WAS: the archive for the WEAVE spectrograph by Guerra, J, Molinari, E, Lodi, M, Martin, A, Dalton, GB, Trager, SC, Abrams, DC, Bonifacio, P, López Aguerri, JA, Vallenari, A, Carrasco Licea, EE, Middleton, KF

“…The WAS1(WEAVE Archive System) is a software architecture for archiving and delivering the data releases for the WEAVE7 instrument at WHT (William Herschel Telescope). …”

The WEAVE observatory control system by Pico, S, Carlos Abrams, D, Benn, C, Dominguez, L, Farina, C, Miguel Delgado, J, Martin, C, Cano, D, Salasnich, B, Guest, S, Gribbin, F, Skvarc, J, Gafton, E, Dalton, G, Middleton, K, Tragger, S, Alfonso Aguerri, J, Bonifacio, P, Vallenari, A, Carrasco, E

“…WEAVE is the next-generation spectroscopic facility for the William Herschel Telescope (WHT) 1,2. …”

WEAVE core processing system by Walton, N, Irwin, M, Lewis, JR, Gonzalez-Solares, E, Dalton, G, Trager, S, Aguerri, J, Allende Prieto, C, Benn, C, Abrams, D, Picó, S, Middleton, K, Lodi, M, Bonifacio, P

“…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). …”

First results of tests on the WEAVE fibres by Sayède, F, Younes, Y, Fasola, G, Dorent, S, Abrams, D, Aguerri, J, Bonifacio, P, Dalton, G, Dee, K, Laporte, P, Lewis, I, Lhome, E, Middleton, K, Pragt, J, Rey, J, Stuik, R, Trager, S, Vallenari, A

“…WEAVE is a new wide-field spectroscopy facility proposed for the prime focus of the 4.2m William Herschel Telescope. …”

Fibre positioning algorithms for the WEAVE spectrograph by Terrett, D, Lewis, I, Dalton, G, Abrams, D, Aguerri, J, Bonifacio, P, Middleton, K, Trager, S

“…WEAVE is the next-generation wide-field optical spectroscopy facility for the William Herschel Telescope (WHT) in La Palma, Canary Islands, Spain. …”

Fibre links for the WEAVE instrument: the making of by Mignot, S, Bonifacio, P, Fasola, G, Dalton, G, Lewis, I

“…The WEAVE instrument nearing completion for the William Herschel Telescope is a fiber-fed spectrograph operating in three different modes. …”

Optimisation of the WEAVE target assignment algorithm by Hughes, S, Dalton, G, Smith, D, Duncan, K, Terrett, D, Abrams, DC, Aguerri, JA, Bishop, G, Bonifacio, P, Carrasco, E, Jin, S, Lewis, I, Trager, S, Vallenari, A

“…WEAVE is the new wide-field spectroscopic facility for the prime focus of the William Herschel Telescope in La Palma, Spain. …”

Calibration at elevation of the WEAVE fibre positioner by Hughes, S, Dalton, G, Dee, K, Abrams, DC, Middleton, K, Lewis, I, Terrett, D, Aguerri, AL, Balcells, M, Bishop, G, Bonifacio, P, Carrasco, E, Trager, SC, Vallenari, A

“…WEAVE is the new wide-field spectroscopy facility for the prime focus of the William Herschel Telescope in La Palma, Spain. …”

Development of the single fibres and IFUs of WEAVE by Guinouard, I, Bonifacio, P, Trager, S, Verheijen, M, Lewis, I, Dalton, G

“…WEAVE is a new wide-field spectroscopy facility proposed for the prime focus of the 4.2m William Herschel telescope. …”

VPHGs for WEAVE: design, manufacturing and characterisation by Bianco, A, Pariani, G, Aliverti, M, Zanutta, A, Arns, J, Pragt, J, Stuik, R, Middleton, K, Tosh, I, Dalton, G, Trager, S, Abrams, DC, Aguerri, JAL, Bonifacio, P, Vallenari, A, Carrasco, E

“…WEAVE is the next-generation optical spectroscopy facility for the William Herschel Telescope (WHT). …”

WEAVE spectrograph cameras: the polishing of the spherical lenses by Izazaga, R, Carrasco, E, Hidalgo, A, Aguirre, D, Terlevich, E, Terlevich, R, Dalton, G, Trager, S, Aguerri, J, Bonifacio, P, Vallenari, A, Abrams, D, Middleton, K

