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Building the cosmic infrared background brick by brick with Herschel/PEP

Building the cosmic infrared background brick by brick with Herschel/PEP

http://www.wikidata.org/entity/Q58911970

about

A DEBRIS disk around the planet hosting M-star GJ 581 spatially resolved withHerschel Resolved debris discs around A stars in the Herschel DEBRIS survey Herschel ★ -ATLAS: properties of dusty massive galaxies at low and high redshifts A Herschel view of the far-infrared properties of submillimetre galaxies Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation HerMES: deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background GOODS-Herschel: identification of the individual galaxies responsible for the 80–290μm cosmic infrared background Mid- to far-infrared properties of star-forming galaxies and active galactic nuclei Dust temperature and CO → H₂ conversion factor variations in the SFR-M∗ plane Probing star formation in the dense environments of z ∼ 1 lensing haloes aligned with dusty star-forming galaxies detected with the South Pole Telescope Multi-wavelength characterisation ofz~ 2 clustered, dusty star-forming galaxies discovered byPlanck The redshift evolution of the distribution of star formation among dark matter halos as seen in the infrared The Herschel PEP/HerMES luminosity function – I. Probing the evolution of PACS selected Galaxies to z ≃ 4 An accurate measurement of the anisotropies and mean level of the cosmic infrared background at 100 μm and 160 μm DUst around NEarby Stars. The survey observational results Herschelobservations of the debris disc around HIP 92043 The composite nature of Dust-Obscured Galaxies (DOGs) atz ∼ 2–3 in the COSMOS field – I. A far-infrared view Upper limit on the cosmological gamma-ray background The host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACS Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observations Mapping the average AGN accretion rate in the SFR–M* plane for Herschel★-selected galaxies at 0 < z ≤ 2.5 Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy atz ~ 3.3 Dust attenuation inz~ 1 galaxies fromHerscheland 3D-HST Hαmeasurements The influence of wavelength, flux, and lensing selection effects on the redshift distribution of dusty, star-forming galaxies The evolution of the dust and gas content in galaxies Black hole accretion preferentially occurs in gas-rich galaxies*The Herschel census of infrared SEDs through cosmic time Panchromatic spectral energy distributions ofHerschelsources Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies TheHerschel -ATLAS data release 1 – I. Maps, catalogues and number counts

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Building the cosmic infrared background brick by brick with Herschel/PEP

http://www.wikidata.org/entity/Q58911970

description

article publié dans la revue scientifique Astronomy and Astrophysics

@fr

im Juli 2011 veröffentlichter wissenschaftlicher Artikel

@de

scientific article published in Astronomy and Astrophysics

@en

wetenschappelijk artikel

@nl

наукова стаття, опублікована в липні 2011

@uk

name

Building the cosmic infrared background brick by brick with Herschel/PEP

@en

Building the cosmic infrared background brick by brick with Herschel/PEP

@nl

type

label

Building the cosmic infrared background brick by brick with Herschel/PEP

@en

Building the cosmic infrared background brick by brick with Herschel/PEP

@nl

prefLabel

Building the cosmic infrared background brick by brick with Herschel/PEP

@en

Building the cosmic infrared background brick by brick with Herschel/PEP

@nl

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P1433

Astronomy and Astrophysics

P1476

Building the cosmic infrared background brick by brick with Herschel/PEP

@en

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A. Cimatti

http://www.w3.org/2001/XMLSchema#string

A. Poglitsch

http://www.w3.org/2001/XMLSchema#string

E. Le Floc’h

http://www.w3.org/2001/XMLSchema#string

E. Sturm

http://www.w3.org/2001/XMLSchema#string

F. Pozzi

http://www.w3.org/2001/XMLSchema#string

H. Castañeda

http://www.w3.org/2001/XMLSchema#string

I. Pérez-Fournon

http://www.w3.org/2001/XMLSchema#string

I. Valtchanov

http://www.w3.org/2001/XMLSchema#string

J. Cepa

http://www.w3.org/2001/XMLSchema#string

L. J. Tacconi

http://www.w3.org/2001/XMLSchema#string

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The Spitzer Space Telescope Mission

High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey

TheCOBEDiffuse Infrared Background Experiment Search for the Cosmic Infrared Background. I. Limits and Detections

TheHerschel-SPIRE instrument and its in-flight performance

The Photodetector Array Camera and Spectrometer (PACS) on the HerschelSpace Observatory

The Large Apex BOlometer Camera survey of the Extended Chandra Deep Field South

A Deep Submillimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution

HerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observations

The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue

Observations of the Hubble Deep Field with the Infrared Space Observatory - III. Source counts and P(D) analysis

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49–49

http://www.w3.org/2001/XMLSchema#string

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scholarly article

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10.1051/0004-6361/201116844

http://www.w3.org/2001/XMLSchema#string

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P478

532

http://www.w3.org/2001/XMLSchema#string

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Roberto Maiolino

Giulia Rodighiero

Benjamin Magnelli

Reinhard Genzel

Natascha M. Förster Schreiber

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2011-07-22T00:00:00Z

http://www.w3.org/2001/XMLSchema#dateTime

P818

1106.3070

http://www.w3.org/2001/XMLSchema#string

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2011A&A...532A..49B

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