activity
20182026
most citedCOSMOS2020: A panchromatic view of the Universe to from two complementary catalogs

485 citations · 1.1k across the 30 of their papers we have counts for

collaborators

29 papers

astro-ph.GA2026

The ASKAP-FLASH survey: A first look at the multiwavelength properties and redshift distribution of compact radio sources

W. Roster, E. M. Sadler, E. K. Mahony +15

We present the characterisation, including a photometric redshift (photo-) analysis, of the optical counterparts (CTPs) to over 45 000 bright ( 30 mJy) comp…

astro-ph.HE2024★ 6 cited

LensWatch. II. Improved Photometry and Time-delay Constraints on the Strongly Lensed Type Ia Supernova 2022qmx ("SN Zwicky") with HST Template Observations

Conor Larison, Justin D. R. Pierel, Max J. B. Newman +34

Strongly lensed supernovae (SNe) are a rare class of transient that can offer tight cosmological constraints that are complementary to methods from other astronomical events. We pr…

astro-ph.GA2023★ 1 cited

The LSST AGN Data Challenge: Selection methods

Đorđe V. Savić, Isidora Jankov, Weixiang Yu +12

Development of the Rubin Observatory Legacy Survey of Space and Time (LSST) includes a series of Data Challenges (DC) arranged by various LSST Scientific Collaborations (SC) that a…

astro-ph.HE2022★ 13 cited

Optical polarization and spectral properties of the H-poor superluminous supernovae SN 2021bnw and SN 2021fpl

F. Poidevin, C. M. B. Omand, Réka Könyves-Tóth +6

New optical photometric, spectrocopic and imaging polarimetry data are combined with publicly available data to study some of the physical properties of the two H-poor superluminou…

astro-ph.CO2022★ 31 cited

LensWatch: I. Resolved HST Observations and Constraints on the Strongly-Lensed Type Ia Supernova 2022qmx ("SN Zwicky")

J. D. R. Pierel, N. Arendse, S. Ertl +39

Supernovae (SNe) that have been multiply-imaged by gravitational lensing are rare and powerful probes for cosmology. Each detection is an opportunity to develop the critical tools…

astro-ph.CO2022★ 43 cited

SALT3-NIR: Taking the Open-Source Type Ia Supernova Model to Longer Wavelengths for Next-Generation Cosmological Measurements

J. D. R. Pierel, D. O. Jones, W. D. Kenworthy +32

A large fraction of Type Ia supernova (SN Ia) observations over the next decade will be in the near-infrared (NIR), at wavelengths beyond the reach of the current standard light-cu…

astro-ph.IM2022★ 3 cited

From Data to Software to Science with the Rubin Observatory LSST

Katelyn Breivik, Andrew J. Connolly, K. E. Saavik Ford +97

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) dataset will dramatically alter our understanding of the Universe, from the origins of the Solar System to the…

astro-ph.GA2022★ 8 cited

The star-formation rates of QSOs

M. Symeonidis, N. Maddox, M. J. Jarvis +13

We examine the far-IR properties of a sample of 5391 optically selected QSOs in the 0.5<z<2.65 redshift range down to log[nuLnu,2500 (erg/s)]>44.7, using SPIRE data from Herschel-A…

astro-ph.GA2022★ 2 cited

Comparison of the star formation of X-ray selected active galactic nuclei in eFEDS with star-forming galaxies

G. Mountrichas, V. Buat, G. Yang +5

We use X-ray Active Galactic Nuclei (AGN) in the eROSITA Final Equatorial-Depth Survey (eFEDS), that span over two orders of magnitude in X-ray luminosity, $\rm L_{X,2-…

astro-ph.HE2022★ 12 cited

Post maximum light and late time optical imaging polarimetry of type I superluminous supernova 2020znr

F. Poidevin, C. M. B. Omand, I. Pérez-Fournon +5

Optical imaging polarimetry was conducted on the hydrogen poor superluminous supernova 2020znr during 3 phases after maximum light (approximately +34 days, +288 days and +289 days)…

astro-ph.GA2021★ 485 cited

COSMOS2020: A panchromatic view of the Universe to from two complementary catalogs

J. R. Weaver, O. B. Kauffmann, O. Ilbert +54

The Cosmic Evolution Survey (COSMOS) has become a cornerstone of extragalactic astronomy. Since the last public catalog in 2015, a wealth of new imaging and spectroscopic data has…

astro-ph.SR2021

Progenitor and Close-In Circumstellar Medium of Type II Supernova 2020fqv from High-Cadence Photometry and Ultra-Rapid UV Spectroscopy

