The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations

Abstract

We present results from the deepest Herschel-PACS (Photodetector Array Camera and Spectrometer) far-infrared blank field extragalactic survey, obtained by combining observations of the GOODS (Great Observatories Origins Deep Survey) fields from the PACS Evolutionary Probe (PEP) and GOODS-Herschel key programmes. We describe data reduction and the construction of images and catalogues. In the deepest parts of the GOODS-S field, the catalogues reach 3-sigma depths of 0.9, 0.6 and 1.3 mJy at 70, 100 and 160 um, respectively, and resolve ~75% of the cosmic infrared background at 100um and 160um into individually detected sources. We use these data to estimate the PACS confusion noise, to derive the PACS number counts down to unprecedented depths and to determine the infrared luminosity function of galaxies down to LIR=10^11 Lsun at z~1 and LIR=10^12 Lsun at z~2, respectively. For the infrared luminosity function of galaxies, our deep Herschel far-infrared observations are fundamental because they provide more accurate infrared luminosity estimates than those previously obtained from mid-infrared observations. Maps and source catalogues (>3-sigma) are now publicly released. Combined with the large wealth of multi-wavelength data available for the GOODS fields, these data provide a powerful new tool for studying galaxy evolution over a broad range of redshifts.

Accepted for publication in A&A; 22 pages, 13 figures; V2: updated to match accepted version

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• ALMA 26 arcmin${}^2$ survey of GOODS-S at one-millimeter (ASAGAO): millimeter properties of stellar mass selected galaxies
• Morphological Evolution of the Hosts of Far-Infrared/Submillimeter Galaxies
• The OTELO survey. III. Demography, morphology, IR luminosity and environment of AGN hosts
• The ALMA Frontier Fields survey V: ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223
• The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at $z\sim 5$
• Diffuse supernova neutrino background with up-to-date star formation rate measurements and long-term multidimensional supernova simulations
• A${}^3$COSMOS: Measuring the cosmic dust-attenuated star formation rate density at $4<z<5$
• Dust Temperature of Compact Star-forming Galaxies at $z\sim 1-3$ in 3D-{\it HST}/CANDELS
• High-z dusty star-forming galaxies: a top-heavy initial mass function?
• Trident: A three-pronged galaxy survey. I. Lyman alpha emitting galaxies at z~2 in GOODS North
• The Infrared Luminosity Function of AKARI 90$\mu$m Galaxies in the Local Universe
• Are z>2 Herschel galaxies proto-spheroids?
• Dust Properties of Local Dust-Obscured Galaxies with the Submillimeter Array
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• The star-forming main sequence and the contribution of dust-obscured star formation since $z\sim 4$ from the FUV+IR luminosity functions
• Probabilistic and progressive deblended far-infrared and sub-millimetre point source catalogues I. Methodology and first application in the COSMOS field
• Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• Confusion of extragalactic sources in the far infrared: a baseline assessment of the performance of PRIMAger in intensity and polarization
• JWST PRIMER: A deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS -- dust-obscured star-formation history back to z $\simeq$ 7
• The Far-Infrared-Radio Correlation in MS0451-03
• Low-frequency radio spectra of submillimetre galaxies in the Lockman Hole
• Kinematics of the ionized and molecular gas in nearby luminous infrared interacting galaxies
• Estimating the confusion noise for the Millimetron space telescope
• Herschel and ALMA Observations of Massive SZE-selected Clusters
• Revealing Dusty Supernovae in High-Redshift (Ultra-)Luminous InfraRed Galaxies Through Near-Infrared Integrated Light Variability
• How accurate are infrared luminosities from monochromatic photometric extrapolation?
• Cosmic star formation history with tomographic cosmic infrared background-galaxy cross-correlation
• Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• Exploring the evolution of star formation and dwarf galaxy properties with JWST/MIRI serendipitous spectroscopic surveys
• Properties of galaxies at the faint end of the H$\alpha$ luminosity function at $z\sim 0.62$
• Multiwavelength characterisation of an ACT-selected, lensed dusty star-forming galaxy at z=2.64
• CONCERTO at APEX -- On-sky performance in continuum
• A${}^3$COSMOS: The dust content of massive quiescent galaxies and its evolution with cosmic time
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Exploring the multiband gravitational wave background with a semi-analytic galaxy formation model
• AKARI and IRAS: From Beam Corrections to SEDs
• The Role of Radio Observations in Studies of Infrared-Bright Galaxies: Prospects for a next-generation Very Large Array
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z=1-6
• A surprising consistency between the far-infrared galaxy luminosity functions of the field and Coma
• Euclid view of dusty star forming galaxies at z>~1.5 detected in wide area submillimetre surveys
• A mock redshift catalogue of the dusty star-forming galaxy population with intrinsic clustering and lensing for deep millimetre surveys
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• A Submillimeter Continuum Survey of Local Dust-Obscured Galaxies
• The Evolution of the Luminosity Function for Luminous Compact Blue Galaxies to z=1
• Probing the Infrared/Radio correlation of the full IRAS Revised Bright Galaxy Sample with MeerKAT and the VLA
• Simulating infrared spectro-photometric surveys with a SPRITZ
• Ultraviolet-to-far-infra-red self-consistent analysis of the stellar populations of massive starburst galaxies at intermediate redshifts
• Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6
• JWST MIRI color classification of mid-infrared selected galaxies: MIRI color classification toward cosmic noon
• Searching Far and Long I: Pilot ALMA 2mm Follow-up of Bright Dusty Galaxies as a Redshift Filter
• The Nature of Hyperluminous Infrared Galaxies