Marc Postman (born April 6, 1958) is an American astronomer at the Space Telescope Science Institute[1] in Baltimore, Maryland, United States. His research interests
include observational studies of the formation and evolution of galaxies and large scale structure in the
universe. His work focuses on determining, observationally, the relationships between galaxy-scale phenomena and the surrounding large-scale environment and matter distribution. His recent research includes characterizing the properties of brightest cluster galaxies [2][3][4][5] and placing new constraints on the cosmic optical background.[6][7]
^Lauer, Tod R.; Postman, Marc; Weaver, Harold A.; Spencer, John R.; Stern, S. Alan; Buie, Marc W.; Durda, Daniel D.; Lisse, Carey M.; Poppe, A. R.; Binzel, Richard P.; Britt, Daniel T.; Buratti, Bonnie J.; Cheng, Andrew F.; Grundy, W. M.; Horányi, Mihaly; Kavelaars, J. J.; Linscott, Ivan R.; McKinnon, William B.; Moore, Jeffrey M.; Núñez, J. I.; Olkin, Catherine B.; Parker, Joel W.; Porter, Simon B.; Reuter, Dennis C.; Robbins, Stuart J.; Schenk, Paul; Showalter, Mark R.; Singer, Kelsi N.; Verbiscer, Anne J.; Young, Leslie A. (2021). "New Horizons Observations of the Cosmic Optical Background". The Astrophysical Journal. 906 (2): 77. arXiv:2011.03052. Bibcode:2021ApJ...906...77L. doi:10.3847/1538-4357/abc881. hdl:1721.1/133770.2. S2CID226277978.
^Lauer, Tod R.; Postman, Marc; Spencer, John R.; Weaver, Harold A.; Stern, S. Alan; Gladstone, G. Randall; Binzel, Richard P.; Britt, Daniel T.; Buie, Marc W.; Buratti, Bonnie J.; Cheng, Andrew F.; Grundy, W. M.; Horányi, Mihaly; Kavelaars, J. J.; Linscott, Ivan R.; Lisse, Carey M.; McKinnon, William B.; McNutt, Ralph L.; Moore, Jeffrey M.; Núñez, J. I.; Olkin, Catherine B.; Parker, Joel W.; Porter, Simon B.; Reuter, Dennis C.; Robbins, Stuart J.; Schenk, Paul M.; Showalter, Mark R.; Singer, Kelsi N.; Verbiscer, Anne. J.; Young, Leslie A. (2022). "Anomalous Flux in the Cosmic Optical Background Detected with New Horizons Observations". The Astrophysical Journal Letters. 927 (1): L8. arXiv:2202.04273. Bibcode:2022ApJ...927L...8L. doi:10.3847/2041-8213/ac573d. S2CID246680032.