187 citations · 537 across the 14 of their papers we have counts for
13 papers · 1 filter
Emission Line Galaxies in the SHARDS Hubble Frontier Fields II: Limits on Lyman-Continuum Escape Fractions of Lensed Emission Line Galaxies at Redshifts 2 < z < 3.5
Alex Griffiths, Christopher J. Conselice, Leonardo Ferreira +10
We present an investigation on escape fractions of UV photons from a unique sample of lensed low-mass emission line selected galaxies at z < 3.5 found in the SHARDS Hubble Frontier…
Identification of single spectral lines in large spectroscopic surveys using UMLAUT: an Unsupervised Machine Learning Algorithm based on Unbiased Topology
I. Baronchelli, C. M. Scarlata, L. Rodriguez-Muñoz +19
The identification of an emission line is unambiguous when multiple spectral features are clearly visible in the same spectrum. However, in many cases, only one line is detected, m…
Differences and similarities of stellar populations in LAEs and LBGs at 3.4 - 6.8
P. Arrabal Haro, J. M. Rodríguez Espinosa, C. Muñoz-Tuñón +6
The differences between the inherent stellar populations (SPs) of LAEs and LBGs are a key factor in understanding early galaxy formation and evolution. We have run a set of SP burs…
A panchromatic spatially-resolved analysis of nearby galaxies -- I. Sub-kpc scale Main Sequence in grand-design spirals
A. Enia, G. Rodighiero, L. Morselli +9
We analyse the spatially resolved relation between stellar mass (M) and star formation rate (SFR) in disk galaxies (i.e. the Main Sequence, MS). The studied sample includ…
ALMA reveals the molecular gas properties of 5 star-forming galaxies across the main sequence at 3 < z < 3.5
Paolo Cassata, Daizhong Liu, Brent Groves +17
We present the detection of CO(5-4) with S/N> 7 - 13 and a lower CO transition with S/N > 3 (CO(4-3) for 4 galaxies, and CO(3-2) for one) with ALMA in band 3 and 4 in five main seq…
The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
Michael Romano, P. Cassata, L. Morselli +31
We report the serendipitous discovery of a bright galaxy (Gal-A) observed as part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE). While this galaxy is detec…
The CANDELS/SHARDS multi-wavelength catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission line fluxes and Star Formation Rates
Guillermo Barro, Pablo G. Perez-Gonzalez, Antonio Cava +52
We present a WFC3 F160W (-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts and…
Inquiring into the nature of the Abell 2667 Brightest Cluster Galaxy: physical properties from MUSE
E. Iani, G. Rodighiero, J. Fritz +21
Based on HST and MUSE data, we probe the stellar and gas properties (i.e. kinematics, stellar mass, star formation rate) of the radio-loud brightest cluster galaxy (BCG) located at…
AGN in Dusty Starbursts at Z=2: Feedback Still To Kick In
G. Rodighiero, A. Enia, I. Delvecchio +18
We investigate a sample of 152 dusty sources at 1:5 < z < 2:5 to understand the connection of enhanced Star-Formation-Rate (SFR) and Black-Hole-Accretion-Rate (BHAR). The sources a…
Rejuvenated galaxies with very old bulges at the origin of the bending of the main sequence and of the "green valley"
Chiara Mancini, Emanuele Daddi, Stéphanie Juneau +11
We investigate the nature of star-forming galaxies with reduced specific star formation rate (sSFR) and high stellar masses, those `green valley' objects that seemingly cause a rep…
Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.20.9
L. Rodríguez-Muñoz, G. Rodighiero, C. Mancini +21
We quantify the star formation (SF) in the inner cores (/0.3) of 24 massive galaxy clusters at 0.20.9 observed by the …
Optically-faint massive Balmer Break Galaxies at z>3 in the CANDELS/GOODS fields
Belén Alcalde Pampliega, Pablo G. Pérez-González, Guillermo Barro +7
We present a sample of 33 Balmer Break Galaxies (BBGs) selected as HST/F160W dropouts in the deepest CANDELS/GOODS fields (~mag) but relatively bright in {\it Spitzer…
The AGN-Star Formation Connection: Future Prospects with JWST
Allison Kirkpatrick, Stacey Alberts, Alexandra Pope +12
The bulk of the stellar growth over cosmic time is dominated by IR luminous galaxies at cosmic noon (z=1-2), many of which harbor a hidden active galactic nucleus (AGN). We use sta…