Zobrazeno 1 - 10
of 89
pro vyhledávání: '"Burchett J"'
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:
ZuHone, J. A., Schellenberger, G., Ogorzalek, A., Oppenheimer, B. D., Stern, J., Bogdan, A., Truong, N., Markevitch, M., Pillepich, A., Nelson, D., Burchett, J. N., Khabibullin, I., Kilbourne, C. A., Kraft, R. P., Nulsen, P. E. J., Veilleux, S., Vogelsberger, M., Wang, Q. D., Zhuravleva, I.
The hot, X-ray-emitting phase of the circumgalactic medium of massive galaxies is believed to be the reservoir of baryons from which gas flows onto the central galaxy and into which feedback from AGN and stars inject mass, momentum, energy, and metal
Externí odkaz:
http://arxiv.org/abs/2307.01269
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:
Tchernyshyov, K., Werk, J. K., Wilde, M. C., Prochaska, J. X., Tripp, T. M., Burchett, J. N., Bordoloi, R., Howk, J. C., Lehner, N., O'Meara, J. M., Tejos, N., Tumlinson, J.
We combine 126 new galaxy-O VI absorber pairs from the CGM$^2$ survey with 123 pairs drawn from the literature to examine the simultaneous dependence of the column density of O VI absorbers ($N_{\rm O VI}$) on galaxy stellar mass, star formation rate
Externí odkaz:
http://arxiv.org/abs/2110.13167
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