papers

Publications (14)

astro-ph.GA2023

CEERS Key Paper VI: JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts

G. Yang, K. I. Caputi, C. Papovich +35

Mid-infrared observations are powerful in identifying heavily obscured Active Galactic Nuclei (AGN) which have weak emission in other wavelengths. Data from the Mid-Infrared Instru…

astro-ph.GA2018

Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field

R. J. McLure, J. S. Dunlop, F. Cullen +12

We present the results of a new study of the relationship between infrared excess (IRX), UV spectral slope (beta) and stellar mass at redshifts 2<z<3, based on a deep Atacama Large…

astro-ph.GA2025

HELM's deep: Highly Extincted Low-Mass galaxies seen by JWST

L. Bisigello, G. Gandolfi, A. Grazian +25

The dust content of star-forming galaxies is generally positively correlated with their stellar mass. However, some recent JWST studies have shown the existence of a population of…

astro-ph.GA2014

Dissecting the origin of the submillimeter emission in nearby galaxies with Herschel and LABOCA

M. Galametz, M. Albrecht, R. Kennicutt +17

We model the infrared to submillimeter spectral energy distribution of 11 nearby galaxies of the KINGFISH sample using Spitzer and Herschel data and compare model extrapolations at…

astro-ph.GA2016

VLA and ALMA Imaging of Intense, Galaxy-Wide Star Formation in z ~ 2 Galaxies

W. Rujopakarn, J. S. Dunlop, G. H. Rieke +30

We present 0-resolution extinction-independent distributions of star formation and dust in 11 star-forming galaxies (SFGs) at . These ga…

astro-ph.GA2024

ReveaLLAGN 0: First Look at JWST MIRI data of Sombrero and NGC 1052

K. Goold, A. Seth, M. Molina +28

We present the first results from the Revealing Low-Luminosity Active Galactic Nuclei (ReveaLLAGN) survey, a JWST survey of seven nearby LLAGN. We focus on two observations with th…

astro-ph.GA2020

Turbulent Gas in Lensed Planck-selected Starbursts at redshifts 1-3.5

Kevin C. Harrington, Axel Weiss, Min S. Yun +26

Dusty star-forming galaxies at high redshift (1 < z < 3) represent the most intense star-forming regions in the Universe. Key aspects to these processes are the gas heating and coo…

astro-ph.GA2016

A deep ALMA image of the Hubble Ultra Deep Field

J. S. Dunlop, R. J. McLure, A. D. Biggs +33

We present the results of the first, deep ALMA imaging covering the full 4.5 sq arcmin of the Hubble Ultra Deep Field (HUDF) as previously imaged with WFC3/IR on HST. Using a mosai…

astro-ph.GA2026

Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS

G. Gandolfi, G. Rodighiero, L. Bisigello +42

The James Webb Space Telescope (JWST) is revolutionizing our understanding of the Universe by unveiling faint, near-infrared dropouts previously beyond our reach, ranging from exce…

astro-ph.GA2023

UV-FIR SED modeling of AGN in IR-luminous galaxies up to z~2.5: Understanding the effects of torus models

Alyssa D. Sokol, M. Yun, A. Pope +2

UV-FIR SED modeling is an effective way to disentangle emission between star formation (SF) and active galactic nuclei (AGN) in galaxies; however, this approach becomes uncertain f…

astro-ph.GA2017

Spatially Resolved Dust, Gas, and Star Formation in the Dwarf Magellanic Irregular NGC4449

D. Calzetti, G. W. Wilson, B. T. Draine +17

We investigate the relation between gas and star formation in sub-galactic regions, ~360 pc to ~1.5 kpc in size, within the nearby starburst dwarf NGC4449, in order to separate the…

astro-ph.GA2016

Towards universal hybrid star formation rate estimators

M. Boquien, R. Kennicutt, D. Calzetti +13

To compute the SFR of galaxies from the rest-frame UV it is essential to take into account the obscuration by dust. To do so, one of the most popular methods consists in combining…

astro-ph.GA2024

ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields

E. Merlin, P. Santini, D. Paris +52

We present a set of photometric catalogs primarily aimed at providing the community with a comprehensive database for the study of galaxy populations in the high redshift Universe.…

astro-ph.IM2021

Great Observatories: The Past and Future of Panchromatic Astrophysics

L. Armus, S. T. Megeath, L. Corrales +30

NASA's Great Observatories have opened up the electromagnetic spectrum from space, providing sustained access to wavelengths not accessible from the ground. Together, Hubble, Compt…