C
C. Badenes
Researcher at University of Pittsburgh
Publications - 7
Citations - 353
C. Badenes is an academic researcher from University of Pittsburgh. The author has contributed to research in topics: Supernova & Star formation. The author has an hindex of 5, co-authored 7 publications receiving 339 citations. Previous affiliations of C. Badenes include Weizmann Institute of Science.
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Journal ArticleDOI
Using the X-ray Morphologies of Young Supernova Remnants to Constrain Explosion Type, Ejecta Distribution, and Chemical Mixing
TL;DR: In this paper, a power-ratio method (a multipole expansion) and wavelet transform analysis were used to measure the global and local morphological properties of the X-ray line and thermal emission in twenty-four supernova remnants.
Journal ArticleDOI
Type II Supernova Energetics and Comparison of Light Curves to Shock-Cooling Models
Adam Rubin,Avishay Gal-Yam,Annalisa De Cia,Assaf Horesh,D. Khazov,Eran O. Ofek,Shrinivas R. Kulkarni,Iair Arcavi,Iair Arcavi,Ilan Manulis,O. Yaron,Paul Vreeswijk,Mansi M. Kasliwal,Sagi Ben-Ami,Daniel A. Perley,Daniel A. Perley,Yi Cao,S. Bradley Cenko,S. Bradley Cenko,Umaa Rebbapragada,Przemek Woźniak,Alexei V. Filippenko,Kelsey I. Clubb,Peter Nugent,Peter Nugent,Yen-Chen Pan,C. Badenes,D. Andrew Howell,D. Andrew Howell,Stefano Valenti,David J. Sand,Jesper Sollerman,Joel Johansson,Douglas C. Leonard,J. Chuck Horst,Stephen F. Armen,Joseph M. Fedrow,Joseph M. Fedrow,Robert M. Quimby,Robert M. Quimby,P. A. Mazzali,Elena Pian,Assaf Sternberg,Thomas Matheson,Mark Sullivan,Kate Maguire,S. Lazarevic +46 more
TL;DR: In this article, a sample of 57 R-band Type II supernovae (SNe) light curves is presented, with greater than 5 detections during the first 10 days after discovery, and a well-constrained time of explosion to within 13 days.
Journal ArticleDOI
Type II supernova energetics and comparison of light curves to shock-cooling models
Adam Rubin,Avishay Gal-Yam,Annalisa De Cia,Assaf Horesh,D. Khazov,Eran O. Ofek,Shrinivas R. Kulkarni,Iair Arcavi,Iair Arcavi,Ilan Manulis,O. Yaron,Paul Vreeswijk,Mansi M. Kasliwal,Sagi Ben-Ami,Daniel A. Perley,Daniel A. Perley,Yi Cao,S. Bradley Cenko,S. Bradley Cenko,Umaa Rebbapragada,Przemek Woźniak,Alexei V. Filippenko,Kelsey I. Clubb,Peter Nugent,Peter Nugent,Yen-Chen Pan,C. Badenes,D. Andrew Howell,D. Andrew Howell,Stefano Valenti,David J. Sand,Jesper Sollerman,Joel Johansson,Douglas C. Leonard,J. Chuck Horst,Stephen F. Armen,Joseph M. Fedrow,Joseph M. Fedrow,Robert M. Quimby,Robert M. Quimby,P. A. Mazzali,Elena Pian,Assaf Sternberg,Thomas Matheson,Mark Sullivan,Kate Maguire,S. Lazarevic +46 more
TL;DR: In this article, a sample of $57$ $R$-band Type II supernovae (SNe) light curves was used to estimate the energy per unit mass (E/M$) of the first few days after the explosion.
Journal ArticleDOI
X-ray studies of supernova remnants: A different view of supernova explosions
TL;DR: The most relevant results on supernova remnants obtained during the first decade of Chandra and the impact that these results have had on open issues in supernova research are reviewed.
Journal ArticleDOI
Statistical time-resolved spectroscopy: A higher fraction of short-period binaries for metal-rich F-type dwarfs in SDSS
TL;DR: In this paper, the authors performed a statistical analysis of 14,000 F-type stars in the Milky Way through time-resolved spectroscopy with the sub-exposures archived in the Sloan Digital Sky Survey.