Shoubaneh Hemmati
Affiliations: | Physics | California Institute of Technology, Pasadena, CA |
Website:
https://pma.caltech.edu/content/shoubaneh-hemmatiGoogle:
"Shoubaneh Hemmati"Bio:
http://escholarship.org/uc/item/3899956x
Mean distance: 13552
Parents
Sign in to add mentor| Bahram Mobasher | grad student | 2015 | UC Riverside | |
| (Resolved (KPC-Scale) Properties of Emission-Line Galaxies at Intermediate Redshifts.) | ||||
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Publications
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| Hemmati S, Mobasher B, Nayyeri H, et al. (2020) Bridging between the integrated and resolved main sequence of star formation The Astrophysical Journal. 896 |
| Shahidi A, Mobasher B, Nayyeri H, et al. (2020) Selection of Massive Evolved Galaxies at 3 ≤ z ≤ 4.5 in the CANDELS Fields The Astrophysical Journal. 897: 44 |
| Darvish B, Scoville NZ, Martin C, et al. (2020) Spectroscopic confirmation of a Coma Cluster progenitor at z~2.2 The Astrophysical Journal. 892: 8 |
| Hemmati S, Capak P, Pourrahmani M, et al. (2019) Bringing Manifold Learning and Dimensionality Reduction to SED Fitters The Astrophysical Journal. 881 |
| Jafariyazani M, Mobasher B, Hemmati S, et al. (2019) Spatially Resolved Properties of Galaxies from CANDELS+MUSE: Radial Extinction Profile and Insights on Quenching The Astrophysical Journal. 887: 204 |
| Rodney SA, Balestra I, Bradac M, et al. (2018) Two peculiar fast transients in a strongly lensed host galaxy Nature Astronomy. 2: 324-333 |
| Rodney SA, Riess AG, Scolnic DM, et al. (2016) ERRATUM: “TWO SNe Ia AT REDSHIFT ∼2: IMPROVED CLASSIFICATION AND REDSHIFT DETERMINATION WITH MEDIUM-BAND INFRARED IMAGING” (2015, AJ, 150, 156) The Astronomical Journal. 151: 47 |
| Peth MA, Lotz JM, Freeman PE, et al. (2016) Beyond spheroids and discs: Classifications of CANDELS galaxy structure at 1.4 < z < 2 via principal component analysis Monthly Notices of the Royal Astronomical Society. 458: 963-987 |
| Khostovan AA, Sobral D, Mobasher B, et al. (2015) Evolution of the Hβ + [O III] and [OII] luminosity functions and the [O II] star formation history of the universe up to z ~ 5 from HiZELS Monthly Notices of the Royal Astronomical Society. 452: 3948-3968 |
| Vivian U, Hemmati S, Darvish B, et al. (2015) A CORRELATION between Ly SPECTRAL LINE PROFILE and REST-FRAME UV MORPHOLOGY Astrophysical Journal. 815 |