“…WEAVE fiber-fed spectrograph offers two resolutions, R ~ 5000 and 20,000. …”

Design of the observation queue scheduler for WEAVE on the WHT by 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

“…The Observation Queue Scheduler (OQS) for WEAVE is described in this paper, with particular emphasis on the scheduling algorithm. …”

Antireflective coatings for the red camera of WEAVE spectrograph by Ortiz, R, Carrasco, E, Paez, G, Reyes, J, Hidalgo, A, Dalton, G, Trager, S, Aguerri, J, Bonifacio, P, Vallenari, A, Abrams, D, Middleton, K

“…In this work we present the coatings of the spectrograph red camera of WEAVE -the new multiobject survey facility for the 4.2m William Herschel Telescope. …”

Low-level control software for the WEAVE spectrograph by Salasnich, B, Pérez, C, Delgado, J, Picó, S, Infantes, D, Stuik, R, Baruffolo, A, Dalton, G, Trager, S, Aguerri, J, Bonifacio, P, Vallenari, A, Carrasco, E, Abrams, D, Middleton, K, WEAVE Instrument Consortium

“…<p>WEAVE is a wide-field spectroscopy facility for WHT which includes a multi-object dual-beam spectrograph which will operate in the visible wavelength range. …”

The WEAVE prime focus Correction: from design to integration by Tomás, A, Canchado, M, Casalta, J, Dalmases, F, Maroto, O, Martín-Nuño, C, Romero, A, Aguerri, J, Harreros, J, Delgado, J, Burgal, J, Abrams, D, Dee, K, Lhomé, E, Dalton, G, Middleton, K, Bonifacio, P, Trager, S, Vallenari, A, Carrasco, E

“…WEAVE is a new wide-field multi-object spectroscopy (MOS) facility proposed for the prime focus of the 4.2m William Herschel Telescope (WHT), situated on the island of La Palma, Canary Islands, Spain. …”

First lab results of the WEAVE fibre positioner system by Schallig, E, Lewis, I, Dalton, G, Brock, M, Terrett, D, Abrams, D, Middleton, K, Bishop, G, Aguerri, J, Bonifacio, P, Licea, E, Trager, S, Vallenari, A

“…WEAVE is the new wide-field spectroscopy facility for the prime focus of the William Herschel Telescope on La Palma in the Canary Islands, Spain. …”

Final assembly, metrology, and testing of the WEAVE fibre positioner by Hughes, S, Schallig, E, Lewis, I, Dalton, G, Terrett, D, Abrams, DC, Trager, S, Brock, M, Bishop, G, Middleton, K, Bonifacio, P, Vallenari, A, Carrasco, E, Aguerri, A

“…WEAVE is the new wide-field spectroscopy facility for the prime focus of the William Herschel Telescope at La Palma, Spain. …”

The hardware control system for WEAVE at the William Herschel telescope by Delgado, J, Mendoza, S, Burgal, J, Herreros, J, Picó, S, Abrams, D, Martin, C, Cano, D, Gribbin, F, Skvarc, J, Dee, K, Lhome, E, Dalton, G, Middleton, K, Trager, S, Aguerri, J, Bonifacio, P, Vallenari, A, Carrasco, E

“…In order, to keep the telescope tracking the field of view selected, the instrument will need to a rotation system for compensating it [1]. The new WEAVE [2] two degrees field of view requires a new field de-rotator on the top-end of the telescope. …”

Towards integrated modelling: full image simulations for WEAVE by Dalton, G, Ham, S, Trager, S, Abrams, D, Bonifacio, P, Aguerri, J, Middleton, K, Benn, C, Rogers, K, Stuik, R, Carrasco, E, Vallenari, A, Jin, S, Lewis, J

“…We present an integrated end-end simulation of the spectral images that will be obtained by the weave spectrograph, which aims to include full modelling of all effects from the top of the atmosphere to the detector. …”

Design of the calibration unit for the WEAVE multi-object spectrograph at the WHT by Dominguez, L, Cano, D, O'Mahony, N, Martin, C, Pico, S, Benn, C, Trager, S, Lhomé, E, Ridings, A, Fariña, C, Abrams, D, Balcells, M, Irwin, M, Lewis, J, Aguerri, J, Bonifacio, P, Vallenari, A, Carrasco, E, Dalton, G

“…The design of the WEAVE calibration unit is now complete.…”