Zobrazeno 1 - 10
of 78
pro vyhledávání: '"KACPRZAK, G. G."'
Autor:
Martínez-Marín, M., Glazebrook, K., Nanayakkara, T., Jacobs, C., Labbé, I., Kacprzak, G. G., Papovich, C., Schreiber, C.
We present a sample of 22 massive galaxies with stellar masses $>10^{10} M_{\odot}$ at $3
Externí odkaz:
http://arxiv.org/abs/2405.12501
Autor:
Augustin, Ramona, Péroux, Céline, Karki, Arjun, Kulkarni, Varsha, Weng, Simon, Hamanowicz, A., Hayes, M., Howk, J. C., Kacprzak, G. G., Klitsch, A., Zwaan, M. A., Fox, A., Biggs, A., Fresco, A. Y., Kassin, S., Kuntschner, H.
The physical processes by which gas is accreted onto galaxies, transformed into stars and then expelled from galaxies are of paramount importance to galaxy evolution studies. Observationally constraining each of these baryonic components in the same
Externí odkaz:
http://arxiv.org/abs/2402.03420
Autor:
Cowley, M. J., Spitler, L. R., Quadri, R. F., Goulding, A. D., Papovich, C., Tran, K. V. H., Labbé, I., Alcorn, L., Allen, R. J., Forrest, B., Glazebrook, K., Kacprzak, G. G., Morrison, G., Nanayakkara, T., Straatman, C. M. S., Tomczak, A. R.
We investigate the relationship between the black hole accretion rate (BHAR) and star formation rate (SFR) for Milky Way (MW) and Andromeda (M31)-mass progenitors from z = 0.2 to 2.5. We source galaxies from the K-s-band-selected ZFOURGE survey, whic
Externí odkaz:
http://hdl.handle.net/10150/627058
http://arizona.openrepository.com/arizona/handle/10150/627058
http://arizona.openrepository.com/arizona/handle/10150/627058
Autor:
Cooke, J., Angus, C., Auchettl, K., Bally, J., Bolin, B., Brough, S., Burchett, J. N., Foley, R., Foran, G., Forbes, D., Gannon, J., Hirai, R., Kacprzak, G. G., Margutti, R., Martinez-Lombilla, C., Mestric, U., Moller, A., Rest, A., Rhodes, J., Rich, R. M., Schussler, F., Wainscoat, R., Walawender, J., Wold, I., Zhang, J.
The Keck Wide-Field Imager (KWFI) is a proposed 1-degree diameter field of view UV-sensitive optical camera for Keck prime focus. KWFI will be the most powerful optical wide-field camera in the world and the only such 8m-class camera sensitive down t
Externí odkaz:
http://arxiv.org/abs/2207.11698
Autor:
Fisher, D. B., Bolatto, A. D., Glazebrook, K., Obreschkow, D., Obreschkow, R. G., Kacprzak, G. G., Nielsen, N. M.
We report on the internal distribution of star formation efficiency in IRAS 08339+6517 (hereafter IRAS08), using $\sim$200~pc resolution CO(2-1) observations from NOEMA. The molecular gas depletion time changes by 2 orders-of-magnitude from disk-like
Externí odkaz:
http://arxiv.org/abs/2202.00024
Autor:
Sameer, Charlton, J. C., Norris, J. M., Gebhardt, M., Churchill, C. W., Kacprzak, G. G., Muzahid, S., Narayanan, Anand, Nielsen, N. M., Richter, Philipp, Wakker, Bart P.
We present a new method aimed at improving the efficiency of component by component ionization modeling of intervening quasar absorption line systems. We carry out cloud-by-cloud, multiphase modeling making use of CLOUDY and Bayesian methods to extra
Externí odkaz:
http://arxiv.org/abs/2012.00021
Autor:
Schreiber, C., Glazebrook, K., Papovich, C., Diaz-Santos, T., Verma, A., Elbaz, D., Kacprzak, G. G., Nanayakkara, T., Oesch, P., Pannella, M., Spitler, L., Straatman, C., Tran, K. -V., Wang, T.
Publikováno v:
A&A 646, A68 (2021)
Understanding the process of quenching is one of the major open questions in galaxy evolution, and crucial insights may be obtained by studying quenched galaxies at high redshifts, at epochs when the Universe and the galaxies were younger and simpler
Externí odkaz:
http://arxiv.org/abs/2011.13700
Akademický článek
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Autor:
Schreiber, C., Glazebrook, K., Nanayakkara, T., Kacprzak, G. G., Labbe, I., Oesch, P., Yuan, T., Tran, K. -V., Papovich, C., Spitler, L., Straatman, C.
Publikováno v:
A&A 618, A85 (2018)
We present Keck-MOSFIRE H and K spectra for a sample of 24 candidate quiescent galaxies (QGs) at 3
Externí odkaz:
http://arxiv.org/abs/1807.02523
Autor:
Rees, G. A., Spitler, L. R., Norris, R. P., Cowley, M. J., Papovich, C., Glazebrook, K., Quadri, R. F., Straatman, C. M. S., Allen, R., Kacprzak, G. G., Labbe, I., Nanayakkara, T., Tomczak, A. R., Tran, K. -V.
In order to reproduce the high-mass end of the galaxy mass-distribution, some process must be responsible for the suppression of star-formation in the most massive of galaxies. Commonly Active Galactic Nuclei (AGN) are invoked to fulfil this role, bu
Externí odkaz:
http://arxiv.org/abs/1511.01988