Marc Postman
Affiliations: | Space Telescope Science Institute |
Area:
galaxy evolution; clusters of galaxies; large-scale structureWebsite:
http://www.stsci.edu/~postman/Home.htmlGoogle:
"Marc Postman"Children
Sign in to add trainee| Kevin Fogarty | grad student | 2012-2017 | Johns Hopkins |
| Bingxiao Xu | grad student | 2012-2017 | Johns Hopkins |
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Publications
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| Kelly PL, Rodney S, Treu T, et al. (2023) Constraints on the Hubble constant from Supernova Refsdal's reappearance. Science (New York, N.Y.). eabh1322 |
| Gültekin K, Burke-Spolaor S, Lauer TR, et al. (2021) Chandra Observations of Abell 2261 Brightest Cluster Galaxy, a Candidate Host to a Recoiling Black Hole The Astrophysical Journal. 906: 48 |
| Mercurio A, Rosati P, Biviano A, et al. (2021) CLASH-VLT: Abell S1063 Astronomy & Astrophysics. 656: A147 |
| Ciocan BI, Ziegler BL, Verdugo M, et al. (2021) The VLT-MUSE and ALMA view of the MACS 1931.8-2635 brightest cluster galaxy Astronomy & Astrophysics. 649: A23 |
| Connor T, Donahue M, Kelson DD, et al. (2020) Erratum: “Crowded Field Galaxy Photometry: Precision Colors in the CLASH Clusters” (2017, ApJ, 848, 37) The Astrophysical Journal. 892: 72 |
| Fogarty K, Postman M, Li Y, et al. (2019) The Dust and Molecular Gas in the Brightest Cluster Galaxy in MACS 1931.8-2635 The Astrophysical Journal. 879: 103 |
| Fujita Y, Donahue M, Ettori S, et al. (2019) Halo Concentrations and the Fundamental Plane of Galaxy Clusters Arxiv: Astrophysics of Galaxies. 7: 8 |
| Fujita Y, Umetsu K, Rasia E, et al. (2019) The new fundamental plane dictating galaxy cluster evolution Proceedings of the International Astronomical Union. 15: 271-272 |
| Siegel SR, Sayers J, Mahdavi A, et al. (2018) Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-Ray, SZ, and Lensing Data The Astrophysical Journal. 861: 71 |
| Umetsu K, Sereno M, Tam S, et al. (2018) The Projected Dark and Baryonic Ellipsoidal Structure of 20 CLASH Galaxy Clusters The Astrophysical Journal. 860: 104 |