papers

Publications (370)

astro-ph.HE2019

On the importance of special relativistic effects in modelling ultra-fast outflows

A. Luminari, F. Tombesi, E. Piconcelli +5

Outflows are observed in a variety of astrophysical sources. Remarkably, ultra-fast (), outflows in the UV and X-ray bands are often seen in AGNs. Depending on their en…

astro-ph.IM2018

HERMES: An ultra-wide band X and gamma-ray transient monitor on board a nano-satellite constellation

F. Fuschino, R. Campana, C. Labanti +49

The High Energy Modular Ensemble of Satellites (HERMES) project is aimed to realize a modular X/gamma-ray monitor for transient events, to be placed on-board of a CubeSat bus. This…

astro-ph.IM2010

The New Hard X-ray Mission

G. Tagliaferri, G. Pareschi, A. Argan +12

The Italian New Hard X-ray Mission (NHXM) has been designed to provide a real breakthrough on a number of hot astrophysical issues that includes: black holes census, the physics of…

astro-ph2002

Polarimetric observations of GRB 011211

S. Covino, D. Lazzati, D. Malesani +13

We present and discuss polarimetric observations performed with the VLT-UT3 (Melipal) on the afterglow of GRB 011211, ~35 hours after the burst onset. The observations yielded a 3-…

astro-ph.GA2025

HYPERION: broad-band X-ray-to-near-infrared emission of Quasars in the first billion years of the Universe

I. Saccheo, A. Bongiorno, E. Piconcelli +41

We aim at characterizing the X-ray-to-optical/near-infrared broad-band emission of luminous QSOs in the first Gyr of cosmic evolution to understand whether they exhibit differences…

astro-ph.CO2013

Massive Molecular Outflows and Evidence for AGN Feedback from CO Observations

C. Cicone, R. Maiolino, E. Sturm +12

We study the properties of massive, galactic-scale outflows of molecular gas and investigate their impact on galaxy evolution. We present new IRAM PdBI CO(1-0) observations of loca…

astro-ph.IM2021

The scientific payload on-board the HERMES-TP and HERMES-SP CubeSat missions

Y. Evangelista, F. Fiore, F. Fuschino +22

HERMES (High Energy Rapid Modular Ensemble of Satellites) Technological and Scientific pathfinder is a space borne mission based on a LEO constellation of nano-satellites. The 3U C…

astro-ph.HE2010

GRB 090313: X-shooter's first shot at a GRB

A. de Ugarte Postigo, P. Goldoni, C. C. Thöne +26

Context. X-shooter is the first second-generation instrument to become operative at the ESO Very Large Telescope (VLT). It is a broad-band medium-resolution spectrograph designed w…

astro-ph.IM2016

High Contrast Imaging in the Visible: First Experimental Results at the Large Binocular Telescope

F. Pedichini, M. Stangalini, A. Ambrosino +13

In February 2014, the SHARK-VIS (System for High contrast And coronography from R to K at VISual bands) Forerunner, a high contrast experimental imager operating at visible wavelen…

astro-ph1997

Hard X--ray detection of NGC 1068 with BeppoSAX

G. Matt, M. Guainazzi, F. Frontera +14

We report on the first detection above ~10 keV of the archetypal Compton-thick Seyfert 2 galaxy NGC 1068. This detection, obtained with the PDS instrument onboard BeppoSAX in the 2…

astro-ph.GA2019

The Lyman continuum escape fraction and the Mean Free Path of hydrogen ionizing photons for bright z~4 QSOs from SDSS DR14

M. Romano, A. Grazian, E. Giallongo +5

One of the major challenges in observational cosmology is related to the redshift evolution of the average hydrogen ionization in the Universe. In order to probe the ionization lev…

astro-ph.CO2013

The incidence of obscuration in active galactic nuclei

A. Merloni, A. Bongiorno, M. Brusa +22

We study the incidence of nuclear obscuration on a complete sample of 1310 AGN selected on the basis of their rest-frame 2-10 keV X-ray flux from the XMM-COSMOS survey, in the reds…

astro-ph2000

BeppoSAX observations of Narrow-Line Seyfert 1 galaxies: II. Ionized iron features in Arakelian 564

