PPT-Type Ia supernovae in the near-infrared:

nickel all over Bruno Leibundgut Suhail Dhawan Jason Spyromilio Kate Maguire The promise of the nearinfrared Extinction is much reduced in the nearIR A H A V 019 Cardelli. Infrared Absorbance. IR- Empirical Comparisons. Identifying functional groups in organic molecules. Region of infrared that is most useful lies between. 2.5-16 . m. m (4000-625 cm. -1. ). depends on transitions between vibrational . Supernovae . J081659.74+511233.7 . and . J07285387+3349106. . with . the BSU . Observatory. Benjamin . Lombard and Sarah Peck . (Mentor: Professor Jamie Kern). Bridgewater State University. Abstract. S. R. Kulkarni. Caltech Optical Observatories. Key Papers. “On Supernovae” Baade & . Zwicky. (1934a). “Cosmic Rays From Supernovae” Baade & . Zwicky. (1934b). “On the Search for Supernovae” . 11-5. IR spectroscopy. . measures the vibrational excitation of atoms around the bonds that connect them.. The positions of the absorption lines are related to the types of functional groups present.. Talk by: John McCann. Paper by: D. . Poznanski. , Z. Kostrzewa-Rutkowska, L. Wyrzykowski & N. . Blagorodnova. OGLE-IV. OGLE – Optical Gravitational Lensing Experiment, Phase four. Las . Benefits. . Problems that do exist will be identified quickly, giving time to assess and repair the problem before a failure. In most cases the problem is identified well before a problem becomes critical.. S.J. . . Smartt. M. Nicholl, . C. . Inserra, A. Jerkstrand, T.W. Chen, M. McCrum, K. Smith, D. Young. Queen’s University Belfast . Not an unbiased review !. See “Handbook of Supernovae”. Andy Howell “Superluminous Supernovae”. #10 Signals from Within. [8:55-20:29]. Infrared Spectroscopy. http. ://www.learner.org/resources/series61.html. region of infrared that is most useful lies between. 2.5-16 . m. m (4000-625 cm. -1. ). light curves and spectral evolution. Bruno . Leibundgut. ESO. The core-collapse SN poster child. SN 1987A. the best observed supernova ever. Suntzeff. (2003). (also . Fransson. et al. 2007). What do we want to learn about supernovae?. Chelsea Braun. Credit: Artist illustration ESO, http. ://www.universetoday.com/wp-content/uploads/2006/12/2006-1130supernova.jpg. Overview. What is a Supernova?. Types of Supernovae. Supernovae in NGC 4088. Herschel. Era. Jason K. . Chu (jasonchu@. ifa.hawaii.edu). Institute for Astronomy, University of Hawai`i. Collaborators: David Sanders (. IfA. ). , Kirsten Larson . (Caltech/IPAC), Joe . Mazzarella. Ruqayyah Askar. PHYS 689 . April 27, 2018. Outline. Introduction. General principles. Historical overview. Types of IR . detectors. Current IR . technologies. Parameters of IR Detectors. Emerging . Technologies. Radiance Observations. Will McCarty. Global Modeling and Assimilation Office. NASA Goddard Space Flight Center . 2015 JCSDA Summer Colloquium . 28 July . 2015. What is Infrared Radiation?. What is Infrared . Properties of III-Nitride . H. eterostructures. Oana . Malis, Purdue University. EPM DMR 1206919. The principal objective of this project . is . to establish the relationship between material growth, atomic structure and infrared optical properties of nitride semiconductors. A.