Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Nicola Malavasi"'
Publikováno v:
The Astrophysical Journal, Vol 961, Iss 1, p 39 (2024)
We present a systematic study of the environmental impact on star formation activities of galaxies using a mass-complete sample of ∼170k galaxies at z < 4 from the latest COSMOS2020 catalog. At z < 1, we find that the mean star formation rate (SFR)
Externí odkaz:
https://doaj.org/article/32c1af9ca72e430eb795bb8e1359d255
Autor:
Yun Huang, Kyoung-Soo Lee, Olga Cucciati, Brian C. Lemaux, Marcin Sawicki, Nicola Malavasi, Vandana Ramakrishnan, Rui Xue, Letizia P. Cassara, Yi-Kuan Chiang, Arjun Dey, Stephen D. J. Gwyn, Nimish Hathi, Laura Pentericci, Moire K. M. Prescott, Gianni Zamorani
The discovery and spectroscopic confirmation of Hyperion, a protosupercluster at z ∼ 2.47, provides an unprecedented opportunity to study distant galaxies in the context of their large-scale environment. We carry out deep narrowband imaging of a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab6e2881f12334a77518defa4b5562d2
Filaments and clusters of the cosmic web have an impact on the properties of galaxies, switching off their star-formation, contributing to the build-up of their stellar mass, and influencing the acquisition of their angular momentum. In this work we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8f5dcd337bc45e1335cf9309e7fa4a7f
https://hal.archives-ouvertes.fr/hal-03378075
https://hal.archives-ouvertes.fr/hal-03378075
We present a detailed characterization of the Lya properties for 93 Lya emitters (LAEs) at z~3.1 selected from the D1 field of the Canada-France-Hawaii-Telescope Legacy Survey, including 24 members of a massive protocluster. The median-stacked Lya im
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::09595d9ef2d37c773dbb83292830aa6c
http://arxiv.org/abs/2104.11354
http://arxiv.org/abs/2104.11354
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.L2. ⟨10.1051/0004-6361/202038521⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.L2. ⟨10.1051/0004-6361/202038521⟩
Astronomy & Astrophysics
We report the first statistical detection of X-ray emission from cosmic web filaments in ROSAT data. We selected 15,165 filaments at 0.2
Comment: 7 pages, 8 figures, published by A&A as Letters
Comment: 7 pages, 8 figures, published by A&A as Letters
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba2388f2beef794a7aefc7acb9a82b57
https://hal.archives-ouvertes.fr/hal-02993736
https://hal.archives-ouvertes.fr/hal-02993736
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, 495 (4), pp.4237-4247. ⟨10.1093/mnras/staa1434⟩
Monthly Notices of the Royal Astronomical Society, 2020, 495 (4), pp.4237-4247. ⟨10.1093/mnras/staa1434⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 495 (4), pp.4237-4247. ⟨10.1093/mnras/staa1434⟩
Monthly Notices of the Royal Astronomical Society, 2020, 495 (4), pp.4237-4247. ⟨10.1093/mnras/staa1434⟩
We investigate the connection between X-ray and radio-loud AGNs and the physical properties of their evolved and massive host galaxies, focussing on the mass-related quenching channel followed by $\mathcal{M}^\star (\simeq 10^{10.6} M_\odot)$ galaxie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f4f3933f127ce2c688539e62f288492
https://hal-cnrs.archives-ouvertes.fr/hal-03100524
https://hal-cnrs.archives-ouvertes.fr/hal-03100524
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 641, pp.A173. ⟨10.1051/0004-6361/202037986⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 641, pp.A173. ⟨10.1051/0004-6361/202037986⟩
Astronomy & Astrophysics
We present a statistical study of the filamentary structures of the cosmic web in the large hydro-dynamical simulations Illustris-TNG, Illustris, and Magneticum at redshift z=0. We focus on the radial distribution of the galaxy density around filamen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b4c9aeb4f2537468fa3d4d70b56dd716
https://hal.archives-ouvertes.fr/hal-02542826
https://hal.archives-ouvertes.fr/hal-02542826
Publikováno v:
Astron.Astrophys.
Astron.Astrophys., 2020, 634, pp.A30. ⟨10.1051/0004-6361/201936629⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 634, pp.A30. ⟨10.1051/0004-6361/201936629⟩
Astron.Astrophys., 2020, 634, pp.A30. ⟨10.1051/0004-6361/201936629⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 634, pp.A30. ⟨10.1051/0004-6361/201936629⟩
The Cosmic Web is a complex network of filaments, walls and voids that represent the largest structures in the Universe. In this network, which is the direct result of structure formation, galaxy clusters occupy central positions as the nodes, connec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2bf5b3bc2a8622204073b4d360f8a25
https://hal.archives-ouvertes.fr/hal-02410547
https://hal.archives-ouvertes.fr/hal-02410547
Autor:
Thibaud Moutard, C. Adami, Nicola Malavasi, Stéphane Arnouts, Marcin Sawicki, Anneya Golob, Jean Coupon, Olivier Ilbert
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, 2018, 479 (2), pp.2147-2160. ⟨10.1093/mnras/sty1543⟩
Monthly Notices of the Royal Astronomical Society, 2018, 479 (2), pp.2147-2160. ⟨10.1093/mnras/sty1543⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 479 (2), pp.2147-2160. ⟨10.1093/mnras/sty1543⟩
Monthly Notices of the Royal Astronomical Society, 2018, 479 (2), pp.2147-2160. ⟨10.1093/mnras/sty1543⟩
We investigate the connection between environment and the different quenching channels that galaxies are prone to follow in the rest-frame NUVrK colour diagram, as identified by Moutard et al. (2016b). Namely, the fast quenching channel followed by $
Publikováno v:
The Astrophysical Journal. 921:103