A. Comastri, G. M. Stirpe, C. Vignali +8

The BeppoSAX observations of the bright Narrow-Line Seyfert 1 galaxy Ark 564 are presented along with a high quality optical spectrum taken at the 1.5m telescope at La Silla. The 0…

astro-ph.GA2023

HYPerluminous quasars at the Epoch of ReionizatION (HYPERION). A new regime for the X-ray nuclear properties of the first quasars

L. Zappacosta, E. Piconcelli, F. Fiore +40

The existence of luminous quasars (QSO) at the Epoch of Reionization (EoR; i.e. z>6) powered by supermassive black holes (SMBH) with masses challenges models…

astro-ph.GA2021

The VANDELS ESO public spectroscopic survey: final Data Release of 2087 spectra and spectroscopic measurements

B. Garilli, R. McLure, L. Pentericci +94

VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we prese…

astro-ph.HE2019

Constraints on gamma-ray and neutrino emission from NGC 1068 with the MAGIC telescopes

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +172

Starburst galaxies and star-forming active galactic nuclei (AGN) are among the candidate sources thought to contribute appreciably to the extragalactic gamma-ray and neutrino backg…

astro-ph.GA2014

The M_BH - M_star relation for X-ray obscured, red QSOs at 1.2< z <2.6

A. Bongiorno, R. Maiolino, M. Brusa +12

We present near-infrared spectra, obtained with SINFONI and XShooter observations at ESO VLT, of nine dusty, red QSOs at 1.2<z<2.6. The sources are hard X-ray detected, characteriz…

astro-ph.HE2017

Extragalactic gamma-ray background from AGN winds and star-forming galaxies in cosmological galaxy formation models

A. Lamastra, N. Menci, F. Fiore +4

We derive the contribution to the extragalactic gamma-ray background (EGB) from AGN winds and star-forming galaxies by including a physical model for the gamma-ray emission produce…

astro-ph2002

The log(N)-log(S) and the Broadband Properties of the Sources in the HELLAS2XMM Survey

A. Baldi, S. Molendi, A. Comastri +3

We present the first results from an XMM-Newton serendipitous medium-deep survey, which covers nearly three square degrees. We show the log(N)-log(S) distributions for the 0.5-2, 2…

astro-ph2002

A BeppoSAX Observation of KS 1731-260 in its Quiescent State: Constraints on the NS Magnetic Field

L. Burderi, T. Di Salvo, L. Stella +10

We report here the results of a 90 ks BeppoSAX observation of the low mass X-ray binary and atoll source KS 1731-260 during a quiescent phase. From this observation we derive a sou…

astro-ph.IM2020

ESA Voyage 2050 white paper -- GrailQuest: hunting for Atoms of Space and Time hidden in the wrinkle of Space-Time

L. Burderi, A. Sanna, T. Di Salvo +30

GrailQuest (Gamma Ray Astronomy International Laboratory for QUantum Exploration of Space-Time) is a mission concept based on a constellation (hundreds/thousands) of nano/micro/sma…

astro-ph1999

BeppoSAX Observations of GRB980425: Detection of the Prompt Event and Monitoring of the Error Box

E. Pian, L. Amati, L. A. Antonelli +25

We present BeppoSAX follow-up observations of GRB980425 obtained with the Narrow Field Instruments (NFI) in April, May, and November 1998. The first NFI observation has detected wi…

astro-ph2002

On the nature of X-ray Bright Optically Normal galaxies

A. Comastri, M. Brusa, P. Ciliegi +10

Multiwavelength observations of the hard X-ray selected sources by Chandra and XMM-Newton surveys have significantly improved our knowledge of the objects responsible of the hard X…

astro-ph.GA2020

SUPER III. Broad Line Region properties of AGN at z2

G. Vietri, V. Mainieri, D. Kakkad +27

The SINFONI survey for Unveiling the Physics and Effect of Radiative feedback (SUPER) was designed to conduct a blind search for AGN-driven outflows on X-ray selected AGN at redshi…

astro-ph2007

Selection effects shaping the Gamma Ray Burst redshift distributions

F. Fiore, D. Guetta, S. Piranomonte +2

Long Gamma Ray Bursts hold the promise of probing star-formation and metal enrichment up to very high redshifts. The present GRB samples with redshift determination are largely inc…

astro-ph2000

An exploratory study of the hard X-ray variability properties of PG quasars with RXTE

