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Crowded Field 3D Spectrophotometry of Extragalactic Planetary Nebulae.

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Title: Crowded Field 3D Spectrophotometry of Extragalactic Planetary Nebulae.
Authors: Leibundgut, B., Stanghellini, L., Walsh, J. R., Douglas, N. G., Roth, Martin M., Becker, Thomas, Böhm, Petra, Schönberner, Detlef, Steffen, Matthias, Exter, Katrina
Source: Planetary Nebulae Beyond the Milky Way; 2006, p239-243, 5p
Abstract: The spectrophotometry of extragalactic planetary nebulae in high surface brightness regions of nearby galaxies is notoriously difficult because of the problem of accurately subtracting the local background of unresolved stars and gaseous emission of the ISM. Conventional slit spectroscopy is not very well suited for providing a good estimate of the two-dimensional surface brightness distribution in the continuum, absorption lines, and superimposed emission lines from all of these background sources. The emergent technique of integral field (3D) spectroscopy holds the promise to overcome these limitations, similar to the advance of CCD photometry vs. photoelectric aperture photometry. We discuss basic properties of 3D spectrophotometry, results from a pilot study with planetary nebulae in the bulge of M31, and some more recent results from observations in other local group galaxies. [ABSTRACT FROM AUTHOR]
Copyright of Planetary Nebulae Beyond the Milky Way is the property of Springer eBooks and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Crowded Field 3D Spectrophotometry of Extragalactic Planetary Nebulae.
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  Data: Planetary Nebulae Beyond the Milky Way; 2006, p239-243, 5p
– Name: Abstract
  Label: Abstract
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  Data: The spectrophotometry of extragalactic planetary nebulae in high surface brightness regions of nearby galaxies is notoriously difficult because of the problem of accurately subtracting the local background of unresolved stars and gaseous emission of the ISM. Conventional slit spectroscopy is not very well suited for providing a good estimate of the two-dimensional surface brightness distribution in the continuum, absorption lines, and superimposed emission lines from all of these background sources. The emergent technique of integral field (3D) spectroscopy holds the promise to overcome these limitations, similar to the advance of CCD photometry vs. photoelectric aperture photometry. We discuss basic properties of 3D spectrophotometry, results from a pilot study with planetary nebulae in the bulge of M31, and some more recent results from observations in other local group galaxies. [ABSTRACT FROM AUTHOR]
– Name: Abstract
  Label:
  Group: Ab
  Data: <i>Copyright of Planetary Nebulae Beyond the Milky Way is the property of Springer eBooks and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1007/3-540-34270-2_36
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      – Code: eng
        Text: English
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        PageCount: 5
        StartPage: 239
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      – TitleFull: Crowded Field 3D Spectrophotometry of Extragalactic Planetary Nebulae.
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            – D: 01
              M: 01
              Text: 2006
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