Multiband photometry of selected areas in a study of galactic structure

P. K. Lu; W. S. Tsay; A. B.C. Chen; R. Chen; W. H. Sun; Y. I. Byun; W. P. Chen; T. H. Chiueh; H. J. Kuo; D. Burstein; J. J. Hester; R. A. Windhorst; L. Z. Fang; J. S. Chen; J. Zhu; L. C. Deng; X. H. Fan; Z. J. Jiang; Y. Li; H. Wu; M. Zhang; Z. Y. Zheng; X. Zhou; F. Z. Chen; Z. G. Deng; Y. Q. Chu; J. Su; Z. H. Shang; H. J. Yan; X. Y. Xia

doi:10.1515/astro-1997-0108

Multiband photometry of selected areas in a study of galactic structure

P. K. Lu, W. S. Tsay, A. B.C. Chen, R. Chen, W. H. Sun, Y. I. Byun, W. P. Chen, T. H. Chiueh, H. J. Kuo, D. Burstein, J. J. Hester, R. A. Windhorst, L. Z. Fang, J. S. Chen, J. Zhu, L. C. Deng, X. H. Fan, Z. J. Jiang, Y. Li, H. WuM. Zhang, Z. Y. Zheng, X. Zhou, F. Z. Chen, Z. G. Deng, Y. Q. Chu, J. Su, Z. H. Shang, H. J. Yan, X. Y. Xia

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Abstract

The BATC (Beijing-Arizona-Taipei-Connecticut) intermediate-band 15 filter photometry system has been tested by using the Michigan Curtis Schmidt telescope at CTIO taking one-degree fields around NGC 288, SA 92, 94, 95, Lp 543-32/33. BVRI and uvby, Hβ filter observations of these same fields were also made using the 0.9 m CTIO telescope. The main purpose of these observations is to compare the results from the standard filter color systems (UBVRI and ubvy, Hβ) to those we can construct from the BATC filter system. These fields were chosen based on available filter color data in those systems. The BATC data are being taken on a Schmidt telescope similar to that at CTIO, so that these observations can provide an independent source of calibration for the BATC data. This is a report on the status of this study.

Original language	English
Pages (from-to)	33-40
Number of pages	8
Journal	Baltic Astronomy
Volume	6
Issue number	1
DOIs	https://doi.org/10.1515/astro-1997-0108
State	Published - 1997
Externally published	Yes

Keywords

Galaxy: structure
Stars: fundamental parameters
Techniques: photometric

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Lu, P. K., Tsay, W. S., Chen, A. B. C., Chen, R., Sun, W. H., Byun, Y. I., Chen, W. P., Chiueh, T. H., Kuo, H. J., Burstein, D., Hester, J. J., Windhorst, R. A., Fang, L. Z., Chen, J. S., Zhu, J., Deng, L. C., Fan, X. H., Jiang, Z. J., Li, Y., ... Xia, X. Y. (1997). Multiband photometry of selected areas in a study of galactic structure. Baltic Astronomy, 6(1), 33-40. https://doi.org/10.1515/astro-1997-0108

@article{490a85f25e424728a18aeea2c2e155fc,

title = "Multiband photometry of selected areas in a study of galactic structure",

abstract = "The BATC (Beijing-Arizona-Taipei-Connecticut) intermediate-band 15 filter photometry system has been tested by using the Michigan Curtis Schmidt telescope at CTIO taking one-degree fields around NGC 288, SA 92, 94, 95, Lp 543-32/33. BVRI and uvby, Hβ filter observations of these same fields were also made using the 0.9 m CTIO telescope. The main purpose of these observations is to compare the results from the standard filter color systems (UBVRI and ubvy, Hβ) to those we can construct from the BATC filter system. These fields were chosen based on available filter color data in those systems. The BATC data are being taken on a Schmidt telescope similar to that at CTIO, so that these observations can provide an independent source of calibration for the BATC data. This is a report on the status of this study.",

keywords = "Galaxy: structure, Stars: fundamental parameters, Techniques: photometric",

author = "Lu, {P. K.} and Tsay, {W. S.} and Chen, {A. B.C.} and R. Chen and Sun, {W. H.} and Byun, {Y. I.} and Chen, {W. P.} and Chiueh, {T. H.} and Kuo, {H. J.} and D. Burstein and Hester, {J. J.} and Windhorst, {R. A.} and Fang, {L. Z.} and Chen, {J. S.} and J. Zhu and Deng, {L. C.} and Fan, {X. H.} and Jiang, {Z. J.} and Y. Li and H. Wu and M. Zhang and Zheng, {Z. Y.} and X. Zhou and Chen, {F. Z.} and Deng, {Z. G.} and Chu, {Y. Q.} and J. Su and Shang, {Z. H.} and Yan, {H. J.} and Xia, {X. Y.}",

