WFIRST & Euclid Jason Rhodes NASA Jet Propulsion Laboratory California Institute of Technology Copyright 2011 California Institute of Technology. Government.
(Recalling the Death of a High-Mass Star…). Neutron stars, although they have 1–3 solar masses, are so dense that they are very small. This image.
Stellar Explosions. Introduction Life after Death for White Dwarfs The End of a High-Mass Star Supernovae Supernova 1987A The Crab Nebula in Motion The.
Results of Recent Grazing Occultation Observations presented 2014 July 13, UMD Obs., College Park, MD 32 nd Annual IOTA Meeting David W. Dunham.
Transit Searches: Results I.Results from individual transit searche programs II. Interesting cases III. Spectroscopic Transits IV. In-transit spectroscopy.
By Tony George for 2013 IOTA Conference. Issues: Many IOTA members are purchasing integrating CCD video cameras to expand the range of occultations.
Extra-Solar Planets Astronomy 311 Professor Lee Carkner Lecture 24.
Energetic Neutral Atoms from Solar Flares H. S. Hudson 1, R. P. Lin 1, A. L. MacKinnon 2, J. C. Raymond 3, A. Y. Shih 1, and Wang, L. 1 1 University of.
The Cleveland Street Variable Star Observatory presents Back due to popular demand and the laws of astrophysics From the neck of the Swan-between Eta Cyg.
Modeling Variability of Blazar Jets with a Turbulent Magnetic Field Alan Marscher Institute for Astrophysical Research, Boston University Research Web.
Seven sisters 20051 How I Stopped Worrying and Learned to Love the Universe Marilena LoVerde Columbia University Hubble Deep Field, NASA.
CAMERA Compact Automated MEMS Rayleigh Adaptive Optics System C. Baranec, S. Kulkarni, R. Dekany, N. Law, E. Ofek, M. Kasliwal, V. Velur, & A. Ramaprakash.