WEAVE core processing system

Nicholas A. Walton; Mike Irwin; James R. Lewis; Eduardo Gonzalez-Solares; Gavin Dalton; Scott Trager; J. Alfonso L. Aguerri; Carlos Allende Prieto; Chris R. Benn; Don Carlos Abrams; Sergio Picó; Kevin Middleton; Marcello Lodi; Piercarlo Bonifacio

doi:10.1117/12.2055457

WEAVE core processing system

Nicholas A. Walton, Mike Irwin, James R. Lewis, Eduardo Gonzalez-Solares, Gavin Dalton, Scott Trager, J. Alfonso L. Aguerri, Carlos Allende Prieto, Chris R. Benn, Don Carlos Abrams, Sergio Picó, Kevin Middleton, Marcello Lodi, Piercarlo Bonifacio

Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic

2 Citations (Scopus)

Abstract

WEAVE is an approved massive wide field multi-object optical spectrograph (MOS) currently entering its build phase, destined for use on the 4.2-m William Herschel Telescope (WHT). It will be commissioned and begin survey operations in 2017. This paper describes the core processing system (CPS) system being developed to process the bulk data flow from WEAVE. We describe the processes and techniques to be used in producing the scientifically validated 'Level 1' data products from the WEAVE data. CPS outputs will include calibrated one-d spectra and initial estimates of basic parameters such as radial velocities (for stars) and redshifts (for galaxies).

Original language	English
Title of host publication	Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
Publisher	SPIE
Volume	91520R
DOIs	https://doi.org/10.1117/12.2055457
Publication status	Published - Jul-2014
Event	SPIE Astronomical Telescopes + Instrumentation, 2014, Montréal, Quebec, Canada - Montréal in Quebec, Canada Duration: 22-Jun-2014 → 27-Jun-2014

Conference

Conference	SPIE Astronomical Telescopes + Instrumentation, 2014, Montréal, Quebec, Canada
Country/Territory	Canada
City	Montréal in Quebec
Period	22/06/2014 → 27/06/2014

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10.1117/12.2055457

http://adsabs.harvard.edu/abs/2014SPIE.9152E..0RW

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Walton, N. A., Irwin, M., Lewis, J. R., Gonzalez-Solares, E., Dalton, G., Trager, S., Aguerri, J. A. L., Allende Prieto, C., Benn, C. R., Abrams, D. C., Picó, S., Middleton, K., Lodi, M., & Bonifacio, P. (2014). WEAVE core processing system. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series (Vol. 91520R). Article 91520R SPIE. https://doi.org/10.1117/12.2055457

@inproceedings{da2b452ee9b84a529619c7b68b578867,

title = "WEAVE core processing system",

abstract = "WEAVE is an approved massive wide field multi-object optical spectrograph (MOS) currently entering its build phase, destined for use on the 4.2-m William Herschel Telescope (WHT). It will be commissioned and begin survey operations in 2017. This paper describes the core processing system (CPS) system being developed to process the bulk data flow from WEAVE. We describe the processes and techniques to be used in producing the scientifically validated 'Level 1' data products from the WEAVE data. CPS outputs will include calibrated one-d spectra and initial estimates of basic parameters such as radial velocities (for stars) and redshifts (for galaxies).",

author = "Walton, {Nicholas A.} and Mike Irwin and Lewis, {James R.} and Eduardo Gonzalez-Solares and Gavin Dalton and Scott Trager and Aguerri, {J. Alfonso L.} and {Allende Prieto}, Carlos and Benn, {Chris R.} and Abrams, {Don Carlos} and Sergio Pic{\'o} and Kevin Middleton and Marcello Lodi and Piercarlo Bonifacio",

year = "2014",

month = jul,

doi = "10.1117/12.2055457",

language = "English",

volume = " 91520R",

booktitle = "Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series",

publisher = "SPIE",

note = " SPIE Astronomical Telescopes + Instrumentation, 2014, Montr{\'e}al, Quebec, Canada ; Conference date: 22-06-2014 Through 27-06-2014",

}

Walton, NA, Irwin, M, Lewis, JR, Gonzalez-Solares, E, Dalton, G, Trager, S, Aguerri, JAL, Allende Prieto, C, Benn, CR, Abrams, DC, Picó, S, Middleton, K, Lodi, M & Bonifacio, P 2014, WEAVE core processing system. in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. vol. 91520R, 91520R, SPIE, SPIE Astronomical Telescopes + Instrumentation, 2014, Montréal, Quebec, Canada, Montréal in Quebec, Canada, 22/06/2014. https://doi.org/10.1117/12.2055457

TY - GEN

T1 - WEAVE core processing system

AU - Walton, Nicholas A.

AU - Irwin, Mike

AU - Lewis, James R.

AU - Gonzalez-Solares, Eduardo

AU - Dalton, Gavin

AU - Trager, Scott

AU - Aguerri, J. Alfonso L.

AU - Allende Prieto, Carlos

AU - Benn, Chris R.

AU - Abrams, Don Carlos

AU - Picó, Sergio

AU - Middleton, Kevin

AU - Lodi, Marcello

AU - Bonifacio, Piercarlo

PY - 2014/7

Y1 - 2014/7

N2 - WEAVE is an approved massive wide field multi-object optical spectrograph (MOS) currently entering its build phase, destined for use on the 4.2-m William Herschel Telescope (WHT). It will be commissioned and begin survey operations in 2017. This paper describes the core processing system (CPS) system being developed to process the bulk data flow from WEAVE. We describe the processes and techniques to be used in producing the scientifically validated 'Level 1' data products from the WEAVE data. CPS outputs will include calibrated one-d spectra and initial estimates of basic parameters such as radial velocities (for stars) and redshifts (for galaxies).

AB - WEAVE is an approved massive wide field multi-object optical spectrograph (MOS) currently entering its build phase, destined for use on the 4.2-m William Herschel Telescope (WHT). It will be commissioned and begin survey operations in 2017. This paper describes the core processing system (CPS) system being developed to process the bulk data flow from WEAVE. We describe the processes and techniques to be used in producing the scientifically validated 'Level 1' data products from the WEAVE data. CPS outputs will include calibrated one-d spectra and initial estimates of basic parameters such as radial velocities (for stars) and redshifts (for galaxies).

UR - http://adsabs.harvard.edu/abs/2014SPIE.9152E..0RW

U2 - 10.1117/12.2055457

DO - 10.1117/12.2055457

M3 - Conference contribution

VL - 91520R

BT - Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

PB - SPIE

T2 - SPIE Astronomical Telescopes + Instrumentation, 2014, Montréal, Quebec, Canada

Y2 - 22 June 2014 through 27 June 2014

ER -

WEAVE core processing system

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