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of 4
pro vyhledávání: '"Juan D. Remolina González"'
Publikováno v:
The Astrophysical Journal
Strong gravitational lensing provides unique opportunities to investigate the mass distribution at the cores of galaxy clusters and to study high redshift galaxies. Using $94$ strong lensing models of $74$ cluster fields from the \textit{Hubble} Fron
Autor:
G. Khullar, Jan Luca van den Busch, Benjamin Floyd, Keren Sharon, Guillaume Mahler, Tim Schrabback, Michael S. Calzadilla, Matthew B. Bayliss, Juan D. Remolina González, Lindsey Bleem, Michael D. Gladders, Antony A. Stark, Michael McDonald
We present an analysis of the mass distribution inferred from strong lensing by SPT-CL J0356-5337, a cluster of galaxies at redshift z = 1.0359 revealed in the follow-up of the SPT-SZ clusters. The cluster has an Einstein radius of Erad=14 for a sour
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eeb9894b4aef09d992ace27791e5b2a7
Autor:
Esra Bulbul, Guillaume Mahler, Bradford Benson, Michael S. Calzadilla, William R. Forman, Vittorio Ghirardini, Michael McDonald, G. Khullar, Sebastian Bocquet, Juan D. Remolina González, Matthew B. Bayliss, Lindsey Bleem, Ralph P. Kraft, Dominique Eckert
Publikováno v:
The Astrophysical Journal
The thermodynamic properties of the hot plasma in galaxy clusters retains information on the processes leading to the formation and evolution of the gas in their deep, dark matter potential wells. These processes are dictated not only by gravity but
Autor:
Samuel J. Dunham, Michael Florian, Benjamin P. Koester, Mohammad Akhshik, Juan D. Remolina González, Jane R. Rigby, Rachel Paterno-Mahler, Katherine T. Murray, Guillaume Mahler, Michael D. Gladders, Matthew B. Bayliss, Traci L. Johnson, Keren Sharon, Eva Wuyts, Håkon Dahle, Katherine E. Whitaker
Publikováno v:
Sharon, K, Bayliss, M B, Dahle, H, Dunham, S J, Florian, M K, Gladders, M D, Johnson, T L, Mahler, G, Paterno-Mahler, R, Rigby, J R, Whitaker, K E, Akhshik, M, Koester, B P, Murray, K, Gonzalez, J D R & Wuyts, E 2020, ' Strong Lens Models for 37 Clusters of Galaxies from the SDSS Giant Arcs Survey ', Astrophysical Journal, Supplement Series, vol. 247, no. 1, 12 . https://doi.org/10.3847/1538-4365/ab5f13
Sharon, K, Bayliss, M B, Dahle, H, Dunham, S J, Florian, M K, Gladders, M D, Johnson, T L, Mahler, G, Paterno-Mahler, R, Rigby, J R, Whitaker, K E, Akhshik, M, Koester, B P, Murray, K, Remolina González, J D & Wuyts, E 2020, ' Strong Lens Models for 37 Clusters of Galaxies from the SDSS Giant Arcs Survey ', Astrophysical Journal Supplement Series, vol. 247, no. 1, 12 . https://doi.org/10.3847/1538-4365/ab5f13
Sharon, K, Bayliss, M B, Dahle, H, Dunham, S J, Florian, M K, Gladders, M D, Johnson, T L, Mahler, G, Paterno-Mahler, R, Rigby, J R, Whitaker, K E, Akhshik, M, Koester, B P, Murray, K, Remolina González, J D & Wuyts, E 2020, ' Strong Lens Models for 37 Clusters of Galaxies from the SDSS Giant Arcs Survey ', Astrophysical Journal Supplement Series, vol. 247, no. 1, 12 . https://doi.org/10.3847/1538-4365/ab5f13
We present strong gravitational lensing models for 37 galaxy clusters from the SDSS Giant Arcs Survey. We combine data from multi-band Hubble Space Telescope WFC3imaging, with ground-based imaging and spectroscopy from Magellan, Gemini, APO, and MMT,