867 citations · 5.9k across the 104 of their papers we have counts for
11 papers · 1 filter
Differential attenuation in star-forming galaxies at 0.3 1.5 in the SHARDS/CANDELS field
L. Rodríguez-Muñoz, G. Rodighiero, P. G. Pérez-González +21
We use a sample of 706 galaxies, selected as [OII]3727 ([OII]) emitters in the Survey for High- Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to stud…
Simulating infrared spectro-photometric surveys with a SPRITZ
L. Bisigello, C. Gruppioni, F. Calura +19
Mid- and far-infrared (IR) photometric and spectroscopic observations are fundamental to a full understanding of the dust-obscured Universe and the evolution of both star formation…
A Peculiar Type~II QSO Identified via Broad-band Detection of Extreme Nebular Line Emission
Yu-Heng Lin, Claudia Scarlata, Matthew Hayes +5
We present S82-20, an unusual redshift 3 object identified in SDSS-Stripe 82 broad-band images. The rest-frame ultraviolet spectrum of S82-20 shows emission lines from hig…
Deciphering stellar metallicities in the early Universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
Jorryt Matthee, Anna Feltre, Michael Maseda +8
Directly characterising the first generations of stars in distant galaxies is a key quest of observational cosmology. We present a case study of ID53 at z=4.77, the UV-brightest (b…
Chemical abundances in Seyfert galaxies -- VII. Direct abundance determination of neon based on optical and infrared emission lines
Mark Armah, O. L. Dors, C. P. Aydar +6
For the first time, neon abundance has been derived in the narrow line region from a sample of Seyfert~2 nuclei. In view of this, we compiled from the literature fluxes of optical…
Spectroscopy of an extreme [OIII] emitting active galactic nucleus at : implications for the reionisation era
Mengtao Tang, Daniel P. Stark, Richard S. Ellis +4
Reionisation-era galaxies often display intense nebular emission lines, both in rest-frame optical ([OIII]+H) and ultraviolet (UV; CIII], CIV). How such strong nebular emission…
Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at
K. B. Schmidt, J. Kerutt, L. Wisotzki +17
[Abbreviated] Rest-frame UV emission lines probe physical parameters of the emitting star-forming galaxies and their environments. The strongest main UV line, Ly, has been instr…
The role of SPICA-like missions and the Origins Space Telescope in the quest for heavily obscured AGN and synergies with Athena
L. Barchiesi, F. Pozzi, C. Vignali +21
In the BH-galaxy co-evolution framework, most of the star-formation (SF) and the black hole (BH) accretion is expected to take place in highly obscured conditions. Thus, obscured A…
Measuring the average molecular gas content of star-forming galaxies at
Leindert A. Boogaard, Rychard J. Bouwens, Dominik Riechers +15
We study the molecular gas content of 24 star-forming galaxies at , with a median stellar mass of M, from the MUSE Hubble Ultra Deep Field (HUDF) Survey…
The MUSE Extremely Deep Field: the Cosmic Web in Emission at High Redshift
Roland Bacon, David Mary, Thibault Garel +29
We report the discovery of diffuse extended Ly-alpha emission from redshift 3.1 to 4.5, tracing cosmic web filaments on scales of 2.5-4 comoving Mpc. These structures have been obs…
FirstLight IV: Diversity in sub-L galaxies at cosmic dawn
Daniel Ceverino, Michaela Hirschmann, Ralf Klessen +3
Using a large sample of sub-L galaxies, with similar UV magnitudes, M at , extracted from the FirstLight simulations, we show the diversity of ga…