Search Publications

unWISE Coadds: The Five-year Data Set
DOI: 10.1088/1538-3873/ab3df4 Bibcode: 2019PASP..131l4504M

Lang, D.; Schlafly, E. F.; Meisner, A. M. +1 more

We present full-sky coadded maps created by uniformly combining the first five years of Wide-field Infrared Survey Explorer (WISE) and NEOWISE imaging at 3.4 µm (W1) and 4.6 µm (W2). By incorporating both pre-hibernation WISE exposures from 2010 to 2011 and the first four years (2013-2017) of post-hibernation exposures from the NEOWISE…

2019 Publications of the Astronomical Society of the Pacific
Gaia 56
The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5
DOI: 10.1093/mnras/stz2693 Bibcode: 2019MNRAS.490.1451F

Smail, I.; Cristiani, S.; D'Odorico, V. +12 more

We present the goals, design, and first results of the MUSE Ultra Deep Field (MUDF) survey, a large programme using the Multi Unit Spectroscopic Explorer (MUSE) instrument at the ESO Very Large Telescope. The MUDF survey is collecting ≈150 h on-source of integral field optical spectroscopy in a 1.5 × 1.2 arcmin2 region which hosts sever…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 56
The AGN fuelling/feedback cycle in nearby radio galaxies I. ALMA observations and early results
DOI: 10.1093/mnras/stz255 Bibcode: 2019MNRAS.484.4239R

Davis, Timothy A.; Bureau, Martin; Mignano, Arturo +7 more

This is the first paper of a series exploring the multifrequency properties of a sample of 11 nearby low-excitation radio galaxies (LERGs) in the southern sky. We are conducting an extensive study of different galaxy components (stars, warm and cold gas, radio jets) with the aim of improving our understanding of the active galactic nucleus (AGN) f…

2019 Monthly Notices of the Royal Astronomical Society
eHST 56
Evidence for Sub-Chandrasekhar Type Ia Supernovae from Stellar Abundances in Dwarf Galaxies
DOI: 10.3847/1538-4357/ab2c02 Bibcode: 2019ApJ...881...45K

Kovalev, Mikhail; McWilliam, Andrew; Shen, Ken J. +6 more

There is no consensus on the progenitors of Type Ia supernovae (SNe Ia) despite their importance for cosmology and chemical evolution. We address this question using our previously published catalogs of Mg, Si, Ca, Cr, Fe, Co, and Ni abundances in dwarf galaxy satellites of the Milky Way (MW) to constrain the mass at which the white dwarf (WD) exp…

2019 The Astrophysical Journal
Gaia 56
The RWST, a comprehensive statistical description of the non-Gaussian structures in the ISM
DOI: 10.1051/0004-6361/201834975 Bibcode: 2019A&A...629A.115A

Boulanger, F.; Levrier, F.; Zhang, S. +5 more

The interstellar medium (ISM) is a complex nonlinear system governed by the interplay between gravity and magneto-hydrodynamics, as well as radiative, thermodynamical, and chemical processes. Our understanding of it mostly progresses through observations and numerical simulations, and a quantitative comparison between these two approaches requires…

2019 Astronomy and Astrophysics
Herschel 56
Transiting exocomets detected in broadband light by TESS in the β Pictoris system
DOI: 10.1051/0004-6361/201935552 Bibcode: 2019A&A...625L..13Z

Zwintz, K.; Kennedy, G. M.; Zieba, S. +1 more


Aims: We search for signs of falling evaporating bodies (FEBs, also known as exocomets) in photometric time series obtained for β Pictoris after fitting and removing its δ Scuti-type pulsation frequencies.
Methods: Using photometric data obtained by the TESS satellite we determined the pulsational properties of the exoplanet host star β …

2019 Astronomy and Astrophysics
Gaia 56
Environmental impacts on molecular gas in protocluster galaxies at z ∼ 2
DOI: 10.1093/pasj/psz005 Bibcode: 2019PASJ...71...40T

Tamura, Yoichi; Kohno, Kotaro; Suzuki, Tomoko L. +12 more

We present the results from ALMA CO(3-2) observations of 66 Hα-selected galaxies in three protoclusters around radio galaxies: PKS 1138-262 (z = 2.16), USS 1558-003 (z = 2.53), and 4C 23.56 (z = 2.49). The pointing areas have an overdensity of ∼100 compared to the mean surface number density of galaxies in field environments. We detect the CO emis…

2019 Publications of the Astronomical Society of Japan
eHST 55
The local and distant Universe: stellar ages and H0
DOI: 10.1088/1475-7516/2019/03/043 Bibcode: 2019JCAP...03..043J

Verde, Licia; Jimenez, Raul; Cimatti, Andrea +2 more

The ages of the oldest stellar objects in our galaxy provide an independent test of the current cosmological model as they give a lower limit to the age of the Universe. Recent accurate parallaxes by the Gaia space mission, accurate measurements of the metallicity of stars, via individual elemental abundances, and advances in the modelling of stel…

2019 Journal of Cosmology and Astroparticle Physics
Gaia 55
Standard Galactic field RR Lyrae II: a Gaia DR2 calibration of the period-Wesenheit-metallicity relation
DOI: 10.1093/mnras/stz2814 Bibcode: 2019MNRAS.490.4254N

Madore, Barry F.; Freedman, Wendy L.; Sarajedini, Ata +9 more

RR Lyrae stars have long been popular standard candles, but significant advances in methodology and technology have been made in recent years to increase their precision as distance indicators. We present multiwavelength (optical UBVRcIc and Gaia G, BP, RP; near-infrared JHKs; mid-infrared [3.6], [4.5]) period-lumi…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 55
Solar Chromospheric Temperature Diagnostics: A Joint ALMA-Hα Analysis
DOI: 10.3847/1538-4357/ab2ba3 Bibcode: 2019ApJ...881...99M

Cranmer, Steven R.; Reardon, Kevin P.; Uitenbroek, Han +4 more

We present the first high-resolution, simultaneous observations of the solar chromosphere in the optical and millimeter wavelength ranges, obtained with the Atacama Large Millimeter Array (ALMA) and the Interferometric Bidimensional Spectrometer at the Dunn Solar Telescope. In this paper we concentrate on the comparison between the brightness temp…

2019 The Astrophysical Journal
IRIS 55