NewEvery arXiv paper, its researchers & institutions — mapped.
papers

Publications (15)

astro-ph1996

Observation of Cosmological Time Dilation using Type Ia Supernovae as Clocks

G. Goldhaber, S. Deustua, S. Gabi +23

astro-ph1996

K Corrections For Type Ia Supernovae and a Test for Spatial Variation of the Hubble Constant

A. Kim, S. Deustua, S. Gabi +23

astro-ph2004

Type Ia supernova rate at a redshift of ~ 0.1

G. Blanc, C. Afonso, C. Alard +58

astro-ph1996

The Type Ia Supernova Rate at z ~ 0.4

R. Pain, I. Hook, S. Perlmutter +23

astro-ph2003

The extended tails of Palomar 5: A ten degree arc of globular cluster tidal debris

M. Odenkirchen, E. K. Grebel, W. Dehnen +7

astro-ph2002

Palomar 5 and its tidal tails: New observational results

M. Odenkirchen, E. K. Grebel, W. Dehnen +4

astro-ph2007

Candidate Milky Way Satellites in the Galactic Halo

C. Liu, J. Hu, H. Newberg +1

astro-ph2008

Improved Cosmological Constraints from New, Old and Combined Supernova Datasets

M. Kowalski, D. Rubin, G. Aldering +67

astro-ph2000

The Chandra Multi-wavelength Project (ChaMP): a serendipitous survey with Chandra archival data

B. J. Wilkes, P. Green, R. Brissenden +34

astro-ph2004

Spectroscopic Observations and Analysis of the Peculiar SN 1999aa

G. Garavini, G. Folatelli, A. Goobar +55

astro-ph2004

A comprehensive model for the Monoceros tidal stream

J. Penarrubia, D. Martinez-Delgado, H. W. Rix +7

astro-ph2008

The Milky Way's Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars

X. -X. Xue, H. -W. Rix, G. Zhao +14

astro-ph2007

The SEGUE Stellar Parameter Pipeline. I. Description and Initial Validation Tests

Y. S. Lee, T. C. Beers, T. Sivarani +10

astro-ph1996

Scheduled Discoveries of 7+ High-Redshift Supernovae: First Cosmology Results and Bounds on q_0

S. Perlmutter, S. Deustua, S. Gabi +23

astro-ph2005

Spectroscopic Observations and Analysis of the Unusual Type Ia SN 1999ac

The Supernova Cosmology Project, :, G. Garavini +55