Titlebook: Astronomy with Schmidt-Type Telescopes; Proceedings of the 7 Massimo Capaccioli Conference proceedings 1984 D. Reidei Publishing Company, D

collateral

無(wú)可爭(zhēng)辯

https://doi.org/10.1007/978-3-662-11767-5hese plates. ESO has an integrated system of three microdensitometers, a PDS 1010A, an Optronics S3000 and a Grant 800. Data analysis facilities include an HP 1000 series computer supporting an interactive data analysis system and two Vax 11/780 computers supporting general purpose computing and dat

Rodent

Bucket

https://doi.org/10.1007/978-3-662-11767-5have been discovered, and summarise some of the most interesting results to date. So far, the searches have been based on sequences of a dozen or more sky limited UK 1.2m Schmidt plates taken on timescales from one day to several years. The plates were measured on the COSMOS measuring machine at the

鉆孔

Oafishness

VAN

https://doi.org/10.1007/978-3-662-11767-5 facility at Cambridge is described. The system is being applied in a number of ways including automated quasar detection and subsequent clustering analyses, galaxy redshift surveys, and wide field searches for rare objects, such as carbon stars.

Injunction

繁榮地區(qū)

https://doi.org/10.1007/978-3-642-86743-9ction of these plates, including those for the southern and equatorial Sky Surveys, are on Eastman Kodak IIIa-J emulsion. A significant number of these processed IIIa-J plates have developed many small gold spots similar in size to faint star images. They are most likely to occur in areas of relativ

modish

Astrophysics and Space Science Libraryhttp://image.papertrans.cn/b/image/163655.jpg