The Nearby Field Galaxy Survey
Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample fo...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Jansen, Rolf A. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2001 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 2001 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 276(2001), 2-4 vom: März, Seite 1151-1159 |
|---|---|
| Übergeordnetes Werk: |
volume:276 ; year:2001 ; number:2-4 ; month:03 ; pages:1151-1159 |
| Links: |
|---|
| DOI / URN: |
10.1023/A:1011954916413 |
|---|
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OLC2066227870 |
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| 520 | |a Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample for high-redshift studies and to study the variation in star formation rates (SFRs), star formation history (SFH),excitation, metallicity, and internal kinematics over a wide range of galaxy luminosities and morphological types. In particular, we extend the work of Kennicutt (1992) to lower-luminosity systems. We present the main results of our analysis so far. In these proceedings, we condense the two atlases presented of 1) images and radial surface brightness profiles and colour profiles, and 2) images and integrated spectra into several example images, profiles and spectra, showing the general trends observed. For the original atlases we refer the reader to the electronic distribution on CDROM or as available on the Web at http://www.astro.rug.nl/∼nfgs/. | ||
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10.1023/A:1011954916413 doi (DE-627)OLC2066227870 (DE-He213)A:1011954916413-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Jansen, Rolf A. verfasserin aut The Nearby Field Galaxy Survey 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample for high-redshift studies and to study the variation in star formation rates (SFRs), star formation history (SFH),excitation, metallicity, and internal kinematics over a wide range of galaxy luminosities and morphological types. In particular, we extend the work of Kennicutt (1992) to lower-luminosity systems. We present the main results of our analysis so far. In these proceedings, we condense the two atlases presented of 1) images and radial surface brightness profiles and colour profiles, and 2) images and integrated spectra into several example images, profiles and spectra, showing the general trends observed. For the original atlases we refer the reader to the electronic distribution on CDROM or as available on the Web at http://www.astro.rug.nl/∼nfgs/. Rotation Curve Surface Brightness Star Formation Rate Nearby Galaxy Virgo Cluster Kannappan, Sheila J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), 2-4 vom: März, Seite 1151-1159 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:2-4 month:03 pages:1151-1159 https://doi.org/10.1023/A:1011954916413 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 2-4 03 1151-1159 |
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10.1023/A:1011954916413 doi (DE-627)OLC2066227870 (DE-He213)A:1011954916413-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Jansen, Rolf A. verfasserin aut The Nearby Field Galaxy Survey 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample for high-redshift studies and to study the variation in star formation rates (SFRs), star formation history (SFH),excitation, metallicity, and internal kinematics over a wide range of galaxy luminosities and morphological types. In particular, we extend the work of Kennicutt (1992) to lower-luminosity systems. We present the main results of our analysis so far. In these proceedings, we condense the two atlases presented of 1) images and radial surface brightness profiles and colour profiles, and 2) images and integrated spectra into several example images, profiles and spectra, showing the general trends observed. For the original atlases we refer the reader to the electronic distribution on CDROM or as available on the Web at http://www.astro.rug.nl/∼nfgs/. Rotation Curve Surface Brightness Star Formation Rate Nearby Galaxy Virgo Cluster Kannappan, Sheila J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), 2-4 vom: März, Seite 1151-1159 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:2-4 month:03 pages:1151-1159 https://doi.org/10.1023/A:1011954916413 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 2-4 03 1151-1159 |
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10.1023/A:1011954916413 doi (DE-627)OLC2066227870 (DE-He213)A:1011954916413-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Jansen, Rolf A. verfasserin aut The Nearby Field Galaxy Survey 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample for high-redshift studies and to study the variation in star formation rates (SFRs), star formation history (SFH),excitation, metallicity, and internal kinematics over a wide range of galaxy luminosities and morphological types. In particular, we extend the work of Kennicutt (1992) to lower-luminosity systems. We present the main results of our analysis so far. In these proceedings, we condense the two atlases presented of 1) images and radial surface brightness profiles and colour profiles, and 2) images and integrated spectra into several example images, profiles and spectra, showing the general trends observed. For the original atlases we refer the reader to the electronic distribution on CDROM or as available on the Web at http://www.astro.rug.nl/∼nfgs/. Rotation Curve Surface Brightness Star Formation Rate Nearby Galaxy Virgo Cluster Kannappan, Sheila J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), 2-4 vom: März, Seite 1151-1159 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:2-4 month:03 pages:1151-1159 https://doi.org/10.1023/A:1011954916413 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 2-4 03 1151-1159 |
