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astro-ph.IMMar 7, 2018
5
citations (OpenAlex)
authors
  • P. M. Plewa
  • S. Gillessen
  • M. Bauböck
  • J. Dexter
  • F. Eisenhauer
  • S. von Fellenberg
  • F. Gao
  • R. Genzel
  • M. Habibi
  • A. Jimenez-Rosales
  • T. Ott
  • O. Pfuhl
  • I. Waisberg
  • F. Widmann
institutions
  • Max Planck Institute for Extraterrestrial Physics
arXiv abstractPDF
paper

Optical Distortion in the NACO Imager

arXiv:1803.02733 · doi:10.3847/2515-5172/aab3df

Abstract

In this research note, we present a set of distortion solutions that may be used to correct geometric optical distortion in images taken with the S13 camera of the NACO adaptive optics imager.

arXiv commentpublished in the RNAAS

References in corpus (4)

  • Monitoring stellar orbits around the Massive Black Hole in the Galactic Center
  • An Update on Monitoring Stellar Orbits in the Galactic Center
  • What is limiting near-infrared astrometry in the Galactic Center?
  • Pinpointing the near-infrared location of Sgr A* by correcting optical distortion in the NACO imager

Cited by in corpus (4)

  • Precise Dynamical Masses of Epsilon Indi Ba and Bb: Evidence of Slowed Cooling at the L/T Transition
  • Hunting for intermediate-mass black holes in globular clusters: an astrometric study of NGC 6441
  • X3: a high-mass Young Stellar Object close to the supermassive black hole Sgr~A*
  • The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. II. Kinematic structure
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