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20192026
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astro-ph.IM2026

Laboratory characterization of iLocater

Marcelo Tala Pinto, Marshall C. Johnson, Julia Brady +18

iLocater is a diffraction-limited, fiber-fed spectrograph designed for the Large Binocular Telescope (LBT), which targets high-precision radial velocity measurements in the near-in…

astro-ph.IM2026

Commissioning and on-sky performance verification of iLocater

Marshall C. Johnson, Marcelo Tala Pinto, Jonathan Crass +59

iLocater is a high-resolution near-infrared extreme precision radial velocity (EPRV) spectrograph that was deployed to the Large Binocular Telescope (LBT) in June 2026. iLocater op…

astro-ph.IM2026

The Calibration System of the iLocater Spectrograph

Sai Vidyud Senthil Nathan, Jonathan Crass, Julia E. Brady +21

iLocater is a new near-infrared, extreme precision radial velocity (EPRV) instrument delivered to the Large Binocular Telescope in the summer of 2026. The instrument utilizes singl…

astro-ph.IM2020

Fiber modal noise mitigation by a rotating double scrambler

Gert Raskin, Jacob Pember, Dmytro Rogozin +2

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 radi…

astro-ph.IM2020

Rubidium transitions as wavelength reference for astronomical Doppler spectrographs

Dmytro Rogozin, Tobias Feger, Christian Schwab +10

Precise wavelength calibration is a critical issue for high-resolution spectroscopic observations. The ideal calibration source should be able to provide a very stable and dense gr…

astro-ph.IM2019

Fiber modal noise mitigation by a rotating double scrambler

Gert Raskin, Dmytro Rogozin, Tom Mladenov +2

Fiber modal noise is a performance limiting factor in high-precision radial velocity measurements with multi-mode fiber-fed high-resolution spectrographs. Traditionally, modal nois…