Wide-field multi-object spectroscopy with MANIFEST

MANIFEST is a multi-object fibre facility for the Giant Magellan Telescope that uses ‘Starbug’ robots to accurately position fibre units across the telescope’s focal plane. MANIFEST, when coupled to the telescope’s planned seeinglimited instruments, offers access to larger fields of view; higher multiplex gains; versatile focal plane reformatting of the focal plane via integral-field-units; image-slicers; and in some cases higher spatial and spectral resolution. The TAIPAN instrument on the UK Schmidt Telescope is now close to science verification which will demonstrate the feasibility of the Starbug concept. We are now moving into the conceptual development phase for MANIFEST, with a focus on developing interfaces for the telescope and for the instruments.

[1]  Matthew Colless,et al.  The MANIFEST fibre positioning system for the Giant Magellan Telescope , 2014, Astronomical Telescopes and Instrumentation.

[2]  J. Bland-Hawthorn The Hector Survey: integral field spectroscopy of 100,000 galaxies , 2014, Proceedings of the International Astronomical Union.

[3]  Ralf Bender,et al.  VIRUS: production and deployment of a massively replicated fiber integral field spectrograph for the upgraded Hobby-Eberly Telescope , 2014, Astronomical Telescopes and Instrumentation.

[4]  T. Prochaska,et al.  GMACS: a wide field, multi-object, moderate-resolution, optical spectrograph for the Giant Magellan Telescope , 2012, Other Conferences.

[5]  Matthew Colless,et al.  The Taipan Galaxy Survey: Scientific Goals and Observing Strategy , 2017, Publications of the Astronomical Society of Australia.

[6]  Scott Case,et al.  TAIPAN: optical spectroscopy with StarBugs , 2014, Astronomical Telescopes and Instrumentation.

[7]  U. Munari,et al.  The GALAH survey: scientific motivation , 2015, Monthly Notices of the Royal Astronomical Society.

[8]  Matthew Colless,et al.  MANIFEST: a many-instrument fiber-positioning system for GMT , 2010, Astronomical Telescopes + Instrumentation.

[9]  M. Viel,et al.  Tomography of the intergalactic medium with Lyα forests in close QSO pairs , 2006 .

[10]  Matthew Colless,et al.  MANIFEST instrument concept and related technologies , 2012, Other Conferences.

[11]  Ross Zhelem,et al.  The MANIFEST prototyping design study , 2016, Astronomical Telescopes + Instrumentation.

[12]  A. Hopkins,et al.  The Sydney-AAO Multi-object Integral field spectrograph , 2011, 1112.3367.

[13]  Damien Jones,et al.  First light results from the High Efficiency and Resolution Multi-Element Spectrograph at the Anglo-Australian Telescope , 2015 .

[14]  M. Asplund,et al.  CHEMICALLY TAGGING THE HR 1614 MOVING GROUP , 2007 .

[15]  Peter Gillingham,et al.  An all-silica three element wide-field corrector for GMT , 2016, Astronomical Telescopes + Instrumentation.

[16]  D. Guzman,et al.  The GMT-CfA, Carnegie, Catolica, Chicago Large Earth Finder (G-CLEF): a general purpose optical echelle spectrograph for the GMT with precision radial velocity capability , 2012, Other Conferences.

[17]  Matthew Colless,et al.  Hector: a high-multiplex survey instrument for spatially resolved galaxy spectroscopy , 2012, Other Conferences.