Analyzing Spiral Galaxies Observed in Near-Infrared

A sample of 54 spiral galaxies was observed in the near-infrared K′ band and used to analyze perturbations in galactic disks. Although it is desirable to perform reductions and analysis as automatic as possible, some steps require manual intervention. These are discussed together with several techniques useful for analysis of spiral galaxies.

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Author and article information

Conference

Publication date: April 2004

Publication date (Print): April 2004

Pages: 1-5

Affiliations

[0001]European Southern Observatory

Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany

Article

DOI: 10.14236/ewic/ADA-III2004.15

SO-VID: b3b1be9f-f69d-4394-9d85-9790fcb5e5ac

License:

This work is licensed under a Creative Commons Attribution 4.0 Unported License. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/

Conference name: ADA-III - Astronomical Data Analysis III Conference

Conference acronym: ADA

Conference number: 3

Conference location: Sant' Agata sui due Golfi, Italy

Conference date: 29 April - 1 May 2004

Conference sponsor: Electronic Workshops in Computing (eWiC)

Conference theme: Astronomical Data Analysis

History

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1477-9358 BCS Learning & Development

Self URI (article page): https://www.scienceopen.com/hosted-document?doi=10.14236/ewic/ADA-III2004.15

Self URI (journal page): https://ewic.bcs.org/

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Analyzing Spiral Galaxies Observed in Near-Infrared

Abstract