910..125P

Holoien, Thomas W. -S.; Vallely, Patrick J.; Auchettl, Katie +24 more

We present the discovery that ASASSN-14ko is a periodically flaring active galactic nucleus at the center of the galaxy ESO 253-G003. At the time of its discovery by the All-Sky Automated Survey for Supernovae (ASAS-SN), it was classified as a supernova close to the nucleus. The subsequent 6 yr of V- and g-band ASAS-SN observations revealed that A…

2021 The Astrophysical Journal
XMM-Newton 105