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20002026
most citedPACS Evolutionary Probe (PEP) - A Herschel Key Program

503 citations · 5.1k across the 69 of their papers we have counts for

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43 papers · 1 filter

astro-ph.CO2025

Thermal Sunyaev-Zel'dovich effect at the core of CL J1226.9+3332 revealed by NOEMA

M. Muñoz-Echeverría, J. -F. Macías-Pérez, R. Neri +58

We present first detailed maps of the thermal Sunyaev-Zel'dovich (tSZ) effect on a cluster with the NOrthern Extended Millimeter Array (NOEMA). The high sensitivity of t…

astro-ph.CO2025

NIKA2 Cosmological Legacy Survey: Blind detection of galaxy clusters in the COSMOS field via the Sunyaev-Zel'dovich effect

D. Chérouvrier, J. F. Macias-Perez, F. X. Désert +59

(Abridged) Clusters of galaxies, formed in the latest stages of structure formation, are unique cosmological probes. With the advent of large CMB surveys like those from the Planck…

astro-ph.CO2024★ 2 cited

Exploiting the high-resolution NIKA2 data to study the intracluster medium and dynamical state of ACT-CL J0240.0+0116

A. Paliwal, M. De Petris, A. Ferragamo +54

Having a detailed knowledge of the intracluster medium (ICM) to infer the exact cluster physics such as the cluster dynamical state is crucial for cluster-based cosmological studie…

astro-ph.CO2014★ 151 cited

J-PAS: The Javalambre-Physics of the Accelerated Universe Astrophysical Survey

N. Benitez, R. Dupke, M. Moles +149

The Javalambre-Physics of the Accelerated Universe Astrophysical Survey (J-PAS) is a narrow band, very wide field Cosmological Survey to be carried out from the Javalambre Observat…

astro-ph.CO2013★ 264 cited

The evolution of the dust temperatures of galaxies in the SFR plane up to

B. Magnelli, D. Lutz, A. Saintonge +38

[Abridged] We study the evolution of the dust temperatures of galaxies in the SFR-M* plane up to z~2 using observations from the Herschel Space Observatory. Starting from a sample…

astro-ph.CO2013★ 15 cited

Lyman break and UV-selected galaxies at z ~ 1: II. PACS-100um/160um FIR detections

I. Oteo, G. Magdis, Á. Bongiovanni +53

We report the PACS-100um/160um detections of a sample of 42 GALEX-selected and FIR-detected Lyman break galaxies (LBGs) at z ~ 1 located in the COSMOS field and analyze their ultra…

astro-ph.CO2013★ 19 cited

The UV to FIR spectral energy distribution of star-forming galaxies in the redshift desert

I. Oteo, Á. Bongiovanni, G. Magdis +6

We analyse the rest-frame UV-to-NIR spectral energy distribution (SED) of Lyman break galaxies (LBGs), star-forming (SF) BzK (sBzK), and UV-selected galaxies at 1.5 < z < 2.5 in th…

astro-ph.CO2013★ 429 cited

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 +34

We present results from the deepest Herschel-PACS (Photodetector Array Camera and Spectrometer) far-infrared blank field extragalactic survey, obtained by combining observations of…

astro-ph.CO2013★ 1 cited

X-ray luminosity functions of different morphological and X-ray type AGN populations

M. Pović, A. M. Pérez García, M. Sánchez-Portal +12

Luminosity functions are one of the most important observational clues when studying galaxy evolution over cosmic time. In this paper we present the X-ray luminosity functions of X…

astro-ph.CO2013★ 440 cited

The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4

C. Gruppioni, F. Pozzi, G. Rodighiero +100

We exploit the deep and extended far infrared data sets (at 70, 100 and 160 um) of the Herschel GTO PACS Evolutionary Probe (PEP) Survey, in combination with the HERschel Multi tie…

astro-ph.CO2013★ 6 cited

Lyman break and UV-selected galaxies at I. Stellar populations from ALHAMBRA survey

I. Oteo, Á. Bongiovanni, J. Cepa +29

We take advantage of the exceptional photometric coverage provided by the combination of GALEX data in the UV and the ALHAMBRA survey in the optical and near-IR to analyze the phys…

astro-ph.CO2012

SAFIR: testing the coexistence of AGN and star formation activity and the nature of the dusty torus in the local universe

