Zobrazeno 1 - 10
of 32 901
pro vyhledávání: '"SIMONS, R."'
Publikováno v:
Annales Aequatoria, 1996 Jan 01. 17, 477-478.
Externí odkaz:
https://www.jstor.org/stable/25837270
Autor:
Huertas-Company, M., Primack, J. R., Dekel, A., Koo, D. C., Lapiner, S., Ceverino, D., Simons, R. C., Snyder, G. F., Bernardi, M., Chen, Z., Domínguez-Sánchez, H., Lee, C. T., Margalef-Bentabol, B., Tuccillo, D.
We use machine learning to identify in color images of high-redshift galaxies an astrophysical phenomenon predicted by cosmological simulations. This phenomenon, called the blue nugget (BN) phase, is the compact star-forming phase in the central regi
Externí odkaz:
http://arxiv.org/abs/1804.07307
Autor:
Lipton, Merle
Publikováno v:
International Affairs (Royal Institute of International Affairs 1944-), 1971 Apr 01. 47(2), 443-445.
Externí odkaz:
https://www.jstor.org/stable/2614007
Autor:
Davis,, R. Hunt
Publikováno v:
The International Journal of African Historical Studies, 1972 Jan 01. 5(3), 498-500.
Externí odkaz:
https://www.jstor.org/stable/217106
Autor:
Hartnett, William E.
Publikováno v:
American Scientist, 1989 Nov 01. 77(6), 607-607.
Externí odkaz:
https://www.jstor.org/stable/27856079
Autor:
Mossayebi Z; Department of Chemical Engineering, The University of Melbourne, Melbourne, Victoria, 3010, Australia.; CSIRO Manufacturing, Melbourne, Victoria, 3169, Australia., Shabani S; Department of Chemical Engineering, The University of Melbourne, Melbourne, Victoria, 3010, Australia., Easton CD; CSIRO Manufacturing, Melbourne, Victoria, 3169, Australia., Gurr PA; Department of Chemical Engineering, The University of Melbourne, Melbourne, Victoria, 3010, Australia., Simons R; CSIRO Manufacturing, Melbourne, Victoria, 3169, Australia., Qiao GG; Department of Chemical Engineering, The University of Melbourne, Melbourne, Victoria, 3010, Australia.
Publikováno v:
Small (Weinheim an der Bergstrasse, Germany) [Small] 2024 Oct; Vol. 20 (43), pp. e2402114. Date of Electronic Publication: 2024 Jul 11.
Autor:
Ramimoghadam D; Manufacturing, Commonwealth Scientific and Industrial Research Organization (CSIRO), Clayton, Victoria, 3168, Australia., Eyckens DJ; Manufacturing, Commonwealth Scientific and Industrial Research Organization (CSIRO), Clayton, Victoria, 3168, Australia., Evans RA; Manufacturing, Commonwealth Scientific and Industrial Research Organization (CSIRO), Clayton, Victoria, 3168, Australia., Moad G; Manufacturing, Commonwealth Scientific and Industrial Research Organization (CSIRO), Clayton, Victoria, 3168, Australia., Holmes S; Manufacturing, Commonwealth Scientific and Industrial Research Organization (CSIRO), Clayton, Victoria, 3168, Australia., Simons R; Manufacturing, Commonwealth Scientific and Industrial Research Organization (CSIRO), Clayton, Victoria, 3168, Australia.
Publikováno v:
Chemistry (Weinheim an der Bergstrasse, Germany) [Chemistry] 2024 Sep 02; Vol. 30 (49), pp. e202401728. Date of Electronic Publication: 2024 Aug 13.
Autor:
Santini, P., Ferguson, H. C., Fontana, A., Mobasher, B., Barro, G., Castellano, M., Finkelstein, S. L., Grazian, A., Hsu, L. T., Lee, B., Lee, S. -K., Pforr, J., Salvato, M., Wiklind, T., Wuyts, S., Almaini, O., Cooper, M. C., Galametz, A., Weiner, B., Amorin, R., Boutsia, K., Conselice, C. J., Dahlen, T., Dickinson, M. E., Giavalisco, M., Grogin, N. A., Guo, Y., Hathi, N. P., Kocevski, D., Koekemoer, A. M., Kurczynski, P., Merlin, E., Mortlock, A., Newman, J. A., Paris, D., Pentericci, L., Simons, R., Willner, S. P.
We present the public release of the stellar mass catalogs for the GOODS-S and UDS fields obtained using some of the deepest near-IR images available, achieved as part of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) pr
Externí odkaz:
http://arxiv.org/abs/1412.5180
Autor:
Papovich, Casey, Labbé, I., Quadri, R., Tilvi, V., Behroozi, P., Bell, E. F., Glazebrook, K., Spitler, L., Straatman, C. M. S., Tran, K. -V., Cowley, M., Davé, R., Dekel, A., Dickinson, M., Ferguson, H., Finkelstein, S. L., Gawiser, E., Inami, H., Faber, S. M., Kacprzak, G. G., Kawinwanchakij, L., Kocevski, D., Koekemoer, A., Koo, D. C., Kurczynski, P., Lotz, J. M., Lu, Y., Lucas, R. A., McIntosh, D., Mehrtens, N., Mobasher, B., Monson, A., Morrison, G., Nanayakkara, T., Perrson, S. E., Salmon, B., Simons, R., Tomczak, A., van Dokkum, P., Weiner, B., Willner, S. P.
Galaxies with stellar masses near M* contain the majority of stellar mass in the universe, and are therefore of special interest in the study of galaxy evolution. The Milky Way (MW) and Andromeda (M31) have present day stellar masses near M*, at 5x10
Externí odkaz:
http://arxiv.org/abs/1412.3806