SF-CHAMP 5 - FROGGER - San Francisco's Newly-updated Travel Model
JR - A Comprsn of Microsp Trfc Flow Sim Systm for Urban Area.pdf
Type Ia Supernovae Progenitors. Type Ia Supernovae Historical defining characteristics: Generally, lack of lines of hydrogen Contain a strong Si II absorption.
The Fraction Alice K. Harding NASA Goddard Space Flight Center Alice K. Harding NASA Goddard Space Flight Center How many UnID -ray sources are radio-quiet.
Primeval Starbursting Galaxies: Presentation of “Lyman-Break Galaxies” by Mauro Giavalisco Jean P. Walker Rutgers University.
Close-by young isolated NSs: A new test for cooling curves Sergei Popov (Sternberg Astronomical Institute) Co-authors: H.Grigorian, R. Turolla, D. Blaschke.
Bayesian Photometric Redshifts (BPZ) Narciso Benítez 1,2 (2000) Narciso Benítez 1,2 et al. (2004) Dan Coe 1,2,3 et al. (2006) Johns Hopkins University.
Close-by young isolated neutron stars (and black holes) Sergey Popov (Sternberg Astronomical Institute)
A Simple Prescription for Envelope Binding Energy ANDREW LOVERIDGE, MARC VAN DER SLUYS, VICKY KALOGERA 1. Introduction Between thirty and fifty percent.
AY202a Galaxies & Dynamics Lecture 1: Introduction Organization, History, Basic Cosmology Prof. John Huchra, P309 TA Joseph Munoz, P203 JPH’s Assistant.
Stefan Ballmer Fermilab May 14, 2013 Experimental Challenges in Gravitational-Wave Astronomy.
A Synthetic Population Generator that Matches Both Household and Person Attribute Distributions Xin Ye, Ram M. Pendyala, Karthik C. Konduri, Bhargava Sana.