M. Guainazzi, F. Fiore, E. Giallongo +3

We have monitored with the RXTE PCA the variability pattern of the 2-20 keV flux in four PG quasars (QSOs) from the Laor et al. (1994) sample. Six observations of each target at re…

astro-ph2006

The multiwavelength afterglow of GRB 050721: a puzzling rebrightening seen in the optical but not in the X-ray

L. A. Antonelli, V. Testa, P. Romano +27

Context. GRB050721 was detected by Swift and promptly followed-up, in the X-ray by Swift itself and, in the optical band, by the VLT operated, for the first time, in rapid response…

astro-ph2000

The evolution of AGN in the Hard X-rays from HELLAS

F. La Franca, F. Fiore, C. Vignali +3

We present optical spectroscopic identification of sources identified in the BeppoSAX MECS fields of the High Energy LLarge Area Survey (HELLAS). In total 62 sources from a sample…

astro-ph2005

Active and passive shielding design optimization and technical solutions for deep sensitivity hard X-ray focusing telescopes

G. Malaguti, G. Pareschi, P. Ferrando +12

The 10-100 keV region of the electromagnetic spectrum contains the potential for a dramatic improvement in our understanding of a number of key problems in high energy astrophysics…

astro-ph2003

Heavy Element Abundances and Dust Depletions in the Host Galaxies of Three Gamma-Ray Bursts

S. Savaglio, S. M. Fall, F. Fiore

We have derived the column densities of heavy elements in three gamma-ray burst (GRB) optical transients, associated with the circumburst or interstellar medium (ISM) of the host g…

astro-ph.GA2011

A low escape fraction of ionizing photons of L>L* Lyman break galaxies at z=3.3

K. Boutsia, A. Grazian, E. Giallongo +12

We present an upper limit for the relative escape fraction (f_{esc}^{rel}) of ionizing radiation at z~3.3 using a sample of 11 Lyman Break Galaxies (LBGs) with deep imaging in the…

astro-ph2007

An X-ray Survey in SA 57 with XMM-Newton

D. Trevese, F. Vagnetti, S. Puccetti +3

The maximum number density of Active Galactic Nuclei (AGNs), as deduced from X-ray studies, occurs at z<~1, with lower luminosity objects peaking at smaller redshifts. Optical stud…

astro-ph1998

The Equilibrium Photoionized Absorber in 3C351

F. Nicastro, F. Fiore, M. Elvis +1

We present two ROSAT PSPC observations of the radio-loud, lobe-dominated quasar 3C 351, which shows an `ionized absorber' in its X-ray spectrum. The factor 1.7 change in flux in th…

astro-ph.HE2013

The Hot and Energetic Universe: Astrophysics of feedback in local AGN

M. Cappi, C. Done, E. Behar +30

Understanding the astrophysics of feedback in active galactic nuclei (AGN) is key to understanding the growth and co-evolution of supermassive black holes and galaxies. AGN-driven…

astro-ph2006

The XMM-Newton wide-field survey in the COSMOS field. IV: X-ray spectral properties of Active Galactic Nuclei

V. Mainieri, G. Hasinger, N. Cappelluti +25

We present a detailed spectral analysis of point-like X-ray sources in the XMM-COSMOS field. Our sample of 135 sources only includes those that have more than 100 net counts in the…

astro-ph.GA2016

AGN host galaxy mass function in COSMOS: is AGN feedback responsible for the mass-quenching of galaxies?

A. Bongiorno, A. Schulze, A. Merloni +11

We investigate the role of supermassive black holes in the global context of galaxy evolution by measuring the host galaxy stellar mass function (HGMF) and the specific accretion r…

astro-ph.CO2010

A Runaway Black Hole in COSMOS: Gravitational Wave or Slingshot Recoil?

