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pro vyhledávání: '"ILLUSTRIS PROJECT"'
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Autor:
Romeel Davé, Antonios Katsianis, Xiaohu Yang, Ping Zhao, Yu Luo, Haojie Xu, Xianzhong Zheng, Weiguang Cui, Claudia del P. Lagos
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Katsianis, A, Xu, H, Yang, X, Luo, Y, Cui, W, Davé, R, Lagos, C D P, Zheng, X & Zhao, P 2021, ' The specific star formation rate function at different mass scales and quenching: a comparison between cosmological models and SDSS ', Monthly Notices of the Royal Astronomical Society, vol. 500, no. 2, pp. 2036-2048 . https://doi.org/10.1093/mnras/staa3236
Katsianis, A, Xu, H, Yang, X, Luo, Y, Cui, W, Dave, R, Lagos, C D P, Zheng, X & Zhao, P 2021, ' The specific star formation rate function at different mass scales and quenching : a comparison between cosmological models and SDSS ', Monthly Notices of the Royal Astronomical Society, vol. 500, no. 2, pp. 2036-2048 . https://doi.org/10.1093/mnras/staa3236
Katsianis, A, Xu, H, Yang, X, Luo, Y, Cui, W, Davé, R, Lagos, C D P, Zheng, X & Zhao, P 2021, ' The specific star formation rate function at different mass scales and quenching: a comparison between cosmological models and SDSS ', Monthly Notices of the Royal Astronomical Society, vol. 500, no. 2, pp. 2036-2048 . https://doi.org/10.1093/mnras/staa3236
Katsianis, A, Xu, H, Yang, X, Luo, Y, Cui, W, Dave, R, Lagos, C D P, Zheng, X & Zhao, P 2021, ' The specific star formation rate function at different mass scales and quenching : a comparison between cosmological models and SDSS ', Monthly Notices of the Royal Astronomical Society, vol. 500, no. 2, pp. 2036-2048 . https://doi.org/10.1093/mnras/staa3236
We present the eddington bias corrected Specific Star Formation Rate Function (sSFRF) at different stellar mass scales from a sub-sample of the Sloan Digital Sky Survey Data Release DR7 (SDSS), which is considered complete both in terms of stellar ma
Publikováno v:
Faisst, A L L, Chary, R R, Brammer, G & Toft, S 2022, ' What Are Those Tiny Things? A First Study of Compact Star Clusters in the SMACS0723 Field with JWST ', Astrophysical Journal Letters, vol. 941, no. 1, L11 . https://doi.org/10.3847/2041-8213/aca1bf
We use the unprecedented resolution and depth of the JWST NIRCam Early Release Observations at 1-5 $\mu$m to study the stellar mass, age, and metallicity of compact star clusters in the neighborhood of the host galaxies in the SMACS J0723.3-7327 gala
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::873cbcdf9b6b6713dc1abaecfb06a379
Autor:
Mark Vogelsberger, Lars Hernquist, Eduardo Bañados, Sébastien Peirani, Shy Genel, Stuart McAlpine, Dylan Nelson, Iskren Y. Georgiev, Mélanie Habouzit, Yohan Dubois, Romeel Davé, Rachel S. Somerville, Daniel Anglés-Alcázar, James Aird, Yetli Rosas-Guevara, Yuan Li
Publikováno v:
Habouzit, M, Somerville, R S, Li, Y, Genel, S, Aird, J, Anglés-Alcázar, D, Davé, R, Georgiev, I Y, McAlpine, S, Rosas-Guevara, Y, Dubois, Y, Nelson, D, Bañados, E, Hernquist, L, Peirani, S & Vogelsberger, M 2022, ' Supermassive black holes in cosmological simulations-II: the AGN population and predictions for upcoming X-ray missions ', Monthly Notices of the Royal Astronomical Society, vol. 509, no. 2, pp. 3015-3042 . https://doi.org/10.1093/mnras/stab3147
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, In press, ⟨10.1093/mnras/stab3147⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, ⟨10.1093/mnras/stab3147⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, In press, ⟨10.1093/mnras/stab3147⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, ⟨10.1093/mnras/stab3147⟩
In large-scale hydrodynamical cosmological simulations, the fate of massive galaxies is mainly dictated by the modeling of feedback from active galactic nuclei (AGN). The amount of energy released by AGN feedback is proportional to the mass that has
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::beb03ed99cae7c946344f78cbd294677
https://hdl.handle.net/20.500.11820/93d8b022-97dd-4464-b5a5-87de4bf04cc0
https://hdl.handle.net/20.500.11820/93d8b022-97dd-4464-b5a5-87de4bf04cc0
Autor:
Mohammad Akhshik, Katherine E. Whitaker, Joel Leja, Johan Richard, Justin S. Spilker, Mimi Song, Gabriel Brammer, Rachel Bezanson, Harald Ebeling, Anna R. Gallazzi, Guillaume Mahler, Lamiya A. Mowla, Erica J. Nelson, Camilla Pacifici, Keren Sharon, Sune Toft, Christina C. Williams, Lillian Wright, Johannes Zabl
Publikováno v:
The Astrophysical Journal, 2023, Vol.943(2) [Peer Reviewed Journal]
Akhshik, M, Whitaker, K E, Leja, J, Richard, J, Spilker, J S, Song, M, Brammer, G, Bezanson, R, Ebeling, H, Gallazzi, A R, Mahler, G, Mowla, L A, Nelson, E J, Pacifici, C, Sharon, K, Toft, S, Williams, C C, Wright, L & Zabl, J 2023, ' REQUIEM-2D : A Diversity of Formation Pathways in a Sample of Spatially Resolved Massive Quiescent Galaxies at z similar to 2 ', Astrophysical Journal, vol. 943, no. 2, 179 . https://doi.org/10.3847/1538-4357/aca677
Akhshik, M, Whitaker, K E, Leja, J, Richard, J, Spilker, J S, Song, M, Brammer, G, Bezanson, R, Ebeling, H, Gallazzi, A R, Mahler, G, Mowla, L A, Nelson, E J, Pacifici, C, Sharon, K, Toft, S, Williams, C C, Wright, L & Zabl, J 2023, ' REQUIEM-2D : A Diversity of Formation Pathways in a Sample of Spatially Resolved Massive Quiescent Galaxies at z similar to 2 ', Astrophysical Journal, vol. 943, no. 2, 179 . https://doi.org/10.3847/1538-4357/aca677
REQUIEM-2D (REsolving QUIEscent Magnified galaxies with 2D grism spectroscopy) is comprised of a sample of 8 massive ($\log M_*/M_\odot > 10.6$) strongly lensed quiescent galaxies at $z\sim2$. REQUIEM-2D combines the natural magnification from strong
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 490:408-416
The problem of the extent of habitable zones in different kinds of galaxies is one of the outstanding challenges for contemporary astrobiology. In the present study, we investigate habitability in a large sample of simulated galaxies from the Illustr
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