activity
20172020
most citedSCALA: In-situ calibration for Integral Field Spectrographs

10 citations · 10 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2020

The SNEMO and SUGAR Companion Datasets

G. Aldering, P. Antilogus, C. Aragon +41

The Nearby Supernova Factory has made spectrophotometric observations of Type Ia supernovae since . This work presents an interim version of the data produced, including $210…

astro-ph.CO2019

SUGAR: An improved empirical model of Type Ia Supernovae based on spectral features

P. -F. Léget, E. Gangler, F. Mondon +40

Type Ia Supernovae (SNe Ia) are widely used to measure the expansion of the Universe. Improving distance measurements of SNe Ia is one technique to better constrain the acceleratio…

astro-ph.HE2019

SN 2012dn from early to late times: 09dc-like supernovae reassessed

S. Taubenberger, A. Floers, C. Vogl +40

As a candidate 'super-Chandrasekhar' or 09dc-like Type Ia supernova (SN Ia), SN 2012dn shares many characteristics with other members of this remarkable class of objects but lacks…

astro-ph.CO2018

SNEMO: Improved Empirical Models for Type Ia Supernovae

C. Saunders, G. Aldering, P. Antilogus +39

Type Ia supernova cosmology depends on the ability to fit and standardize observations of supernova magnitudes with an empirical model. We present here a series of new models of Ty…

astro-ph.CO2018

Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate

M. Rigault, V. Brinnel, G. Aldering +40

As part of an on-going effort to identify, understand and correct for astrophysics biases in the standardization of Type Ia supernovae (SNIa) for cosmology, we have statistically c…

astro-ph.CO2018

Correcting for peculiar velocities of Type Ia Supernovae in clusters of galaxies

P. -F. Léget, M. V. Pruzhinskaya, A. Ciulli +43

Type Ia Supernovae (SNe Ia) are widely used to measure the expansion of the Universe. To perform such measurements the luminosity and cosmological redshift () of the SNe Ia have…