The Magnetar Primer Shriharsh P. Tendulkar California Institute of Technology S. R. Kulkarni P. B. Cameron.
SPECTROSCOPY OVERVIEW The Science Case: High Resolution Spectroscopy of (cool) stars Basic tools for specifications and verification One example of similar.
Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen.
The Birth and Assembly of Galaxies: the Relationship Between Science Capabilities and Telescope Aperture Betsy Barton Center for Cosmology University of.
The Far-Infrared Universe: from the Universe’s oldest light to the birth of its youngest stars Jeremy P. Scott, on behalf of Locke D. Spencer Physics and.
A wide field multi-wavelength survey of two clusters at z~0.5 Tommaso Treu (UCSB)
Cool gas in the distant Universe Epoch of galaxy assembly (z~1 to 5) Massive galaxy formation: imaging hyper-starbursts Main sequence galaxies: gas.
Lecture #4 Observational facts Olivier Le Fèvre – LAM Cosmology Summer School 2014.
Galaxies - Chapter 24 vs. 1. First spiral nebula found in 1845 by the Earl of Rosse. Speculated it was beyond our Galaxy. 1920 - "Great Debate" between.
Neutron stars - Chapter 21 1. Neutron stars The remains of cores of some massive stars that have become supernovae. Cores are a degenerate gas of mostly.
Constraining Astronomical Populations with Truncated Data Sets Brandon C. Kelly (CfA, Hubble Fellow, [email protected]) 6/11/2015Brandon C. Kelly,
Integral field spectroscopy in the IR: Gemini-CIRPASS observations and the star-formation history in the nucleus of M83 While HST offers excellent spatial.