The DOI matches its Crossref record; 27 of the 27 references it cites were found in a registry or an index.
The Size Evolution of High-Redshift Galaxies
Open accessAbstract
Hubble Space Telescope images of high-redshift galaxies selected via color and photometric redshifts are used to examine the size and axial ratio distribution of galaxies as a function of redshift at look-back times t > 8 Gyr. These parameters are measured at rest-frame UV wavelengths (1200 Å < λ < 2000 Å) on images with a rest-frame resolution of less than 0.8 kpc. Galaxy radii are found to scale with redshift approximately as the Hubble parameter H -1 ( z ). This is in accord with the theoretical expectation that the typical sizes of the luminous parts of galaxies should track the expected evolution in the virial radius of dark matter halos. The mean ratio of the semimajor axis to the semiminor axis for a bright well-resolved sample of galaxies at z ~ 4 is b / a = 0.65, suggesting that these Lyman break galaxies are not drawn from a spheroidal population. However, the median concentration index of this sample is C = 3.5, which is closer to the typical concentration indices of nearby elliptical galaxies ( C ~ 4) than to the values for local disk galaxies of type Sb and later ( C < 2).
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Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
SExtractor: Software for source extraction
Bertin, E., & Arnouts, S. (1996) · Astronomy and Astrophysics Supplement Series · doi:10.1051/aas:1996164 · Cited by 10,866
The Dust Content and Opacity of Actively Star‐forming Galaxies
Calzetti, D., Armus, L., Bohlin, R. C., Kinney, A. L., Koornneef, J., & Storchi‐Bergmann, T. (2000) · The Astrophysical Journal · doi:10.1086/308692 · Cited by 5,717
Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering
White, S. D. M., & Rees, M. J. (1978) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/183.3.341 · Cited by 3,919
Sloan 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
Galaxy formation through hierarchical clustering
White, S. D. M., & Frenk, C. S. (1991) · The Astrophysical Journal · doi:10.1086/170483 · Cited by 2,354
The formation of galactic discs
Mo, H. J., Mao, S., & White, S. D. M. (1998) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1998.01227.x · Cited by 2,155
The formation and evolution of galaxies within merging dark matter haloes*
Kauffmann, G., White, S. D. M., & Guiderdoni, B. (1993) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/264.1.201 · Cited by 1,884
Spectral evolution of stellar populations using isochrone synthesis
Bruzual A., G., & Charlot, S. (1993) · The Astrophysical Journal · doi:10.1086/172385 · Cited by 1,808
The Great Observatories Origins Deep Survey: Initial Results from Optical and Near-Infrared Imaging
Giavalisco, M., Ferguson, H. C., Koekemoer, A. M., Dickinson, M., Alexander, D. M., Bauer, F. E., Bergeron, J., Biagetti, C., Brandt, W. N., Casertano, S., et al. (2004) · The Astrophysical Journal · doi:10.1086/379232 · Cited by 1,678
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Cited by
MORPHOLOGIES OF ∼190,000 GALAXIES AT z = 0–10 REVEALED WITH HST LEGACY DATA. I. SIZE EVOLUTION
Shibuya, T., Ouchi, M., & Harikane, Y. (2015) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/219/2/15 · Cited by 426
Bouwens, R. J., Illingworth, G. D., Blakeslee, J. P., & Franx, M. (2006) · The Astrophysical Journal · doi:10.1086/498733 · Cited by 344
ZFOURGE/CANDELS: ON THE EVOLUTION OF M* GALAXY PROGENITORS FROM z= 3 TO 0.5
Papovich, C., Labbé, I., Quadri, R., Tilvi, V., Behroozi, P., Bell, E. F., Glazebrook, K., Spitler, L., Straatman, C. M. S., Tran, K.-V., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/803/1/26 · Cited by 143
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Metadata
- Authors
- Ferguson, H. C., Dickinson, M., Giavalisco, M., Kretchmer, C., Ravindranath, S., Idzi, R., Taylor, E., Conselice, C. J., Fall, S. M., Gardner, J. P., Livio, M., Madau, P., Moustakas, L. A., Papovich, C. M., Somerville, R. S., Spinrad, H., & Stern, D.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2004-01-09
- Volume
- 600
- Issue
- 2
- Pages
- L107-L110
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2116427483
- Cited by
- 371
- References
- 27
- FWCI
- 17.53
- Type
- journal article
- Language
- en
- Open access
- bronze
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