Search Publications

The LOFAR Two-metre Sky Survey: Deep Fields data release 1. V. Survey description, source classifications, and host galaxy properties
DOI: 10.1093/mnras/stad1308 Bibcode: 2023MNRAS.523.1729B

Bondi, M.; Prandoni, I.; Małek, K. +26 more

Source classifications, stellar masses, and star-formation rates are presented for ≈80 000 radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey (LoTSS) Deep Fields, which represents the widest deep radio survey ever undertaken. Using deep multi-wavelength data spanning from the ultraviolet to the far-infrared, …

2023 Monthly Notices of the Royal Astronomical Society
Herschel 66
ALMA confirmation of an obscured hyperluminous radio-loud AGN at z = 6.853 associated with a dusty starburst in the 1.5 deg2 COSMOS field
DOI: 10.1093/mnras/stad266 Bibcode: 2023MNRAS.520.4609E

Fan, Xiaohui; Stark, Daniel P.; Endsley, Ryan +7 more

We present band 6 ALMA observations of a heavily obscured radio-loud (L1.4 GHz = 1025.4 W Hz-1) active galactic nucleus (AGN) candidate at zphot = 6.83 ± 0.06 found in the 1.5 deg2 COSMOS field. The ALMA data reveal detections of exceptionally strong [C II]158 $\mu$m (z[C II] = 6.85…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 56
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions - XV. Steady accretion from global collapse to core feeding in massive hub-filament system SDC335
DOI: 10.1093/mnras/stad012 Bibcode: 2023MNRAS.520.3259X

Zhang, Yong; Tej, Anandmayee; Soam, Archana +37 more

We present ALMA Band-3/7 observations towards 'the Heart' of a massive hub-filament system (HFS) SDC335, to investigate its fragmentation and accretion. At a resolution of ~0.03 pc, 3 mm continuum emission resolves two massive dense cores MM1 and MM2, with $383(^{\scriptscriptstyle +234}_{\scriptscriptstyle -120})$ M (10-24 % mass of '…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 43
An empirical study of dust properties at the earliest epochs
DOI: 10.1093/mnras/stad1470 Bibcode: 2023MNRAS.523.3119W

Maiolino, Roberto; Jones, Gareth C.; Smit, Renske +2 more

We present an empirical analysis of the properties of dust-continuum emission in a sample of 17 galaxies in the early Universe (4 < z < 8) with well-sampled far-infrared spectral energy distributions (SEDs) compiled from the literature. We place our results into context by self-consistently comparing to samples of nearby star-forming galaxie…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 33
The ALMA REBELS Survey: the first infrared luminosity function measurement at z ∼ 7
DOI: 10.1093/mnras/stad1259 Bibcode: 2023MNRAS.522.3926B

Inami, H.; Schneider, R.; Oesch, P. A. +18 more

We present the first observational infrared luminosity function (IRLF) measurement in the Epoch of Reionization (EoR) based on a ultraviolet (UV)-selected galaxy sample with the Atacama Large Millimeter Array (ALMA) spectroscopic observations. Our analysis is based on the ALMA large program Reionization Era Bright Emission Line Survey (REBELS), wh…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 29
Spatially resolved dust properties and quasar-galaxy decomposition of a hyper-luminous infrared galaxy at z = 4.4
DOI: 10.1093/mnras/stad1464 Bibcode: 2023MNRAS.523.4654T

Krumholz, Mark R.; Wisnioski, Emily; Tsukui, Takafumi +1 more

We report spatially resolved dust properties of the quasar host galaxy BRI1335-0417 at redshift z = 4.4 constrained by the Atacama Large Millimetre/submillimetre Array observations. The dust temperature map, derived from a greybody fit to rest frame 90 and 161 µm continuum images, shows a steep increase towards the centre, reaching 57.1 ± 0.…

2023 Monthly Notices of the Royal Astronomical Society
Gaia Herschel eHST 25
The bright extragalactic ALMA redshift survey (BEARS) - II. Millimetre photometry of gravitational lens candidates
DOI: 10.1093/mnras/stac3771 Bibcode: 2023MNRAS.522.2995B

Berta, S.; Andreani, P.; Pérez-Fournon, I. +49 more

We present 101- and 151-GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500-µm flux densities >80 mJy and 250-500-µm colours consistent with z > 2, most of which are expected to be gravitationally lensed or hyperluminous infrared galaxies. Approximately half of the Herschel 500-µm sourc…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 24
The LOFAR Two-metre Sky Survey: the radio view of the cosmic star formation history
DOI: 10.1093/mnras/stad1602 Bibcode: 2023MNRAS.523.6082C

Prandoni, I.; Hardcastle, M. J.; Röttgering, H. J. A. +9 more

We present a detailed study of the cosmic star formation history over 90 per cent of cosmic time (0 ≲ z ≲ 4), using deep, radio continuum observations that probe star formation activity independent of dust. The Low Frequency Array Two Metre Sky Survey has imaged three well-studied extragalactic fields, Elais-N1, Boötes, and the Lockman Hole, reach…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 23
Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
DOI: 10.1093/mnras/stad1147 Bibcode: 2023MNRAS.522.3092L

Kauffmann, Guinevere; Naab, Thorsten; Lahén, Natalia +6 more

We present new GRIFFIN project hydrodynamical simulations that model the formation of galactic star cluster populations in low-metallicity (Z = 0.00021) dwarf galaxies, including radiation, supernova, and stellar wind feedback of individual massive stars. In the simulations, stars are sampled from the stellar initial mass function (IMF) down to th…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 23
Bright extragalactic ALMA redshift survey (BEARS) III: detailed study of emission lines from 71 Herschel targets
DOI: 10.1093/mnras/stad784 Bibcode: 2023MNRAS.521.5508H

Berta, S.; Ivison, R. J.; Omont, A. +55 more

We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies between redshifts 1.4 and 4.6 detected by the Atacama Large Millimeter/submillimeter Array. These lines include a total of 156 CO, [C I], and H2O emission lines. For 46 galaxies, we detect two transitions of CO lines, and for these galaxies we fin…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 21