918 citations · 19.7k across the 225 of their papers we have counts for
25 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…
Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission
Luigi Spinoglio, Sabrina Mordini, Juan Antonio Fernandez-Ontiveros +31
We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to demonstrate how deep spectrophotometric surveys covering large cosmological volu…
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…
A panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals
Laura Morselli, Giulia Rodighiero, Andrea Enia +13
In the second work of this series, we analyse the connection between the availability of gas and the position of a region with respect to the spatially resolved main sequence (MS)…
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…
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 …
Optical spectroscopic survey of a sample of Unidentified Fermi objects: II
Simona Paiano, Renato Falomo, Aldo Treves +2
We report on optical spectroscopy obtained at the 10.4m Gran Telescopio Canarias of 28 Fermi gamma-ray sources that completes the study of a sample of 60 targets of unidentified ob…
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…
The Herschel-ATLAS: magnifications and physical sizes of m-selected strongly lensed galaxies
A. Enia, M. Negrello, M. Gurwell +10
We perform lens modelling and source reconstruction of Submillimeter Array (SMA) data for a sample of 12 strongly lensed galaxies selected at 500m in the Herschel Astrophysical…
Optical spectroscopic survey of a sample of Unidentified Fermi objects
Simona Paiano, Renato Falomo, Alberto Franceschini +2
We present optical spectroscopy secured at the 10m Gran Telescopio Canarias of the counterparts of 20 extragalactic gamma-ray sources detected by the Fermi satellite. The observati…
Tracing the evolution of dust obscured star-formation and accretion back to the reionisation epoch with SPICA
C. Gruppioni, L. Ciesla, E. Hatziminaoglou +35
Our current knowledge of star formation and accretion luminosity at high-redshift (z>3-4), as well as the possible connections between them, relies mostly on observations in the re…
Galaxy evolution studies with the SPace IR telescope for Cosmology and Astrophysics (SPICA): the power of IR spectroscopy
L. Spinoglio, A. Alonso-Herrero, L. Armus +65
IR spectroscopy in the range 12-230 micron with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes that govern the formation and evolu…
The Bright and Dark Sides of High-Redshift starburst galaxies from {\it Herschel} and {\it Subaru} observations
A. Puglisi, E. Daddi, A. Renzini +15
We present rest-frame optical spectra from the FMOS-COSMOS survey of twelve \textit{Herschel} starburst galaxies, with Star Formation Rate (SFR) elevated by 8,…
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 st…
Star Formation in Herschel's Monsters versus Semi-Analytic Models
C. Gruppioni, F. Calura, F. Pozzi +9
We present a direct comparison between the observed star formation rate functions (SFRF) and the state-of-the-art predictions of semi-analytic models (SAM) of galaxy formation and…
HerMES: Current Cosmic Infrared Background Estimates Can be Explained by Known Galaxies and their Faint Companions at z < 4
M. P. Viero, L. Moncelsi, R. F. Quadri +28
We report contributions to cosmic infrared background (CIB) intensities originating from known galaxies and their faint companions at submillimeter wavelengths. Using the publicly-…
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…
Combining Physical galaxy models with radio observations to constrain the SFRs of high-z dusty star forming galaxies
B. Lo Faro, L. Silva, A. Franceschini +2
We complement our previous analysis of a sample of z~1-2 luminous and ultra-luminous infrared galaxies ((U)LIRGs), by adding deep VLA radio observations at 1.4 GHz to a large data-…
Linking the X-ray and infrared properties of star-forming galaxies at z<1.5
M. Symeonidis, A. Georgakakis, M. J. Page +16
We present the most complete study to date of the X-ray emission from star-formation in high redshift (median z=0.7; z<1.5), IR-luminous (L_IR=10^10-10^13 L_sun) galaxies detected…
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…
Black hole accretion preferentially occurs in gas rich galaxies
Fabio Vito, Roberto Maiolino, Paola Santini +15
We have investigated the gas content of a sample of several hundred AGN host galaxies at z1 and compared it with a sample of inactive galaxies, matched in bins of stellar mass a…