10.6k citations
- National Institute for AstrophysicsIT3k papers
- Centre National de la Recherche ScientifiqueFR1.3k papers
- Brera Astronomical ObservatoryIT946 papers
- Osservatorio Astronomico di PadovaIT883 papers
- European Southern ObservatoryCL826 papers
- Trieste Astronomical ObservatoryIT819 papers
- Agenzia Spaziale ItalianaIT797 papers
- University of PaduaIT797 papers
- University of Rome Tor VergataIT793 papers
- University of BolognaIT773 papers
- Arcetri Astrophysical ObservatoryIT743 papers
- Max Planck Institute for Extraterrestrial PhysicsDE723 papers
225 papers · 1 filter
The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3
A. Durkalec, O. Le Fèvre, S. de la Torre +45
The relation between the galaxy stellar mass M_star and the dark matter halo mass M_h gives important information on the efficiency in forming stars and assembling stellar mass in…
Chandra deep observation of XDCP J0044.0-2033, a massive galaxy cluster at z>1.5
P. Tozzi, J. S. Santos, M. J. Jee +11
We report the analysis of the Chandra observation of XDCP J0044.0-2033, a massive, distant (z=1.579) galaxy cluster discovered in the XDCP survey. The total exposure time of 380 ks…
The reversal of the SF-density relation in a massive, X-ray selected galaxy cluster at z=1.58: results from Herschel
Joana S. Santos, . Bruno Altieri, Ivan Valtchanov +8
Dusty, star-forming galaxies have a critical role in the formation and evolution of massive galaxies in the Universe. Using deep far-infrared imaging in the range 100-500um obtaine…
The hidden quasar nucleus of a WISE-selected, hyperluminous, dust-obscured galaxy at z ~ 2.3
E. Piconcelli, C. Vignali, S. Bianchi +8
We present the first X-ray spectrum of a Hot dust-obscured galaxy (DOG), namely W1835+4355 at z ~ 2.3. Hot DOGs represent a very rare population of hyperluminous (>= 10^47 erg/s),…
AGB stars in the LMC: evolution of dust in circumstellar envelopes
F. Dell'Agli, P. Ventura, R. Schneider +4
We calculated theoretical evolutionary sequences of asymptotic giant branch (AGB) stars, including formation and evolution of dust grains in their circumstellar envelope. By consid…
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…