Difference between revisions 2243871 and 2243978 on enwikiversity

[[Image:Detectors summary 3.png|thumb|right|250px|This tree diagram shows the relationship between types and classification of most common particle detectors. Credit: [[commons:User:Wdcf|Wdcf]].]]
'''Radiation detectors''' provide a signal that is converted to an electric current. The device is designed so that the current provided is proportional to the characteristics of the incident radiation.

(contracted; show full)|pages=103-6
|url=
|arxiv=
|bibcode=1992ESASP.356..103F
|doi=
|pmid=
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|accessdate=2013-05-24 }}</ref>

"A0620-00 [is observed] with the [Faint Object Spectrograph] FOS blue detector" while aboard the Hubble Space Telescope.<ref name="McClintock">{{cite book
|author=Jeffrey McClintock
|title=Black Hole A0620-00 and Advection-Dominated Accretion, In: ''HST Proposal ID #7393''
|publisher=STSci
|location=Baltimore, Maryland USA
|date=December 1997
|editor=
|pages=
|url=
|arxiv=
|bibcode=1997hst..prop.7393M
|doi=
|pmid=
|isbn=
|accessdate=2013-05-24 }}</ref>

==Cyans==
{{main|Radiation astronomy/Cyans|Cyans}}
The Wide Field/Planetary Camera (PC-1) had an F469N, F487N, and F492M cyan filters in the filter wheel.<ref name="Krist"/>

The Wide Field Planetary Camera (PC-2) replaced PC-1 on the Hubble Space Telescope and carried the following cyan filters on the same filter wheels: F467M, F469N, F487N.<ref name="Krist">{{cite book
|author=John Krist
(contracted; show full){{tlx|Radiation astronomy resources}}{{Principles of radiation astronomy}}{{Sisterlinks|Radiation detectors}}

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[[Category:Radiation astronomy/Lectures]]
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