Matthieu Bethermin - Dissemin

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Papers authored by Matthieu Bethermin

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2010 M. Jauzac

ORCID

, H. Dole, E. Le Floc’h, H. Aussel, K. Caputi, O. Ilbert, M. Salvato, N. Bavouzet, A. Beelen, M. Béthermin

ORCID

ORCID

, G. Lagache, J.-L. Puget

The cosmic far-infrared background buildup since redshift 2 at 70 and 160 microns in the COSMOS and GOODS fields

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J. Glenn, A. Conley, M. Béthermin

ORCID

, B. Altieri, A. Amblard, V. Arumugam, H. Aussel, T. Babbedge, A. Blain, J. Bock, A. Boselli, V. Buat, N. Castro-Rodríguez, A. Cava

ORCID

, P. Chanial and 59 other authors

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

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I.~G G. Roseboom, S.~J J. Oliver, M. Kunz, B. Altieri, A. Amblard, V. Arumugam, R. Auld, H. Aussel, T. Babbedge, M. Béthermin

ORCID

, A. Blain, J. Bock, A. Boselli, D. Brisbin, V. Buat and 71 other authors

The Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE images

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M. Béthermin

ORCID

, H. Dole, M. Cousin, N. Bavouzet

Submillimeter number counts at 250 μm, 350 μm and 500 μm in BLAST data

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This paper was not found in any repository, but could be made available legally by the author.

M. Béthermin

ORCID

, H. Dole, A. Beelen, H. Aussel

Spitzerdeep and wide legacy mid- and far-infrared number counts and lower limits of cosmic infrared background

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This paper was not found in any repository; the policy of its publisher is unknown or unclear.

M. Béthermin

ORCID

, H. Dole, G. Lagache, D. Le Borgne, A. Penin

Modeling the evolution of infrared galaxies with a backward evolution model

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This paper was not found in any repository; the policy of its publisher is unknown or unclear.

M. Béthermin

ORCID

, H. Dole, M. Cousin, N. Bavouzet

Submillimeter number counts at 250 μ m, 350 μ m and 500 μ m in BLAST data

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This paper was not found in any repository; the policy of its publisher is unknown or unclear.

M. Bethermin

ORCID

, H. Dole

Measurements of the spectral energy distribution of the cosmic infrared background

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