activity
20032009
most citedRates and properties of type Ia supernovae as a function of mass and star-formation in their host galaxies

562 citations · 2.2k across the 13 of their papers we have counts for

collaborators

16 papers

astro-ph.CO2009321 cited

The 0.4 < z < 1.3 star formation history of the Universe as viewed in the far-infrared

B. Magnelli, D. Elbaz, R. R Chary +4

[Abridged] We use the deepest existing mid- and far-infrared observations (reaching ~3 mJy at 70 um) obtained with Spitzer in the GOODS and FIDEL fields to derive the evolution of…

astro-ph2008182 cited

Spectroscopic ages and metallicities of stellar populations: validation of full spectrum fitting

M. Koleva, Ph. Prugniel, P. Ocvirk +2

Fitting whole spectra at intermediate spectral resolution (R = 1000 -- 3000), to derive physical properties of stellar populations, appears as an optimized alternative to methods b…

astro-ph20075 cited

Analysis of stellar populations with large empirical libraries at high spectral resolution

Philippe Prugniel, Mina Koleva, Pierre Ocvirk +2

The stellar population models dramatically progressed with the arrival of large and complete libraries, ELODIE, CFLIB (=Indo-US) and MILES at a relatively high resolution. We show…

astro-ph2007

Comparison of different spectral population models

Mina Koleva, Philippe Prugniel, Pierre Ocvirk +3

We have compared simple stellar populations (SSPs) generated with different population synthesis tools: BC03, Vazdekis and Pegase.HR and different stellar libraries: ELODIE3.1, Ste…

astro-ph2007

Age and metallicity of Galactic clusters from full spectrum fitting

Mina Koleva, Philippe Prugniel, Pierre Ocvirk +1

We are using full spectrum fitting to determine the ages and metallicities of Galactic clusters (M67 and globular clusters). We find that the method is very accurate to measure the…

astro-ph200723 cited

A Compact Cluster of Massive Red Galaxies at a Redshift of 1.51

P. J. McCarthy, H. Yan, R. G. Abraham +15

We describe a compact cluster of massive red galaxies at z=1.51 discovered in one of the Gemini Deep Deep Survey (GDDS) fields. Deep imaging with the Near Infrared Camera and Multi…