activity
20102015
most citedThe XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

272 citations · 1.4k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.CO2015★ 272 cited

The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

M. Pierre, F. Pacaud, C. Adami +89

We present the XXL Survey, the largest XMM programme totaling some 6.9 Ms to date and involving an international consortium of roughly 100 members. The XXL Survey covers two extrag…

astro-ph.GA2014★ 77 cited

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…

astro-ph.IM2014★ 41 cited

The Pointing System of the Herschel Space Observatory. Description, Calibration, Performance and Improvements

Miguel Sánchez-Portal, Anthony Marston, Bruno Altieri +14

We present the activities carried out to calibrate and characterise the performance of the elements of attitude control and measurement on board the Herschel spacecraft. The main c…

astro-ph.GA2014★ 52 cited

Star formation in the massive cluster merger Abell 2744

T. D. Rawle, B. Altieri, E. Egami +8

We present a comprehensive study of star-forming (SF) galaxies in the HST Frontier Field recent cluster merger A2744 (z=0.308). Wide-field, ultraviolet-infrared (UV-IR) imaging ena…

astro-ph.EP2013★ 39 cited

Herschel celestial calibration sources: Four large main-belt asteroids as prime flux calibrators for the far-IR/sub-mm range

T. G. Mueller, Z. Balog, M. Nielbock +9

Celestial standards play a major role in observational astrophysics. They are needed to characterise the performance of instruments and are paramount for photometric calibration. D…

astro-ph.IM2013★ 177 cited

The Herschel-PACS photometer calibration: Point-source flux calibration for scan maps

Zoltan Balog, Thomas Müller, Markus Nielbock +9

This paper provides an overview of the PACS photometer flux calibration concept, in particular for the principal observation mode, the scan map. The absolute flux calibration is ti…

astro-ph.IM2013★ 20 cited

The Herschel PACS photometer calibration - A time dependent flux calibration for the PACS chopped point-source photometry AOT mode

Markus Nielbock, Thomas Müller, Ulrich Klaas +7

We present a flux calibration scheme for the PACS chopped point-source photometry observing mode based on the photometry of five stellar standard sources. This mode was used for sc…

astro-ph.IM2012★ 17 cited

The effect of the high-pass filter data reduction technique on the Herschel PACS Photometer PSF and noise

P. Popesso, B. Magnelli, S. Buttiglione +36

We investigate the effect of the "high-pass filter" data reduction technique on the Herschel PACS PSF and noise of the PACS maps at the 70, 100 and 160 um bands and in medium and f…

astro-ph.CO2012★ 70 cited

Rapid Coeval Black Hole and Host Galaxy Growth in MRC 1138-262: The Hungry Spider

N. Seymour, B. Altieri, C. De Breuck +30

We present a detailed study of the infrared spectral energy distribution of the high-redshift radio galaxy MRC 1138-26 at z = 2.156, also known as the Spiderweb Galaxy. By combinin…

astro-ph.CO2012★ 18 cited

The starburst-AGN connection in the merger galaxy Mrk 938: an infrared and X-ray view

P. Esquej, A. Alonso-Herrero, A. M. Pérez-García +14

Mrk938 is a luminous infrared galaxy in the local Universe believed to be the remnant of a galaxy merger. It shows a Seyfert 2 nucleus and intense star formation according to optic…

astro-ph.CO2012★ 26 cited

PACS-Herschel FIR detections of Lyman-alpha emitters at 2.0<z<3.5

I. Oteo, A. Bongiovanni, A. M. Pérez García +23

In this work we analyze the physical properties of a sample of 56 spectroscopically selected star-forming (SF) Ly emitting galaxies at 2.0z3.5 using both a s…

astro-ph.CO2011★ 12 cited

Far infrared constraints on the contamination by dust obscured galaxies of high-z dropout searches

F. Boone, D. Schaerer, R. Pello +23

The spectral energy distributions (SED) of dusty galaxies at intermediate redshift may look similar to very high redshift galaxies in the optical/near infrared (NIR) domain. This c…

astro-ph.CO2011★ 27 cited

Resolving the nuclear dust distribution of the Seyfert 2 galaxy NGC 3081

C. Ramos Almeida, M. Sanchez-Portal, A. M. Perez-Garcia +13

We report far-infrared (FIR) imaging of the Seyfert 2 galaxy NGC 3081 in the range 70-500 micron, obtained with an unprecedented angular resolution, using the Herschel Space Observ…

astro-ph.CO2011★ 256 cited

GOODS-Herschel: The far-infrared view of star formation in AGN host galaxies since z~3

J. R. Mullaney, M. Pannella, E. Daddi +28

We present a study of the infrared properties of X-ray selected, moderate luminosity (Lx=10^{42}-10^{44}ergs/s) active galactic nuclei (AGNs) up to z~3, to explore the links betwee…

astro-ph.CO2010★ 166 cited

Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel

H. S. Hwang, D. Elbaz, G. E. Magdis +112

We study the dust properties of galaxies in the redshift range 0.1<z<2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-Nort…

astro-ph.CO2010★ 19 cited

Unveiling Far-Infrared Counterparts of Bright Submillimeter Galaxies Using PACS Imaging

H. Dannerbauer, E. Daddi, G. E. Morrison +35

We present a search for Herschel-PACS counterparts of dust-obscured, high-redshift objects previously selected at submillimeter and millimeter wavelengths in the Great Observatorie…

astro-ph.CO2010★ 39 cited

Measures of star formation rates from Infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields

V. Buat, E. Giovannoli, D. Burgarella +75

The reliability of infrared (IR) and ultraviolet (UV) emissions to measure star formation rates in galaxies is investigated for a large sample of galaxies observed with the SPIRE a…

astro-ph.CO2010★ 69 cited

HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements

Asantha Cooray, A. Amblard, L. Wang +77

We measure the angular correlation function, w(theta), from 0.5 to 30 arcminutes of detected sources in two wide fields of the Herschel Multi-tiered Extragalactic Survey (HerMES).…