The DOI matches its Crossref record; 21 of the 21 references it cites were found in a registry or an index.
Estimating Fixed-Frame Galaxy Magnitudes in the Sloan Digital Sky Survey
Open accessAbstract
Broadband measurements of flux for galaxies at different redshifts measure different regions of the rest-frame galaxy spectrum. Certain astronomical questions, such as the evolution of the luminosity function of galaxies, require transforming these inherently redshift-dependent magnitudes into redshift-independent quantities. To prepare to address these astronomical questions, investigated in detail in subsequent papers, we fit spectral energy distributions (SEDs) to broadband photometric observations in the context of the optical observations of the Sloan Digital Sky Survey (SDSS). Linear combinations of four spectral templates can reproduce the five SDSS magnitudes of all galaxies to the precision of the photometry. Expressed in the appropriate coordinate system, the locus of the coefficients multiplying the templates is planar and, in fact, nearly linear. The resulting reconstructed SEDs can be used to recover fixed-frame magnitudes over a range of redshifts. This process yields consistent results in the sense that, within each sample, the intrinsic colors of similar type galaxies are nearly constant with redshift. We compare our results with simpler interpolation methods and galaxy spectrophotometry from the SDSS. The software that generates these results is publicly available and easily adapted to handle a wide range of galaxy observations.
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Cites
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Self-citationSavitzky-Golay Smoothing Filters
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The Sloan Digital Sky Survey: Technical Summary
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Self-citationThe Sloan Digital Sky Survey Photometric System
Fukugita, M., Ichikawa, T., Gunn, J. E., Doi, M., Shimasaku, K., & Schneider, D. P. (1996) · The Astronomical Journal · doi:10.1086/117915 · Cited by 3,033
Self-citationSecondary standard stars for absolute spectrophotometry
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Self-citationSloan Digital Sky Survey: Early Data Release
Stoughton, C., Lupton, R. H., Bernardi, M., Blanton, M. R., Burles, S., Castander, F. J., Connolly, A. J., Eisenstein, D. J., Frieman, J. A., Hennessy, G. S., et al. (2002) · The Astronomical Journal · doi:10.1086/324741 · Cited by 2,390
Self-citationSpectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
Strauss, M. A., Weinberg, D. H., Lupton, R. H., Narayanan, V. K., Annis, J., Bernardi, M., Blanton, M., Burles, S., Connolly, A. J., Dalcanton, J., et al. (2002) · The Astronomical Journal · doi:10.1086/342343 · Cited by 1,909
Self-citationSpectral evolution of stellar populations using isochrone synthesis
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The Sloan Digital Sky Survey Photometric Camera
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Self-citationSmith, J. A., Tucker, D. L., Kent, S., Richmond, M. W., Fukugita, M., Ichikawa, T., Ichikawa, S.-I., Jorgensen, A. M., Uomoto, A., Gunn, J. E., et al. (2002) · The Astronomical Journal · doi:10.1086/339311 · Cited by 1,621
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Cited by
Tremonti, C. A., Heckman, T. M., Kauffmann, G., Brinchmann, J., Charlot, S., White, S. D. M., Seibert, M., Peng, E. W., Schlegel, D. J., Uomoto, A., et al. (2004) · The Astrophysical Journal · doi:10.1086/423264 · Cited by 3,608
Self-citationThe Optical and Near‐Infrared Properties of Galaxies. I. Luminosity and Stellar Mass Functions
Bell, E. F., McIntosh, D. H., Katz, N., & Weinberg, M. D. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/378847 · Cited by 2,295
Cole, S., Percival, W. J., Peacock, J. A., Norberg, P., Baugh, C. M., Frenk, C. S., Baldry, I., Bland-Hawthorn, J., Bridges, T., Cannon, R., et al. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09318.x · Cited by 2,094
Conroy, C., Gunn, J. E., & White, M. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/699/1/486 · Cited by 1,891
Self-citationThe clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z=0.15
Ross, A. J., Samushia, L., Howlett, C., Percival, W. J., Burden, A., & Manera, M. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv154 · Cited by 1,745
“They include K-corrected absolute magnitudes, determined using the methods of Blanton et al. (2003), and detailed information on the mask.”
Method
Metadata
- Authors
- Blanton, M. R., Brinkmann, J., Csabai, I., Doi, M., Eisenstein, D., Fukugita, M., Gunn, J. E., Hogg, D. W., & Schlegel, D. J.
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2003-05
- Volume
- 125
- Issue
- 5
- Pages
- 2348-2360
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W1847269195
- Cited by
- 542
- References
- 21
- FWCI
- 27.26
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Blanton, M. R., Brinkmann, J., Csabai, I., Doi, M., Eisenstein, D., Fukugita, M., Gunn, J. E., Hogg, D. W., & Schlegel, D. J. (2003). Estimating Fixed-Frame Galaxy Magnitudes in the Sloan Digital Sky Survey. The Astronomical Journal. https://doi.org/10.1086/342935
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