Archive of the University Observatory

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o:292378 Kategorie F: Sternwarten, Astronomische Gebäude, Instrumente
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Objects found (14)

o:102634 XXX

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o:102635 XXX

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o:102636 XXX

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o:102637 XXX

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Farbempfindlichkeit einiger gebräuchlicher Methoden
Farbempfindlichkeit einiger in der Astrophotometrie gebräuchlicher Methoden. show more
Farbempfindlichkeit einiger in der Astrophotometrie gebräuchlicher Methoden.
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Astigmatismus
Astigmatismus schiefer Büschel. (Nach H. Boegehold, die geometrische Theorie der optischen Abbildung. Czapski-Effekt, Grundzüge der Theorie der optischen Instrumente. 3. Aufl. Leipzig 1924, S. 26). show more
Astigmatismus schiefer Büschel. (Nach H. Boegehold, die geometrische Theorie der optischen Abbildung. Czapski-Effekt, Grundzüge der Theorie der optischen Instrumente. 3. Aufl. Leipzig 1924, S. 26).
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Farbdispersion in Kron- und Flintglas
2 Graphiken. 1. Verteilung der einzelnen Farbdispersionen bei Kron- und Flintglas; 2. Aussehen der Sternspektren in verschiedenen Objektivabständen. Quelle: Graff, Astrophysik, S. 47 – 49 show more
2 Graphiken. 1. Verteilung der einzelnen Farbdispersionen bei Kron- und Flintglas; 2. Aussehen der Sternspektren in verschiedenen Objektivabständen. Quelle: Graff, Astrophysik, S. 47 – 49
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Gewöhnliches und achromatisches Prisma
Gewöhnliches und achromatisches Prisma. Quelle: Graff, Astrophysik, S. 47 – 49 show more
Gewöhnliches und achromatisches Prisma. Quelle: Graff, Astrophysik, S. 47 – 49
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CC BY-NC 3.0 AT

Crossley-Reflektor
Amateur astronomer Andrew A. Common built the Crossley Reflector in Great Britain in 1879, around the time that the Great Lick Refractor was built. The Great Refractor was one of the last large refractors built, and the Crossley was one of the first... show more
Amateur astronomer Andrew A. Common built the Crossley Reflector in Great Britain in 1879, around the time that the Great Lick Refractor was built. The Great Refractor was one of the last large refractors built, and the Crossley was one of the first large reflectors built. Large reflectors became practical after 1880, when a new technology for making concave, silver-coated glass mirrors was perfected. Prior to this, such mirrors required constant polishing to remain reflective. With his reflector, A.A. Common was the first to discover that stars too faint to be seen through a telescope with the eye could be imaged in photographs taken through the telescope using a long exposure time. This discovery is the basis for all modern astrophotography and spectroscopy. For these early astronomical photographs, Common was awarded the Royal Astronomical Society gold medal for Astronomy. After deciding to build a larger telescope, Common sold the 36-inch reflector to Edward Crossley in 1885. Crossley built a new dome enclosure to protect the telescope and observers from the harsh Halifax (UK) weather, but this climate was far from ideal for observation. After about 10 years, Crossley donated both telescope and dome to Lick Observatory, where it was put into operation in 1896.
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Große Treppe der Wiener Universitätssternwarte, Ansicht von unten
Die Großen Treppe des Instituts für Astronomie der Universität Wien vom Eingangsbereich aus aufgenommen show more
Die Großen Treppe des Instituts für Astronomie der Universität Wien vom Eingangsbereich aus aufgenommen
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CC BY-NC 2.0 AT

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