A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images

被引：0

作者：

Huertas-Company, M. ^{[1
,3
]}

Tasca, L. ^{[2
]}

Rouan, D. ^{[1
]}

Pelat, D. ^{[4
]}

Kneib, J.P. ^{[2
]}

Le Fèvre, O. ^{[2
]}

Capak, P. ^{[7
,8
]}

Kartaltepe, J. ^{[9
]}

Koekemoer, A. ^{[11
]}

McCracken, H.J. ^{[5
]}

Salvato, M. ^{[6
,7
]}

Sanders, D.B. ^{[9
]}

Willott, C. ^{[10
]}

机构：

[1] LESIA-Paris Observatory, 5 place Jules Janssen, 92195 Meudon, France

[2] LAM, CNRS, Université de Provence, 38 rue Frédric Joliot-Curie, 13388 Marseille Cedex 13, France

[3] IAA-C/ Camino Bajo de Huétor, 50 - 18008 Granada, Spain

[4] LUTH-Paris Observatory, 5 place Jules Janssen, 92195 Meudon, France

[5] IAP, CNRS, Université Pierre et Marie Curie, 98 boulevard Arago, 75014 Paris, France

[6] Caltech, Pasadena, CA 91125, United States

[7] 105-24 Caltech, Pasadena, CA 91125, United States

[8] Spitzer Science Center, 314-6 Caltech, Pasadena, CA 91125, United States

[9] Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, United States

[10] Physics Department, University of Ottawa, MacDonald Hall, 150 Louis Pasteur, Ottawa, ON K1N 6N5, Canada

[11] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD 21218, United States

来源：

Astronomy and Astrophysics | 2009年 / 497卷 / 03期

关键词：

Galaxies;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Journal article (JA)

引用

页码：743 / 753

共 50 条

[1] A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images
Huertas-Company, M.
Rouan, D.
Tasca, L.
Soucail, G.
Le Fevre, O.
[J]. ASTRONOMY & ASTROPHYSICS, 2008, 478 (03) : 971 - 980
[2] A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images: I. Method description
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Rouan, D.
Tasca, L.
Soucail, G.
Le Fèvre, O.
[J]. Astronomy and Astrophysics, 1600, 478 (03): : 971 - 980
[3] A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images II. Quantifying morphological k-correction in the COSMOS field at 1 < z < 2: Ks band vs. I band
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Rouan, D.
Pelat, D.
Kneib, J. P.
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Capak, P.
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Koekemoer, A.
McCracken, H. J.
Salvato, M.
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