Zobrazeno 1 - 10
of 244
pro vyhledávání: '"Crain, R."'
Autor:
Stephenson, H. M. O., Stott, J. P., Cullen, F., Bielby, R. M., Amos, N., Dutta, R., Fumagalli, M., Tejos, N., Burchett, J. N., Crain, R. A., Prochaska, J. X.
We present analysis of the mass-metallicity relation (MZR) for a sample of 67 [OIII]-selected star-forming galaxies at a redshift range of $z=1.99 - 2.32$ ($z_{\text{med}} = 2.16$) using \emph{Hubble Space Telescope} Wide Field Camera 3 grism spectro
Externí odkaz:
http://arxiv.org/abs/2311.10140
Autor:
Stott, J. P., Bielby, R. M., Cullen, F., Burchett, J. N., Tejos, N., Fumagalli, M., Crain, R. A., Morris, S. L., Amos, N., Bower, R. G., Prochaska, J. X.
Publikováno v:
2020, MNRAS, 497, 3083
We demonstrate that the UV brightest quasars at z=1-2 live in overdense environments. This is based on an analysis of deep Hubble Space Telescope WFC3 G141 grism spectroscopy of the galaxies along the lines-of-sight to UV luminous quasars in the reds
Externí odkaz:
http://arxiv.org/abs/2006.07384
Autor:
Koribalski, B. S., Staveley-Smith, L., Westmeier, T., Serra, P., Spekkens, K., Wong, O. I., Lagos, C. D. P., Obreschkow, D., Ryan-Weber, E. V., Zwaan, M., Kilborn, V., Bekiaris, G., Bekki, K., Bigiel, F., Boselli, A., Bosma, A., Catinella, B., Chauhan, G., Cluver, M. E., Colless, M., Courtois, H. M., Crain, R. A., de Blok, W. J. G., Dénes, H., Duffy, A. R., Elagali, A., Fluke, C. J., For, B. -Q., Heald, G., Henning, P. A., Hess, K. M., Holwerda, B. W., Howlett, C., Jarrett, T., Jones, D. H., Jones, M. G., Józsa, G. I. G., Jurek, R., Jütte, E., Kamphuis, P., Karachentsev, I., Kerp, J., Keiner, D., Kraan-Korteweg, R. C., Lee-Waddell, K., López-Sánchez, A. R., Madrid, J., Meyer, M., Mould, J., Murugeshan, C., Norris, R. P., Oh, S. -H., Oosterloo, T. A., Popping, A., Putman, M., Reynolds, T. N., Rhee, J., Robotham, A. S. G., Ryder, S., Schröder, A. C., Shao, Li, Stevens, A. R. H., Taylor, E. N., van der Hulst, J. M., Verdes-Montenegro, L., Wakker, B. P., Wang, J., Whiting, M., Winkel, B., Wolf, C.
Publikováno v:
Ap&SS 365, 118 (2020) - https://rdcu.be/b5Bfg
The Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) is a next-generation survey of neutral hydrogen (HI) in the Local Universe. It uses the widefield, high-resolution capability of the Australian Square Kilometer Array Pathfinder (ASKAP)
Externí odkaz:
http://arxiv.org/abs/2002.07311
Autor:
Pawlik, M. M., McAlpine, S., Trayford, J. W., Wild, V., Bower, R., Crain, R. A., Schaller, M., Schaye, J.
About 35 years ago a class of galaxies with unusually strong Balmer absorption lines and weak emission lines was discovered in distant galaxy clusters. These objects, alternatively referred to as post-starburst, E+A or k+a galaxies, are now known to
Externí odkaz:
http://arxiv.org/abs/1903.11050
Autor:
Bielby, R. M., Stott, J. P., Cullen, F., Tripp, T. M., Burchett, J., Fumagalli, M., Morris, S. L., Tejos, N., Crain, R. A., Bower, R. G., Prochaska, J. X.
We present the first results from a study of OVI absorption around galaxies at $z<1.44$ using data from a near-infrared grism spectroscopic Hubble Space Telescope Large Program, the Quasar Sightline and Galaxy Evolution (QSAGE) survey. QSAGE is the f
Externí odkaz:
http://arxiv.org/abs/1809.05544
Autor:
Tescari, E., Cortese, L., Power, C., Wyithe, J. S. B., Ho, I. -T., Crain, R. A., Bland-Hawthorn, J., Croom, S. M., Kewley, L. J., Schaye, J., Bower, R. G., Theuns, T., Schaller, M., Barnes, L., Brough, S., Bryant, J. J., Goodwin, M., Gunawardhana, M. L. P., Lawrence, J. S., Leslie, S. K., López-Sánchez, Á. R., Lorente, N. P. F., Medling, A. M., Richards, S. N., Sweet, S. M., Tonini, C.
This work presents a study of galactic outflows driven by stellar feedback. We extract main sequence disc galaxies with stellar mass $10^9\le$ M$_{\star}/$M$_{\odot} \le 5.7\times10^{10}$ at redshift $z=0$ from the highest resolution cosmological sim
Externí odkaz:
http://arxiv.org/abs/1709.01939
Autor:
Furlong, M., Bower, R. G., Crain, R. A., Schaye, J., Theuns, T., Trayford, J. W., Qu, Y., Schaller, M., Berthet, M., Helly, J. C.
We present the evolution of galaxy sizes, from redshift 2 to 0, for actively star forming and passive galaxies in the cosmological hydrodynamical 1003 cMpc3 simulation of the EAGLE project. We find that the sizes increase with stellar mass , but that
Externí odkaz:
http://arxiv.org/abs/1510.05645
Autor:
Calore, F., Bozorgnia, N., Lovell, M., Bertone, G., Schaller, M., Frenk, C. S., Crain, R. A., Schaye, J., Theuns, T., Trayford, J. W.
Publikováno v:
JCAP 12 (2015) 053
We study high-resolution hydrodynamic simulations of Milky Way type galaxies obtained within the "Evolution and Assembly of GaLaxies and their Environments" (EAGLE) project, and identify the those that best satisfy observational constraints on the Mi
Externí odkaz:
http://arxiv.org/abs/1509.02164
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Furlong, M., Bower, R. G., Theuns, T., Schaye, J., Crain, R. A., Schaller, M., Vecchia, C. Dalla, Frenk, C. S., McCarthy, I. G., Helly, J., Jenkins, A., Rosas-Guevara, Y. M.
Publikováno v:
2015, MNRAS, 450, 4486
We investigate the evolution of galaxy masses and star formation rates in the Evolution and Assembly of Galaxies and their Environment (EAGLE) simulations. These comprise a suite of hydrodynamical simulations in a $\Lambda$CDM cosmogony with subgrid
Externí odkaz:
http://arxiv.org/abs/1410.3485