Published March 4, 2025
| Version Accepted version
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A panchromatic view of N2CLS GOODS-N: the evolution of the dust cosmic density since z~7. Figure E.1
Authors/Creators
- Berta, S. (Contact person)1
- Lagache, G. (Project leader)2
- Beelen, A. (Project leader)2
- Adam, R. (Project member)3
- Ade, P. (Project member)4
- Ajeddig, H. (Project member)5
- Amarantidis, S. (Project member)6
- André, P. (Project member)5
- Aussel, H. (Project member)5
- Benoit, A. (Project member)7
- et al. Show all 61 authors
Authors/Creators
- Berta, S. (Contact person)1
- Lagache, G. (Project leader)2
- Beelen, A. (Project leader)2
- Adam, R. (Project member)3
- Ade, P. (Project member)4
- Ajeddig, H. (Project member)5
- Amarantidis, S. (Project member)6
- André, P. (Project member)5
- Aussel, H. (Project member)5
- Benoit, A. (Project member)7
- Bethermin, M. (Project member)8
- Bing, L. J. (Project member)9
- Bongiovanni, A. (Project member)6
- Bounmy, J. (Project member)10
- Bourrion, O. (Project member)10
- Calvo, M. (Project member)7
- Catalano, A. (Project member)10
- Chérouvrier, D. (Project member)10
- Ciesla, L. (Project member)2
- De Petris, M. (Project member)11
- Désert, F. X. (Project member)12
- Doyle, S. (Project member)13
- Driessen, E. F. C. (Project member)1
- Ejlali, G. (Project member)14
- Elbaz, D. (Project member)5
- Ferragamo, A. (Project member)11, 15
- Gomez, A. (Project member)16
- Goupy, J. (Project member)7
- Hanser, C. (Project member)10
- Katsioli, S. (Project member)17, 18
- Kéruzoré, F. (Project member)19
- Kramer, C. (Project member)1
- Ladjelate, B. (Project member)6
- Leclercq, S. (Project member)1
- Lestrade, J. F. (Project member)20
- Macias-Perez, J. F. (Project member)10
- Madden, S. C. (Project member)5
- Maury, A. (Project member)21, 22, 23
- Mayet, F. (Project member)10
- Messias, H. (Project member)24, 25
- Monfardini, A. (Project member)7
- Moyer-Anin, A. (Project member)10
- Muñoz-Echeverria, M. (Project member)26
- Myserlis, I. (Project member)6
- Neri, R. (Project member)1
- Paliwal, A. (Project member)11
- Perotto, L. (Project member)10
- Pisano, G. (Project member)11
- Ponthieu, N. (Project leader)12
- Revéret, V. (Project member)5
- Rigby, A. J. (Project member)27
- Ritacco, A.28, 29
- Roussel, H. (Project member)30
- Rupin, F. (Project member)31
- Sanchez-Portal, M. (Project member)6
- Savorgnano, S. (Project member)10
- Schuster, K. (Project member)1
- Sievers, A. (Project member)6
- Tucker, C. (Project member)13
- Xiao, M. Y. (Project member)32
- Zylka, R. (Project member)1
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1.
Institut de Radioastronomie Millimétrique
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2.
Laboratoire d'Astrophysique de Marseille
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3.
Observatoire de la Côte d'Azur
- 4. Cardiff University, School of Physics and Astronomy
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5.
CEA Paris-Saclay - Etablissement de Saclay
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6.
Instituto de Radioastronomía Milimétrica
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7.
Institut Néel
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8.
Université de Strasbourg
- 9. Astronomy Centre, University of Sussex
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10.
Laboratoire de Physique Subatomique et de Cosmologie
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11.
Sapienza University of Rome
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12.
Institut de Planétologie et d'Astrophysique de Grenoble
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13.
Cardiff University
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14.
Institute for Research in Fundamental Sciences
- 15. Universita' di Napoli, Federico II
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16.
Centro de Astrobiología
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17.
National Observatory of Athens
- 18. University of Athens, Department of Astrophysics
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19.
Argonne National Laboratory
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20.
Laboratoire d'Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères
- 21. Institute of Space Sciences (ICE), Barcelona
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22.
Catalonian Institute for Acances Studies and Research
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23.
CEA Paris-Saclay
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24.
Atacama Large Millimeter Submillimeter Array
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25.
European Southern Observatory
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26.
Institut de Recherche en Astrophysique et Planétologie
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27.
University of Leeds
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28.
University of Rome Tor Vergata
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29.
École Normale Supérieure - PSL
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30.
Institut d'Astrophysique de Paris
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31.
Institut de Physique des 2 Infinis de Lyon
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32.
University of Geneva
Description
Supplementary material of the paper "A panchromatic view of N2CLS GOODS-N: the evolution of the dust cosmic density since z~7", accepted for publication on Astronomy & Astrophysics.
Figure E.1: N2GN individual sources: multi-wavelength postage stamps and SED fitting results.