activity
20042015
most citedSpectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation

1.4k citations · 1.8k across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2015★ 27 cited

Type Ia supernova Hubble diagram with near-infrared and optical observations

V. Stanishev, A. Goobar, R. Amanullah +10

We main goal of this paper is to test whether the NIR peak magnitudes of SNe Ia could be accurately estimated with only a single observation obtained close to maximum light, provid…

astro-ph.SR2012★ 164 cited

SN 2006oz: rise of a super-luminous supernova observed by the SDSS-II SN Survey

G. Leloudas, E. Chatzopoulos, B. Dilday +21

We study SN 2006oz, a newly-recognized member of the class of H-poor, super-luminous supernovae. We present multi-color light curves from the SDSS-II SN Survey, that cover the rise…

astro-ph.CO2011★ 4 cited

Line Profiles of Intermediate Redshift Type Ia Supernovae

Kohki Konishi, Joshua A. Frieman, Ariel Goobar +6

We present the temporal evolution of line profiles ranging from near ultraviolet to optical wavelengths by analyzing 59 Subaru telescope spectra of normal Type Ia Supernovae (SNe I…

astro-ph.CO2011★ 3 cited

Subaru Spectroscopy of SDSS-II Supernovae

Kohki Konishi, Naoki Yasuda, Kouichi Tokita +11

The Sloan Digital Sky Survey II (SDSS-II) Supernova Survey discovered Type Ia supernovae (SNe Ia) in an almost unexplored intermediate redshift range of and provid…

astro-ph.CO2010★ 26 cited

Spectral properties of Type Ia supernovae up to z~0.3

J. Nordin, L. Ostman, A. Goobar +10

Aims: Spectroscopic observations of Type Ia supernovae obtained at the New Technology Telescope (NTT) and the Nordic Optical Telescope (NOT), in conjunction with the SDSS-II Supern…

astro-ph.CO2010★ 47 cited

NTT and NOT spectroscopy of SDSS-II supernovae

L. Ostman, J. Nordin, A. Goobar +18

Context. The SDSS-II Supernova Survey, conducted between 2005 and 2007, was designed to detect a large number of Type Ia supernovae (SNe Ia) around z~0.2, the redshift "gap" betwee…