Paper
25 July 2000 NOAO queue-observing experiment on the WIYN Telescope
Abhijit Saha, Dianne L. Harmer, Paul S. Smith, Daryl W. Willmarth
Author Affiliations +
Abstract
For the last 3 years, most of NOAO's 40 percent observing share on the WIYN 3.5 m telescope has been used for queued observing, with the goal of facilitating highly ranked science proposals that require rare observing conditions and/or synoptic or 'target of opportunity' observations. The ease of switching between imaging on one Nasmyth focus and multi- object fiber fed bench spectroscopy on the other Nasmyth port offers the choice of making the best use of the extant observing conditions. We assess the results of this experiment and highlight some of the forefront observing programs that have been executed. We discuss algorithms that facilitate making decisions on both long and short time scales so that we can provide the best match of program requirements and observing conditions. We suggest a way of quantifying the prioritization of programs beyond simple ranking that will greatly aid decision making, and evolve the procedures to where queued observations better serve the emphases placed by the time allocation process, without compromising the intent of the scientific investigators.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Abhijit Saha, Dianne L. Harmer, Paul S. Smith, and Daryl W. Willmarth "NOAO queue-observing experiment on the WIYN Telescope", Proc. SPIE 4010, Observatory Operations to Optimize Scientific Return II, (25 July 2000); https://doi.org/10.1117/12.392499
Lens.org Logo
CITATIONS
Cited by 4 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Databases

Spectroscopy

Imaging spectroscopy

Spectrographs

Mirrors

Gamma radiation

RELATED CONTENT

Mass-producing spectra: the SDSS spectrographic system
Proceedings of SPIE (September 30 2004)
Spectro-imaging of the extreme-UV solar corona
Proceedings of SPIE (September 27 2005)
Optical design for a 1-deg. FOV 30-m telescope
Proceedings of SPIE (August 02 2000)

Back to Top