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10.1023/A:1011954916413 doi (DE-627)OLC2066227870 (DE-He213)A:1011954916413-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Jansen, Rolf A. verfasserin aut The Nearby Field Galaxy Survey 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample for high-redshift studies and to study the variation in star formation rates (SFRs), star formation history (SFH),excitation, metallicity, and internal kinematics over a wide range of galaxy luminosities and morphological types. In particular, we extend the work of Kennicutt (1992) to lower-luminosity systems. We present the main results of our analysis so far. In these proceedings, we condense the two atlases presented of 1) images and radial surface brightness profiles and colour profiles, and 2) images and integrated spectra into several example images, profiles and spectra, showing the general trends observed. For the original atlases we refer the reader to the electronic distribution on CDROM or as available on the Web at http://www.astro.rug.nl/∼nfgs/. Rotation Curve Surface Brightness Star Formation Rate Nearby Galaxy Virgo Cluster Kannappan, Sheila J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), 2-4 vom: März, Seite 1151-1159 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:2-4 month:03 pages:1151-1159 https://doi.org/10.1023/A:1011954916413 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 2-4 03 1151-1159 |
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10.1023/A:1011954916413 doi (DE-627)OLC2066227870 (DE-He213)A:1011954916413-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Jansen, Rolf A. verfasserin aut The Nearby Field Galaxy Survey 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample for high-redshift studies and to study the variation in star formation rates (SFRs), star formation history (SFH),excitation, metallicity, and internal kinematics over a wide range of galaxy luminosities and morphological types. In particular, we extend the work of Kennicutt (1992) to lower-luminosity systems. We present the main results of our analysis so far. In these proceedings, we condense the two atlases presented of 1) images and radial surface brightness profiles and colour profiles, and 2) images and integrated spectra into several example images, profiles and spectra, showing the general trends observed. For the original atlases we refer the reader to the electronic distribution on CDROM or as available on the Web at http://www.astro.rug.nl/∼nfgs/. Rotation Curve Surface Brightness Star Formation Rate Nearby Galaxy Virgo Cluster Kannappan, Sheila J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), 2-4 vom: März, Seite 1151-1159 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:2-4 month:03 pages:1151-1159 https://doi.org/10.1023/A:1011954916413 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 2-4 03 1151-1159 |
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Jansen, Rolf A. |
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the nearby field galaxy survey |
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The Nearby Field Galaxy Survey |
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Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample for high-redshift studies and to study the variation in star formation rates (SFRs), star formation history (SFH),excitation, metallicity, and internal kinematics over a wide range of galaxy luminosities and morphological types. In particular, we extend the work of Kennicutt (1992) to lower-luminosity systems. We present the main results of our analysis so far. In these proceedings, we condense the two atlases presented of 1) images and radial surface brightness profiles and colour profiles, and 2) images and integrated spectra into several example images, profiles and spectra, showing the general trends observed. For the original atlases we refer the reader to the electronic distribution on CDROM or as available on the Web at http://www.astro.rug.nl/∼nfgs/. © Kluwer Academic Publishers 2001 |
| abstractGer |
Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample for high-redshift studies and to study the variation in star formation rates (SFRs), star formation history (SFH),excitation, metallicity, and internal kinematics over a wide range of galaxy luminosities and morphological types. In particular, we extend the work of Kennicutt (1992) to lower-luminosity systems. We present the main results of our analysis so far. In these proceedings, we condense the two atlases presented of 1) images and radial surface brightness profiles and colour profiles, and 2) images and integrated spectra into several example images, profiles and spectra, showing the general trends observed. For the original atlases we refer the reader to the electronic distribution on CDROM or as available on the Web at http://www.astro.rug.nl/∼nfgs/. © Kluwer Academic Publishers 2001 |
| abstract_unstemmed |
Abstract We report on our observing programme to obtain integrated spectrophotometry, intermediate- and high-resolution major-axis spectra, and UBR surface photometry of a representative sample of ∼ 200galaxies in the nearby field. The main goal of this programme is to provide a comparison sample for high-redshift studies and to study the variation in star formation rates (SFRs), star formation history (SFH),excitation, metallicity, and internal kinematics over a wide range of galaxy luminosities and morphological types. In particular, we extend the work of Kennicutt (1992) to lower-luminosity systems. We present the main results of our analysis so far. In these proceedings, we condense the two atlases presented of 1) images and radial surface brightness profiles and colour profiles, and 2) images and integrated spectra into several example images, profiles and spectra, showing the general trends observed. For the original atlases we refer the reader to the electronic distribution on CDROM or as available on the Web at http://www.astro.rug.nl/∼nfgs/. © Kluwer Academic Publishers 2001 |
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The Nearby Field Galaxy Survey |
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Kannappan, Sheila J. |
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