PyCosmic: a robust method to detect cosmics in CALIFA and other fiber-fed integral-field spectroscopy datasets
B. Husemann (1), S. Kamann (1), C. Sandin (1), S. F. S\'anchez (2 and, 3), R. Garc\'ia-Benito (2), D. Mast (2, 3) ((1) Leibniz-Institut f\"ur, Astrophysik Potsdam, (2) Instituto de Astrof\'isica de Andaluc\'ia, (3), Centro Astron\'omico Hispano Alem\'an de Calar Alto)

TL;DR
PyCosmic is a new, robust cosmic ray detection algorithm tailored for fiber-fed integral-field spectroscopy data, outperforming existing methods in accuracy and reliability, and integrated into major data reduction pipelines.
Contribution
We introduce PyCosmic, a novel cosmic ray detection algorithm that combines edge detection with PSF convolution, optimized for fiber-fed IFS data, and demonstrate its superior performance over existing methods.
Findings
PyCosmic achieves >90% detection rate with <5% false positives.
It outperforms L.A.Cosmic and DCR in robustness and efficiency.
It is integrated into CALIFA and P3D pipelines.
Abstract
[Abridged] Detecting cosmic ray hits (cosmics) in fiber-fed IFS data of single exposures is a challenging task, because of the complex signal recorded by IFS instruments. Existing detection algorithms are commonly found to be unreliable in the case of IFS data and the optimal parameter settings are usually unknown a-priori for a given dataset. The CALIFA survey generates hundreds of IFS datasets for which a reliable and robust detection algorithm for cosmics is required as an important part of the fully automatic CALIFA data reduction pipeline. We developed a novel algorithm, PyCosmic, which combines the edge-detection algorithm of L.A.Cosmic with a point-spread function convolution scheme. We generated mock data to compute the efficiency of different algorithms for a wide range of characteristic fibre-fed IFS datasets using the PMAS and VIMOS IFS instruments as representative cases.…
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