PampelMuse: Crowded-field 3D spectroscopy

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Ada Coda
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PampelMuse: Crowded-field 3D spectroscopy

Post by Ada Coda » Thu May 24, 2018 9:34 pm

PampelMuse: Crowded-field 3D spectroscopy

Abstract: PampelMuse analyzes integral-field spectroscopic observations of crowded stellar fields and provides several subroutines to perform the individual steps of the data analysis. All analysis steps assume that the IFS data has been properly reduced and that all the instrumental artifacts have been removed. PampelMuse is designed to correctly handle IFS data regardless of which instrument was used to observe the data. In addition to the actual data, the software also requires an estimate of the variances for the analysis; optionally, it can use a bad pixel mask. The analysis relies on the presence of a reference catalogue, containing coordinates and magnitudes of the stars in and around the observed field.

Credit: Kamann, Sebastian

Site: https://gitlab.gwdg.de/skamann/pampelmuse
https://ui.adsabs.harvard.edu/abs/2020ApJ...896...13B

Bibcode: 2018ascl.soft05021K

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2013A%26A...549A..71K

ID: ascl:1805.021
Last edited by Ada Coda on Tue Jul 07, 2020 8:19 am, edited 1 time in total.
Reason: Updated code entry.

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