Abstract
Two almost identical échelle spectrographs are under construction: for the 3.9m Anglo-Australian (AAT) and the 4.2m William Herschel (WHT) telescopes. The versatility of the optical design requires the simultaneous control of many mechanical functions, so a high level of automation under computer control is essential. The control and data reduction software packages will be highly interactive and will be implemented at the observatories and at home institutions, allowing prospective users to test the feasibility of proposed observing programs. Then, at the observatory, the accumulating data can be preliminarily reduced allowing real-time decisions to be made. The data reduction package should find applications to échelle data generally and the control system may easily be adapted to other instruments.
Original language | English |
---|---|
Title of host publication | Instrumentation in Astronomy VI |
Editors | David L. Crawford |
Publisher | SPIE |
Pages | 721-729 |
Number of pages | 9 |
Volume | 0627 |
ISBN (Print) | 9780892526628 |
DOIs | |
Publication status | Published - 13 Oct 1986 |
Externally published | Yes |
Event | 1986 Astronomy Conferences - Tucson, United States Duration: 1 Mar 1986 → 2 Mar 1986 Conference number: 4 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
---|---|
Publisher | SPIE |
Volume | 0627 |
ISSN (Print) | 0277-786X |
ISSN (Electronic) | 1996-756X |
Conference
Conference | 1986 Astronomy Conferences |
---|---|
Country/Territory | United States |
City | Tucson |
Period | 1/03/86 → 2/03/86 |