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Proceedings Paper

Astronomical optical frequency comb generation and test in a fiber-fed MUSE spectrograph
Author(s): J. M. Chavez Boggio; T. Fremberg; B. Moralejo; M. Rutowska; E. Hernandez; M. Zajnulina; A. Kelz; D. Bodenmüller; C. Sandin; M. Wysmolek; H. Sayinc; J. Neumann; R. Haynes; M. M. Roth
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Paper Abstract

We here report on recent progress on astronomical optical frequency comb generation at innoFSPEC-Potsdam and present preliminary test results using the fiber-fed Multi Unit Spectroscopic Explorer (MUSE) spectrograph. The frequency comb is generated by propagating two free-running lasers at 1554.3 and 1558.9 nm through two dispersionoptimized nonlinear fibers. The generated comb is centered at 1590 nm and comprises more than one hundred lines with an optical-signal-to-noise ratio larger than 30 dB. A nonlinear crystal is used to frequency double the whole comb spectrum, which is efficiently converted into the 800 nm spectral band. We evaluate first the wavelength stability using an optical spectrum analyzer with 0.02 nm resolution and wavelength grid of 0.01 nm. After confirming the stability within 0.01 nm, we compare the spectra of the astro-comb and the Ne and Hg calibration lamps: the astro-comb exhibits a much larger number of lines than lamp calibration sources. A series of preliminary tests using a fiber-fed MUSE spectrograph are subsequently carried out with the main goal of assessing the equidistancy of the comb lines. Using a P3d data reduction software we determine the centroid and the width of each comb line (for each of the 400 fibers feeding the spectrograph): equidistancy is confirmed with an absolute accuracy of 0.4 pm.

Paper Details

Date Published: 28 July 2014
PDF: 7 pages
Proc. SPIE 9151, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation, 915120 (28 July 2014); doi: 10.1117/12.2056684
Show Author Affiliations
J. M. Chavez Boggio, Leibniz-Institut für Astrophysik Potsdam (Germany)
T. Fremberg, Leibniz-Institut für Astrophysik Potsdam (Germany)
B. Moralejo, Leibniz-Institut für Astrophysik Potsdam (Germany)
M. Rutowska, Leibniz-Institut für Astrophysik Potsdam (Germany)
E. Hernandez, Leibniz-Institut für Astrophysik Potsdam (Germany)
M. Zajnulina, Leibniz-Institut für Astrophysik Potsdam (Germany)
A. Kelz, Leibniz-Institut für Astrophysik Potsdam (Germany)
D. Bodenmüller, Leibniz-Institut für Astrophysik Potsdam (Germany)
C. Sandin, Leibniz-Institut für Astrophysik Potsdam (Germany)
M. Wysmolek, Ctr. for Quantum Engineering and Space-Time Research (Germany)
H. Sayinc, Laser Zentrum Hannover e.V. (Germany)
J. Neumann, Laser Zentrum Hannover e.V. (Germany)
Ctr. for Quantum Engineering and Space-Time Research (Germany)
R. Haynes, Leibniz-Institut für Astrophysik Potsdam (Germany)
M. M. Roth, Leibniz-Institut für Astrophysik Potsdam (Germany)

Published in SPIE Proceedings Vol. 9151:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation
Ramón Navarro; Colin R. Cunningham; Allison A. Barto, Editor(s)

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