IDS Spectroscopy of Faint Emission-Line Objects

Details IDS Spectroscopy of Faint Emission-Line Objects IDS Spectroscopy of Faint Emission-Line Objects

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984msngr..37...35l&link_type=abstract

The Messenger, No. 37, P.35, 1984

Physics

5

Scientific paper

Ouring the last decades we have seen the advent of new technology detectors, which no longer contain a photographic emulsion as a last step. These detectors, such as the lOS (Image Oissector Scanner) for spectroscopic work and the CCO (Charge-Coupled Oevice) for field imaging, produce digitized data, which can easily be stored on a disk or on a magnetic tape. In this short article we will report some of our experiences of the lOS devices of ESO. The lOS at the 3.6 m telescope was taken into use in 1978 and the one at the 1.52 m telescope followed two years later. Although we have had the opportunity to use both instruments we will concentrate on a programme performed exclusively with the 1.52 m telescope.

Affiliated with

Also associated with

No associations

Rating

IDS Spectroscopy of Faint Emission-Line Objects does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with IDS Spectroscopy of Faint Emission-Line Objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IDS Spectroscopy of Faint Emission-Line Objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1396767