140 research outputs found
'Modal-noise' in single-mode fibers: A cautionary note for high precision radial velocity instruments
Exploring the use of single-mode fibers (SMFs) in high precision Doppler
spectrometers has become increasingly attractive since the advent of
diffraction-limited adaptive optics systems on large-aperture telescopes.
Spectrometers fed with these fibers can be made significantly smaller than
typical 'seeing-limited' instruments, greatly reducing cost and overall
complexity. Importantly, classical mode interference and speckle issues
associated with multi-mode fibers, also known as 'modal noise', are mitigated
when using SMFs, which also provide perfect radial and azimuthal image
scrambling. However, these fibers do support multiple polarization modes, an
issue that is generally ignored for larger-core fibers given the large number
of propagation modes. Since diffraction gratings used in most high resolution
astronomical instruments have dispersive properties that are sensitive to
incident polarization changes, any birefringence variations in the fiber can
cause variations in the efficiency profile, degrading illumination stability.
Here we present a cautionary note outlining how the polarization properties of
SMFs can affect the radial velocity measurement precision of high resolution
spectrographs. This work is immediately relevant to the rapidly expanding field
of diffraction-limited, extreme precision RV spectrographs that are currently
being designed and built by a number of groups.Comment: 6 pages, 5 figures, accepted for publication in ApJ Letter
Frequency stability characterization of a broadband fiber Fabry-Perot interferometer
An optical etalon illuminated by a white light source provides a broadband
comb-like spectrum that can be employed as a calibration source for
astronomical spectrographs in radial velocity (RV) surveys for extrasolar
planets. For this application the frequency stability of the etalon is
critical, as its transmission spectrum is susceptible to frequency fluctuations
due to changes in cavity temperature, optical power and input polarization. In
this paper we present a laser frequency comb measurement technique to
characterize the frequency stability of a custom-designed fiber Fabry-Perot
interferometer (FFP). Simultaneously probing the stability of two etalon
resonance modes, we assess both the absolute stability of the etalon and the
long-term stability of the cavity dispersion. We measure mode positions with
MHz precision, which corresponds to splitting the FFP resonances by a part in
500 and to RV precision of ~1 m/s. We address limiting systematic effects,
including the presence of parasitic etalons, that need to be overcome to push
the metrology of this system to the equivalent RV precision of 10 cm/s. Our
results demonstrate a means to characterize environmentally-driven
perturbations of etalon resonance modes across broad spectral bandwidths, as
well as motivate the benefits and challenges of FFPs as spectrograph
calibrators.Comment: 15 pages, 9 figures, accepted to Opt. Expres
Development of a New, Precise Near-infrared Doppler Wavelength Reference: A Fiber Fabry-Perot Interferometer
We present the ongoing development of a commercially available Micron Optics
fiber-Fabry Perot Interferometer as a precise, stable, easy to use, and
economic spectrograph reference with the goal of achieving <1 m/s long term
stability. Fiber Fabry-Perot interferometers (FFP) create interference patterns
by combining light traversing different delay paths. The interference creates a
rich spectrum of narrow emission lines, ideal for use as a precise Doppler
reference. This fully photonic reference could easily be installed in existing
NIR spectrographs, turning high resolution fiber-fed spectrographs into precise
Doppler velocimeters. First light results on the Sloan Digital Sky Survey III
(SDSS-III) Apache Point Observatory Galactic Evolution Experiment (APOGEE)
spectrograph and several tests of major support instruments are also presented.
These instruments include a SuperK Photonics fiber supercontinuum laser source
and precise temperature controller. A high resolution spectrum obtained using
the NIST 2-m Fourier transform spectrometer (FTS) is also presented. We find
our current temperature control precision of the FFP to be 0.15 mK,
corresponding to a theoretical velocity stability of 35 cm/s due to temperature
variations of the interferometer cavity.Comment: 16 pages, 11 figures. To appear in the proceedings of the SPIE 2012
Astronomical Instrumentation and Telescopes conferenc
Seeing-limited Coupling of Starlight into Single-mode Fiber with a Small Telescope
An optical fiber link to a telescope provides many advantages for
spectrometers designed to detect and characterize extrasolar planets through
precise radial velocity (PRV) measurements. In the seeing-limited regime, a
multi-mode fiber is typically used so that a significant amount of starlight
may be captured. In the near-diffraction-limited case, either with an adaptive
optics system or with a small telescope at an excellent site, efficiently
coupling starlight into a much smaller, single-mode fiber may be possible. In
general, a spectrometer designed for single-mode fiber input will be
substantially less costly than one designed for multi-mode fiber input. We
describe the results of tests coupling starlight from a 70 cm telescope at Mt.
Hopkins, Arizona into the single-mode fiber of the MINERVA-Red spectrometer at
a wavelength of ~850 nm using a low-speed tip/tilt image stabilization system
comprising all commercial, off-the-shelf components. We find that approximately
0.5% of the available starlight is coupled into the single-mode fiber under
seeing conditions typical for observatories hosting small telescopes, which is
close to the theoretical expectation. We discuss scientific opportunities for
small telescopes paired with inexpensive, high-resolution spectrometers, as
well as upgrade paths that should significantly increase the coupling
efficiency for the MINERVA-Red system.Comment: 8 pages, 4 figures. Accepted for publication in Astronomische
Nachrichte
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