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Titlebook: Optical Detectors for Astronomy; Proceedings of an ES James W. Beletic,Paola Amico Conference proceedings 1998 Springer Science+Business Me

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发表于 2025-3-21 17:07:13 | 显示全部楼层 |阅读模式
书目名称Optical Detectors for Astronomy
副标题Proceedings of an ES
编辑James W. Beletic,Paola Amico
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Optical Detectors for Astronomy; Proceedings of an ES James W. Beletic,Paola Amico Conference proceedings 1998 Springer Science+Business Me
描述The Workshop "Optical Detectors for Astronomy" was held during October 8-10, 1996 at the headquarters of the European Southern Observatory in Garching, Germany. This was the third meeting of its kind, previous meetings being held in 1991 and 1993, but this is the first ESO "CCD Workshop" that has published proceedings. Most of the leading manufacturers and major astronomical observatories were represented, with the 117 attendees coming together from 14 different countries that spanned every continent on Earth. The motivation for the ESO CCD Workshop series is the creation of informal and open venue of information exchange about astronomical CCD detectors and systems. Judging from the reaction and feedback of the participants, the 1996 workshop was as successful as the previous editions, which is a credit to all who attended. The Workshop was organized as a mixture of invited talks, oral presentations, poster sessions and roundtable discussions, the latter used to foster a free exchange of ideas among participants. These technical sessions were complemented by an opening reception and a congenial evening in downtown Munich, which included a walking tour of the historic area followed
出版日期Conference proceedings 1998
关键词Astrometry; CCD; Observatories; Sensor; astronomy; electronics; instruments
版次1
doihttps://doi.org/10.1007/978-94-011-5262-4
isbn_softcover978-94-010-6214-5
isbn_ebook978-94-011-5262-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 1998
The information of publication is updating

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The Astronomical CCD Development Program at Copenhagen Universitywar, the system is designed to accommodate a variety of commonly used CCDs up to the Loral 2kx2k devices in up to 2 x 2 mosaics, read through up to 8 parallel channels. The PC/MC68020 based controller performs in all essential respects on a par with other systems currently in use at major observator
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A Drift Scan Camera for Astrometrygets of the project are both scientific (galactic populations statistics, parallaxes) and technological (acquisition of expertise on drift scan technique for high accuracy astrometric ground based and spaceborne surveys). In particular, the issues of field distortions and timing accuracy are discuss
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RGO (and ING) CCDs — Current Developments of their focal plane requirements. The current status of the RGO programmes of CCD-upgrades is also discussed. We present details of ‘recent’ RGO detector work (since the previous 1993 ESO workshop), together with plans for the future.
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High Precision Shutter for the T.N.G. CCD Camerage dimensions or the combination of CCDs to form mosaics. The TNG optical imager, for example, will use a 6 cm squared CCD detector (2 X 2 Loral chips). Furthermore, modern fast optics telescopes, such as the NTT or the TNG, use, for standard star calibration, exposure times real-time control softwa
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ESO’s New CCD Testbencht step in this process is the CCD characterization and optimization that is done after the device is received from the manufacturer. In order to accommodate the new large CCDs and to interface to the new FIERA controller, ESO is building a new CCD testing facility in Garching. Among the measurements
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