Instrumentation progress at the Giant Magellan Telescope project
Instrumentation progress at the Giant Magellan Telescope project
复制标题
巨型麦哲伦望远镜项目的仪器进展
DOI:
10.1117/12.2232809
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发表时间:
2016
影响因子:
2.8
通讯作者:
B. Walls
中科院分区:
文献类型:
--
作者:
G. Jacoby;R. Bernstein;A. Bouchez;M. Colless;J. Crane;D. Depoy;B. Espeland;T. Hare;D. Jaffe;J. Lawrence;J. Marshall;P. Mcgregor;S. Shectman;R. Sharp;A. Szentgyorgyi;A. Uomoto;B. Walls
Instrument development for the 24m Giant Magellan Telescope (GMT) is described: current activities, progress, status, and schedule. One instrument team has completed its preliminary design and is currently beginning its final design (GCLEF, an optical 350-950 nm, high-resolution and precision radial velocity echelle spectrograph). A second instrument team is in its conceptual design phase (GMACS, an optical 350-950 nm, medium resolution, 6-10 arcmin field, multi-object spectrograph). A third instrument team is midway through its preliminary design phase (GMTIFS, a near-IR YJHK diffraction-limited imager/integral-field-spectrograph), focused on risk reduction prototyping and design optimization. A fourth instrument team is currently fabricating the 5 silicon immersion gratings needed to begin its preliminary design phase (GMTNIRS, a simultaneous JHKLM high-resolution, AO-fed, echelle spectrograph). And, another instrument team is focusing on technical development and prototyping (MANIFEST, a facility robotic, multifiber feed, with a 20 arcmin field of view). In addition, a medium-field (6 arcmin, 0.06 arcsec/pix) optical imager will support telescope and AO commissioning activities, and will excel at narrow-band imaging. In the spirit of advancing synergies with other groups, the challenges of running an ELT instrument program and opportunities for cross-ELT collaborations are discussed.