Michel A. Zamojski, Ph.D.
Affiliations: | 2008 | Columbia University, New York, NY |
Area:
Astronomy and AstrophysicsGoogle:
"Michel Zamojski"Parents
Sign in to add mentor| David Schiminovich | grad student | 2008 | Columbia | |
| (Morphological properties of star-forming galaxies: Connecting the morphological evolution of galaxies and the decline of the star formation rate density of the Universe in the past 9 billion years.) | ||||
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Publications
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| Dessauges-Zavadsky M, Zamojski M, Rujopakarn W, et al. (2017) Molecular gas properties of a lensed star-forming galaxy at z similar to 3.6: a case study Astronomy and Astrophysics. 605 |
| Elvis M, Hao H, Civano F, et al. (2012) Spectral energy distributions of type 1 active galactic nuclei in the Cosmos survey. I. the XMM-Cosmos sample Astrophysical Journal. 759 |
| Williams MJ, Zamojski MA, Bureau M, et al. (2011) The stellar kinematics and populations of boxy bulges: Cylindrical rotation and vertical gradients Monthly Notices of the Royal Astronomical Society. 414: 2163-2172 |
| Yan H, Yan L, Zamojski MA, et al. (2011) Probing very bright end of galaxy luminosity function at z ≳ 7 using Hubble Space Telescope Pure Parallel observations Astrophysical Journal Letters. 728 |
| Zamojski M, Yan L, Dasyra K, et al. (2011) HST/NICMOS imaging of bright high-redshift 24 μm selected galaxies: Merging properties Astrophysical Journal. 730 |
| Brusa M, Civano F, Comastri A, et al. (2010) The XMM-newton wide-field survey in the cosmos field (XMM-COSMOS): Demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei Astrophysical Journal. 716: 348-369 |
| Yan L, Tacconi LJ, Fiolet N, et al. (2010) Detections of CO Molecular Gas in 24 μm Bright ULIRGs at z ~ 2 in the Spitzer First Look Survey The Astrophysical Journal. 714: 100-114 |
| Ilbert O, Salvato M, Le Floc'H E, et al. (2010) Galaxy stellar mass assembly between 0.2 < z < 2 from the s-cosmos survey Astrophysical Journal. 709: 644-663 |
| Vibert D, Zamojski M, Conseil S, et al. (2009) Photometry in UV astronomical images of extended sources in crowded field using deblended images in optical visible bands as Bayesian priors Proceedings of Spie. 7246: 72460 |
| Caputi KI, Lilly SJ, Aussel H, et al. (2009) The optical spectra of spitzer 24 μm galaxies in the cosmic evolution survey field. II. Faint infrared sources in the zCosmos-Bright 10k catalog Astrophysical Journal. 707: 1387-1403 |