year = "1997",

doi = "10.1515/astro-1997-0108",

language = "English",

volume = "6",

pages = "33--40",

journal = "Baltic Astronomy",

issn = "1392-0049",

publisher = "Walter de Gruyter GmbH",

number = "1",

}

Lu, PK, Tsay, WS, Chen, ABC, Chen, R, Sun, WH, Byun, YI, Chen, WP, Chiueh, TH, Kuo, HJ, Burstein, D, Hester, JJ, Windhorst, RA, Fang, LZ, Chen, JS, Zhu, J, Deng, LC, Fan, XH, Jiang, ZJ, Li, Y, Wu, H, Zhang, M, Zheng, ZY, Zhou, X, Chen, FZ, Deng, ZG, Chu, YQ, Su, J, Shang, ZH, Yan, HJ & Xia, XY 1997, 'Multiband photometry of selected areas in a study of galactic structure', Baltic Astronomy, vol. 6, no. 1, pp. 33-40. https://doi.org/10.1515/astro-1997-0108

TY - JOUR

T1 - Multiband photometry of selected areas in a study of galactic structure

AU - Lu, P. K.

AU - Tsay, W. S.

AU - Chen, A. B.C.

AU - Chen, R.

AU - Sun, W. H.

AU - Byun, Y. I.

AU - Chen, W. P.

AU - Chiueh, T. H.

AU - Kuo, H. J.

AU - Burstein, D.

AU - Hester, J. J.

AU - Windhorst, R. A.

AU - Fang, L. Z.

AU - Chen, J. S.

AU - Zhu, J.

AU - Deng, L. C.

AU - Fan, X. H.

AU - Jiang, Z. J.

AU - Li, Y.

AU - Wu, H.

AU - Zhang, M.

AU - Zheng, Z. Y.

AU - Zhou, X.

AU - Chen, F. Z.

AU - Deng, Z. G.

AU - Chu, Y. Q.

AU - Su, J.

AU - Shang, Z. H.

AU - Yan, H. J.

AU - Xia, X. Y.

PY - 1997

Y1 - 1997

N2 - The BATC (Beijing-Arizona-Taipei-Connecticut) intermediate-band 15 filter photometry system has been tested by using the Michigan Curtis Schmidt telescope at CTIO taking one-degree fields around NGC 288, SA 92, 94, 95, Lp 543-32/33. BVRI and uvby, Hβ filter observations of these same fields were also made using the 0.9 m CTIO telescope. The main purpose of these observations is to compare the results from the standard filter color systems (UBVRI and ubvy, Hβ) to those we can construct from the BATC filter system. These fields were chosen based on available filter color data in those systems. The BATC data are being taken on a Schmidt telescope similar to that at CTIO, so that these observations can provide an independent source of calibration for the BATC data. This is a report on the status of this study.

AB - The BATC (Beijing-Arizona-Taipei-Connecticut) intermediate-band 15 filter photometry system has been tested by using the Michigan Curtis Schmidt telescope at CTIO taking one-degree fields around NGC 288, SA 92, 94, 95, Lp 543-32/33. BVRI and uvby, Hβ filter observations of these same fields were also made using the 0.9 m CTIO telescope. The main purpose of these observations is to compare the results from the standard filter color systems (UBVRI and ubvy, Hβ) to those we can construct from the BATC filter system. These fields were chosen based on available filter color data in those systems. The BATC data are being taken on a Schmidt telescope similar to that at CTIO, so that these observations can provide an independent source of calibration for the BATC data. This is a report on the status of this study.

KW - Galaxy: structure

KW - Stars: fundamental parameters

KW - Techniques: photometric

UR - http://www.scopus.com/inward/record.url?scp=0039758513&partnerID=8YFLogxK

U2 - 10.1515/astro-1997-0108

DO - 10.1515/astro-1997-0108

M3 - Article

AN - SCOPUS:0039758513

SN - 1392-0049

VL - 6

SP - 33

EP - 40

JO - Baltic Astronomy

JF - Baltic Astronomy

IS - 1

ER -

Multiband photometry of selected areas in a study of galactic structure

Abstract

Keywords

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