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BUDHIES III: The fate of HI and the quenching of galaxies in evolving environments

Y. Jaffé, M. Verheijen, C. Haines, H. Yoon, R. Cybulski, M. Montero-Castaño, R. Smith, A. Chung, B. Deshev, X. Fernández, J. van Gorkom, B. Poggianti, M. Yun, A. Finoguenov, G. Smith, и N. Okabe. (2016)cite arxiv:1604.07832Comment: 21 pages (including appendix). Accepted for publication in MNRAS.

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Alexis Lebedeff

Alexis Rozenknop

Alexis Hoen

Alexis Rump

Alexis Hofmeister

Другие публикации лиц с тем же именем

A filament of dark matter between two clusters of galaxiesJ. Dietrich, N. Werner, D. Clowe, A. Finoguenov, T. Kitching, L. Miller, и A. Simionescu. (2012)cite arxiv:1207.0809Comment: Nature, in press.Building robust AGN mock catalogs to unveil black hole evolution and for survey planningV. Allevato, F. Shankar, C. Marsden, U. Rasulov, A. Viitanen, A. Georgakakis, A. Ferrara, и A. Finoguenov. (2021)cite arxiv:2105.02883Comment: Accepted for publication in the Astrophysical Journal.Discovery of a galaxy cluster with a violently starbursting core at z=2.506T. Wang, D. Elbaz, E. Daddi, A. Finoguenov, D. Liu, C. Schreiber, S. Martin, V. Strazzullo, F. Valentino, R. van der Burg и 9 other автор(ы). (2016)cite arxiv:1604.07404Comment: submitted.Chemical Enrichment RGS cluster sample (CHEERS): Constraints on turbulenceC. Pinto, J. Sanders, N. Werner, J. de Plaa, A. Fabian, Y. Zhang, J. Kaastra, A. Finoguenov, и J. Ahoranta. (06.01.2015)Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical propertiesM. Bethermin, M. Kilbinger, E. Daddi, J. Gabor, A. Finoguenov, H. McCracken, M. Wolk, H. Aussel, V. Strazzulo, E. Floc'h и 6 other автор(ы). (2014)cite arxiv:1405.0492Comment: 18 pages, 16 figures, Accepted by A&A.The integrated stellar content of dark matter halosA. Leauthaud, M. George, P. Behroozi, K. Bundy, J. Tinker, R. Wechsler, C. Conroy, A. Finoguenov, и M. Tanaka. (2011)cite arxiv:1109.0010Comment: Submitted to ApJ. 16 Pages, 11 Figures. Comments Welcome.Do group dynamics play a role in the evolution of member galaxies?A. Hou, L. Parker, M. Balogh, S. McGee, D. Wilman, J. Connelly, W. Harris, A. Mok, J. Mulchaey, R. Bower и 1 other автор(ы). (2013)cite arxiv:1308.1406Comment: 14 pages, 6 figures, MNRAS accepted.BUDHIES III: The fate of HI and the quenching of galaxies in evolving environmentsY. Jaffé, M. Verheijen, C. Haines, H. Yoon, R. Cybulski, M. Montero-Castaño, R. Smith, A. Chung, B. Deshev, X. Fernández и 6 other автор(ы). (2016)cite arxiv:1604.07832Comment: 21 pages (including appendix). Accepted for publication in MNRAS.CANDELS: Constraining the AGN-Merger Connection with Host Morphologies at z~2D. Kocevski, S. Faber, M. Mozena, A. Koekemoer, K. Nandra, C. Rangel, E. Laird, M. Brusa, S. Wuyts, J. Trump и 28 other автор(ы). (2011)cite arxiv:1109.2588 Comment: 10 Pages, 5 Figures, Revised draft submitted to ApJ.LoCuSS: Pre-processing in galaxy groups falling into massive galaxy clusters at z=0.2M. Bianconi, G. Smith, C. Haines, S. McGee, A. Finoguenov, и E. Egami. (2017)cite arxiv:1710.04230Comment: 5 pages, 2 figures. Accepted for publication in MNRAS Letters.

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