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. …”

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. …”

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. …”

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. …”

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.…”

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. …”

Testing process for the WEAVE prime focus corrector lenses for the William Herschel Telescope by Bogunivic, D, Jonas, G, Cochrane, D, Rakich, A, Connor, P, Romeril, J, Gers, L, Howick, E, Young, C, Reed, T, Tosh, I, Lhomé, E, Dee, K, Dalton, G, Trager, S, Agerri, J, Bonifacio, P, Vallenari, A, Carrasco, E, Abrams, D, Middleton, K

“…A new prime focus corrector for the WEAVE project for the William Herschel Telescope is being produced. …”

WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope by Dalton, G, Trager, S, Abrams, D, Carter, D, Bonifacio, P, Aguerri, J, MacIntosh, M, Evans, C, Lewis, I, Navarro, R, Agocs, T, Dee, K, Rousset, S, Tosh, I, Middleton, K, Pragt, J, Terrett, D, Brock, M, Benn, C, Verheijen, M, Cano, D, Bevil, C, Steele, I, Mottram, C, Bates, S

“…We present the preliminary design of the WEAVE next generation spectroscopy facility for the William Herschel Telescope (WHT), principally targeting optical ground-based follow up of upcoming ground-based (LOFAR) and space-based (Gaia) surveys. …”

Construction progress of WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope by Dalton, G, Trager, S, Abrams, D, Lewis, I, Brock, M, Schallig, E, al., E

“…We present an update on the overall construction progress of the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT), now that all the major fabrication contracts are in place. …”

Manufacturing process for the WEAVE Prime Focus Corrector optics for the 4.2m William Herschel Telescope by Lhomé, E, Agócs, T, Abrams, D, Dee, K, Middleton, K, Tosh, I, Jaskó, A, Connor, P, Cochrane, D, Gers, L, Jonas, G, Rakich, A, Dalton, G, Benn, C, Balcells, M, Trager, S, Carrasco, E, Vallenari, A, Bonifacio, P, Aguerri, J

“…In this paper, we detail the manufacturing process for the lenses that will constitute the new two-degree field-of-view Prime Focus Corrector (PFC) for the 4.2m William Herschel Telescope (WHT) optimised for the upcoming WEAVE Multi-Object Spectroscopy (MOS) facility. The corrector, including an Atmospheric Dispersion Corrector (ADC), is made of six large lenses, the largest being 1.1-meter diameter. …”

Final design and progress of WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope by Dalton, G, Trager, S, Abrams, D, Bonifacio, P, Aguerri, J, Middleton, K, Benn, C, Dee, K, Sayède, F, Lewis, I, Pragt, J, Pico, S, Walton, N, Rey, J, Prieto, C, Peñate, J, Lhome, E, Agócs, T, Alonso, J, Terrett, D, Brock, M, Gilbert, J, Schallig, E, Ridings, A, Guinouard, I, Verheijen, M, Tosh, I, Rogers, K, Lee, M, Steele, I, Stuik, R, Tromp, N, Jasko, A, Carrasco, E, Farcas, S, Kragt, J, Lesman, D, Kroes, G, Mottram, C, Bates, S, Gribbin, F, Rodriguez, L, Delgado, J, Herreros, J, Martin, C, Cano, D, Navarro, R, Irwin, M, Lewis, J, Solares, E, Murphy, D, Worley, C, O'Mahony, N, Bassom, R, Bianco, A, Zurita, C, ter Horst, R, Molinari, E, Lodi, M, Guerra, J, Martin, A, Vallenari, A, Salasnich, B, Baruffolo, A, Jin, S, Hill, V, Smith, D, Drew, J, Poggianti, B, Pieri, M, Palmero, L, Farina, C

“…We present the Final Design of the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT), together with a status update on the details of manufacturing, integration and the overall project schedule now that all the major fabrication contracts are in place. …”