Design of the observation queue scheduler for WEAVE on the WHT
The Observation Queue Scheduler (OQS) for WEAVE is described in this paper, with particular emphasis on the scheduling algorithm. WEAVE is the new 2-deg field of view multi-object (1000 multiplex) spectroscopy facility (R5000 and R20000) at the 4.2-m William Herschel Telescope. The OQS helps to maxi...
Main Authors: | , , , , , , , , , , , , , |
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Format: | Conference item |
Language: | English |
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Society of Photo-Optical Instrumentation Engineers
2018
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_version_ | 1797075027833651200 |
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author | Farina, C Dominguez-Palmero, L Benn, C Guest, S Morris, H Pico, S Carlos Abrams, D Aguerri, JAL Bonifacio, P Carrasco, E Dalton, G Middleton, K Trager, S Vallenari, A |
author_facet | Farina, C Dominguez-Palmero, L Benn, C Guest, S Morris, H Pico, S Carlos Abrams, D Aguerri, JAL Bonifacio, P Carrasco, E Dalton, G Middleton, K Trager, S Vallenari, A |
author_sort | Farina, C |
collection | OXFORD |
description | The Observation Queue Scheduler (OQS) for WEAVE is described in this paper, with particular emphasis on the scheduling algorithm. WEAVE is the new 2-deg field of view multi-object (1000 multiplex) spectroscopy facility (R5000 and R20000) at the 4.2-m William Herschel Telescope. The OQS helps to maximize the scientific impact of WEAVE observations by optimising the schedule of the observing blocks, taking into account the science priority, required instrument configuration and observing constraints. On a nightly basis the OQS will assist the observer in creating a flexible queue of suitable observing blocks to be executed. It will be also possible to run a version of the OQS for extended periods of time to provide guidance on the longer-term planning of WEAVE surveys. |
first_indexed | 2024-03-06T23:44:35Z |
format | Conference item |
id | oxford-uuid:7074fa5c-df55-477e-8079-cb60cfbaefe5 |
institution | University of Oxford |
language | English |
last_indexed | 2024-03-06T23:44:35Z |
publishDate | 2018 |
publisher | Society of Photo-Optical Instrumentation Engineers |
record_format | dspace |
spelling | oxford-uuid:7074fa5c-df55-477e-8079-cb60cfbaefe52022-03-26T19:37:21ZDesign of the observation queue scheduler for WEAVE on the WHTConference itemhttp://purl.org/coar/resource_type/c_5794uuid:7074fa5c-df55-477e-8079-cb60cfbaefe5EnglishSymplectic ElementsSociety of Photo-Optical Instrumentation Engineers2018Farina, CDominguez-Palmero, LBenn, CGuest, SMorris, HPico, SCarlos Abrams, DAguerri, JALBonifacio, PCarrasco, EDalton, GMiddleton, KTrager, SVallenari, AThe Observation Queue Scheduler (OQS) for WEAVE is described in this paper, with particular emphasis on the scheduling algorithm. WEAVE is the new 2-deg field of view multi-object (1000 multiplex) spectroscopy facility (R5000 and R20000) at the 4.2-m William Herschel Telescope. The OQS helps to maximize the scientific impact of WEAVE observations by optimising the schedule of the observing blocks, taking into account the science priority, required instrument configuration and observing constraints. On a nightly basis the OQS will assist the observer in creating a flexible queue of suitable observing blocks to be executed. It will be also possible to run a version of the OQS for extended periods of time to provide guidance on the longer-term planning of WEAVE surveys. |
spellingShingle | Farina, C Dominguez-Palmero, L Benn, C Guest, S Morris, H Pico, S Carlos Abrams, D Aguerri, JAL Bonifacio, P Carrasco, E Dalton, G Middleton, K Trager, S Vallenari, A Design of the observation queue scheduler for WEAVE on the WHT |
title | Design of the observation queue scheduler for WEAVE on the WHT |
title_full | Design of the observation queue scheduler for WEAVE on the WHT |
title_fullStr | Design of the observation queue scheduler for WEAVE on the WHT |
title_full_unstemmed | Design of the observation queue scheduler for WEAVE on the WHT |
title_short | Design of the observation queue scheduler for WEAVE on the WHT |
title_sort | design of the observation queue scheduler for weave on the wht |
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