Introduction to Astronomical Photometry:
Saved in:
| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Dordrecht
Springer Netherlands
1974
|
| Series: | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews
41 |
| Subjects: | |
| Online Access: | Volltext |
| Item Description: | The material given in this 'Introduction to astronomical photometry' is the subject matter of a lecture at the University of Geneva. It is, therefore, intended for those students, physicists or mathematicians, who have completed their bachelor's degree or diploma, and are intending to work for their Ph.D. in astronomy. We assume then the elementary ideas of astrophysics, magnitude, colour index, spectral classes, luminosity classes, gradient, atmospheric extinction are already known. The student may find it useful to re-read the work of Schatzman [1], Dufay [2] and Aller [254] before embarking upon the study of this 'Introduction to astronomical photometry'. It is not our aim in this book to deal with every aspect of stellar photometry. On the contrary, we shall restriet ourselves to looking at subjects ofwhich knowledge seems to us essential for someone who has to use photometrie quantities in his astronomical research. We are, therefore, keeping the interests of the photometrie measurements user partieularly in mind. We shall only discuss very superficially the technical prob lems and reduction methods for atmospheric extinction. These problems are dealt with very clearly in Astronomical Techniques [3]; the first by A. Lallemand, H. L. |
| Physical Description: | 1 Online-Ressource (IX, 366 p) |
| ISBN: | 9789401021692 9789401021715 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-010-2169-2 |
Staff View
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| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 520 - Astronomy and allied sciences |
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| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-010-2169-2 |
| format | Electronic eBook |
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| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:57Z |
| institution | BVB |
| isbn | 9789401021692 9789401021715 |
| issn | 0067-0057 |
| language | English |
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| physical | 1 Online-Ressource (IX, 366 p) |
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| series2 | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews |
| spelling | Golay, M. Verfasser aut Introduction to Astronomical Photometry by M. Golay Dordrecht Springer Netherlands 1974 1 Online-Ressource (IX, 366 p) txt rdacontent c rdamedia cr rdacarrier Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews 41 0067-0057 The material given in this 'Introduction to astronomical photometry' is the subject matter of a lecture at the University of Geneva. It is, therefore, intended for those students, physicists or mathematicians, who have completed their bachelor's degree or diploma, and are intending to work for their Ph.D. in astronomy. We assume then the elementary ideas of astrophysics, magnitude, colour index, spectral classes, luminosity classes, gradient, atmospheric extinction are already known. The student may find it useful to re-read the work of Schatzman [1], Dufay [2] and Aller [254] before embarking upon the study of this 'Introduction to astronomical photometry'. It is not our aim in this book to deal with every aspect of stellar photometry. On the contrary, we shall restriet ourselves to looking at subjects ofwhich knowledge seems to us essential for someone who has to use photometrie quantities in his astronomical research. We are, therefore, keeping the interests of the photometrie measurements user partieularly in mind. We shall only discuss very superficially the technical prob lems and reduction methods for atmospheric extinction. These problems are dealt with very clearly in Astronomical Techniques [3]; the first by A. Lallemand, H. L. Physics Astronomy, Observations and Techniques Astronomie (DE-588)4003311-9 gnd rswk-swf Fotometrie (DE-588)4174524-3 gnd rswk-swf Astronomie (DE-588)4003311-9 s Fotometrie (DE-588)4174524-3 s 1\p DE-604 https://doi.org/10.1007/978-94-010-2169-2 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Golay, M. Introduction to Astronomical Photometry Physics Astronomy, Observations and Techniques Astronomie (DE-588)4003311-9 gnd Fotometrie (DE-588)4174524-3 gnd |
| subject_GND | (DE-588)4003311-9 (DE-588)4174524-3 |
| title | Introduction to Astronomical Photometry |
| title_auth | Introduction to Astronomical Photometry |
| title_exact_search | Introduction to Astronomical Photometry |
| title_full | Introduction to Astronomical Photometry by M. Golay |
| title_fullStr | Introduction to Astronomical Photometry by M. Golay |
| title_full_unstemmed | Introduction to Astronomical Photometry by M. Golay |
| title_short | Introduction to Astronomical Photometry |
| title_sort | introduction to astronomical photometry |
| topic | Physics Astronomy, Observations and Techniques Astronomie (DE-588)4003311-9 gnd Fotometrie (DE-588)4174524-3 gnd |
| topic_facet | Physics Astronomy, Observations and Techniques Astronomie Fotometrie |
| url | https://doi.org/10.1007/978-94-010-2169-2 |
| work_keys_str_mv | AT golaym introductiontoastronomicalphotometry |