M. Sanchez-Portal, M. Castillo-Fraile, C. Ramos Almeida +16

We present the Seyfert and star formation Activity in the Far-InfraRed (SAFIR) project, a small (15.1h) Herschel guaranteed time proposal performing PACS and SPIRE imaging of a sma…

astro-ph.CO2012

Status of the OTELO Project

J. Cepa, A. Bongiovanni, A. M. Perez Garcia +10

The OTELO project is the extragalactic survey currently under way using the tunable filters of the OSIRIS instrument at the GTC. OTELO is already providing the deepest emission lin…

astro-ph.CO2012★ 13 cited

Physical properties of Lyman-alpha emitters at from UV-to-FIR measurements

I. Oteo, A. Bongiovanni, A. M. Pérez García +25

The analysis of the physical properties of low-redshift Ly emitters (LAEs) can provide clues in the study of their high-redshift analogues. At , LAEs are bright enou…

astro-ph.CO2012★ 299 cited

The Mean Star Formation Rate of X-ray selected Active Galaxies and its Evolution from z=2.5: Results from PEP-Herschel

D. J. Rosario, P. Santini, D. Lutz +37

(Abridged) We study relationships between the SFR and the nuclear properties of X-ray selected AGNs out to z=2.5, using far-IR data in three extragalactic deep fields as part of th…

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.CO2012★ 287 cited

A Herschel view of the far-infrared properties of submillimetre galaxies

B. Magnelli, D. Lutz, P. Santini +48

We study a sample of 61 submillimetre galaxies (SMGs) selected from ground-based surveys, with known spectroscopic redshifts and observed with Herschel as part of the PACS Evolutio…

astro-ph.CO2012★ 221 cited

Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observations

P. Santini, D. J. Rosario, L. Shao +35

We compare the average star formation (SF) activity in X-ray selected AGN hosts with mass-matched control inactive galaxies,including star forming and quiescent sources, at 0.5<z<2…

astro-ph.CO2011★ 14 cited

SDSS galaxies with double-peaked emission lines: double starbursts or AGNs?

L. S. Pilyugin, I. A. Zinchenko, B. Cedres +4

With the aim of investigating galaxies with two strong simultaneous starbursts, we have extracted a sample of galaxies with double-peaked emission lines in their global spectra fro…

astro-ph.CO2011★ 13 cited

FIR measurements of Ly- emitters at z1.0: dust attenuation from PACS-\emph{Herschel}

I. Oteo, A. Bongiovanni, A. M. Pérez García +24

One remaining open question regarding the physical properties of Ly emitters (LAEs) is their dust content and its evolution with redshift. The variety of results is large and wi…

astro-ph.CO2011★ 417 cited

On Star Formation Rates and Star Formation Histories of Galaxies out to z ~ 3

Stijn Wuyts, Natascha M. Forster Schreiber, Dieter Lutz +23

We compare multi-wavelength SFR indicators out to z~3 in GOODS-South. Our analysis uniquely combines U-to-8um photometry from FIREWORKS, MIPS 24um and PACS 70, 100, and 160um photo…

astro-ph.CO2011★ 503 cited

PACS Evolutionary Probe (PEP) - A Herschel Key Program

D. Lutz, A. Poglitsch, B. Altieri +35

Deep far-infrared photometric surveys studying galaxy evolution and the nature of the cosmic infrared background are a key strength of the Herschel mission. We describe the scienti…

astro-ph.CO2011★ 104 cited

The impact of evolving infrared spectral energy distributions of galaxies on star formation rate estimates

R. Nordon, D. Lutz, R. Genzel +27

We combine Herschel-PACS data from the PEP program with Spitzer 24 um and 16 um photometry and ultra deep IRS mid-infrared spectra, to measure the mid- to far-infrared spectral ene…

astro-ph.CO2011★ 58 cited

The effect of environment on star forming galaxies at redshift 1 - First insight from PACS

P. Popesso, G. Rodighiero, A. Saintonge +4

We use deep 70, 100 and 160 um observations taken with PACS, the Photodetector Array Camera and Spectrometer on board of Herschel, as part of the PACS Evolutionary Probe (PEP) guar…