F. Civano, M. Elvis, G. Lanzuisi +39

We present a detailed study of a peculiar source in the COSMOS survey at z=0.359. Source CXOCJ100043.1+020637 (CID-42) presents two compact optical sources embedded in the same gal…

astro-ph.CO2010

The XMM-Newton Wide-Field Survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous AGN

M. Brusa, F. Civano, A. Comastri +64

We report the final optical identifications of the medium-depth (~60 ksec), contiguous (2 deg^2) XMM-Newton survey of the COSMOS field. XMM-Newton has detected ~800 X-ray sources d…

astro-ph.CO2009

Spectroscopic identifications of Spitzer sources in the SWIRE/XMM-NEWTON/ELAIS-S1 field: a large fraction of Active Galactic Nuclei with high F(24micron)/F(R) ratio

N. Sacchi, F. La Franca, C. Feruglio +20

We present a catalog of optical spectroscopic identifications of sources detected by Spitzer at 3.6 or 24 micron down to 10 and 280 microJy, respectively, in the SWIRE/XMM-Newton/E…

astro-ph.GA2017

The WISSH Quasars Project III. X-ray properties of hyper-luminous quasars

S. Martocchia, E. Piconcelli, L. Zappacosta +14

We perform a survey of the X-ray properties of 41 objects from the WISE/SDSS selected Hyper-luminous (WISSH) quasars sample, composed by 86 broad-line quasars (QSOs) with bolometri…

astro-ph.GA2017

The Lyman Continuum escape fraction of faint galaxies at z~3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC

A. Grazian, E. Giallongo, D. Paris +41

The reionization of the Universe is one of the most important topics of present day astrophysical research. The most plausible candidates for the reionization process are star-form…

astro-ph.CO2011

X-ray spectroscopy of the Compton-thick Seyfert 2 ESO 138-G1

E. Piconcelli, S. Bianchi, C. Vignali +2

We report on our analysis of XMM-Newton observations of the Seyfert 2 galaxy ESO 138-G1 (z = 0.0091). These data reveal a complex spectrum in both its soft and hard portions. The 0…

astro-ph.CO2010

The HELLAS2XMM survey. XIII. Multi-component analysis of the spectral energy distribution of obscured AGN

F. Pozzi, C. Vignali, A. Comastri +9

We combine near-to-mid-IR Spitzer data with shorter wavelength observations (optical to X-rays) to get insights on the properties of a sample of luminous, obscured Active Galactic…

astro-ph2001

Iron line emission in X-ray afterglows

D. Lazzati, G. Ghisellini, M. Vietri +2

Recent observations of X-ray afterglows reveal the presence of a redshifted Kalpha iron line in emission in four bursts. In GRB 991216, the line was detected by the low energy grat…

astro-ph1999

The BeppoSAX view of the hot cluster Abell 2319

S. Molendi, S. De Grandi, R. Fusco-Femiano +4

We present results from a BeppoSAX observation of the rich cluster Abell 2319. The broad band spectrum (2-50 keV) of the cluster can be adequately represented by an optically thin…

astro-ph2002

The BeppoSAX High Energy Large Area Survey -V. The nature of the hard X-ray source populations and its evolution

F. La Franca, F. Fiore, C. Vignali +7

We present optical spectroscopic identifications of hard X-ray (5-10 keV) selected sources belonging to the HELLAS sample obtained with BeppoSAX down to a 5-10 keV flux limit of f_…

astro-ph1998

High resolution imaging of the X-ray afterglow of GRB970228 with ROSAT

F. Frontera, J. Greiner, L. A. Antonelli +6

We report results of a ROSAT High-Resolution Imager (HRI) observation of the X-ray error box given by the BeppoSAX Wide Field Camera for the gamma-ray burst that occurred on 1997 F…

astro-ph.HE2018

The NuSTAR Extragalactic Surveys: X-ray spectroscopic analysis of the bright hard-band selected sample

L. Zappacosta, A. Comastri, F. Civano +23

We discuss the spectral analysis of a sample of 63 Active Galactic Nuclei (AGN) detected above a limiting flux of keV erg/s/cm in the multi-tiered N…

astro-ph.HE2009

GRB090426: the farthest short gamma-ray burst?

L. A. Antonelli, P. D Avanzo, R. Perna +23

Aims. With an observed and rest-frame duration of < 2s and < 0.5s, respectively, GRB090426 could be classified as a short GRB. The prompt detection, both from space and ground-base…

astro-ph2007

Can we use Gamma Ray Bursts to probe high redshift star-formation?

