Type II Supernovae as Probes of Cosmology (2009)
Poznanski, Dovi, Baron, Eddie, Blondin, Stephane, Bloom, Joshua S., D'Andrea, Christopher B., Della Valle, Massimo, ...
- Constraining the cosmological parameters and understanding Dark Energy have tremendous implications for the nature of the Universe and its physical laws. - The pervasive limit of systematic...
Stellar Explosions: How Big Can They Get? (2007)
100 billion stars. Supernovae release their energy in a variety of forms (neutrinos, the kinetic energy of material, optical light, and radio waves), but they are usually detected on earth via their...
The New Standard Stellar Population Models (NSSPM) -- The Prologue (2007)
Lee, Hyun-chul, Worthey, Guy, Trager, Scott C., Dotter, Aaron, Chaboyer, Brian, Ferguson, Jason W., ...
We are developing a brand new stellar population models with flexible chemistry (isochrones plus stellar colors and spectra) in order to set a new standard of completeness and excellence. Here we...
Crotts, Arlin, Garnavich, Peter, Priedhorsky, William, Habib, Salman, Heitmann, Katrin, Wang, Yun, ...
JEDI will probe dark energy in three independent ways by measuring the expansion history of the universe: (1) using type Ia supernovae as cosmological standard candles over a range of distances, (2)...
Non-LTE model atmosphere analysis of the early ultraviolet spectra of nova OS Andromedae 1986 (1996)
Schwarz, Greg, Hauschildt, Peter H., Starrfield, Sumner, Baron, Eddie, Allard, France, Shore, Steve, ...
We have analyzed the early optically thick ultraviolet spectra of Nova OS And 1986 using a grid of spherically symmetric, non-LTE, line-blanketed, expanding model atmospheres and synthetic spectra...