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The ALPINE−ALMA [C ii] Survey: on the nature of an extremely obscured serendipitous galaxy

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 496, pp.875-887. ⟨10.1093/mnras/staa1546⟩
Monthly Notices of the Royal Astronomical Society, 496(1), 875-887
Romano, M, Cassata, P, Morselli, L, Lemaux, B C, Bethermin, M, Capak, P, Faisst, A, Le Fevre, O, Schaerer, D, Silverman, J, Yan, L, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Enia, A, Fudamoto, Y, Fujimoto, S, Ginolfi, M, Gruppioni, C, Hathi, N P, Ibar, E, Jones, G C, Koekemoer, A M, Loiacono, F, Mancini, C, Riechers, D A, Rodighiero, G, Rodriguez-Munoz, L, Talia, M, Vallini, L, Vergani, D, Zamorani, G & Zucca, E 2020, ' The ALPINE ALMA [C II] Survey : on the nature of an extremely obscured serendipitous galaxy ', Monthly Notices of the Royal Astronomical Society, vol. 496, no. 1, pp. 875-887 . https://doi.org/10.1093/mnras/staa1546

We report the serendipitous discovery of a bright galaxy (Gal-A) observed as part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE). While this galaxy is detected both in line and continuum emission in ALMA Band 7, it is complete

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28b6c63da46606e298e0f0bf35412702
https://doi.org/10.1093/mnras/staa1546

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Euclid: the selection of quiescent and star-forming galaxies using observed colours

Autor: F. J. Castander, Rafael Toledo-Moreo, L. Bisigello, Marc Sauvage, M. Poncet, Ulrike Kuchner, H. Israel, R. Cledassou, S. Kermiche, Crescenzo Tortora, F. Sureau, Sebastiano Ligori, R. Kohley, Sandrine Pires, Jarle Brinchmann, Mauro Roncarelli, Michele Moresco, G. Zamorani, Andy Taylor, G. Meylan, Andrea Cimatti, Natalia Auricchio, J. Carretero, B. Kubik, M. Wetzstein, Lucia Pozzetti, Thomas D. Kitching, Felix Hormuth, Stefano Andreon, E. Franceschi, Claudia Maraston, M. Bolzonella, Roberto P. Saglia, Martin Kunz, Simona Mei, D. Masters, M. Frailis, Andrew Humphrey, Leonardo Corcione, A. Secroun, Mark Cropper, Ismael Tereno, G. Polenta, V. Capobianco, Jason Rhodes, L. Valenziano, Ivan Lloro, S. Serrano, Peter Schneider, Elisabetta Maiorano, L. Conversi, Fabio Pasian, Ole Marggraf, G. Congedo, P. B. Lilje, S. Dusini, S. Paltani, Y. Mellier, Valeria Pettorino, P. Franzetti, C. J. Conselice, F. Raison, B. Garilli, Yu Wang, Marco Castellano, M. Fumana, O. Le Fevre, Richard Massey, Knud Jahnke, Pierre-Alain Duc, Stefano Cavuoti, Emanuel Rossetti, C. Padilla, Julien Zoubian

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 494 (2), pp.2337-2354. ⟨10.1093/mnras/staa885⟩
Congedo, G & Taylor, A N 2020, ' Euclid: The selection of quiescent and star-forming galaxies using observed colours? ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 2, pp. 2337-2354 . https://doi.org/10.1093/mnras/staa885
Monthly Notices of the Royal Astronomical Society, 2020, 494 (2), pp.2337-2354. ⟨10.1093/mnras/staa885⟩

The Euclid mission will observe well over a billion galaxies out to $z\sim6$ and beyond. This will offer an unrivalled opportunity to investigate several key questions for understanding galaxy formation and evolution. The first step for many of these

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5df23b5f5cdef750af13d84c6731db12
https://doi.org/10.1093/mnras/staa885

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Establishing a new technique for discovering large-scale structure using the ORELSE survey

Autor: Brian C. Lemaux, Dale D. Kocevski, Lu Shen, G. K. Squires, Roy R. Gal, Debora Pelliccia, Simona Mei, O. Cucciati, Lori M. Lubin, O. Le Fevre, Adam Tomczak, Denise Hung, Po-Feng Wu

