Malcolm S. Hicken, Ph.D.
Affiliations: | 2009 | Harvard University, Cambridge, MA, United States |
Area:
observational astronomyGoogle:
"Malcolm Hicken"Mean distance: 15.07
Cross-listing: Astronomy Tree
Parents
Sign in to add mentor| Robert P. Kirshner | grad student | 2009 | Harvard | |
| (Doubling the nearby Supernova Type Ia sample.) | ||||
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Publications
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| Pierel JDR, Rodney S, Avelino A, et al. (2018) Extending Supernova Spectral Templates for Next-generation Space Telescope Observations Publications of the Astronomical Society of the Pacific. 130: 114504 |
| Hicken M, Friedman AS, Blondin S, et al. (2017) Type II Supernova Light Curves and Spectra from the CfA The Astrophysical Journal Supplement Series. 233: 6 |
| Blondin S, Prieto JL, Patat F, et al. (2017) Erratum: “A Second Case of Variable Na I D Lines in a Highly-reddened Type Ia Supernova” (2009, ApJ, 693, 207) The Astrophysical Journal. 844: 88 |
| Narayan G, Rest A, Tucker BE, et al. (2016) LIGHT CURVES of 213 TYPE Ia SUPERNOVAE from the ESSENCE SURVEY Astrophysical Journal, Supplement Series. 224 |
| Kelly PL, Filippenko AV, Burke DL, et al. (2015) Distances with <4% precision from type Ia supernovae in young star-forming environments. Science (New York, N.Y.). 347: 1459-62 |
| Friedman AS, Wood-Vasey WM, Marion GH, et al. (2015) CfAIR2: Near-infrared light curves of 94 type Ia supernovae Astrophysical Journal, Supplement Series. 220 |
| Bianco FB, Modjaz M, Hicken M, et al. (2014) Multi-color optical and near-infrared light curves of 64 stripped-envelope core-collapse supernovae Astrophysical Journal, Supplement Series. 213 |
| Modjaz M, Blondin S, Kirshner RP, et al. (2014) Optical spectra of 73 stripped-envelope core-collapse supernovae Astronomical Journal. 147 |
| Drout MR, Soderberg AM, Mazzali PA, et al. (2013) The fast and furious decay of the peculiar type Ic supernova 2005ek Astrophysical Journal. 774 |
| Turnbull SJ, Hudson MJ, Feldman HA, et al. (2012) Cosmic flows in the nearby universe from Type Ia supernovae Monthly Notices of the Royal Astronomical Society. 420: 447-454 |