most citedPRIMA: PRIMAger, a far-infrared hyperspectral and polarimetric instrument

7 citations · 8 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2025

PRIMA General Observer Science Book Volume 2

A. Moullet, D. Burgarella, T. Kataria +8

The PRobe far-Infrared Mission for Astrophysics (PRIMA) mission concept is a proposed mission to NASA's Astrophysics Probe Explorer (APEX) call. The concept features a cryogenicall…

astro-ph.GA2025

PRIMAger General Observer programs: a {\Large }-sr Infrared Survey and other General Observer wide-field programs

Denis Burgarella, Matthieu Bethermin, Alessandro Boselli +5

The PRobe far-Infrared Mission for Astrophysics (PRIMA) is a cryogenically-cooled, far-infrared (far-IR) observatory expected to begin serving the astronomical community by early 2…

astro-ph.GA2025

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies

Carlotta Gruppioni, Lee Armus, Matthieu Bethermin +10

One of the main open issues in galaxy formation and evolution is the early assembly of the most massive galaxies and their contribution to the stellar mass and star formation rate…

astro-ph.IM20257 cited

PRIMA: PRIMAger, a far-infrared hyperspectral and polarimetric instrument

Laure Ciesla, Charles Darren Dowell, Marc Sauvage +27

The PRobe far-Infrared Mission for Astrophysics (PRIMA) is an infrared observatory for the next decade, currently in Phase A, with a 1.8m telescope actively cooled to 4.5K. On boar…

astro-ph.GA2025

Very bright, very blue, and very red: JWST CAPERS analysis of highly luminous galaxies with extreme UV slopes at

Callum T. Donnan, Mark Dickinson, Anthony J. Taylor +37

We present JWST/NIRSpec PRISM observations of three luminous () galaxies at observed with the CAPERS Cycle 3 program. These galaxies exhibit extreme UV sl…

astro-ph.GA2025

Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities

Nikko J. Cleri, Grace M. Olivier, Bren E. Backhaus +24

High-redshift observations from JWST indicate that optical strong line ratios do not carry the same constraining power as they do at low redshifts. Critically, this prevents a sepa…