10.6k citations · 40k across the 238 of their papers we have counts for
72 papers · 1 filter
A pilot sample of Planck-selected strongly lensed sub-mm galaxies: NOEMA observations and physical characterisation
Leonardo Trobbiani, Matteo Bonato, Ivano Baronchelli +6
The extreme brightness of high- strongly lensed galaxies detected by Planck surveys, thanks to their exceptionally large gravitational magnifications, offers a unique opportunit…
Breathless BEARS: [O] 88m Emission of Dusty Star-Forming Galaxies at
T. J. L. C. Bakx, Hiddo S. B. Algera, Prachi Prajapati +13
We present [O] 88m observations towards four -selected dusty star-forming galaxies (DSFGs; log L/L = 13.5 - 14 at $z…
ALMACAL. XV. Band 3 ALMA Survey and Number Counts
Matteo Bonato, Ivano Baronchelli, Gianfranco De Zotti +10
The ALMACAL project leverages ALMA maps of calibrator-centered fields to conduct deep mm/sub-mm surveys, enabling the detection of extragalactic sources with flux densities orders…
Investigating the physical properties of dusty star-forming galaxies at z>=1.5 in the GOODS-South field using JWST
Dipanjan Mitra, Mattia Negrello, Gianfranco De Zotti
We investigated how well the physical properties of progenitors of present-day massive spheroidal galaxies (proto-spheroids) can be constrained by the JWST Advanced Deep Extragalac…
A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
Matteo Bonato, David Leisawitz, Gianfranco De Zotti +10
Far-infrared (FIR) surveys are critical to probing the co-evolution of black holes and galaxies, since of order half the light from accreting black holes and active star formation…
Correlations between IR Luminosity, Star Formation Rate, and CO Luminosity in the Local Universe
Matteo Bonato, Ivano Baronchelli, Viviana Casasola +5
We exploit the DustPedia sample of galaxies within approximately 40 Mpc, selecting 388 sources, to investigate the correlations between IR luminosity (L), the star forma…
Galaxy populations and redshift dependence of the correlation between infrared and radio luminosity
G. De Zotti, M. Bonato, M. Giulietti +4
We argue that the difference in infrared-to-radio luminosity ratio between local and high-redshift star-forming galaxies reflects {the alternative physical conditions} -- including…
Euclid view of dusty star forming galaxies at z>~1.5 detected in wide area submillimetre surveys
Dipanjan Mitra, Mattia Negrello, Gianfranco De Zotti +1
We investigate the constraints provided by the Euclid space observatory on the physical properties of dusty star forming galaxies (DSFGs) at z>~1.5 detected in wide area sub millim…
The Tiered Radio Extragalactic Continuum (T-RECS) simulation II: HI emission and continuum-HI cross-correlation
Anna Bonaldi, Philippa Hartley, Tommaso Ronconi +2
In this paper we extend the Tiered Radio Extragalactic Continuum Simulation (T-RECS) to include HI emission. The HI T-RECS model is based on the most recent HI mass function estima…
The star-formation rates of QSOs
M. Symeonidis, N. Maddox, M. J. Jarvis +13
We examine the far-IR properties of a sample of 5391 optically selected QSOs in the 0.5<z<2.65 redshift range down to log[nuLnu,2500 (erg/s)]>44.7, using SPIRE data from Herschel-A…
Selecting a complete sample of blazars in sub-millimetre catalogues
M. Massardi, M. Bonato, M. Lopez-Caniego +6
The \textit{Herschel} Astrophysical Terahertz Large Area Survey (H-ATLAS), that has covered about 642 sq. deg. in 5 bands from 100 to 500 , allows a blind flux-limited sele…
Modelling high-resolution ALMA observations of strongly lensed dustystar forming galaxies detected by Herschel
Jacob Maresca, Simon Dye, Aristeidis Amvrosiadis +15
We present modelling of ~0.1arcsec resolution Atacama Large Millimetre/sub-millimeter Array imaging of seven strong gravitationally lensed galaxies detected by the Herschel Space O…
The infrared-radio relation in the local universe
K. Tisanić, G. De Zotti, A. Amiri +3
The Square Kilometer Array (SKA) is expected to detect high-redshift galaxies with star formation rates (SFRs) up to two orders of magnitude lower than Herschel surveys and will th…
The LOFAR Two-metre Sky Survey Deep fields: A new analysis of low-frequency radio luminosity as a star-formation tracer in the Lockman Hole region
M. Bonato, I. Prandoni, G. De Zotti +14
We have exploited LOFAR deep observations of the Lockman Hole field at 150 MHz to investigate the relation between the radio luminosity of star-forming galaxies (SFGs) and their st…
Planck intermediate results. LV. Reliability and thermal properties of high-frequency sources in the Second Planck Catalogue of Compact Sources
Planck Collaboration, Y. Akrami, M. Ashdown +117
We describe an extension of the most recent version of the Planck Catalogue of Compact Sources (PCCS2), produced using a new multi-band Bayesian Extraction and Estimation Package (…
A New Multi-Wavelength Census of Blazars
A. Paggi, M. Bonato, C. M. Raiteri +3
Context:Blazars are the rarest and most powerful active galactic nuclei, playing a crucial and growing role in today multi-frequency and multi-messenger astrophysics. Current blaza…
Extragalactic astrophysics with next-generation CMB experiments
G. De Zotti, M. Bonato, M. Negrello +7
Planck, SPT and ACT surveys have clearly demonstrated that Cosmic Microwave Background (CMB) experiments, while optimised for cosmological measurements, have made important contrib…
Role of environment on nuclear activity
Amirnezam Amiri, Saeed Tavasoli, Gianfranco De Zotti
Motivated by the apparently conflicting results reported in the literature on the effect of environment on nuclear activity, we have carried out a new analysis by comparing the fra…
Herschel-ATLAS : The spatial clustering of low and high redshift submillimetre galaxies
A. Amvrosiadis, E. Valiante, J. Gonzalez-Nuevo +12
We present measurements of the angular correlation function of sub-millimeter (sub-mm) galaxies (SMGs) identified in four out of the five fields of the Herschel Astrophysical Terah…
Planck 2018 results. XI. Polarized dust foregrounds
Planck Collaboration, Y. Akrami, M. Ashdown +131
The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization. We use new Planck maps to characterize Galactic du…
Characterization of polarimetric and total intensity behaviour of a complete sample of PACO radio sources in the radio bands
Vincenzo Galluzzi, Marcella Massardi, Anna Bonaldi +17
We present high sensitivity (mJy) polarimetric observations in seven bands, from to GHz, of a complete sample of compact extragalactic radio sou…
Chandra and ALMA observations of the nuclear activity in two strongly lensed star forming galaxies
M. Massardi, A. F. M. Enia, M. Negrello +7
Nuclear activity and star formation play relevant roles in the early stages of galaxy formation. We aim at identifying them in high redshift galaxies by exploiting high-resolution…
H-ATLAS/GAMA: Magnification Bias Tomography. Astrophysical constraints above arcmin
J. González-Nuevo, A. Lapi, L. Bonavera +14
In this work we measure and study the cross-correlation signal between a foreground sample of GAMA galaxies with spectroscopic redshifts in the range , and a background…
Multi-frequency polarimetry of a complete sample of PACO radio sources
V. Galluzzi, M. Massardi, A. Bonaldi +16
We present high sensitivity polarimetric observations in 6 bands covering the 5.5-38 GHz range of a complete sample of 53 compact extragalactic radio sources brighter than 200 mJy…