Standard

Study of BTA, Hubble, and Spitzer GRB 021004 deep fields. / Sokolov, I.V.; Bravo Calle, O.J.A.; Baryshev, Yu.V.

EAS Publication Series. Cambridge University Press, 2013. p. 435-437.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Research › peer-review

Harvard

Sokolov, IV, Bravo Calle, OJA & Baryshev, YV 2013, Study of BTA, Hubble, and Spitzer GRB 021004 deep fields. in EAS Publication Series. Cambridge University Press, pp. 435-437. https://doi.org/10.1051/eas/1361070

APA

Sokolov, I. V., Bravo Calle, O. J. A., & Baryshev, Y. V. (2013). Study of BTA, Hubble, and Spitzer GRB 021004 deep fields. In EAS Publication Series (pp. 435-437). Cambridge University Press. https://doi.org/10.1051/eas/1361070

Vancouver

Sokolov IV, Bravo Calle OJA, Baryshev YV. Study of BTA, Hubble, and Spitzer GRB 021004 deep fields. In EAS Publication Series. Cambridge University Press. 2013. p. 435-437 https://doi.org/10.1051/eas/1361070

Author

Sokolov, I.V. ; Bravo Calle, O.J.A. ; Baryshev, Yu.V. / Study of BTA, Hubble, and Spitzer GRB 021004 deep fields. EAS Publication Series. Cambridge University Press, 2013. pp. 435-437

BibTeX

@inproceedings{d61a13dc98fb4a948399d8f09dca1062,
title = "Study of BTA, Hubble, and Spitzer GRB 021004 deep fields",
abstract = "The photometric redshifts were derived, based on photometry data in visual and infrared. Deep fields were observed during gamma-ray bursts investigation with the SAO RAS 6-meter telescope (BTA), Spitzer and Hubble Space Telescope. BTA BVRI images were used, as well as F475W, F606W, F814W of ACS at the Hubble Space Telescope and Spitzer IRAC ch1 3.6 μm, ch3 5.7 μm. Each BTA BVRI exposure was about one-hour long, reaching objects up to the ~27th stellar magnitude. The GRB 021004 field was investigated. A catalog of 874 discovered objects is being made as well as color diagrams and Hubble diagram for these objects.",
author = "I.V. Sokolov and {Bravo Calle}, O.J.A. and Yu.V. Baryshev",
year = "2013",
doi = "10.1051/eas/1361070",
language = "English",
pages = "435--437",
booktitle = "EAS Publication Series",
publisher = "Cambridge University Press",
address = "United Kingdom",

}

RIS

TY - GEN

T1 - Study of BTA, Hubble, and Spitzer GRB 021004 deep fields

AU - Sokolov, I.V.

AU - Bravo Calle, O.J.A.

AU - Baryshev, Yu.V.

PY - 2013

Y1 - 2013

N2 - The photometric redshifts were derived, based on photometry data in visual and infrared. Deep fields were observed during gamma-ray bursts investigation with the SAO RAS 6-meter telescope (BTA), Spitzer and Hubble Space Telescope. BTA BVRI images were used, as well as F475W, F606W, F814W of ACS at the Hubble Space Telescope and Spitzer IRAC ch1 3.6 μm, ch3 5.7 μm. Each BTA BVRI exposure was about one-hour long, reaching objects up to the ~27th stellar magnitude. The GRB 021004 field was investigated. A catalog of 874 discovered objects is being made as well as color diagrams and Hubble diagram for these objects.

AB - The photometric redshifts were derived, based on photometry data in visual and infrared. Deep fields were observed during gamma-ray bursts investigation with the SAO RAS 6-meter telescope (BTA), Spitzer and Hubble Space Telescope. BTA BVRI images were used, as well as F475W, F606W, F814W of ACS at the Hubble Space Telescope and Spitzer IRAC ch1 3.6 μm, ch3 5.7 μm. Each BTA BVRI exposure was about one-hour long, reaching objects up to the ~27th stellar magnitude. The GRB 021004 field was investigated. A catalog of 874 discovered objects is being made as well as color diagrams and Hubble diagram for these objects.

U2 - 10.1051/eas/1361070

DO - 10.1051/eas/1361070

M3 - Conference contribution

SP - 435

EP - 437

BT - EAS Publication Series

PB - Cambridge University Press

ER -

ID: 7398695