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An 8 Channel Imager/Polarimeter for ...

Taylor, Brian W.

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An 8 Channel Imager/Polarimeter for Astronomical Observations.

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	An 8 Channel Imager/Polarimeter for Astronomical Observations./
作者:	Taylor, Brian W.
出版者:	Ann Arbor : ProQuest Dissertations & Theses, : 2019,
面頁冊數:	73 p.
附註:	Source: Masters Abstracts International, Volume: 80-07.
Contained By:	Masters Abstracts International80-07.
標題:	Optics. -
電子資源:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=13426342
ISBN:	9780438804500

An 8 Channel Imager/Polarimeter for Astronomical Observations.
Taylor, Brian W.

An 8 Channel Imager/Polarimeter for Astronomical Observations. - Ann Arbor : ProQuest Dissertations & Theses, 2019 - 73 p.

Source: Masters Abstracts International, Volume: 80-07.

Thesis (M.S.)--The University of Arizona, 2019.

This item must not be sold to any third party vendors.

Discussion of optical designs and instrument polarization for an Eight Channel Imager/Po- larimeter are presented. The designs will cover the optical and Near Infrared(NIR) wavelengths from 330nm to 2400nm in a simultaneous acquisition mode for eight distinct broad bands. The simultaneous acquisition provides capabilities to study unique events such as supernovae, Gamma Ray Bursts(GRBs), and occultations. It also increases the efficiency of long term monitoring pro- grams such as the study of blazars. The selection of the wavelength bands were specifically chosen to match the Sloan Digital Sky Survey(u', g', r', i',z') and the 2MASS(J,H,K) catalogs.

ISBN: 9780438804500Subjects--Topical Terms:

517925
Optics.

An 8 Channel Imager/Polarimeter for Astronomical Observations.
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506 $a This item must not be sold to any third party vendors.
520 $a Discussion of optical designs and instrument polarization for an Eight Channel Imager/Po- larimeter are presented. The designs will cover the optical and Near Infrared(NIR) wavelengths from 330nm to 2400nm in a simultaneous acquisition mode for eight distinct broad bands. The simultaneous acquisition provides capabilities to study unique events such as supernovae, Gamma Ray Bursts(GRBs), and occultations. It also increases the efficiency of long term monitoring pro- grams such as the study of blazars. The selection of the wavelength bands were specifically chosen to match the Sloan Digital Sky Survey(u', g', r', i',z') and the 2MASS(J,H,K) catalogs.
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