Measuring Astronomical Seeing: The DA/IAC DIMM
Accurate, absolute, and reproducible measurements are the expected qualities of any instrument. A differential image motion monitor (DIMM) is presented which assesses astronomical seeing with those requirements. It has been designed (with collaboration of the staff of the Département d'Astrophy...
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Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 1995-03, Vol.107 (709), p.265-272 |
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creator | Vernin, Jean Muñoz-Tuñón, Casiana |
description | Accurate, absolute, and reproducible measurements are the expected qualities of any instrument. A differential image motion monitor (DIMM) is presented which assesses astronomical seeing with those requirements. It has been designed (with collaboration of the staff of the Département d'Astrophysique de l'Université de Nice and the Instituto de Astrofísica de Canarias: DA/IAC) also to be reliable, simple, transportable, and easy to set up, operate, and maintain. Its accuracy has been studied, both from theoretical and experimental points of view, mainly with respect to CCD sampling, photon noise, and threshold influence on centroid determination. The DA/IAC DIMM has been cross calibrated with the existing ESO DIMM. It monitors the seeing with a temporal resolution better than half a minute. This type of instrument is essential for testing new and already existing sites and to ascertain that the surroundings of telescopes do not generate additional turbulence. It is also indispensable to optimize astronomical instrument selection in "flexible scheduling." |
doi_str_mv | 10.1086/133549 |
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A differential image motion monitor (DIMM) is presented which assesses astronomical seeing with those requirements. It has been designed (with collaboration of the staff of the Département d'Astrophysique de l'Université de Nice and the Instituto de Astrofísica de Canarias: DA/IAC) also to be reliable, simple, transportable, and easy to set up, operate, and maintain. Its accuracy has been studied, both from theoretical and experimental points of view, mainly with respect to CCD sampling, photon noise, and threshold influence on centroid determination. The DA/IAC DIMM has been cross calibrated with the existing ESO DIMM. It monitors the seeing with a temporal resolution better than half a minute. This type of instrument is essential for testing new and already existing sites and to ascertain that the surroundings of telescopes do not generate additional turbulence. 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It is also indispensable to optimize astronomical instrument selection in "flexible scheduling."</description><subject>Astronomical Instrumentation</subject><subject>Astronomical magnitude</subject><subject>Centroids</subject><subject>Image intensifiers</subject><subject>Noise measurement</subject><subject>Photons</subject><subject>Pixels</subject><subject>Stars</subject><subject>Telescopes</subject><subject>Turbulence</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1995</creationdate><recordtype>article</recordtype><recordid>eNo9j8FKxDAURYMoWEf9A6Erd515Ly9pE3elM2phigvHdUnTVDvMTCWpC__eSsXVhcvhcg9jtwhLBJWukEgKfcYilKQSUhmdswgARJJyBZfsKoQ9AKJCiNiyciZ8-f70Hudh9MNpOPbWHOJX56buId59uHidr8q8iNdlVV2zi84cgrv5ywV7e9zsiudk-_JUFvk2sTyjMeGyUWknU2FbLYxRVmaZEy2C1qrlrekcEDnNDYIlZ5QSTddkTWNEy6f3mhbsft61fgjBu67-9P3R-O8aof61rGfLCbybwX0YB_9PCUgVSEL6AWI3Sus</recordid><startdate>19950301</startdate><enddate>19950301</enddate><creator>Vernin, Jean</creator><creator>Muñoz-Tuñón, Casiana</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19950301</creationdate><title>Measuring Astronomical Seeing: The DA/IAC DIMM</title><author>Vernin, Jean ; Muñoz-Tuñón, Casiana</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c273t-25b86f564cd94aa8c577e4d10998d2dafe033e92a10c3ea884bfb7bba4d233593</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1995</creationdate><topic>Astronomical Instrumentation</topic><topic>Astronomical magnitude</topic><topic>Centroids</topic><topic>Image intensifiers</topic><topic>Noise measurement</topic><topic>Photons</topic><topic>Pixels</topic><topic>Stars</topic><topic>Telescopes</topic><topic>Turbulence</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Vernin, Jean</creatorcontrib><creatorcontrib>Muñoz-Tuñón, Casiana</creatorcontrib><collection>CrossRef</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Vernin, Jean</au><au>Muñoz-Tuñón, Casiana</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Measuring Astronomical Seeing: The DA/IAC DIMM</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1995-03-01</date><risdate>1995</risdate><volume>107</volume><issue>709</issue><spage>265</spage><epage>272</epage><pages>265-272</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><abstract>Accurate, absolute, and reproducible measurements are the expected qualities of any instrument. A differential image motion monitor (DIMM) is presented which assesses astronomical seeing with those requirements. It has been designed (with collaboration of the staff of the Département d'Astrophysique de l'Université de Nice and the Instituto de Astrofísica de Canarias: DA/IAC) also to be reliable, simple, transportable, and easy to set up, operate, and maintain. Its accuracy has been studied, both from theoretical and experimental points of view, mainly with respect to CCD sampling, photon noise, and threshold influence on centroid determination. The DA/IAC DIMM has been cross calibrated with the existing ESO DIMM. It monitors the seeing with a temporal resolution better than half a minute. This type of instrument is essential for testing new and already existing sites and to ascertain that the surroundings of telescopes do not generate additional turbulence. It is also indispensable to optimize astronomical instrument selection in "flexible scheduling."</abstract><pub>American Institute of Physics</pub><doi>10.1086/133549</doi><tpages>8</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Astronomical Instrumentation Astronomical magnitude Centroids Image intensifiers Noise measurement Photons Pixels Stars Telescopes Turbulence |
title | Measuring Astronomical Seeing: The DA/IAC DIMM |
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