Starfinder: a code for crowded stellar fields analysis
天体物理学
2019-08-17 v1
摘要
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 Optics observations and exploit this knowledge to improve the analysis of the observed field. A description of the method and applications to real AO data are presented.
引用
@article{arxiv.astro-ph/9911354,
title = {Starfinder: a code for crowded stellar fields analysis},
author = {E. Diolaiti and O. Bendinelli and D. Bonaccini and L. Close and D. Currie and G. Parmeggiani},
journal= {arXiv preprint arXiv:astro-ph/9911354},
year = {2019}
}
备注
4 pages, 3 postscript figures, uses adassconf.sty. To be published in the Adass 99 Conference Proceedings