F. Fiore, D. Guetta, S. Piranomonte +2

We present a detailed analysis of the selection effects that plague GRB observations. We find that these effects may partially explain the different redshift distributions between…

astro-ph.GA2018

The rest-frame UV-to-optical spectroscopy of APM 08279+5255 - BAL classification and black hole mass estimates

F. G. Saturni, M. Bischetti, E. Piconcelli +9

We present the analysis of the rest-frame optical-to-UV spectrum of APM 08279+5255, a well-known lensed broad absorption line (BAL) quasar at . The spectroscopic data ar…

astro-ph.GA2016

A fast ionised wind in a Star Forming-Quasar system at z~1.5 resolved through Adaptive Optics assisted near-infrared data

M. Brusa, M. Perna, G. Cresci +15

Outflows are invoked in co-evolutionary models to link the growth of SMBH and galaxies through feedback phenomena, and from the analysis of both galaxies and Active Galactic Nuclei…

astro-ph.CO2009

On the cosmic evolution of the scaling relations between black holes and their host galaxies: Broad Line AGN in the zCOSMOS survey

A. Merloni, A. Bongiorno, M. Bolzonella +56

(Abriged) We report on the measurement of the rest frame K-band luminosity and total stellar mass of the hosts of 89 broad line Active Galactic Nuclei detected in the zCOSMOS surve…

astro-ph.GA2019

Triggering nuclear and galaxy activity in the Bullet cluster

S. Puccetti, F. Fiore, A. Bongiorno +3

The analysis of the cluster environment is a valuable instrument to investigate the origin of AGN and star-forming galaxies gas fuelling and trigger mechanisms. To this purpose, we…

astro-ph.GA2009

The Fraction of Quiescent Massive Galaxies in the Early Universe

A. Fontana, P. Santini, A. Grazian +9

Aims: The aim of this work is to collect a complete, mass--selected sample of galaxies with very low specific star formation rate, for a comparison with the prediction of recent th…

astro-ph2001

The BeppoSAX High Energy Large Area Survey HELLAS, II: Number counts and X-ray spectral properties

F. Fiore, P. Giommi, C. Vignali +7

The BeppoSAX High Energy Large Area Survey (HELLAS) has surveyed about 85 deg^2 of sky in the 5-10 keV band down to a flux of 4-5 10^-14 erg cm-2 s-1. The source surface density of…

astro-ph2006

The ESO-Spitzer Imaging extragalactic Survey (ESIS) I: WFI B,V,R deep observations of ELAIS-S1 and comparison to Spitzer and GALEX data

S. Berta, S. Rubele, A. Franceschini +15

The ESO-Spitzer extragalactic Imaging Survey (ESIS) is the optical follow up of the Spitzer Wide-Area InfraRed Extragalactic (SWIRE) survey in the ELAIS-S1 area. This paper present…

astro-ph.GA2019

The gentle monster PDS 456: the kpc scale molecular outflow and its implications for QSO feedback

M. Bischetti, E. Piconcelli, C. Feruglio +12

We report on the first ALMA observation of the CO(32) and rest-frame ~340 GHz continuum emission in PDS 456, which is the most luminous, radio-quiet QSO in the local Universe ($…

astro-ph2000

Chandra study of an overdensity of X-ray sources around two distant (z~0.5) clusters

M. Cappi, P. Mazzotta, M. Elvis +21

We present results from a Chandra X-ray Observatory study of the field X-ray source populations in 4 different observations: two high-redshift (z~0.5) clusters of galaxies 3C295 an…

astro-ph1998

X-Ray Surveys

P. Giommi, F. Fiore, M. Perri

A review of recent developments in the field of X-ray surveys, especially in the hard (2-10 and 5-10 keV) bands, is given. A new detailed comparison between the measurements in the…

astro-ph.CO2011

A Compton-thick AGN at z~5 in the 4 Ms Chandra Deep Field South

R. Gilli, J. Su, C. Norman +13

We report the discovery of a Compton-thick Active Galactic Nucleus (AGN) at z=4.76 in the 4 Ms Chandra Deep Field South. This object was selected as a V-band dropout in HST/ACS ima…

astro-ph2000

On the peculiar X-ray properties of the bright nearby radio-quiet quasar PDS456

C. Vignali, A. Comastri, F. Nicastro +3

BeppoSAX and ASCA observations of the nearby (z=0.184), high-luminosity, radio-quiet quasar PDS456 are presented. The X-ray spectrum is characterized by a prominent ionized edge at…

astro-ph.HE2016

Galactic outflow driven by the active nucleus and the origin of the gamma-ray emission in NGC 1068

