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The performance of fiber-fed astronomical spectrographs is highly influenced by the properties of fibers. The near-field and far-field scrambling characteristics have a profound impact on the line spread function (LSF) of the spectra. Focal…

Instrumentation and Methods for Astrophysics · Physics 2024-08-16 Man-Yin Leo Lee , Zhiheng Lin , Chit-Ho Hui , Renbin Yan , YiuHung Cheung , Horace Tsz-Hong Hung , Matthew A. Bershady , Sabysachi Chattopadhyay , Michael P. Smith

Optical fibers are a key component for high-resolution spectrographs to attain high precision in radial velocity measurements. We present a custom fiber with a novel core geometry - a 'D'-shape. From a theoretical standpoint, such a fiber…

Instrumentation and Methods for Astrophysics · Physics 2016-12-07 Julian Stürmer , Christian Schwab , Stephan Grimm , Andre Kalide , Adam P. Sutherland , Andreas Seifahrt , Kay Schuster , Jacob L. Bean , Andreas Quirrenbach

In astronomical spectroscopy, optical fibres are abundantly used for multiplexing and decoupling the spectrograph from the telescope to provide stability in a controlled environment. However, fibres are less than perfect optical components…

Instrumentation and Methods for Astrophysics · Physics 2021-05-05 E. Hernandez , M. M. Roth , K. Petermann , A. Kelz , B. Moralejo , K. Madhav

The performance of highly-multiplexed spectrographs is limited by focal degradation (FRD) in the optical fibres. It has already been shown that this is caused mainly by processes concentrated around the mounting points at the ends of the…

Instrumentation and Methods for Astrophysics · Physics 2015-06-17 Jeremy Allington-Smith , Colin Dunlop , Graham Murray , Ulrike Lemke

Modal noise is a common source of noise introduced to the measurements by optical fibres and is particularly important for fibre-fed spectroscopic instruments, especially for high-resolution measurements. This noise source can limit the…

Instrumentation and Methods for Astrophysics · Physics 2016-03-16 D. P. Sablowski , D. Plüschke , M. Weber , K. G. Strassmeier , A. Järvinen

We report on the scrambling performance and focal-ratio-degradation (FRD) of various octagonal and rectangular fibers considered for MAROON-X. Our measurements demonstrate the detrimental effect of thin claddings on the FRD of octagonal and…

Instrumentation and Methods for Astrophysics · Physics 2016-12-07 Adam P. Sutherland , Julian Stürmer , Katrina R. Miller , Andreas Seifahrt , Jacob L. Bean

Modal noise in fibers has been shown to limit the signal-to-noise ratio achievable in fiber-coupled, high-resolution spectrographs if it is not mitigated via modal scrambling techniques. Modal noise become significantly more important as…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 Keegan McCoy , Lawrence Ramsey , Suvrath Mahadevan , Samuel Halverson , Stephen L. Redman

For fiber-fed spectrographs with a stable external wavelength source, scrambling properties of optical fibers and, homogeneity and stability of the instrument illumination are important for the accuracy of radial-velocimetry. Optical…

Instrumentation and Methods for Astrophysics · Physics 2015-05-14 I. Boisse , F. Bouchy , B. Chazelas , S. Perruchot , F. Pepe , C. Lovis , G. Hebrard

Fiber modal noise is a performance limiting factor in high-resolution spectroscopy, both with respect to achieving high signal-to-noise ratios or when targeting high-precision radial velocity measurements, with multi-mode fiber-fed…

Instrumentation and Methods for Astrophysics · Physics 2020-12-16 Gert Raskin , Jacob Pember , Dmytro Rogozin , Christian Schwab , David Coutts

We investigate the dependence on length of optical fibres used in astronomy, especially the focal ratio degradation (FRD) which places constraints on the performance of fibre-fed spectrographs used for multiplexed spectroscopy. To this end…

Instrumentation and Methods for Astrophysics · Physics 2015-05-18 C. L. Poppett , J. R. Allington-Smith

Fiber modal noise is a performance limiting factor in high-precision radial velocity measurements with multi-mode fiber-fed high-resolution spectrographs. Traditionally, modal noise is mitigated by agitating the fiber, this way…

Instrumentation and Methods for Astrophysics · Physics 2019-11-20 Gert Raskin , Dmytro Rogozin , Tom Mladenov , Christian Schwab , David Coutts

When coherent light propagates through a multimode optical fiber, the modes interfere at the fiber exit boundary, producing a high-contrast speckle interference pattern called modal noise. This non-uniform interference pattern introduces…

Starting from our puzzling on-sky experience with the GIANO-TNG spectrometer we set up an infrared high resolution spectrometer in our laboratory and used this instrument to characterize the modal noise generated in fibers of different…

Instrumentation and Methods for Astrophysics · Physics 2019-11-27 E. Oliva , M. Rainer , A. Tozzi , N. Sanna , M. Iuzzolino , A. Brucalassi

We present the design and test results of a compact optical fiber double-scrambler for high-resolution Doppler radial velocity instruments. This device consists of a single optic: a high-index $n$$\sim$2 ball lens that exchanges the near…

Instrumentation and Methods for Astrophysics · Physics 2015-06-17 Samuel Halverson , Arpita Roy , Suvrath Mahadevan , Lawrence Ramsey , Eric Levi , Christian Schwab , Fred Hearty , Nick MacDonald

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…

Instrumentation and Methods for Astrophysics · Physics 2015-12-02 Samuel Halverson , Arpita Roy , Suvrath Mahadevan , Christian Schwab

Focal Ratio Degradation (FRD) in fibres is a crucial factor to control in astronomical instruments in order to minimize light loss. As astronomical instrumentation has advanced, the integration of large populations of fibres has become…

Instrumentation and Methods for Astrophysics · Physics 2023-06-30 Weimin Sun , Xudong Chen , Jiabin Wang , Hang Jiang , Anzhi Wang , Qi Yan , Zhenyu Ma , Shengjia Wang , Tao Geng , Yue Zhong , Zhongquan Qu , Yunxiang Yan

High-precision spectrographs play a key role in exoplanet searches using the radial velocity technique. But at the accuracy level of 1 m.s-1, required for super-Earth characterization, stability of fiber-fed spectrograph performance is…

Instrumentation and Methods for Astrophysics · Physics 2015-05-30 S. Perruchot , F. Bouchy , B. Chazelas , R. F. Diaz , G. Hébrard , K. Arnaud , L. Arnold , G. Avila , X. Delfosse , I. Boisse , G. Moreaux , F. Pepe. Y. Richaud , A. Santerne , R. Sottile , D. Tezier

In modern particle physics experiments wavelength-shifting and scintillating fibres based on plastic polymers are used for tracking and calorimetry. In this review the role of photon trapping efficiencies, transmission functions and signal…

Nuclear Experiment · Physics 2007-05-23 C. P. Achenbach

When multimode optical fibers are perturbed, the data that is transmitted through them is scrambled. This presents a major difficulty for many possible applications, such as multimode fiber-based telecommunication and endoscopy. To overcome…

Image and Video Processing · Electrical Eng. & Systems 2022-02-17 Shachar Resisi , Sebastien M. Popoff , Yaron Bromberg

Fibre modal noise occurs in high spectral resolution, high signal-to-noise applications. It imposes fundamental limits on the photometric accuracy of state-of-the-art fibre-spectrograph systems. In order to maximize the performance of…

Instrumentation and Methods for Astrophysics · Physics 2015-05-28 U. Lemke , J. Corbett , J. Allington-Smith , G. Murray
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