918 citations · 19.7k across the 225 of their papers we have counts for
13 papers · 2 filters
Models for Evolution of Dusty Galaxies and E/S0s Seen in Multiband Surveys
C. K. Xu, C. J. Lonsdale, D. L. Shupe +3
Phenomenological models for evolution of dusty galaxies and E/S0 galaxies, respectively, are developed to address two major questions concenring galaxy populations in deep infrared…
XMM-Newton observations of ULIRGs I: A Compton-thick AGN in IRAS19254-7245
V. Braito, A. Franceschini, R. Della Ceca +8
We present the XMM-Newton observation of the merging system IRAS 19254-7245, also known as The Superantennae, whose southern nucleus is classified as a Seyfert 2 galaxy. The XMM-Ne…
An enshrouded AGN in the merging starburst system Arp~299 revealed by BeppoSAX
R. Della Ceca, L. Ballo, F. Tavecchio +9
Using a long (=150 ksec), broad-band (0.1--40 keV) BeppoSAX observation of the merging starburst system Arp 299 (=IC 694 + NGC 3690) we found the first unambiguous evidence of the…
Spectro-Polarimetric search for hidden AGNs in four southern Ultraluminous Infrared Galaxies
C. Pernechele, S. Berta, A. Marconi +5
We report on a spectro-polarimetric analysis of four southern Ultra-Luminous Infrared Galaxies (ULIRGs), aimed at constraining the presence of hidden broad AGN lines. For IRAS 1925…
The LARI Method for ISO-CAM/PHOT Data Reduction and Analysis
Carlo Lari, Mattia Vaccari, Giulia Rodighiero +5
The techniques and software tools developed for the reduction and analysis of ISO-CAM/PHOT data with the LARI method are presented. The method, designed for the detection of faint…
Kinematics of Galaxies in the Hubble Deep Field South: Discovery of a Very Massive Spiral at z=0.6
D. Rigopoulou, A. Franceschini, H. Aussel +3
We report the first results from a study of the internal kinematics, based on spatially resolved H_alpha velocity profiles, of three galaxies at redshift z~0.6 and one at redshift…
Origin of the X-Ray Background and AGN Unification: New Perspectives
A. Franceschini, V. Braito, D. Fadda
We critically review the basic assumptions of the standard model for the synthesis of the XRB in the light of new data from ultradeep surveys by Chandra and XMM, resolving major pa…
New Method for ISOCAM Data Reduction - II. Mid-Infrared Extragalactic Source Counts in the Southern ELAIS Field
C. Gruppioni, C. Lari, F. Pozzi +5
We present the 15 micron extragalactic source counts from the Final Analysis Catalogue of the European Large Area ISO Survey southern hemisphere field S1, extracted using the Lari…
The SWIRE SIRTF Legacy Program: Studying the Evolutionary Mass Function and Clustering of Galaxies
Alberto Franceschini, Carol Lonsdale, the SWIRE Co-Investigator Team
The SIRTF Wide-area Infrared Extragalactic (SWIRE) survey is a "Legacy Program" using 851 hours of SIRTF observing time to conduct a set of large-area (67 sq. deg. split into 7 fie…
An XMM-Newton Survey of Ultra-Luminous Infrared Galaxies
V. Braito, A. Franceschini, R. Della Ceca +8
We present preliminary results of XMM-Newton observations of 5 Ultra-luminous Infrared Galaxies (ULIRGs), part of a mini-survey program dedicated to 10 ULIRGs selected from the bri…
The Bulk of the Cosmic Infrared Background Resolved by ISOCAM
D. Elbaz, C. Cesarsky, P. Chanial +4
We have computed the 15 microns integrated galaxy light produced by ISOCAM galaxies above a sensitivity limit of 50 microJy. It sets a lower limit to the 15 microns extragalactic b…
Observations of the Hubble Deep Field South with the Infrared Space Observatory - II. Associations and star formation rates
R. G. Mann, S. Oliver, R. Carballo +15
We present results from a deep mid-IR survey of the Hubble Deep Field South (HDF-S) region performed at 7 and 15um with the CAM instrument on board ISO. We found reliable optical/n…
Observations of the Hubble Deep Field South with the Infrared Space Observatory - I. Observations, data reduction and mid-infrared source counts
S. Oliver, R. G. Mann, R. Carballo +14
We present results from a deep mid-infrared survey of the Hubble Deep Field South (HDF-S) region performed at 7 and 15 micron with the CAM instrument on board the Infrared Space Ob…