A. Lamastra, F. Fiore, D. Guetta +6

We compute the non-thermal emissions produced by relativistic particles accelerated by the AGN-driven shocks in NGC 1068, and we compare the model predictions with the observed gam…

astro-ph2002

An XMM-Newton Study of Hard X-ray Sources

E. Piconcelli, L. Bassani, M. Cappi +3

We briefly report on an on-going spectroscopic study of hard X-ray sources selected serendipitously in 12 XMM-Newton fields. Results for the analysis of the 41 sources from the fir…

astro-ph2008

The short GRB070707 afterglow and its very faint host galaxy

S. Piranomonte, P. D'Avanzo, S. Covino +18

We present the results from an ESO/VLT campaign aimed at studying the afterglow properties of the short/hard gamma ray burst GRB 070707. Observations were carried out at ten differ…

astro-ph2007

Compton thick AGN in the Suzaku era

A. Comastri, R. Gilli, C. Vignali +3

Suzaku observations of two hard X-ray (> 10 keV) selected nearby Seyfert 2 galaxies are presented. Both sources were clearly detected with the PIN Hard X-ray Detector up to several…

astro-ph2003

The HELLAS2XMM 1dF survey: on the nature of high X-ray to optical flux ratio sources

F. Fiore, M. Brusa, F. Cocchia +12

We present results from the photometric and spectroscopic identification of 122 X-ray sources discovered by XMM-Newton in the 2-10 keV band (the HELLAS2XMM 1dF sample). One of the…

astro-ph.IM2021

A summary on an investigation of GAGG:Ce afterglow emission in the context of future space applications within the HERMES nanosatellite mission

G. Dilillo, R. Campana, N. Zampa +18

GAGG:Ce (Cerium-doped Gadolinium Aluminium Gallium Garnet) is a promising new scintillator crystal. A wide array of interesting features, such as high light output, fast decay time…

astro-ph2002

Flux and spectral variations in the Circinus Galaxy

S. Bianchi, G. Matt, F. Fiore +3

We report on a dramatic flux (50 % increase in the LECS and MECS band) and spectral variation between two BeppoSAX observations of the Circinus Galaxy performed almost three years…

astro-ph.CO2013

Diffuse optical intracluster light as a measure of stellar tidal stripping: the cluster CL0024+17 at 0.4 observed at LBT

E. Giallongo, N. Menci, A. Grazian +9

We have evaluated the diffuse intracluster light (ICL) in the central core of the galaxy cluster CL0024+17 at observed with the prime focus camera (LBC) at LBT. The mea…

astro-ph.HE2021

Distributed Architectures and Constellations for Gamma-Ray Burst Science

F. Fiore, N. Werner, E. Behar

The gravitational wave/gamma-ray burst GW/GRB170817 event marked the beginning of the era of multi-messenger astrophysics, in which new observations of Gravitational Waves (GW) are…

astro-ph2004

HEXIT-SAT: a mission concept for X-ray grazing incidence telescopes from 0.5 to 70 keV

F. Fiore, G. C. Perola, G. Pareschi +3

While the energy density of the Cosmic X-ray Background (CXB) provides a statistical estimate of the super massive black hole (SMBH) growth and mass density in the Universe, the la…

astro-ph.CO2013

The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology

N. Menci, F. Fiore, A. Lamastra

Recent measurements of the abundance of AGN with low-luminosities (L_X< 10^44 erg/s in the 2-10 keV energy band) at high redshifts z>4 provide a serious challenge for Cold Dark Mat…

astro-ph1998

Signatures of Resonant Absoprtion in X-ray Spectra of Type 1 AGN

F. Nicastro, F. Fiore, G. Matt

We present photoionization models accounting for both photoelectric and resonant absorption. We demonstrate that resonance absorption lines are detectable even in moderate resoluti…

astro-ph2000

An X-ray and optical study of the cluster A33

S. Colafrancesco, C. R. Mullis, A. Wolter +11

We report the first detailed X-ray and optical observations of the medium-distant cluster A33 obtained with the Beppo-SAX satellite and with the UH 2.2m and Keck II telescopes at M…

