D 2010

MUNI-FITS-Utils

CHRASTINA, Marek, Miloslav ZEJDA and Zdeněk MIKULÁŠEK

Basic information

Original name

MUNI-FITS-Utils

Name in Czech

MUNI-FITS-Utils

Authors

CHRASTINA, Marek (703 Slovakia, guarantor, belonging to the institution), Miloslav ZEJDA (203 Czech Republic, belonging to the institution) and Zdeněk MIKULÁŠEK (203 Czech Republic, belonging to the institution)

Edition

San Francisco, Binaries - key to comprehension of the universe, p. 83-84, 2 pp. 2010

Publisher

Astronomical society of the Pacific

Other information

Language

English

Type of outcome

Stať ve sborníku

Field of Study

10308 Astronomy

Country of publisher

United States of America

Confidentiality degree

není předmětem státního či obchodního tajemství

Publication form

printed version "print"

RIV identification code

RIV/00216224:14310/10:00049405

Organization unit

Faculty of Science

ISBN

978-1-58381-750-6

UT WoS

000289880000017

Keywords in English

FITS; CCD; photometry

Tags

Tags

International impact, Reviewed
Změněno: 28/1/2013 10:17, doc. RNDr. Miloslav Zejda, Ph.D.

Abstract

V originále

The FITS standard allows arbitrary use of name-space for keywords,except some reserved keywords.Results of this freedom is that several keywords have the same meaning.Similar problem is that values of keywords have different physical units.These facts complicate automated data processing and also creation of FITS file archives with simple structure.MUNI-FITS-Utils is a package of Python scripts which have been developed in PyFITS, a Python FITS Module.Scripts are user-friendly and allow manipulating FITS headers to get uniform shape.Further functions will be added soon.

Links

GD205/08/H005, research and development project
Name: Fyzika Slunce, hvězd a hvězdných soustav
Investor: Czech Science Foundation, Physics of Sun, stars, and stellar systems
IAA301630901, research and development project
Name: Rozložení energie ve spektru horkých hvězd a jeho proměnnost
Investor: Academy of Sciences of the Czech Republic, Spectral energy distribution of hot stars and its variability