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A photometric study of faint galaxies in the field of GRB 000926. / Fatkhullin, T. A.; Vasil'ev, A. A.; Reshetnikov, V. P.

In: Astronomy Letters, Vol. 30, No. 5, 01.05.2004, p. 283-292.

Research output: Contribution to journal › Article › peer-review

Harvard

Fatkhullin, TA, Vasil'ev, AA & Reshetnikov, VP 2004, 'A photometric study of faint galaxies in the field of GRB 000926', Astronomy Letters, vol. 30, no. 5, pp. 283-292. https://doi.org/10.1134/1.1738151

APA

Fatkhullin, T. A., Vasil'ev, A. A., & Reshetnikov, V. P. (2004). A photometric study of faint galaxies in the field of GRB 000926. Astronomy Letters, 30(5), 283-292. https://doi.org/10.1134/1.1738151

Vancouver

Fatkhullin TA, Vasil'ev AA, Reshetnikov VP. A photometric study of faint galaxies in the field of GRB 000926. Astronomy Letters. 2004 May 1;30(5):283-292. https://doi.org/10.1134/1.1738151

Author

Fatkhullin, T. A. ; Vasil'ev, A. A. ; Reshetnikov, V. P. / A photometric study of faint galaxies in the field of GRB 000926. In: Astronomy Letters. 2004 ; Vol. 30, No. 5. pp. 283-292.

BibTeX

@article{ecd035eede3c4983b0689586ca064a51,
title = "A photometric study of faint galaxies in the field of GRB 000926",
abstract = "We present our B, V, Rc, and Ic observations of a 3′.6 × 3′ field centered on the host galaxy of GRB 000926 (α2000.0 = 17h04m11s, δ2000.0 = +51°47′9″.8). The observations were carried out on the 6-m Special Astrophysical Observatory telescope using the SCORPIO instrument. The catalog of galaxies detected in this field includes 264 objects for which the signal-to-noise ratio is larger than 5 in each photometric band. The following limiting magnitudes in the catalog correspond to this limitation: 26.6 (B), 25.7 (V), 25.8 (R), and 24.5 (I). The differential galaxy counts are in good agreement with previously published CCD observations of deep fields. We estimated the photometric redshifts for all of the cataloged objects and studied the color variations of the galaxies with z. For luminous spiral galaxies with M(B) < -18, we found no evidence for any noticeable evolution of their linear sizes to z ∼ 1.",
keywords = "Distant galaxies, Photometric observations",
author = "Fatkhullin, {T. A.} and Vasil'ev, {A. A.} and Reshetnikov, {V. P.}",
year = "2004",
month = may,
day = "1",
doi = "10.1134/1.1738151",
language = "English",
volume = "30",
pages = "283--292",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "5",

}

RIS

TY - JOUR

T1 - A photometric study of faint galaxies in the field of GRB 000926

AU - Fatkhullin, T. A.

AU - Vasil'ev, A. A.

AU - Reshetnikov, V. P.

PY - 2004/5/1

Y1 - 2004/5/1

N2 - We present our B, V, Rc, and Ic observations of a 3′.6 × 3′ field centered on the host galaxy of GRB 000926 (α2000.0 = 17h04m11s, δ2000.0 = +51°47′9″.8). The observations were carried out on the 6-m Special Astrophysical Observatory telescope using the SCORPIO instrument. The catalog of galaxies detected in this field includes 264 objects for which the signal-to-noise ratio is larger than 5 in each photometric band. The following limiting magnitudes in the catalog correspond to this limitation: 26.6 (B), 25.7 (V), 25.8 (R), and 24.5 (I). The differential galaxy counts are in good agreement with previously published CCD observations of deep fields. We estimated the photometric redshifts for all of the cataloged objects and studied the color variations of the galaxies with z. For luminous spiral galaxies with M(B) < -18, we found no evidence for any noticeable evolution of their linear sizes to z ∼ 1.

AB - We present our B, V, Rc, and Ic observations of a 3′.6 × 3′ field centered on the host galaxy of GRB 000926 (α2000.0 = 17h04m11s, δ2000.0 = +51°47′9″.8). The observations were carried out on the 6-m Special Astrophysical Observatory telescope using the SCORPIO instrument. The catalog of galaxies detected in this field includes 264 objects for which the signal-to-noise ratio is larger than 5 in each photometric band. The following limiting magnitudes in the catalog correspond to this limitation: 26.6 (B), 25.7 (V), 25.8 (R), and 24.5 (I). The differential galaxy counts are in good agreement with previously published CCD observations of deep fields. We estimated the photometric redshifts for all of the cataloged objects and studied the color variations of the galaxies with z. For luminous spiral galaxies with M(B) < -18, we found no evidence for any noticeable evolution of their linear sizes to z ∼ 1.

KW - Distant galaxies

KW - Photometric observations

UR - http://www.scopus.com/inward/record.url?scp=2942690213&partnerID=8YFLogxK

U2 - 10.1134/1.1738151

DO - 10.1134/1.1738151

M3 - Article

AN - SCOPUS:2942690213

VL - 30

SP - 283

EP - 292

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 5

ER -

ID: 33073404