Zobrazeno 1 - 10 of 336 pro vyhledávání: '"Jee, Mj"'
1
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GALEX UV Color-Magnitude Relations and Evidence for Recent Star Formation in Early-type Galaxies
Autor: Yi, S, Yoon, SJ, Kaviraj, S, Deharveng, JM, Rich, RM, Salim, S, Boselli, A, Lee, YW, Ree, CH, Sohn, YJ, Rey, SC, Lee, JW, Rhee, J, Bianchi, L, Byun, YI, Donas, J, Friedman, PG, Heckman, TM, Jelinsky, P, Madore, BF, Malina, R, Martin, DC, Milliard, B, Morrissey, P, Neff, S, Schiminovich, D, Siegmund, O, Small, T, Szalay, AS, Jee, MJ, Kim, SW, Barlow, T, Forster, K, Welsh, B, Wyder, TK
Publikováno v: Astrophys.J.619:L111-L114,2005
We have used the GALEX UV photometric data to construct a first near-ultraviolet (NUV) color-magnitude relation (CMR) for the galaxies pre-classified as early-type by SDSS studies. The NUV CMR is a powerful tool for tracking the recent star formation
Externí odkaz: http://arxiv.org/abs/astro-ph/0411327
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2
Precise Mass Determination of SPT-CL J2106-5844, the Most Massive Cluster at z > 1
Autor: Kim, J, Jee, MJ, Perlmutter, S, Hayden, B, Rubin, D, Huang, X, Aldering, G, Ko, J
Publikováno v: The Astrophysical Journal: an international review of astronomy and astronomical physics, vol 887, iss 1
© 2019. The American Astronomical Society. All rights reserved.. We present a detailed high-resolution weak-lensing study of SPT-CL J2106-5844 at z = 1.132, claimed to be the most massive system discovered at z > 1 in the South Pole Telescope Sunyae
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::65ead8601beaf08a52a47c8d07c4b00b
https://escholarship.org/uc/item/1fd8d566
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3
First Weak-lensing Results from 'See Change': Quantifying Dark Matter in the Two z ≳ 1.5 High-redshift Galaxy Clusters SPT-CL J2040–4451 and IDCS J1426+3508
Autor: Jee, MJ, Ko, J, Perlmutter, S, Gonzalez, A, Brodwin, M, Linder, E, Eisenhardt, P
Publikováno v: The Astrophysical Journal, vol 847, iss 2
Astrophysical Journal, vol 847, iss 2
We present a weak-lensing study of SPT-CL J2040-4451 and IDCS J1426+3508 at z = 1.48 and 1.75, respectively. The two clusters were observed in our "See Change" program, a Hubble Space Telescope survey of 12 massive high-redshift clusters aimed at hig
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3226b0ada91ac1ecc1c0d9825fb1a164
https://escholarship.org/uc/item/0dj743wz
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4
MC 2: Constraining the dark matter distribution of the violent merging galaxy cluster CIZA J2242.8+5301 by piercing through the milky way
Autor: Jee, MJ, Stroe, A, Dawson, W, Wittman, D, Hoekstra, H, Brüggen, M, Röttgering, H, Sobral, D, Van Weeren, RJ
Publikováno v: Astrophysical Journal, vol 802, iss 1
The galaxy cluster CIZA J2242.8+5301 at z = 0.19 is a merging system with a prominent (2 Mpc long) radio relic, which together with the morphology of the X-ray emission provides strong evidence for a violent collision along the north-south axis. We p
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od_______325::e84c4709a24b440d133f1685102159b3
https://escholarship.org/uc/item/4vb9t3f7
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5
Cluster galaxies in XMMU J2235-2557: galaxy population properties in most massive environments at z similar to 1.4
Autor: Strazzullo, V, Rosati, P, Pannella, M, Gobat, R, Santos, Js, Nonino, M, Demarco, R, Lidman, C, Tanaka, M, Mullis, Cr, Nunez, C, Rettura, A, Jee, Mj, Bohringer, H, Bender, R, Bouwens, Rj, Dawson, K, Fassbender, R, Franx, M, Perlmutter, S, Postman, M
We present a multi-wavelength study of galaxy populations in the core of the massive, X-ray luminous cluster XMMU J2235 at z = 1.39, based on high quality VLT and HST photometry at optical and near-infrared wavelengths. We derive luminosity functions
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::cc99c8f453db2d4a8603db72342c36e4
https://hdl.handle.net/11368/2956865
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8
GALEX UV Color-Magnitude Relations and Evidence for Recent Star Formation in Early-type Galaxies
Autor: Yi, S, Yoon, Sj, Kaviraj, S, Deharveng, Jm, Rich, Rm, Salim, S, Ree, Ch, Sohn, Yj, Rey, Sc, Rhee, J, Byun, Yi, Friedman, Pg, Heckman, Tm, Madore, Bf, Siegmund, O, Small, T, Szalay, As, Jee, Mj, Kim, Sw, Bianchi, L., Boselli, A., Donas, J., Martin, D. C., Milliard, B., Morrissey, P., Neff, Susan Gale, Malina, R. F., Wyder, Ted, Lee, Y. -W., Rich, Robert Michael, Schiminovich, David, Jelinsky, P. N., Welsh, B., Barlow, T., Forster, K.
Publikováno v: The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2005, 619, pp.111-114. ⟨10.1086/422811⟩
The Astrophysical journal letters, 2005, 619, pp.111-114. ⟨10.1086/422811⟩
We have used the GALEX UV photometric data to construct a first near-ultraviolet (NUV) color-magnitude relation (CMR) for the galaxies pre-classified as early-type by SDSS studies. The NUV CMR is a powerful tool for tracking the recent star formation
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f2d7191a06d7e736e7e60858b3bb591d
https://hal.archives-ouvertes.fr/hal-00013794
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9
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10
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