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Dust emission from the bulk of galaxies at the Epoch of Reionization
L. Ciesla, S. Adscheid, B. Magnelli +6
[Abridged] Our view of dust in primordial galaxies is limited towards a few tens of z~7 galaxies, pre-selected from UV-optical observations, and are thus not necessarily representa…
NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at in the COSMOS field
Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis +41
The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at in six deep fields. We report spectroscopic confirmation of eight g…
ACOSMOS: Measuring the cosmic dust-attenuated star formation rate density at
Benjamin Magnelli, Sylvia Adscheid, Tsan-Ming Wang +14
[Abridged] In recent years, conflicting results have provided an uncertain view of the dust-attenuated properties of star-forming galaxies (SFGs). To solve this, we used the…
Overcoming Confusion Noise with Hyperspectral Imaging from PRIMAger
James M. S. Donnellan, Seb J. Oliver, Matthieu Bethermin +11
The PRobe far-Infrared Mission for Astrophysics (PRIMA) concept aims to perform mapping with spectral coverage and sensitivities inaccessible to previous FIR space telescopes. PRIM…
Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
L. Bisigello, C. Gruppioni, A. Bolatto +11
The most active phases of star formation and black hole accretion are strongly affected by dust extinction, making far-infrared (far-IR) observations the best way to disentangle an…
Confusion of extragalactic sources in the far infrared: a baseline assessment of the performance of PRIMAger in intensity and polarization
Matthieu Béthermin, Alberto D. Bolatto, François Boulanger +11
Because of their limited angular resolution, far-infrared telescopes are usually affected by confusion phenomenon. Since several galaxies can be located in the same instrumental be…