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 491, pp.5524-5554. ⟨10.1093/mnras/stz3164⟩

The Observations of Redshift Evolution in Large Scale Environments (ORELSE) survey is an ongoing imaging and spectroscopic campaign initially designed to study the effects of environment on galaxy evolution in high-redshift ($z\sim1$) large-scale str

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0b78a0ae476c9d06b42bc737dbfc0852
https://doi.org/10.1093/mnras/stz3164

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An Optical Observational Cluster Mass Function at $z\sim1$ with the ORELSE Survey

Autor: Dale D. Kocevski, O. Cucciati, Lori M. Lubin, G. Zamorani, G. K. Squires, Po-Feng Wu, Lu Shen, Brian C. Lemaux, Roy R. Gal, Christopher D. Fassnacht, Denise Hung, Debora Pelliccia, Adam Tomczak, O. Le Fevre

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 502 (3), pp.3942-3954. ⟨10.1093/mnras/stab300⟩
Monthly Notices of the Royal Astronomical Society, 2021, 502 (3), pp.3942-3954. ⟨10.1093/mnras/stab300⟩

We present a new mass function of galaxy clusters and groups using optical/near-infrared wavelength spectroscopic and photometric data from the Observations of Redshift Evolution in Large-Scale Environments (ORELSE) survey. At $z\sim1$, cluster mass

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b413e92e1d788fed1e1462171a739e3d
http://arxiv.org/abs/2101.02215

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The ALPINE-ALMA [CII] Survey: Kinematic Diversity & Rotation in Massive Star Forming Galaxies at z~4.4-5.9

Publikováno v: Monthly Notices of the Royal Astronomical Society (MNRAS)
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 507 (3), pp.3540-3563. ⟨10.1093/mnras/stab2226⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 507 (3), pp.3540-3563. ⟨10.1093/mnras/stab2226⟩

While the kinematics of galaxies up to z~3 have been characterized in detail, only a handful of galaxies at high redshift (z>4) have been examined in such a way. The Atacama Large Millimeter/submillimeter Array (ALMA) Large Program to INvestigate [CI

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e88c93d1f4b88b0b9dd42bb8e73480bc

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Less and more IGM-transmitted galaxies from z ∼ 2.7 to z ∼ 6 from VANDELS and VUDS

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 650, pp.A63. ⟨10.1051/0004-6361/202038438⟩
Astronomy and Astrophysics-A&A, 2021, 650, pp.A63. ⟨10.1051/0004-6361/202038438⟩

Aim. Our aim is to analyse the variance of the Inter-Galactic Medium transmission (IGM) by studying this parameter in the rest-frame UV spectra of a large sample of high redshift galaxies. Method. We make use of the VIMOS Ultra Deep Survey and the VA

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::25517bc34e6a41908675cab926919f07
https://hal.archives-ouvertes.fr/hal-03178619

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The ALPINE-ALMA [C II] Survey: [C II] 158 μm Emission Line Luminosity Functions at z ~ 4–6

Publikováno v: The Astrophysical Journal, 905(2), 147
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2020, 905 (2), pp.147. ⟨10.3847/1538-4357/abc41c⟩

We present the [CII]158$\mu$m line luminosity functions (LFs) at $z\sim4-6$ using the ALMA observations of 118 sources, which are selected to have UV luminosity $M_{1500A}10^9L_{\odot}$, suggesting that UV-faint but [CII]-bright sources likely make a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5897f1c29a2717a789d5a64594223d84
https://resolver.caltech.edu/CaltechAUTHORS:20200824-123559194

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The ALPINE-ALMA [CII] survey:Molecular gas budget in the early Universe as traced by [CII]

