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19932007
most citedAnalysis of isoplanatic high resolution stellar fields by Starfinder code

401 citations · 638 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2007★ 28 cited

The extended structure of the remote cluster B514 in M31. Detection of extra-tidal stars

L. Federici, M. Bellazzini, S. Galleti +3

We present a study of the density profile of the remote M31 globular cluster B514, obtained from HST/ACS observations. Coupling the analysis of the distribution of the integrated l…

astro-ph2003

Correlations of Globular Cluster Properties: Their Interpretations and Uses

S. G. Djorgovski, P. Cote, G. Meylan +7

Correlations among the independently measured physical properties of globular clusters (GCs) can provide powerful tests for theoretical models and new insights into their dynamics,…

astro-ph2000★ 401 cited

Analysis of isoplanatic high resolution stellar fields by Starfinder code

E. Diolaiti, O. Bendinelli, D. Bonaccini +3

We describe a new code for the deep analysis of stellar fields, designed for Adaptive Optics Nyquist-sampled images with high and low Strehl ratio. The Point Spread Function is ext…

astro-ph2000★ 121 cited

StarFinder: an IDL GUI based code to analyze crowded fields with isoplanatic correcting PSF fitting

E. Diolaiti, O. Bendinelli, D. Bonaccini +3

StarFinder is a new code for the deep analysis of stellar fields, designed for well-sampled images with high and low Strehl ratio. It is organized in the form of a self-contained I…

astro-ph1999★ 3 cited

Starfinder: a code for crowded stellar fields analysis

E. Diolaiti, O. Bendinelli, D. Bonaccini +3

Starfinder is an IDL code for the deep analysis of stellar fields, designed for well-sampled images with high and low Strehl factor. An important feature is represented by the poss…

astro-ph1996★ 84 cited

The \mv vs \fe Calibration: I. HST Color-Magnitude Diagrams of 8 Globular Clusters in M 31

F. Fusi Pecci, R. Buonanno, C. Cacciari +6

Color Magnitude Diagrams (CMDs) of individual stars in 8 Globular Clusters in M31 down to about 1 mag fainter (V) than the Horizontal Branch have been obtained with the…