AO assisted spectroscopy with SINFONI: PSF, background, and interpolation
arXiv:astro-ph/0703044 · doi:10.1007/978-3-540-76963-7_35
Abstract
I discuss 3 widely applicable aspects concerning calibration of the near infrared adaptive optics integral field spectrometer SINFONI: (1) the accuracy with which one needs to quantify the PSF and how this might be achieved in practice; (2) how it is possible to fine tune the background subtraction to minimise the residual OH airglow; and (3) how an altered perspective on calibration data might lead to improvements in interpolation and greater flexibility in reconstructing datacubes.
9 pages, invited contribution to the 2007 ESO Instrument Calibration Workshop
References in corpus (12)
- Detailed Structural Decomposition of Galaxy Images
- SINFONI - Integral Field Spectroscopy at 50 milli-arcsecond resolution with the ESO VLT
- A method to remove residual OH emission from near infrared spectra
- The Star-Forming Torus and Stellar Dynamical Black Hole Mass in the Seyfert 1 Nucleus of NGC3227
- The Nuclear Gas Dynamics and Star Formation of NGC 7469
- SINFONI adaptive optics integral field spectroscopy of the Circinus Galaxy
- The Nuclear Gas Dynamics and Star Formation of Markarian 231
- Unveiling the central parsec region of an AGN: the Circinus nucleus in the near infrared with the VLT
- The Anisoplanatic Point Spread Function in Adaptive Optics
- Characterizing the Adaptive Optics Off-Axis Point-Spread Function - I: A Semi-Empirical Method for Use in Natural-Guide-Star Observations
- Accounting for anisoplanatic point spread function in deep wide-field adaptive optics images
- Galaxy morphology and evolution from SWAN Adaptive Optics imaging