TY - GEN
T1 - Raven, a harbinger of Multi-Object adaptive optics based instruments at the subaru telescope
AU - Conan, Rodolphe
AU - Bradley, Colin
AU - Lardière, Olivier
AU - Blain, Celia
AU - Venn, Kim
AU - Andersen, David
AU - Simard, Luc
AU - Véran, Jean Pierre
AU - Herriot, Glen
AU - Loop, David
AU - Usuda, Tomonori
AU - Oya, Shin
AU - Hayano, Yutaka
AU - Terada, Hiroshi
AU - Akiyama, Masayuki
PY - 2010
Y1 - 2010
N2 - In the context of instrumentation for Extremely Large Telescopes (ELTs), an Integral Field Spectrographs (IFSs), fed with a Multi-Object Adaptive Optics (MOAO) system, has many scientific and technical advantages. Integrated with an ELT, a MOAO system will allow the simultaneous observation of up to 20 targets in a several arc-minute fieid-of-view, each target being viewed, with unprecedented sensitivity and resolution. However, before building a MOAO instrument for an ELT, several critical issues, such as open-loop control and calibration, must be solved. The Adaptive Optics Laboratory of the University of Victoria, in collaboration with the Herzberg Institute of Astrophysics, the Subaru telescope and two industrial partners, is starting the construction of a MOAO pathfinder, called Raven. The goal of Raven is two fold: first, Raven has to demonstrate that MOAO technical challenges can be solved and implemented reliably for routine on-sky observations. Secondly, Raven must demonstrate that reliable science can be delivered with multiplexed AO systems. In order to achieve these goals, the Raven science channels will be coupled to the Subaru's spectrograph (IRCS) on the infrared Nasmyth platform. This paper will present the status of the project, including the conceptual instrument design and a discussion of the science program.
AB - In the context of instrumentation for Extremely Large Telescopes (ELTs), an Integral Field Spectrographs (IFSs), fed with a Multi-Object Adaptive Optics (MOAO) system, has many scientific and technical advantages. Integrated with an ELT, a MOAO system will allow the simultaneous observation of up to 20 targets in a several arc-minute fieid-of-view, each target being viewed, with unprecedented sensitivity and resolution. However, before building a MOAO instrument for an ELT, several critical issues, such as open-loop control and calibration, must be solved. The Adaptive Optics Laboratory of the University of Victoria, in collaboration with the Herzberg Institute of Astrophysics, the Subaru telescope and two industrial partners, is starting the construction of a MOAO pathfinder, called Raven. The goal of Raven is two fold: first, Raven has to demonstrate that MOAO technical challenges can be solved and implemented reliably for routine on-sky observations. Secondly, Raven must demonstrate that reliable science can be delivered with multiplexed AO systems. In order to achieve these goals, the Raven science channels will be coupled to the Subaru's spectrograph (IRCS) on the infrared Nasmyth platform. This paper will present the status of the project, including the conceptual instrument design and a discussion of the science program.
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U2 - 10.1117/12.856567
DO - 10.1117/12.856567
M3 - Conference contribution
AN - SCOPUS:77957830410
SN - 9780819482266
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Adaptive Optics Systems II
T2 - Adaptive Optics Systems II
Y2 - 27 June 2010 through 2 July 2010
ER -