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Paper
IPM / Astronomy / 18189 |
School of Astronomy
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Title: |
A panchromatic view of N2CLS GOODS-N: the evolution of the dust cosmic density since z~7
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Author(s): |
| 1. |
S. Berta
| | 2. |
G. Lagache
| | 3. |
A. Beelen
| | 4. |
R. Adam
| | 5. |
P. Ade
| | 6. |
H. Ajeddig
| | 7. |
S. Amarantidis
| | 8. |
P. Andre
| | 9. |
H. Aussel
| | 10. |
A. Benoit
| | 11. |
M. Bethermin
| | 12. |
L.J. Bing
| | 13. |
A. Bongiovanni
| | 14. |
J. Bounmy
| | 15. |
O. Bourrion
| | 16. |
M. Calvo
| | 17. |
A. Catalano
| | 18. |
D. Cherouvrier
| | 19. |
L. Ciesla
| | 20. |
M. De Petris
| | 21. |
F.X. Desert
| | 22. |
S. Doyle
| | 23. |
E.F.C. Driessen
| | 24. |
G. Ejlali
| | 25. |
D. Elbaz
| | 26. |
A. Ferragamo
| | 27. |
A. Gomez
| | 28. |
J. Goupy
| | 29. |
C. Hanser
| | 30. |
S. Katsioli
| | 31. |
F. Mayet
| | 32. |
C. Kramer
| | 33. |
B. Ladjelate
| | 34. |
F. Keruzore
| | 35. |
S. Leclercq
| | 36. |
J.F. Lestrade
| | 37. |
J.F. Macias-Perez
| | 38. |
S.C. Madden
| | 39. |
A. Maury
| | 40. |
P. Mauskopf
| | 41. |
F. Mayet
| | 42. |
J.B. Melin
| | 43. |
A. Monfardini
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A. Moyer-Anin
| | 45. |
M. Munoz-Echeverria
| | 46. |
L. Perotto
| | 47. |
G. Pisano
| | 48. |
E. Pointecouteau
| | 49. |
N. Ponthieu
| | 50. |
G.W. Pratt
| | 51. |
V. Reveret
| | 52. |
A.J. Rigby
| | 53. |
A. Ritacco
| | 54. |
C. Romero
| | 55. |
H. Roussel
| | 56. |
F. Ruppin
| | 57. |
K. Schuster
| | 58. |
A. Sievers
| | 59. |
C. Tucker
| | 60. |
M.Y. Xiao
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R. Zylka
| | 62. |
H. Messias
| | 63. |
I. Myserlis
| | 64. |
R. Neri
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A. Paliwal
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Status: |
Published
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Journal: |
Astronomy & Astrophysics
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No.: |
193
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Vol.: |
696
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Year: |
2025
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Pages: |
1-48
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Supported by: |
IPM
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Abstract: |
To understand early star formation, it is essential to determine the dust mass budget of high-redshift galaxies. Sub-millimeter rest-frame emission, dominated by cold dust, is an unbiased tracer of dust mass. The NIKA2 camera conducted a deep blank field survey at 1.2 and 2.0 mm in the GOODS-N field as part of the NIKA2 Cosmological Legacy Survey (N2CLS), detecting 65 sources with SNR>=4.2. Thanks to a dedicated interferometric program with NOEMA and other high-angular resolution data, we identify the multi-wavelength counterparts of these sources and resolve them into 71 individual galaxies. We build detailed SEDs and assign a redshift to 68 of them, over the range 0.6
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