Search Publications

Dust Attenuation Curves in the Local Universe: Demographics and New Laws for Star-forming Galaxies and High-redshift Analogs
DOI: 10.3847/1538-4357/aabf3c Bibcode: 2018ApJ...859...11S

Boquien, Médéric; Salim, Samir; Lee, Janice C.

We study the dust attenuation curves of 230,000 individual galaxies in the local universe, ranging from quiescent to intensely star-forming systems, using GALEX, SDSS, and WISE photometry calibrated on the Herschel ATLAS. We use a new method of constraining SED fits with infrared luminosity (SED+LIR fitting), and parameterized attenuation curves d…

2018 The Astrophysical Journal
Herschel 464
ATLASGAL - properties of a complete sample of Galactic clumps
DOI: 10.1093/mnras/stx2258 Bibcode: 2018MNRAS.473.1059U

König, C.; Menten, K. M.; Smith, M. D. +15 more

The APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) is an unbiased 870 µm submillimetre survey of the inner Galactic plane (|ℓ| < 60° with |b| < 1.5°). It is the largest and most sensitive ground-based submillimetre wavelength Galactic survey to date and has provided a large and systematic inventory of all massive, dense clum…

2018 Monthly Notices of the Royal Astronomical Society
Herschel 284
GOODS-ALMA: 1.1 mm galaxy survey. I. Source catalog and optically dark galaxies
DOI: 10.1051/0004-6361/201832928 Bibcode: 2018A&A...620A.152F

Magnelli, B.; Daddi, E.; Elbaz, D. +36 more


Aims: We present a 69 arcmin2 ALMA survey at 1.1 mm, GOODS-ALMA, matching the deepest HST-WFC3 H-band part of the GOODS-South field.
Methods: We tapered the 0″24 original image with a homogeneous and circular synthesized beam of 0″60 to reduce the number of independent beams - thus reducing the number of purely statistical spu…

2018 Astronomy and Astrophysics
Gaia Herschel eHST 210
Galaxy growth in a massive halo in the first billion years of cosmic history
DOI: 10.1038/nature24629 Bibcode: 2018Natur.553...51M

Bayliss, M. B.; Béthermin, M.; Murphy, E. J. +34 more

According to the current understanding of cosmic structure formation, the precursors of the most massive structures in the Universe began to form shortly after the Big Bang, in regions corresponding to the largest fluctuations in the cosmic density field. Observing these structures during their period of active growth and assembly—the first few hu…

2018 Nature
Herschel eHST 205
Dust temperature and mid-to-total infrared color distributions for star-forming galaxies at 0 < z < 4
DOI: 10.1051/0004-6361/201731506 Bibcode: 2018A&A...609A..30S

Elbaz, D.; Franco, M.; Ciesla, L. +3 more

We present a new, publicly available library of dust spectral energy distributions (SEDs). These SEDs are characterized by only three parameters: the dust mass (Mdust), the dust temperature (Tdust), and the mid-to-total infrared color (IR8 ≡ LIR/L8). The latter measures the relative contribution of polyc…

2018 Astronomy and Astrophysics
Herschel eHST 204
The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-redshift Galaxies
DOI: 10.3847/1538-4357/aaa3e7 Bibcode: 2018ApJ...853...56R

van Dokkum, Pieter G.; Illingworth, Garth D.; Labbé, Ivo +13 more

We use a newly assembled sample of 3545 star-forming galaxies with secure spectroscopic, grism, and photometric redshifts at z = 1.5-2.5 to constrain the relationship between UV slope (β) and dust attenuation (L IR/L UV ≡ IRX). Our sample significantly extends the range of L UV and β probed in previous UV-selected …

2018 The Astrophysical Journal
Herschel eHST 200
A massive core for a cluster of galaxies at a redshift of 4.3
DOI: 10.1038/s41586-018-0025-2 Bibcode: 2018Natur.556..469M

Béthermin, M.; Murphy, E. J.; Greve, T. R. +35 more

Massive galaxy clusters have been found that date to times as early as three billion years after the Big Bang, containing stars that formed at even earlier epochs1-3. The high-redshift progenitors of these galaxy clusters—termed `protoclusters'—can be identified in cosmological simulations that have the highest overdensities (greater-th…

2018 Nature
Herschel 188
Starbursts in and out of the star-formation main sequence
DOI: 10.1051/0004-6361/201732370 Bibcode: 2018A&A...616A.110E

Daddi, E.; Elbaz, D.; Franco, M. +13 more


Aims: We use high-resolution continuum images obtained with the Atacama Large Millimeter Array (ALMA) to probe the surface density of star formation in z ~ 2 galaxies and study the different physical properties between galaxies within and above the star-formation main sequence of galaxies.
Methods: We use ALMA images at 870 µm with…

2018 Astronomy and Astrophysics
AKARI Herschel eHST 166
“Super-deblended” Dust Emission in Galaxies. II. Far-IR to (Sub)millimeter Photometry and High-redshift Galaxy Candidates in the Full COSMOS Field
DOI: 10.3847/1538-4357/aad4af Bibcode: 2018ApJ...864...56J

Calabrò, Antonello; Dickinson, Mark; Daddi, Emanuele +17 more

We present a “super-deblended” far-infrared (FIR) to (sub)millimeter photometric catalog in the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by Liu et al., with key adaptations. We obtain point-spread function fitting photometry at fixed prior positions including 88,008 galaxies detected in VLA 1.4, 3 GHz, and/or M…

2018 The Astrophysical Journal
Herschel 156
The VLA Nascent Disk and Multiplicity Survey of Perseus Protostars (VANDAM). IV. Free-Free Emission from Protostars: Links to Infrared Properties, Outflow Tracers, and Protostellar Disk Masses
DOI: 10.3847/1538-4365/aaceae Bibcode: 2018ApJS..238...19T

Dunham, Michael M.; Kratter, Kaitlin M.; Li, Zhi-Yun +11 more

Emission from protostars at centimeter radio wavelengths has been shown to trace the free-free emission arising from ionizing shocks as a result of jets and outflows driven by protostars. Therefore, measuring properties of protostars at radio frequencies can provide valuable insights into the nature of their outflows and jets. We present a C-band …

2018 The Astrophysical Journal Supplement Series
Herschel XMM-Newton 144