Poster + Paper
25 July 2024 The ERIS pipeline
Erich A. Wiezorrek, John Lightfoot, Andrea Modigliani, Mark J. Neeser, Alex Agudo Berbel, Yixian Cao, Lars Lundin, Ric Davies, Robert J. De Rosa, Kateryna Kravchenko, Harald Kuntschner, Laura Mascetti, Isabelle Percheron, William Taylor
Author Affiliations +
Conference Poster
Abstract
The ERIS data reduction pipeline, as part of the ESO-VLT Data Flow System, provides recipes for the reduction of ERIS data, the support of Operations, and a monitoring of instrument health and data quality. The pipeline generates science-ready data products that are ingested into the ESO archive. The Enhanced Resolution Imager and Spectrograph (ERIS) is an instrument that both extends and enhances the fundamental diffraction-limited imaging and spectroscopic capabilities of the VLT. The observational modes ERIS provides are integral field spectroscopy at 1-2.5 um, done with ERIS-SPIFFIER, imaging at 1-5 um with several options for high-contrast imaging, and long-slit spectroscopy at 3-4 um, done with ERIS-NIX and ERIS-LSS, respectively. The pipeline recipes can be executed either with EsoRex at the command-line level, through the ESOReflex graphical interface, or using the new ESO Data Processing System. This poster will present the main functionalities of the ERIS-NIX and ERIS-SPIFFIER pipelines.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Erich A. Wiezorrek, John Lightfoot, Andrea Modigliani, Mark J. Neeser, Alex Agudo Berbel, Yixian Cao, Lars Lundin, Ric Davies, Robert J. De Rosa, Kateryna Kravchenko, Harald Kuntschner, Laura Mascetti, Isabelle Percheron, and William Taylor "The ERIS pipeline", Proc. SPIE 13101, Software and Cyberinfrastructure for Astronomy VIII, 131012X (25 July 2024); https://doi.org/10.1117/12.3018743
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KEYWORDS
Equipment

Stars

Calibration

Distortion

Sensors

Adaptive optics

Imaging systems

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