MOSES is a vacuum-stabilized white-pupil echelle spectrograph designed for >80,000 resolution over 380-680 nm and sub-2 m/s RV precision via dual-fiber simultaneous Fabry-Pérot calibration on the MONET telescope.
Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , year = 2016, series =
6 Pith papers cite this work. Polarity classification is still indexing.
6
Pith papers citing it
years
2026 6verdicts
UNVERDICTED 6representative citing papers
Introduces a reflection spectroscopy metric and uses KELT-9 injection-recovery tests to demonstrate that rotational line broadening from rapid stellar rotation and large misalignments must be included when assessing detectability of exoplanet reflected spectra.
Archival RV and astrometric data plus three-body simulations constrain an unseen outer perturber in the GJ 436 system to sub-Jovian masses at a_c ≳ 6.8 AU, supporting Kozai-Lidov migration as the source of the hot Neptune's polar eccentric orbit.
Resolves six speculative companions into one giant planet, one eccentric brown dwarf, two low-mass stars, and two stars with no detectable companions.
Describes a fiber-coupling setup for Bruker IFS 125 FTS with hexagonal fibers for mode scrambling and dichroic combining for dual-source measurements.
The paper reports the in-house design, development, and 2022 installation of the CAMPAS Cassegrain module containing focal reducer, atmospheric dispersion corrector, fiber mounts, and calibration unit for the PARAS-2 spectrograph.
citing papers explorer
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MOSES -- The MONET Star and Exoplanet Spectrograph
MOSES is a vacuum-stabilized white-pupil echelle spectrograph designed for >80,000 resolution over 380-680 nm and sub-2 m/s RV precision via dual-fiber simultaneous Fabry-Pérot calibration on the MONET telescope.
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Spinning out of focus: The challenge of rotational line broadening in exoplanet reflection spectroscopy
Introduces a reflection spectroscopy metric and uses KELT-9 injection-recovery tests to demonstrate that rotational line broadening from rapid stellar rotation and large misalignments must be included when assessing detectability of exoplanet reflected spectra.
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Observational and Dynamical Constraints on an Unseen Outer Perturber in the GJ 436 Hot Neptune System
Archival RV and astrometric data plus three-body simulations constrain an unseen outer perturber in the GJ 436 system to sub-Jovian masses at a_c ≳ 6.8 AU, supporting Kozai-Lidov migration as the source of the hot Neptune's polar eccentric orbit.
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The Pan-Pacific Planet Search -- IX. A menagerie of companions orbiting evolved stars
Resolves six speculative companions into one giant planet, one eccentric brown dwarf, two low-mass stars, and two stars with no detectable companions.
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Fiber-coupling of Fourier Transform Spectrographs
Describes a fiber-coupling setup for Bruker IFS 125 FTS with hexagonal fibers for mode scrambling and dichroic combining for dual-source measurements.
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Design and Development of Cassegrain Module for PARAS-2 Spectrograph (CAMPAS)
The paper reports the in-house design, development, and 2022 installation of the CAMPAS Cassegrain module containing focal reducer, atmospheric dispersion corrector, fiber mounts, and calibration unit for the PARAS-2 spectrograph.