1997BaltA...6...33L

Query : 1997BaltA...6...33L

1997BaltA...6...33L - Baltic Astronomy, 6, 33-40 (1997/February-0)

Multiband photometry of selected areas in a study of galactic structure.

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., WU H., ZHANG M., ZHENG Z.Y., ZHOU X., CHEN F.Z., DENG Z.G., CHU Y.Q., SU J., SHANG Z.H., YAN H.J. and XIA X.Y.

Abstract (from CDS):

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, H beta 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, H beta) 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 report on the status of this study.

Abstract Copyright: ∼

Journal keyword(s): techniques: photometric - stars: fundamental parameters - Galaxy: structure

Simbad objects: 7

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Number of rows : 7
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NGC 288 GlC 00 52 45.24 -26 34 57.4   10 8.13     ~ 1130 0
2 SA 92- reg 00 55 03.80 +00 47 13.2           ~ 102 0
3 SA 94- reg 02 55 58.10 +00 30 03.6           ~ 47 0
4 SA 95- reg 03 53 21.0 -00 01 10           ~ 85 0
5 EGGR 426 WD* 07 50 14.5843350628 +07 11 48.917000372   17.9   16.2   DC9 74 0
6 EGGR 427 WD* 07 50 15.3418409575 +07 11 37.097929321   17.6   16.1   DC9 72 0
7 NGC 2682 OpC 08 51 23.5 +11 48 54           ~ 2528 0

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