WEAVE Detectors Completion
Lead Research Organisation:
Liverpool John Moores University
Department Name: Astrophysics Research Institute
Abstract
This grant is to complete the production and commissioning of the detector system for the WEAVE spectrograph.
Planned Impact
ARI has a long tradition of strong industrial and PUS engagement. For this particular project we will continue our policy of engagement with engineering firms who will be commissioned to manufacture the structure of the instrument. In the past this has allowed firms working with us to upgrade their skills and machinery to deliver the high precision needed for astronomical instrumentation, allowing them to received grants and R&D tax credits in order to upgrade their precision machining capability and safeguarding a number of jobs at the time. In addition such firms have been able to use their work on astronomical instrumentation to enhance their reputation with other customers and has assisted them in gaining access to new markets (for example contracts with ING and CERN).
Publications
Antoja T
(2017)
Asymmetric metallicity patterns in the stellar velocity space with RAVE
in Astronomy & Astrophysics
Gonzalez-Perez V
(2017)
The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5
in Monthly Notices of the Royal Astronomical Society
Monreal-Ibero A
(2017)
Measuring diffuse interstellar bands with cool stars Improved line lists to model background stellar spectra?
in Astronomy & Astrophysics
Youakim K
(2017)
The Pristine survey - III. Spectroscopic confirmation of an efficient search for extremely metal-poor stars
in Monthly Notices of the Royal Astronomical Society
Schönrich R
(2017)
Assessing distances and consistency of kinematics in Gaia/TGAS
in Monthly Notices of the Royal Astronomical Society
Starkenburg E
(2017)
The Pristine survey - I. Mining the Galaxy for the most metal-poor stars
in Monthly Notices of the Royal Astronomical Society
DomĂnguez-Tenreiro R
(2017)
The Radial Distribution of Mono-metallicity Populations in the Galactic Disk as Evidence for Two-phase Disk Formation
in The Astrophysical Journal
Erkal D
(2017)
A sharper view of Pal 5's tails: discovery of stream perturbations with a novel non-parametric technique
in Monthly Notices of the Royal Astronomical Society
Pancino E
(2017)
The Gaia -ESO Survey: Calibration strategy
in Astronomy & Astrophysics
Sesar B
(2017)
Machine-learned Identification of RR Lyrae Stars from Sparse, Multi-band Data: The PS1 Sample
in The Astronomical Journal
Blanton M
(2017)
Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
in The Astronomical Journal
Peñarrubia J
(2017)
Stellar envelopes of globular clusters embedded in dark mini-haloes
in Monthly Notices of the Royal Astronomical Society: Letters
Liu C
(2017)
Determination of robust metallicities for metal-rich red giant branch stars An application to the globular cluster NGC 6528???
in Astronomy & Astrophysics
Freeman K
(2017)
Galaxies, Globular Clusters, and Dark Matter
in Annual Review of Astronomy and Astrophysics
Conrad C
(2017)
A RAVE investigation on Galactic open clusters II. Open cluster pairs, groups and complexes?
in Astronomy & Astrophysics
Debattista V
(2017)
Separation of stellar populations by an evolving bar: implications for the bulge of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Ting ?? Y
(2017)
Measuring 14 Elemental Abundances with R = 1800 LAMOST Spectra
in The Astrophysical Journal Letters
Rosslowe C
(2017)
A deep near-infrared spectroscopic survey of the Scutum-Crux arm for Wolf-Rayet stars?
