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20032013
most citedThe influence of chemical composition on the properties of Cepheid stars. II-The iron content

227 citations · 483 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2013★ 186 cited

Chemistry of the Sagittarius Dwarf Galaxy: a Top-Light IMF, Outflows and the R-Process

Andrew McWilliam, George Wallerstein, Marta Mottini

From chemical abundance analysis of stars in the Sagittarius dwarf spheroidal galaxy (Sgr), we conclude that the alpha-element deficiencies cannot be due to the Type Ia supernova (…

astro-ph.SR2009★ 3 cited

The Dependency of the Cepheid Period-Luminosity Relation on Chemical Composition

M. Romaniello, F. Primas, M. Mottini +6

The dependency of the Cepheid Period-Luminosity Relation on chemical composition at different wavelengths is assessed via direct detailed abundance analysis of Galactic and Magella…

astro-ph.HE2009

The Brera Multi-scale Wavelet Chandra Survey. The serendipitous source catalogue

P. Romano, S. Campana, R. P. Mignani +4

We present the Brera Multi-scale Wavelet Chandra (BMW-Chandra) source catalogue drawn from essentially all Chandra ACIS-I pointed observations with an exposure time in excess of 10…

astro-ph.HE2009

The BMW-Chandra survey. Serendipitous Source Catalogue

P. Romano, R. P. Mignani, S. Campana +4

We present the BMW-Chandra source catalogue derived from Chandra ACIS-I observations (exposure time >10ks) public as of March 2003 by using a wavelet detection algorithm (Lazzati e…

astro-ph2008★ 12 cited

The Brera Multi-scale Wavelet Chandra Survey. I. Serendipitous source catalogue

P. Romano, S. Campana, R. P. Mignani +4

We present the BMW-Chandra source catalogue drawn from essentially all Chandra ACIS-I pointed observations with an exposure time in excess of 10ks public as of March 2003 (136 obse…

astro-ph2008★ 227 cited

The influence of chemical composition on the properties of Cepheid stars. II-The iron content

M. Romaniello, F. Primas, M. Mottini +6

The Cepheid period-luminosity (PL) relation is unquestionably one of the most powerful tools at our disposal for determining the extragalactic distance scale. While significant pro…