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20022008
most citedImproved Cosmological Constraints from New, Old and Combined Supernova Datasets

1.6k citations · 1.7k across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph20081.6k cited

Improved Cosmological Constraints from New, Old and Combined Supernova Datasets

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

We present a new compilation of Type Ia supernovae (SNe Ia), a new dataset of low-redshift nearby-Hubble-flow SNe and new analysis procedures to work with these heterogeneous compi…

astro-ph200838 cited

Supernova progenitors and iron density evolution from SN rate evolution measurements

Guillaume Blanc, Laura Greggio

Using an extensive compilation of literature supernova rate data we study to which extent its evolution constrains the star formation history, the distribution of the type Ia super…

astro-ph200764 cited

Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study

G. Garavini, G. Folatelli, S. Nobili +44

We develop a method to measure the strength of the absorption features in Type Ia supernova (SN Ia) spectra and use it to make a quantitative comparison between the spectra of Type…

astro-ph20062 cited

The OGLE-II event sc5_2859 : a Classical Nova outburst?

C. Afonso, J. F. Glicenstein, A. Gould +3

The OGLE-II event sc5_2859 was previously identified as the third longest microlensing event ever observed. Additional photometric observations from the EROS (Experience de Recherc…

astro-ph2003

Bulge Microlensing Optical Depth from EROS 2 observations

C. Afonso, J. -N. Albert, C. Alard +7

We present a measurement of the microlensing optical depth toward the Galactic bulge based on the analysis of 15 contiguous1 square degrees fields centered on (l=2.5 deg, b=-4.0 de…

astro-ph2002

The Hubble Diagram of Type Ia Supernovae as a Function of Host Galaxy Morphology

M. Sullivan, R. S. Ellis, G. Aldering +41

(Abridged) We present new results on the Hubble diagram of distant type Ia supernovae (SNe Ia) segregated according to the type of host galaxy. This makes it possible to check earl…