in Monthly Notices of the Royal Astronomical Society
Lagarde N
(2017)
Population synthesis to constrain Galactic and stellar physics I. Determining age and mass of thin-disc red-giant stars
in Astronomy & Astrophysics
Lofthouse E
(2017)
Local analogues of high-redshift star-forming galaxies: integral field spectroscopy of green peas
in Monthly Notices of the Royal Astronomical Society
Griv E
(2017)
The Spiral Arm Segments of the Galaxy within 3 kpc from the Sun: A Statistical Approach
in The Astrophysical Journal
Breedt E
(2017)
Using large spectroscopic surveys to test the double degenerate model for Type Ia supernovae
in Monthly Notices of the Royal Astronomical Society
Ichikawa K
(2017)
Foreground effect on the J-factor estimation of classical dwarf spheroidal galaxies
in Monthly Notices of the Royal Astronomical Society
Figueras F
(2017)
Outskirts of Galaxies
Mateu C
(2017)
Predictions for the detection of tidal streams with Gaia using great-circle methods
in Monthly Notices of the Royal Astronomical Society
Morabito L
(2017)
Investigating the unification of LOFAR-detected powerful AGN in the Boötes field
in Monthly Notices of the Royal Astronomical Society
Ted Mackereth J
(2017)
The age-metallicity structure of the Milky Way disc using APOGEE
in Monthly Notices of the Royal Astronomical Society
Miglio A
(2017)
PLATO as it is : A legacy mission for Galactic archaeology
in Astronomische Nachrichten
Majewski S
(2017)
The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
in The Astronomical Journal
Childress M
(2017)
OzDES multifibre spectroscopy for the Dark Energy Survey: 3-yr results and first data release
in Monthly Notices of the Royal Astronomical Society
Simpson C
(2017)
Extragalactic radio surveys in the pre-Square Kilometre Array era.
in Royal Society open science
Pato M
(2017)
galkin: A new compilation of Milky Way rotation curve data
in SoftwareX
Hansen C
(2017)
Something borrowed, something blue: The nature of blue metal-poor stars inferred from their colours and chemical abundances
in Astronomy & Astrophysics
Jofré P
(2017)
Gaia FGK benchmark stars: opening the black box of stellar element abundance determination
in Astronomy & Astrophysics
Kalfountzou E
(2017)
Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
in Monthly Notices of the Royal Astronomical Society
Monreal-Ibero A
(2017)
The Wolf-Rayet star population in the dwarf galaxy NGC 625
in Astronomy & Astrophysics
Kushniruk I
(2017)
Kinematic structures of the solar neighbourhood revealed by Gaia DR1/TGAS and RAVE
in Astronomy & Astrophysics
Geier S
(2017)
The population of hot subdwarf stars studied with Gaia I. The catalog of known hot subdwarf stars?
in Astronomy & Astrophysics
Simpson J
(2017)
Siriusly, a newly identified intermediate-age Milky Way stellar cluster: a spectroscopic study of Gaia 1
in Monthly Notices of the Royal Astronomical Society
Shimwell T
(2017)
The LOFAR Two-metre Sky Survey I. Survey description and preliminary data release?
in Astronomy & Astrophysics
Burden A
(2017)
Mitigating the impact of the DESI fiber assignment on galaxy clustering
in Journal of Cosmology and Astroparticle Physics
Williams A
(2017)
On the run: mapping the escape speed across the Galaxy with SDSS
in Monthly Notices of the Royal Astronomical Society
Traven G
(2017)
The Galah Survey: Classification and Diagnostics with t-SNE Reduction of Spectral Information
in The Astrophysical Journal Supplement Series
Thygesen A
(2017)
An Investigation of the Formation and Line Properties of MgH in 3D Hydrodynamical Model Stellar Atmospheres
in The Astrophysical Journal
Ting ?? Y
(2017)
Prospects for Measuring Abundances of >20 Elements with Low-resolution Stellar Spectra
in The Astrophysical Journal
Jofré P
(2017)
Climbing the cosmic ladder with stellar twins in RAVE with Gaia
in Monthly Notices of the Royal Astronomical Society
Bosma A
(2017)
Outskirts of Galaxies
Catalán-Torrecilla C
(2017)
Star Formation in the Local Universe from the CALIFA Sample. II. Activation and Quenching Mechanisms in Bulges, Bars, and Disks
in The Astrophysical Journal
Crnojevic D
(2017)
Outskirts of Galaxies
Jean-Baptiste I
(2017)
On the kinematic detection of accreted streams in the Gaia era: a cautionary tale
in Astronomy & Astrophysics
| Description | The WEAVE detector system was successfully built to specification and is now in use at the WHT. |
| Exploitation Route | Scientific Exploitation of WEAVE |
| Sectors | Other |
| URL | https://www.ing.iac.es/astronomy/instruments/weave/weaveinst.html |