Zobrazeno 1 - 10
of 263
pro vyhledávání: '"Foltz, R"'
Autor:
Foltz, R., Wilson, G., Muzzin, A., Cooper, M. C., Nantais, J., van der Burg, R. F. J., Cerulo, P., Chan, J., Fillingham, S. P., Surace, J., Webb, T., Noble, A., Lacy, M., McDonald, M., Rudnick, G., Lidman, C., Demarco, R., Hlavacek-Larrondo, J., Yee, H. K. C., Perlmutter, S., Hayden, B.
Using a sample of 4 galaxy clusters at $1.35 < z < 1.65$ and 10 galaxy clusters at $0.85 < z < 1.35$, we measure the environmental quenching timescale, $t_Q$, corresponding to the time required after a galaxy is accreted by a cluster for it to fully
Externí odkaz:
http://arxiv.org/abs/1803.03305
Autor:
Delahaye, A. G., Webb, T. M. A., Nantais, J., DeGroot, A., Wilson, G., Muzzin, A., Yee, H. K. C., Foltz, R., Noble, A. G., Demarco, R., Tudorica, A., Cooper, M. C., Lidman, C., Perlmutter, S., Hayden, B., Boone, K., Surace, J.
We compile a sample of spectroscopically- and photometrically-selected cluster galaxies from four high-redshift galaxy clusters ($1.59 < z < 1.71$) from the Spitzer Adaptation of the Red-Sequence Cluster Survey (SpARCS), and a comparison field sample
Externí odkaz:
http://arxiv.org/abs/1705.10849
Autor:
Noble, A. G., McDonald, M., Muzzin, A., Nantais, J., Rudnick, G., van Kampen, E., Webb, T. M. A., Wilson, G., Yee, H. K. C., Boone, K., Cooper, M. C., DeGroot, A., Delahaye, A., Demarco, R., Foltz, R., Hayden, B., Lidman, C., Manilla-Robles, A., Perlmutter, S.
Publikováno v:
The Astrophysical Journal Letters, Volume 842, Number 2 (2017)
We present ALMA CO (2-1) detections in 11 gas-rich cluster galaxies at z~1.6, constituting the largest sample of molecular gas measurements in z>1.5 clusters to date. The observations span three galaxy clusters, derived from the Spitzer Adaptation of
Externí odkaz:
http://arxiv.org/abs/1705.03062
Autor:
Prestwich, A. H., Tsantaki, M., Zezas, A., Jackson, F. E., Roberts, T. P., Foltz, R., Linden, T., Kalogera, V.
Ultra-Luminous X-ray sources (ULX) are X-ray binaries with Lx>1E^39 ergs/s. The most spectacular examples of ULX occur in starburst galaxies and are now understood to be young, luminous High Mass X-ray Binaries. The conditions under which ULX form ar
Externí odkaz:
http://arxiv.org/abs/1302.6203
Autor:
Holland, Andrew D., Beletic, James, Holmes, W., Aghakians, H., Avasapian, S., Bahraman, A., Berg, A., Beyer, A., Boehmer, E., Calvet, R., Cheung, S., Cho, B., Cho, H., Cillis, A., DelCastillo, L., Dickie, M., Delo, G., Farris, M., Feizi, A., Ferraro, N., Fischer, L., Foltz, R., Hambarsoumian, N., Hong, K., Huang, T., Jhabvala, M., Kan, Er., Kopp, R., Krohn, B., Lewis, D., Loose, M., MacNeal, K., Maiten, J., Markley, D., Maldonado, G., Mehta, J., Melendez, J., Morgan, A. R., Mulder, J., Ngyuen, M., Ovee, N., Pniel, M., Pravdo, S., Randall, D., Riendeau, J., Runkle, A., Runyan, M., Seiffert, M., Skalare, M., Tan, P., Turner, A., Van Nostrand, S., Waczynski, A., Wu, J.
Publikováno v:
Proceedings of SPIE; August 2022, Vol. 12191 Issue: 1 p121911U-121911U-13, 12069203p
Autor:
Coyle, Laura E., Matsuura, Shuji, Perrin, Marshall D., Focardi, M., Noce, V., Merola, P., Di Giorgio, A., Ligori, S., Corcione, L., Capobianco, V., Bonino, D., V. Nunez, M., Chiarucci, S., Medinaceli, E., Auricchio, N., Farina, M., Giusi, G., Russi, A., Tortora, A., Serafini, L., Pannocchia, A., Giglio, G., Passerai, M., Verna, M., Del Vecchio Blanco, C., Morgante, G., Ateca, J., Bosch, J., Carmona, M., Casas, A., Gomez, J. M., Lopez, P., Marti, L., Royo, A., Ruiz, O., Serre, C., Skup, K. R., Rutkowski, K., Sobiecki, M., Ber, K., Sobolewski, M., Thernstrom, N., Winklera, M., Ciarka, M., Berthé, M., Cara, C., Fontignie, J., Martignac, J., Kaszubiak, G., Leguay, N., Grimoldi, R., Ober, G., Goullioud, R., Holmes, W., Swain, M., Vasisht, G., Cho, H., Mulder, J., Allen, G. D., Runkle, A., Guzman, E., Weilert, M., Weber, C., Tan, P., Morales, J., Hunacek, J., Rieck, A., Bolduc, A., Aaron, K., Turner, A., Krohn, B., Lew, M., Cillis, A., Foltz, R., Hewagama, T., Loose, M., Crook, M., Hills, M., Gilley, G., Mäkinen, S., Caldwell, A., Bishop, G., Desjonqueres, L., Drummond, R., Eccleston, P., Davidson, A., Umesh, P., Pace, E., Preti, G., Micela, G., Malaguti, G., Tinetti, G.
Publikováno v:
Proceedings of SPIE; August 2024, Vol. 13092 Issue: 1 p1309249-1309249-29
Autor:
Foltz, R, Wilson, G, Muzzin, A, Cooper, MC, Nantais, J, Van Der Burg, RFJ, Cerulo, P, Chan, J, Fillingham, SP, Surace, J, Webb, T, Noble, A, Lacy, M, McDonald, M, Rudnick, G, Lidman, C, Demarco, R, Hlavacek-Larrondo, J, Yee, HKC, Perlmutter, S, Hayden, B
Publikováno v:
The Astrophysical Journal, vol 866, iss 2
Astrophysical Journal, vol 866, iss 2
Astrophysical Journal, vol 866, iss 2
Using a sample of four galaxy clusters at 1.35 < z < 1.65 and 10 galaxy clusters at 0.85 < z < 1.35, we measure the environmental quenching timescale, t Q, corresponding to the time required after a galaxy is accreted by a cluster for it to fully cea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::b3075fbfd11a6a00d959a9e02707bb41
https://escholarship.org/uc/item/2cq5q7rp
https://escholarship.org/uc/item/2cq5q7rp
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Akademický článek
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