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. …”

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. …”

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. …”

The polishing of WEAVE spectrograph collimator mirror by Izazaga, R, Carrasco, E, Hidalgo, A, Dalton, G, Trager, S, Aguerri, J, Bonifacion, P, Vallenari, A, Abrams, D, Middleton, K

“…WEAVE is the new wide field multi-object and integral field survey facility for the prime focus of the 4.2 m 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. …”

The WEAVE focus translation system: from design to construction by Canchado, M, Romero, A, Maroto, O, Tomàs, A, Martin-Nuño, C, Casalta, J, Prida, J, Aguerri, J, Herreros, J, Delgado, J, Burgal, J, Abrams, D, Dee, K, Dalton, G, Bonfacio, P, Trager, S, Vallenari, A

“…<p>WEAVE is a new wide-field spectroscopy facility proposed for the prime focus of the 4.2m William Herschel Telescope (WHT), placed in La Palma, Canary Islands, Spain.…”

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.…”

Thermal and mechanical design and test of the CCD mount for the WEAVE spectrograph cryostats by Bates, S, Steele, IA, Mottram, CJ, Jermak, HE, Tromp, N, Kragt, J, Elswijk, E, Pragt, J, Stuik, R, Barnsley, R, Monroe, C, Dalton, G, Trager, S, Aguerri, JAL, Bonifacio, P, Vallenari, A, Carrasco, E, Abrams, DC, Middleton, K

“…<p>WEAVE is the new multi-object spectrograph for the William Herschel Telescope on La Palma. …”

Developments in fibre positioning technology for the WEAVE instrument for the William Herschel Telescope by Schallig, E, Lewis, I, Gilbert, J, Dalton, G, Brock, M, Abrams, D, Middleton, K, Aguerri, J, Bonifacio, P, Carrasco, E, Trager, S, Vallenari, A

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