Zobrazeno 1 - 10
of 196
pro vyhledávání: '"Parmeggiani G"'
Publikováno v:
In Journal of Algebra 15 October 2023 632:641-723
Publikováno v:
In Journal of Algebra 1 November 2020 561:295-354
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 light with star counts we can reliably follow the profile of the cluste
Externí odkaz:
http://arxiv.org/abs/0706.2337
Publikováno v:
In Journal of Algebra 1 December 2018 515:19-51
Publikováno v:
In Journal of Algebra 1 February 2018 495:264-288
Autor:
Djorgovski, S. G., Cote, P., Meylan, G., Castro, S., Federici, L., Parmeggiani, G., Cacciari, C., Pecci, F. Fusi, Rich, R. M., Jou, T.
Correlations among the independently measured physical properties of globular clusters (GCs) can provide powerful tests for theoretical models and new insights into their dynamics, formation, and evolution. We review briefly some of the previous work
Externí odkaz:
http://arxiv.org/abs/astro-ph/0302129
Autor:
Aloisi, A., Clampin, M., Diolaiti, E., Greggio, L., Leitherer, Claus, Nota, A., Origlia, L., Parmeggiani, G., Tosi, M.
We present HST NICMOS photometry of the resolved stellar population in NGC 1569. The CMD in the F110W and F160W photometric bands contains ~2400 stars with a formal photometric error < 0.1 mag down to J~23.5 and H~22.5. We describe the data processin
Externí odkaz:
http://arxiv.org/abs/astro-ph/0011510
Publikováno v:
Astron.Astrophys.Suppl.Ser. 147 (2000) 335-346
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 extracted directly from the image frame, to take into account the actual
Externí odkaz:
http://arxiv.org/abs/astro-ph/0009177
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 IDL widget-based application, with a 'user-friendly' graphic interface.
Externí odkaz:
http://arxiv.org/abs/astro-ph/0004101
Publikováno v:
ASP Conf.Ser.216:623-626,2000
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 possibility to measure the anisoplanatic effect in wide-field Adaptive Opt
Externí odkaz:
http://arxiv.org/abs/astro-ph/9911354