Brian P. Schmidt
|1995-||Research School of Astronomy and Astrophysics||Australian National University, Acton, Australian Capital Territory, Australia|
Google:"Brian P. Schmidt"
The Nobel Prize in Physics 2011 was divided, one half awarded to Saul Perlmutter, the other half jointly to Brian P. Schmidt and Adam G. Riess "for the discovery of the accelerating expansion of the Universe through observations of distant supernovae".
Mean distance: 15.07
Cross-listing: Astronomy Tree
ParentsSign in to add mentor
ChildrenSign in to add trainee
You can help our author matching system! If you notice any publications incorrectly attributed to this author, please sign in and mark matches as correct or incorrect.
|Hsiao EY, Phillips MM, Marion GH, et al. (2018) Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program Publications of the Astronomical Society of the Pacific. 131: 014002|
|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|
|Galbany L, Hamuy M, Phillips MM, et al. (2016) UBVRIz light curves of 51 type II supernovae Astronomical Journal. 151|
|Howes LM, Asplund M, Keller SC, et al. (2016) The EMBLA survey - metal-poor stars in the Galactic bulge Monthly Notices of the Royal Astronomical Society. 460: 884-901|
|Howes LM, Casey AR, Asplund M, et al. (2015) Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way. Nature|
|Childress MJ, Hillier DJ, Seitenzahl I, et al. (2015) Measuring nickel masses in Type Ia supernovae using cobalt emission in nebular phase spectra Monthly Notices of the Royal Astronomical Society. 454: 3816-3842|
|Nicholl M, Smartt SJ, Jerkstrand A, et al. (2015) On the diversity of superluminous supernovae: Ejected mass as the dominant factor Monthly Notices of the Royal Astronomical Society. 452: 3869-3893|
|Yuan F, Lidman C, Davis TM, et al. (2015) OzDES multifibre spectroscopy for the Dark Energy Survey: First-year operation and results Monthly Notices of the Royal Astronomical Society. 452: 3047-3063|
|Zhou G, Bayliss D, Hartman JD, et al. (2015) A0.24+0.18 M|
|Barbarino C, Dall'Ora M, Botticella MT, et al. (2015) SN 2012ec: Mass of the progenitor from PESSTO follow-up of the photospheric phase Monthly Notices of the Royal Astronomical Society. 448: 2312-2331|