astro-ph.GA2016

The Chandra COSMOS Legacy survey: overview and point source catalog

F. Civano, S. Marchesi, A. Comastri +39

The COSMOS-Legacy survey is a 4.6 Ms Chandra program that has imaged 2.2 deg of the COSMOS field with an effective exposure of 160 ks over the central 1.5 deg and o…

astro-ph1997

BeppoSAX observations of Narrow-Line Seyfert 1 galaxies:I. Ton S 180

A. Comastri, F. Fiore, M. Guainazzi +10

We report on the first spectrum up to 10 keV of the bright narrow-line Seyfert 1 galaxy Ton S 180, obtained with the imaging instruments onboard BeppoSAX. This is the first observe…

astro-ph.CO2009

A Comprehensive Study of Large Scale Structures in the GOODS-SOUTH Field up to z \sim 2.5

S. Salimbeni, M. Castellano, L. Pentericci +14

The aim of this paper is to identify and study the properties and galactic content of groups and clusters in the GOODS-South field up to z\sim2.5, and to analyse the physical prope…

astro-ph2007

A study of the prompt and afterglow emission of the Short GRB 061201

G. Stratta, P. D'Avanzo, S. Piranomonte +30

Our knowledge of the intrinsic properties of short duration Gamma-Ray Bursts has relied, so far, only upon a few cases for which the estimate of the distance and an extended, multi…

astro-ph.GA2018

A high space density of L* Active Galactic Nuclei at z~4 in the COSMOS field

K. Boutsia, A. Grazian, E. Giallongo +2

Identifying the source population of ionizing radiation, responsible for the reionization of the universe, is currently a hotly debated subject with conflicting results. Studies of…

astro-ph2003

X-Ray Sources Overdensity Around the 3C 295 Galaxy Cluster

V. D'Elia, F. Fiore, M. Elvis +4

We present a statistical analysis of the Chandra observation of the source field around the 3C 295 galaxy cluster (). The logN-logS of this field is in good agreement with…

astro-ph.HE2011

On the nature of the absorber in IRAS 09104+4109: the X-ray and mid-infrared view

C. Vignali, E. Piconcelli, G. Lanzuisi +8

We present a long (~76 ks) Chandra observation of IRAS 09104+4109, a hyper-luminous galaxy, optically classified as a Type 2 AGN hosted in a cD galaxy in a cluster at z=0.442. We a…

astro-ph1998

The BeppoSAX High Energy Large Area Survey (HELLAS)

F. Fiore, P. Giommi, F. La Franca +9

We have surveyed about 50 deg-2 of sky in the largely unexplored 5-10 keV band using the BeppoSAX MECS instrument, finding 180 sources. After correction for the non uniform sky cov…

astro-ph.GA2025

A deep X-ray look to the most obscured quasar at z~3.6 and its environment

I. Villani, L. Zappacosta, E. Piconcelli +17

The most luminous and obscured quasars (QSOs) detected in infrared all-sky surveys could represent a key co-evolutionary phase from nuclear to circum-galactic (CG) scales in the fo…

astro-ph2000

The BeppoSAX HELLAS survey: on the nature of faint hard X-ray selected sources

F. Fiore, L. A. Antonelli, P. Ciliegi +8

The BeppoSAX 4.5-10 keV High Energy Large Area Survey has covered about 80 square degrees of sky down to a flux of F(5-10keV)~5E-14 cgs. Optical spectroscopic identification of abo…

astro-ph1997

Spectral Properties of the Prompt X-ray emission and Afterglow from the Gamma-Ray Burst of 28 February 1997

F. Frontera, E. Costa, L. Piro +18

We report high-energy spectral data of the prompt emission of GRB970228 and its X-ray afterglow. We establish that the nature of the X-ray afterglow emission is non-thermal and sim…

astro-ph.CO2010

The M_BH-M_star relation of obscured AGNs at high redshift

J. E. Sarria, R. Maiolino, F. La Franca +5

We report the detection of broad Halpha emission in three X-ray selected obscured AGNs at z=1-2. By exploiting the Halpha width and the intrinsic X-ray luminosity, we estimate thei…

astro-ph2002

The nuclear accretion in the FR I radio galaxy IC4296 from CHANDRA and VLBA observations

