找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

Titlebook: Optical Detectors For Astronomy II; State-of-the-Art at Paola Amico,James W. Beletic Book 2000 Springer Science+Business Media Dordrecht 2

[復制鏈接]
樓主: Scuttle
31#
發(fā)表于 2025-3-26 21:54:08 | 只看該作者
CCD Mosaicing technique for Suprime-Cam (SUbaru PRIME focus CAMera)We have developed a procedure of placing high-precision 2K×4K CCDs manufactured by SITe and MIT into a mosaic for a CCD camera, the SUbaru PRIME focus CAMera (Suprime-Cam). We used this procedure to install 8 CCDs, achieving our requirement of co-planarity of the CCD surfaces to within ±15 μm.
32#
發(fā)表于 2025-3-27 03:25:29 | 只看該作者
33#
發(fā)表于 2025-3-27 07:29:40 | 只看該作者
https://doi.org/10.1007/978-94-011-4361-5CCD; Observatories; Sensor; astronomy; electronics; integrated circuit; metal-oxide-semiconductor transist
34#
發(fā)表于 2025-3-27 12:37:33 | 只看該作者
35#
發(fā)表于 2025-3-27 15:13:42 | 只看該作者
36#
發(fā)表于 2025-3-27 18:23:22 | 只看該作者
37#
發(fā)表于 2025-3-27 23:30:47 | 只看該作者
CFH12K: Optimising 12 MIT/LL CCID-20 CCDs for a direct imaging applicationr imaging mode. Adaptation to the CFHT prime focus environment included modifications to reduce the scattered light seen by the CFH12K. Science data taken by the camera has proven the success of CFHT’s new capability for 42×28 square arcminute imaging with high-resolution subarcsecond seeing.
38#
發(fā)表于 2025-3-28 04:22:59 | 只看該作者
The current state of the art in large CCD mosaic cameras, and a new strategy for wide field, high reution (FWHM ≈ O”.12) deep images over large fields of view (l°×l°) using an array of modest telescopes (D ~ 1.5-1.8m) equipped with mosaics of independently-addressable orthogoral transfer CCD (OTCCD) arrays.
39#
發(fā)表于 2025-3-28 10:17:22 | 只看該作者
40#
發(fā)表于 2025-3-28 13:50:31 | 只看該作者
BUSCA: A simultaneous 4 colour camera with 4K×4K CCDsansmission fluctuations (non-photometric conditions) have almost no effect on colour index determination as colour bands are observed simultaneously. The instrument has been tested at the 1 m telescope of Bonn University’s “Hoher List” Observatory and will have its first Calar Alto run in Spring 2000.
 關于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學 Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結 SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學 Yale Uni. Stanford Uni.
QQ|Archiver|手機版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-9 00:06
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權所有 All rights reserved
快速回復 返回頂部 返回列表
平陆县| 远安县| 新乐市| 天镇县| 云阳县| 漾濞| 衡阳县| 崇明县| 酒泉市| 河源市| 连山| 巴彦淖尔市| 上饶县| 赤城县| 金寨县| 信阳市| 岐山县| 平定县| 康平县| 广元市| 云龙县| 吐鲁番市| 阿拉善右旗| 长葛市| 若尔盖县| 格尔木市| 同仁县| 深泽县| 怀宁县| 南投市| 辽阳县| 丹巴县| 和政县| 哈密市| 南阳市| 大关县| 横峰县| 叙永县| 静乐县| 蛟河市| 鄂温|