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...

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Main Authors: 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
Format: Conference item
Language:English
Published: Society of Photo-Optical Instrumentation Engineers 2018
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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.
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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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