Samaporn Tinyanont, Ryan Ridden-Harper, Ryan Foley +35

We present observations of SN 2020fqv, a Virgo-cluster Type II core-collapse supernova (CCSN) with a high temporal resolution light curve from the Transiting Exoplanet Survey Satel…

astro-ph.GA2021

The Galaxy Evolution Probe

Jason Glenn, Charles M. Bradford, Erik Rosolowsky +21

The Galaxy Evolution Probe (GEP) is a concept for a mid- and far-infrared space observatory to measure key properties of large samples of galaxies with large and unbiased surveys.…

astro-ph.GA2021★ 11 cited

Getting ready for the LSST data -- estimating the physical properties of main sequence galaxies

Gabriele Riccio, Katarzyna Małek, Ambra Nanni +8

In this work we study how to employ the upcoming Legacy Survey of Space and Time (LSST) data to constrain physical properties of normal, star forming galaxies. We use simulated LSS…

astro-ph.GA2021★ 36 cited

The role of AGN and its obscuration on the position of the host galaxy relative to Main Sequence

G. Mountrichas, V. Buat, G. Yang +5

We use X-ray Active Galactic Nuclei (AGN) observed by the Chandra X-ray Observatory within the 9.3 deg Botes field of the NDWFS to study whether there is a correl…

astro-ph.GA2021★ 96 cited

HELP: The Herschel Extragalactic Legacy Project

R. Shirley, K. Duncan, M. C. Campos Varillas +29

We present the Herschel Extragalactic Legacy Project (HELP). This project collates, curates, homogenises, and creates derived data products for most of the premium multi-wavelength…

astro-ph.GA2021★ 19 cited

A hyperluminous obscured quasar at a redshift of z ~ 4.3

Andreas Efstathiou, Katarzyna Malek, Denis Burgarella +9

In this work we report the discovery of the hyperluminous galaxy HELP_J100156.75+022344.7 at the photometric redshift of z ~ 4.3. The galaxy was discovered in the Cosmological Evol…

astro-ph.GA2020★ 37 cited

A Spitzer survey of Deep Drilling Fields to be targeted by the Vera C. Rubin Observatory Legacy Survey of Space and Time

M. Lacy, J. A. Surace, D. Farrah +60

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will observe several Deep Drilling Fields (DDFs) to a greater depth and with a more rapid cadence than the main…

astro-ph.GA2020★ 36 cited

Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS

U. Dudzevičiūtė, I. Smail, A. M. Swinbank +16

We analyse the physical properties of 121 SNR 5 sub-millimetre galaxies (SMGs) from the STUDIES 450-m survey. We model their UV-to-radio spectral energy distributions usi…

physics.ao-ph2020★ 1 cited

An empirical, Bayesian approach to modelling the impact of weather on crop yield: maize in the US

Raphael Shirley, Edward Pope, Myles Bartlett +8

We apply an empirical, data-driven approach for describing crop yield as a function of monthly temperature and precipitation by employing generative probabilistic models with param…

astro-ph.GA2019★ 22 cited

Rest-frame UV Properties of Luminous Strong Gravitationally Lensed Ly Emitters from the BELLS GALLERY Survey

R. Marques-Chaves, I. Pérez-Fournon, Y. Shu +15

We present deep rest-frame UV spectroscopic observations using the Gran Telescopio Canarias of six gravitationally lensed Lya emitters (LAEs) at selected from the BEL…

astro-ph.GA2019★ 13 cited

The role of environment in galaxy evolution in the SERVS Survey I: density maps and cluster candidates

Nick Krefting, Anna Sajina, Mark Lacy +10

We use photometric redshifts derived from new -band through 4.5m Spitzer IRAC photometry in the 4.8\,deg of the XMM-LSS field to construct surface density maps in the red…

astro-ph.GA2019★ 37 cited

SCUBA-2 Ultra Deep Imaging Eao Survey (Studies) III: Multi-wavelength properties, luminosity functions and preliminary source catalog of 450-m-selected galaxies

Chen-Fatt Lim, Wei-Hao Wang, Ian Smail +35

We construct a SCUBA-2 450-m map in the COSMOS field that covers an area of 300 arcmin and reaches a 1 noise level of 0.65 mJy in the deepest region. We extract 256 sou…

astro-ph.GA2019★ 9 cited

Have we seen all the galaxies that comprise the cosmic infrared background at 250\,m 500\,m?

S. Duivenvoorden, S. Oliver, M. Bethermin +11

The cosmic infrared background (CIB) provides a fundamental observational constraint on the star-formation history of galaxies over cosmic history. We estimate the contribution to…