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Cited by 428

The DOI matches its Crossref record; 46 of the 46 references it cites were found in a registry or an index.

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

Open access
Magnelli, B., Popesso, P., Berta, S., Pozzi, F., Elbaz, D., Lutz, D., Dickinson, M., Altieri, B., Andreani, P., Aussel, H., Béthermin, M., Bongiovanni, A., Cepa, J., Charmandaris, V., Chary, R.-R., Cimatti, A., Daddi, E., Förster Schreiber, N. M., Genzel, R., Gruppioni, C., Harwit, M., Hwang, H. S., Ivison, R. J., Magdis, G., Maiolino, R., Murphy, E., Nordon, R., Pannella, M., Pérez García, A., Poglitsch, A., Rosario, D., Sanchez-Portal, M., Santini, P., Scott, D., Sturm, E., Tacconi, L. J., Valtchanov, I.·2013·Astronomy & Astrophysics
DOI 10.1051/0004-6361/201321371
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Abstract

We present results from the deepest Herschel-Photodetector Array Camera and Spectrometer (PACS) far-infrared blank field extragalactic survey, obtained by combining observations of the Great Observatories Origins Deep Survey (GOODS) fields from the PACS Evolutionary Probe (PEP) and GOODS-Herschel key programmes. We describe data reduction and theconstruction of images and catalogues. In the deepest parts of the GOODS-S field, the catalogues reach 3σ depths of 0.9, 0.6 and 1.3 mJy at 70, 100 and 160 μm, respectively, and resolve ~75% of the cosmic infrared background at 100 μm and 160 μm 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 = 1011 L⊙ at z ~ 1 and LIR = 1012 L⊙ 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 (>3σ) 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.

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Authors
Magnelli, B., Popesso, P., Berta, S., Pozzi, F., Elbaz, D., Lutz, D., Dickinson, M., Altieri, B., Andreani, P., Aussel, H., Béthermin, M., Bongiovanni, A., Cepa, J., Charmandaris, V., Chary, R.-R., Cimatti, A., Daddi, E., Förster Schreiber, N. M., Genzel, R., Gruppioni, C., Harwit, M., Hwang, H. S., Ivison, R. J., Magdis, G., Maiolino, R., Murphy, E., Nordon, R., Pannella, M., Pérez García, A., Poglitsch, A., Rosario, D., Sanchez-Portal, M., Santini, P., Scott, D., Sturm, E., Tacconi, L. J., & Valtchanov, I.
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2013-05
Volume
553
Pages
A132
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
DOI
10.1051/0004-6361/201321371
OpenAlex
W2114816526
Cited by
428
References
46
FWCI
24.43
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations. https://app.cochat.ai/papers/10.1051/0004-6361/201321371
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Magnelli, B., Popesso, P., Berta, S., Pozzi, F., Elbaz, D., Lutz, D., Dickinson, M., Altieri, B., Andreani, P., Aussel, H., Béthermin, M., Bongiovanni, A., Cepa, J., Charmandaris, V., Chary, R.-R., Cimatti, A., Daddi, E., Förster Schreiber, N. M., Genzel, R., . . . Valtchanov, I. (2013). The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201321371

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.