100 citations · 204 across the 6 of their papers we have counts for
6 papers
The Rich JWST Spectrum of the Western Nucleus of Arp 220: Shocked Hot Core Chemistry Dominates the Inner Disk
Victorine Buiten, Paul van der Werf, Serena Viti +20
We present full 3-28 JWST MIRI/MRS and NIRSpec/IFU spectra of the western nucleus of Arp 220, the nearest ultraluminous infrared galaxy. This nucleus has long been su…
MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field
Göran Östlin, Pablo G. Pérez-González, Jens Melinder +41
The recently launched James Webb Space Telescope (JWST) is opening new observing windows on the distant universe. Among JWST's instruments, the Mid Infrared Instrument (MIRI) offer…
Early-type massive stars in Carina Nebula within the Gaia-ESO Survey
S. R. Berlanas, A. Herrero, F. Martins +4
The Gaia-ESO Survey (GES) is obtaining high quality spectra of 10 stars in our Galaxy, providing an homogeneous and unique overview of all the main components of the Mi…
On the LINER nuclear obscuration, Compton-thickness and the existence of the dusty torus; Clues from Spitzer/IRS spectra
O. Gonzalez-Martin, J. Masegosa, I. Marquez +7
Most of the optically classified low ionisation narrow emission-line regions (LINERs) nuclei host an active galactic nuclei (AGN). However, how they fit into the unified model (UM)…
Why X-ray--Selected AGN Appear Optically Dull
J. R. Rigby, G. H. Rieke, J. L. Donley +2
We investigate why half of X-ray--selected active galactic nuclei (AGN) in deep surveys lack signs of accretion in their optical spectra. The majority of these ``optically--dull''…
Why Optically--Faint AGN Are Faint: The Spitzer Perspective
J. R. Rigby, G. H. Rieke, P. G. Perez-Gonzalez +5
Optically--faint X-ray sources (those with f_X/f_R > 10) constitute about 20% of X-ray sources in deep surveys, and are potentially highly obscured and/or at high redshift. Their f…