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Developing arrayed waveguide grating spectrographs for multi-object astronomical spectroscopyNick Cvetojevic, Nemanja Jovanovic, Jon Lawrence, Michael Withford, and Joss Bland-Hawthorn »View Author Affiliations
Nick Cvetojevic,1,2,4,*
Nemanja Jovanovic,1,2,3
Jon Lawrence,1,2,3
Michael Withford,1,2,4
and Joss Bland-Hawthorn5,6
1MQ Photonics Research Centre, Department of Physics and Astronomy, Macquarie University, NSW 2109, Australia 2Centre for Astronomy, Astrophysics and Astrophotonics, Macquarie University, Australia 3Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia 4Centre for Ultrahigh Bandwidth Devices for Optical Systems, Australia 5Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006, Australia 6Institute of Photonics and Optical Science, School of Physics, University of Sydney, NSW 2006, Australia *Corresponding author: nick.cvetojevic@mq.edu.au |
Optics Express, Vol. 20, Issue 3, pp. 2062-2072 (2012)
http://dx.doi.org/10.1364/OE.20.002062
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Abstract
With the aim of utilizing arrayed waveguide gratings for multi-object spectroscopy in the field of astronomy, we outline several ways in which standard telecommunications grade chips should be modified. In particular, by removing the parabolic-horn taper or multimode interference coupler, and injecting with an optical fiber directly, the resolving power was increased threefold from 2400 ± 200 (spectral resolution of 0.63 ± 0.2 nm) to 7000 ± 700 (0.22 ± 0.02 nm) while attaining a throughput of 77 ± 5%. More importantly, the removal of the taper enabled simultaneous off-axis injection from multiple fibers, significantly increasing the number of spectra that can be obtained at once (i.e. the observing efficiency). Here we report that ~12 fibers can be injected simultaneously within the free spectral range of our device, with a 20% reduction in resolving power for fibers placed at 0.8 mm off-centre.
© 2012 OSA
OCIS Codes
(110.5100) Imaging systems : Phased-array imaging systems
(130.3120) Integrated optics : Integrated optics devices
(230.1150) Optical devices : All-optical devices
(300.6190) Spectroscopy : Spectrometers
(350.1260) Other areas of optics : Astronomical optics
ToC Category:
Integrated Optics
History
Original Manuscript: September 22, 2011
Revised Manuscript: November 11, 2011
Manuscript Accepted: December 23, 2011
Published: January 17, 2012
Citation
Nick Cvetojevic, Nemanja Jovanovic, Jon Lawrence, Michael Withford, and Joss Bland-Hawthorn, "Developing arrayed waveguide grating spectrographs for multi-object astronomical spectroscopy," Opt. Express 20, 2062-2072 (2012)
http://www.opticsinfobase.org/oe/abstract.cfm?URI=oe-20-3-2062
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References
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- J. Allington-Smith and J. Bland-Hawthorn, “Astrophotonic spectroscopy: defining the potential advantage,” Mon. Not. R. Astron. Soc.404, 232–238 (2010).
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- N. Cvetojevic, J. S. Lawrence, S. C. Ellis, J. Bland-Hawthorn, R. Haynes, and A. Horton, “Characterization and on-sky demonstration of an integrated photonic spectrograph for astronomy,” Opt. Express17(21), 18643–18650 (2009). [CrossRef] [PubMed]
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- J. Bland-Hawthorn and A. Horton, “Instruments without optics: an integrated photonic spectrograph,” Proc. SPIE6269, 62690N, 62690N-14 (2006). [CrossRef]
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- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
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- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- V. Coudé du Foresto, M. Faucherre, N. Hubin, and P. Gitton, “Using single-mode fibers to monitor fast Strehl ratio fluctuations. Application to a 3.6 m telescope corrected by adaptive optics,” Astron. Astrophys.145(2), 305–310 (2000).
- J. Lawrence, J. Bland-Hawthorn, N. Cvetojevic, R. Haynes, and N. Jovanovic, “Miniture astronomical spectrographs using arrayed waveguide gratings: Capabilities and limitations,” Proc. SPIE7739, 773941 (2010).
- J. Bland-Hawthorn, J. Lawrence, G. Robertson, S. Campbell, B. Pope, C. Betters, S. Leon-Saval, T. Birks, R. Haynes, N. Cvetojevic, and N. Jovanovic, “PIMMS: photonic integrated multimode microspectrograph,” Proc. SPIE7735, 77350N, 77350N-9 (2010). [CrossRef]
- N. Cvetojevic, J. S. Lawrence, S. C. Ellis, J. Bland-Hawthorn, R. Haynes, and A. Horton, “Characterization and on-sky demonstration of an integrated photonic spectrograph for astronomy,” Opt. Express17(21), 18643–18650 (2009). [CrossRef] [PubMed]
- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- S. C. Ellis, J. Bland-Hawthorn, J. S. Lawrence, J. Bryant, R. Haynes, A. Horton, S. Lee, S. Leon-Saval, H. G. Löhmannsröben, J. Mladenoff, J. O'Byrne, W. Rambold, C. Roth, and C. Trinh, “GNOSIS: an OH suppression unit for near-infrared spectrographs,” Proc. SPIE7735, 773516, 773516-10 (2010). [CrossRef]
- N. Cvetojevic, J. S. Lawrence, S. C. Ellis, J. Bland-Hawthorn, R. Haynes, and A. Horton, “Characterization and on-sky demonstration of an integrated photonic spectrograph for astronomy,” Opt. Express17(21), 18643–18650 (2009). [CrossRef] [PubMed]
- V. Coudé du Foresto, M. Faucherre, N. Hubin, and P. Gitton, “Using single-mode fibers to monitor fast Strehl ratio fluctuations. Application to a 3.6 m telescope corrected by adaptive optics,” Astron. Astrophys.145(2), 305–310 (2000).
- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- V. Coudé du Foresto, M. Faucherre, N. Hubin, and P. Gitton, “Using single-mode fibers to monitor fast Strehl ratio fluctuations. Application to a 3.6 m telescope corrected by adaptive optics,” Astron. Astrophys.145(2), 305–310 (2000).
- W. J. Percival, C. M. Baugh, J. Bland-Hawthorn, T. Bridges, R. Cannon, S. Cole, M. Colless, C. Collins, W. Couch, G. Dalton, R. De Propris, S. P. Driver, G. Efstathiou, R. S. Ellis, C. S. Frenk, K. Glazebrook, C. Jackson, O. Lahav, I. Lewis, S. Lumsden, S. Maddox, S. Moody, P. Norberg, J. A. Peacock, B. A. Peterson, W. Sutherland, and K. Taylor, “The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,” Mon. Not. R. Astron. Soc.327(4), 1297–1306 (2001). [CrossRef]
- J. Bland-Hawthorn, J. Lawrence, G. Robertson, S. Campbell, B. Pope, C. Betters, S. Leon-Saval, T. Birks, R. Haynes, N. Cvetojevic, and N. Jovanovic, “PIMMS: photonic integrated multimode microspectrograph,” Proc. SPIE7735, 77350N, 77350N-9 (2010). [CrossRef]
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