Publications (19)
The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel
P. Popesso, A. Biviano, G. Rodighiero +40
Star formation in massive galaxies is quenched at some point during hierarchical mass assembly. To understand where and when the quenching processes takes place, we study the evolu…
Dust attenuation in z 1 galaxies from Herschel and 3D-HST H measurements
A. Puglisi, G. Rodighiero, A. Franceschini +12
We combined the spectroscopic information from the 3D-HST survey with \textit{Herschel} data to characterize the H dust attenuation properties of a sample of 79 main sequence s…
A high redshift population of galaxies at the North Ecliptic Pole: unveiling the main sequence of dusty galaxies
L. Barrufet, C. Pearson, S. Serjeant +16
Dusty high-z galaxies are extreme objects with high star formation rates (SFRs) and luminosities. Characterising the properties of this population and analysing their evolution ove…
The lesser role of starbursts for star formation at z=2
G. Rodighiero, E. Daddi, I. Baronchelli +31
Two main modes of star formation are know to control the growth of galaxies: a relatively steady one in disk-like galaxies, defining a tight star formation rate (SFR)-stellar mass…
The Spitzer-IRAC/MIPS Extragalactic Survey (SIMES): II enhanced nuclear accretion rate in galaxy groups at z0.2
I. Baronchelli, G. Rodighiero, H. I. Teplitz +22
For a sample of star forming galaxies in the redshift interval 0.15z0.3, we study how both the relative strength of the AGN infra-red emission, compared to that due to the st…
Co-evolution of black hole accretion and star formation in galaxies up to z=3.5
R. Carraro, G. Rodighiero, P. Cassata +15
We study the co-evolution between the black hole accretion rate (BHAR) and the star formation rate (SFR) in different galaxy life phases: main sequence star-forming galaxies, quies…
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…
ALMACAL IV: A catalogue of ALMA calibrator continuum observations
M. Bonato, E. Liuzzo, A. Giannetti +12
We present a catalogue of ALMA flux density measurements of 754 calibrators observed between August 2012 and September 2017, for a total of 16,263 observations in different bands a…
The FMOS-COSMOS survey of star-forming galaxies at z~1.6 III. Survey design, performance, and sample characteristics
J. D. Silverman, D. Kashino, D. Sanders +27
We present a spectroscopic survey of galaxies in the COSMOS field using the Fiber Multi-Object Spectrograph (FMOS), a near-infrared instrument on the Subaru Telescope. Our survey i…
Differential attenuation in star-forming galaxies at 0.3 1.5 in the SHARDS/CANDELS field
L. RodrÃguez-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 stu…
Emission-line galaxies at from near-IR HST Slitless Spectroscopy: metallicities, star formation rates and redshift confirmations from VLT/FORS2 spectroscopy
K. Boyett, A. J. Bunker, J Chevallard +14
We follow up emission line galaxies identified through the near-infrared slitless HST/WFC3 WISP survey with VLT/FORS2 optical spectroscopy. Over 4 WISP fields, we targetted 85 of 1…
Relationship between star formation rate and black hole accretion at z=2: The different contributions in quiescent, normal and starburst galaxies
G. Rodighiero, M. Brusa, E. Daddi +12
We investigate the co-evolution of black-hole-accretion-rate (BHAR) and star-formation-rate (SFR) in galaxies displaying a greater diversity of star-forming properties…
The average dust attenuation curve at z~1.3 based on HST grism surveys
A. J. Battisti, M. B. Bagley, I. Baronchelli +12
We present the first characterisation of the average dust attenuation curve at by combining rest-frame ultraviolet through near-IR photometry with Balmer decrement ($\ma…
A Multiwavelength Consensus on the Main Sequence of Star-Forming Galaxies at z~2
G. Rodighiero, A. Renzini, E. Daddi +18
We compare various star formation rate (SFR) indicators for star-forming galaxies at in the COSMOS field. The main focus is on the SFRs from the far-IR (PACS-Herschel d…
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…
Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.20.9
L. RodrÃguez-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 …
Identification of single spectral lines through supervised machine learning in a large HST survey (WISP): a pilot study for Euclid and WFIRST
I. Baronchelli, C. M. Scarlata, G. Rodighiero +13
Future surveys focusing on understanding the nature of dark energy (e.g., Euclid and WFIRST) will cover large fractions of the extragalactic sky in near-IR slitless spectroscopy. T…
The Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole field
I. Baronchelli, C. Scarlata, G. Rodighiero +25
We present the Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole (SEP) field. The large area covered (7.7 deg), together with one of the lowest Galactic…
WFC3 Infrared Spectroscopic Parallel (WISP) Survey: Photometric and Emission Line Data Release
A. J. Battisti, M. B. Bagley, M. Rafelski +21
We present reduced images and catalogues of photometric and emission line data (230,000 and 8,000 sources, respectively) for the WFC3 Infrared Spectroscopic Parallel (W…