Publikováno v: Dessauges-Zavadsky, M, Ginolfi, M, Pozzi, F, Bethermin, M, Le Fevre, O, Fujimoto, S, Silverman, J D, Jones, G C, Vallini, L, Schaerer, D, Faisst, A L, Khusanova, Y, Fudamoto, Y, Cassata, P, Loiacono, F, Capak, P L, Yan, L, Amorin, R, Bardelli, S, Boquien, M, Cimatti, A, Gruppioni, C, Hathi, N P, Ibar, E, Koekemoer, A M, Lemaux, B C, Narayanan, D, Oesch, P A, Rodighiero, G, Romano, M, Talia, M, Toft, S, Vergani, D, Zamorani, G & Zucca, E 2020, ' The ALPINE-ALMA [CII] survey : Molecular gas budget in the early Universe as traced by [CII] ', Astronomy & Astrophysics, vol. 643, A5 . https://doi.org/10.1051/0004-6361/202038231
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 643, ⟨10.1051/0004-6361/202038231⟩
Astronomy & Astrophysics, 643, A5

The molecular gas content of normal galaxies at z>4 is poorly constrained, because the commonly used molecular gas tracers become hard to detect. We use the [CII]158um luminosity, recently proposed as a molecular gas tracer, to estimate the molecular

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1fcbb1d016117b012c3b7aa057d50166
https://curis.ku.dk/portal/da/publications/the-alpinealma-cii-survey(e8a9d6ba-a0e3-4f24-be9f-9140d62b5251).html

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The ALPINE-ALMA [CII] survey: Small Ly$\alpha$-[CII] velocity offsets in main-sequence galaxies at 4.4 < z < 6

Publikováno v: Cassata, P, Morselli, L, Faisst, A, Ginolfi, M, Bethermin, M, Capak, P, Le Fevre, O, Schaerer, D, Silverman, J, Yan, L, Lemaux, B C, Romano, M, Talia, M, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Fudamoto, Y, Fujimoto, S, Giavalisco, M, Hathi, N P, Ibar, E, Jones, G, Koekemoer, A M, Mendez-Hernandez, H, Mancini, C, Oesch, P A, Pozzi, F, Riechers, D A, Rodighiero, G, Vergani, D, Zamorani, G & Zucca, E 2020, ' The ALPINE-ALMA [CII] survey : Small Ly alpha-[CII] velocity offsets in main-sequence galaxies at 4.4 Astron.Astrophys.
Astron.Astrophys., 2020, 643, pp.A6. ⟨10.1051/0004-6361/202037517⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 643, pp.A6. ⟨10.1051/0004-6361/202037517⟩

The Lya line in the UV and the [CII] line in the FIR are widely used tools to identify galaxies and to obtain insights into ISM properties in the early Universe. By combining data obtained with ALMA in band 7 at ~ 320 GHz as part of the ALMA Large Pr

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c3df405c180d2eccbb93f50ec657e422
https://hal.archives-ouvertes.fr/hal-02491249

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The ALPINE-ALMA [CII] survey: Survey strategy, observations and sample properties of 118 star-forming galaxies at $4 < z < 6$

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A1. ⟨10.1051/0004-6361/201936965⟩
Le Fevre, O, Bethermin, M, Faisst, A, Jones, G C, Capak, P, Cassata, P, Silverman, J D, Schaerer, D, Yan, L, Amorin, R, Bardelli, S, Boquien, M, Cimatti, A, Dessauges-Zavadsky, M, Giavalisco, M, Hathi, N P, Fudamoto, Y, Fujimoto, S, Ginolfi, M, Gruppioni, C, Hemmati, S, Ibar, E, Koekemoer, A, Khusanova, Y, Lagache, G, Lemaux, B C, Loiacono, F, Maiolino, R, Mancini, C, Narayanan, D, Morselli, L, Mendez-Hernandez, H, Oesch, P A, Pozzi, F, Romano, M, Riechers, D, Scoville, N, Talia, M, Tasca, L A M, Thomas, R, Toft, S, Vallini, L, Vergani, D, Walter, F, Zamorani, G & Zucca, E 2020, ' The ALPINE-ALMA [CII] survey Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 Astronomy and Astrophysics-A&A, 2020, 643, pp.A1. ⟨10.1051/0004-6361/201936965⟩
Astronomy & Astrophysics
Astronomy & Astrophysics, 643, A1

The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) features 118 galaxies observed in the [CII]-158$\mu$m line and far infrared (FIR

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f3bdadb79da4f3a1d2fd1e7cd920bad
https://hal.archives-ouvertes.fr/hal-02432539

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