Follow
Bruno Altieri
Title
Cited by
Cited by
Year
XMM-Newton observatory-I. The spacecraft and operations
F Jansen, D Lumb, B Altieri, J Clavel, M Ehle, C Erd, C Gabriel, ...
Astronomy & Astrophysics 365 (1), L1-L6, 2001
25532001
GOODS-Herschel: an infrared main sequence for star-forming galaxies
D Elbaz, M Dickinson, HS Hwang, T Díaz-Santos, G Magdis, B Magnelli, ...
arXiv preprint arXiv:1105.2537, 2011
13442011
Euclid definition study report
R Laureijs, J Amiaux, S Arduini, JL Augueres, J Brinchmann, R Cole, ...
arXiv preprint arXiv:1110.3193, 2011
11582011
The Herschel Multi-tiered Extragalactic Survey: HerMES
SJ Oliver, J Bock, B Altieri, A Amblard, V Arumugam, H Aussel, ...
Monthly Notices of the Royal Astronomical Society 424 (3), 1614-1635, 2012
9502012
ISOCAM in flight
CJ Cesarsky, A Sargent
Astronomy and Astrophysics 315 (2), L32-L37, 1996
7121996
The spectrum of comet Hale-Bopp (C/1995 O1) observed with the Infrared Space Observatory at 2.9 astronomical units from the Sun
J Crovisier, K Leech, D Bockelee-Morvan, TY Brooke, MS Hanner, ...
Science 275 (5308), 1904-1907, 1997
6591997
A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34
DA Riechers, CM Bradford, DL Clements, CD Dowell, I Pérez-Fournon, ...
Nature 496 (7445), 329-333, 2013
6432013
PACS Evolutionary Probe (PEP)-a Herschel key program
D Lutz, A Poglitsch, B Altieri, P Andreani, H Aussel, S Berta, ...
arXiv preprint arXiv:1106.3285, 2011
6102011
The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations
B Magnelli, P Popesso, S Berta, F Pozzi, D Elbaz, D Lutz, M Dickinson, ...
arXiv preprint arXiv:1303.4436, 2013
5462013
XMM-Newton observation of the Lockman Hole; I. The X-ray Data
G Hasinger, B Altieri, M Arnaud, X Barcons, J Bergeron, H Brunner, ...
arXiv preprint astro-ph/0011271, 2000
5442000
The Herschel PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4
C Gruppioni, F Pozzi, G Rodighiero, I Delvecchio, S Berta, L Pozzetti, ...
Monthly Notices of the Royal Astronomical Society 432 (1), 23-52, 2013
5362013
On Star Formation Rates and Star Formation Histories of Galaxies Out to z∼ 3
S Wuyts, NMF Schreiber, D Lutz, R Nordon, S Berta, B Altieri, P Andreani, ...
The Astrophysical Journal 738 (1), 106, 2011
5082011
The Mean Star Formation Rate of X-ray selected Active Galaxies and its Evolution from z= 2.5: Results from PEP-Herschel
DJ Rosario, P Santini, D Lutz, L Shao, R Maiolino, DM Alexander, B Altieri, ...
arXiv preprint arXiv:1203.6069, 2012
3482012
A Herschel view of the far-infrared properties of submillimetre galaxies
B Magnelli, D Lutz, P Santini, A Saintonge, S Berta, M Albrecht, B Altieri, ...
arXiv preprint arXiv:1202.0761, 2012
3442012
The first Herschel view of the mass-SFR link in high-z galaxies
G Rodighiero, A Cimatti, C Gruppioni, P Popesso, P Andreani, B Altieri, ...
arXiv preprint arXiv:1005.1089, 2010
3402010
GOODS-Herschel: the far-infrared view of star formation in active galactic nucleus host galaxies since z ≈ 3
JR Mullaney, M Pannella, E Daddi, DM Alexander, D Elbaz, RC Hickox, ...
Monthly Notices of the Royal Astronomical Society 419 (1), 95-115, 2012
3262012
The far-infrared/radio correlation as probed by Herschel
RJ Ivison, B Magnelli, E Ibar, P Andreani, D Elbaz, B Altieri, A Amblard, ...
arXiv preprint arXiv:1005.1072, 2010
3142010
HerMES: SPIRE galaxy number counts at 250, 350 and 500 microns
SJ Oliver, L Wang, AJ Smith, B Altieri, A Amblard, V Arumugam, R Auld, ...
arXiv preprint arXiv:1005.2184, 2010
3002010
The first XMM-Newton slew survey catalogue: XMMSL1
RD Saxton, AM Read, P Esquej, MJ Freyberg, B Altieri, D Bermejo
arXiv preprint arXiv:0801.3732, 2008
2952008
Goods-Herschel measurements of the dust attenuation of typical star-forming galaxies at high redshift: observations of ultraviolet-selected galaxies at z∼ 2
N Reddy, M Dickinson, D Elbaz, G Morrison, M Giavalisco, R Ivison, ...
The Astrophysical Journal 744 (2), 154, 2011
2922011
The system can't perform the operation now. Try again later.
Articles 1–20