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FLUX CALIBRATION METHOD OF SLIT SPECTROMETER FOR EXTENDED SOURCES

  • Lee, Sung-Ho (Korea Astronomy and Space Science Institute) ;
  • Park, Soo-Jong (Department of Astronomy and Space Science, Kyung Hee University)
  • Published : 2006.12.31

Abstract

Long slit spectrometers are widely used in optical and infrared bands in astronomy. Absolute flux calibration for extended sources, however, is not straightforward, because a portion of the radiation energy from a flux calibration star is blocked by the narrow slit width. Assuming that the point spread function(PSF) of the star is circularly symmetric, we develop a robust method to extrapolate the detected stellar flux to the unobscured flux using the measured PSF along the slit-length direction. We apply this method to our long slit data and prove that the uncertainty of the absolute flux calibration is less than a few percents.

Keywords

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Cited by

  1. Three‐Dimensional Observations of H2Emission around Sgr A East. I. Structure in the Central 10 pc of Our Galaxy vol.674, pp.1, 2008, https://doi.org/10.1086/524128
  2. Fluorescent H2 Emission Lines from the Reflection Nebula NGC 7023 Observed with IGRINS vol.841, pp.1, 2017, https://doi.org/10.3847/1538-4357/aa6bf7