S. Pellegrini, T. Venturi, A. Comastri +5

A high angular resolution study of the nucleus of the FR I galaxy IC4296 using Chandra ACIS-S and VLBA observations is presented, with the aim of studying the nature of the accreti…

astro-ph.GA2016

The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars

M. Bischetti, E. Piconcelli, G. Vietri +19

Models and observations suggest that both power and effects of AGN feedback should be maximised in hyper-luminous (L_Bol>10^47 erg/s) quasars, i.e. objects at the brightest end of…

astro-ph.GA2024

Supermassive Black Hole Winds in X-rays -- SUBWAYS. III. A population study on ultra-fast outflows

V. E. Gianolli, S. Bianchi, P-O Petrucci +44

The detection of blue-shifted absorption lines likely associated with ionized Iron K-shell transitions in the X-ray spectra of many Active Galactic Nuclei (AGN) suggests the presen…

astro-ph.GA2014

Triggering Active Galactic Nuclei in Hierarchical Galaxy Formation: Disk instability vs. Interactions

N. Menci, M. Gatti, F. Fiore +1

Using a semi analytic model for galaxy formation we investigate the effects of Black Hole accretion triggered by disk instabilities (DI) in isolated galaxies on the evolution of AG…

astro-ph.GA2015

Physical properties of AGN host galaxies as a probe of SMBH feeding mechanisms

M. Gatti, A. Lamastra, N. Menci +2

Using an advanced semi analytic model (SAM) for galaxy formation, we have investigated the statistical effects of assuming two different mechanisms for triggering AGN activity on t…

astro-ph.GA2014

Very extended cold gas, star formation and outflows in the halo of a bright QSO at z>6

C. Cicone, R. Maiolino, S. Gallerani +6

Past observations of QSO host galaxies at z >6 have found cold gas and star formation on compact scales of a few kiloparsecs. We present new high sensitivity IRAM PdBI follow-up ob…

astro-ph1999

Broad band spectral properties of Seyfert 1 galaxies observed with BeppoSAX

L. Piro, A. De Rosa, M. Dadina +8

We will present some results on the broad--band observations of BeppoSAX of the bright Seyfert galaxies NGC 4151 and NGC 5548.

astro-ph.CO2009

GRB 090423 at a redshift of z~8.1

R. Salvaterra, M. Della Valle, S. Campana +42

Gamma-ray bursts (GRBSs) are produced by rare types of massive stellar explosions. Their rapidly fading afterglows are often bright enough at optical wavelengths, that they are det…

astro-ph.CO2012

Accreting SMBHs in the COSMOS field and the connection to their host galaxies

A. Bongiorno, A. Merloni, M. Brusa +22

Using the wide multi-band photometry available in the COSMOS field we explore the host galaxy properties of a large sample of Active Galactic Nuclei (AGN) obtained by combining X-r…

astro-ph.CO2009

Revealing X-ray obscured quasars in SWIRE sources with extreme mid-IR/optical flux ratios

G. Lanzuisi, E. Piconcelli, F. Fiore +4

Recent works have suggested that selection criteria based on MIR colors can be used to reveal a population of dust-enshrouded, extremely luminous quasars at z>1. However the X-ray…

astro-ph.CO2011

The Population of High Redshift AGNs in the Chandra COSMOS survey

F. Civano, M. Brusa, A. Comastri +19

We present the high redshift (3<z<5.3) 0.5-2 keV number counts and the 2-10 keV (rest frame) space density of X-ray selected AGNs detected in the Chandra COSMOS survey. The sample…

astro-ph2006

The XMM-Newton survey of the ELAIS-S1 field. I: Number counts, angular correlation function and X-ray spectral properties

S. Puccetti, F. Fiore, V. D'Elia +16

We have surveyed with XMM-Newton the central ~0.6 deg2 region of the ELAIS-S1 field down to flux limits of ~5.5X10-16 cgs (0.5-2 keV, S band), ~2X10-15 cgs (2-10 keV, H band), and…

astro-ph.GA2019

The WISSH quasars project VI. Fraction and properties of BAL quasars in the hyper-luminosity regime

G. Bruni, E. Piconcelli, T. Misawa +9

The WISSH quasars project aims at studying the nuclear and host galaxy properties of the most luminous quasars ( erg/s, ). Nuclear winds are manifested…