J/PASP/122/347      Chinese Small Telescope ARray (CSTAR)    (Zhou+, 2010)

The first release of the CSTAR Point Source Catalog from Dome A, Antarctica. Zhou X., Fan Z., Jiang Z., Ashley M.C.B., Cui X., Feng L., Gong X., Hu J., Kulesa C.A., Lawrence J.S., Liu G., Luong-van D.M., Ma J., Moore A.M., Qin W., Shang Z., Storey J.W.V., Sun B., Travouillon T., Walker C.K., Wang J., Wang L., Wu J., Wu Z., Xia L., Yan J., Yang J., Yang H., Yuan X., York D., Zhang Z., Zhu Z. <Publ. Astron. Soc. Pac., 122, 347-353 (2010)> =2010PASP..122..347Z 2010PASP..122..347Z
ADC_Keywords: Surveys ; Galactic pole, south ; Photometry, SDSS Abstract: In 2008 January the twenty-fourth Chinese expedition team successfully deployed the Chinese Small Telescope ARray (CSTAR) to Dome A, the highest point on the Antarctic plateau. CSTAR consists of four 14.5cm optical telescopes, each with a different filter (g,r,i, and open) and has a 4.5°x4.5° field of view (FOV). It operates robotically as part of the Plateau Observatory, PLATO, with each telescope taking an image every ∼30s throughout the year whenever it is dark. During 2008, CSTAR 1 performed almost flawlessly, acquiring more than 0.3 million -band images for a total integration time of 1728hr during 158 days of observations. For each image taken under good sky conditions, more than 10,000 sources down to magnitude could be detected. We performed aperture photometry on all the sources in the field to create the catalog described herein. Since CSTAR has a fixed pointing centered on the south celestial pole (Dec=-90°), all the sources within the FOV of CSTAR were monitored continuously for several months. The photometric catalog can be used for studying any variability in these sources, and for the discovery of transient sources such as supernovae, gamma-ray bursts, and minor planets. Description: CSTAR observed robotically at Dome A (Antartica) from 2008 March 4 until 2008 August 8, taking an image with each telescope whenever it was dark enough to do so. The exposure time was changed from 20s to 30s on April 4. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file cstar1.dat 66 21845 Chinese Small Telescope ARray (CSTAR), Version 2008 -------------------------------------------------------------------------------- See also: http://casdc.china-vo.org/data/cstar : CSTAR home page Byte-by-byte Description of file: cstar1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Right ascension (J2000) 4- 5 I2 min RAm Right ascension (J2000) 7- 12 F6.3 s RAs Right ascension (J2000) 14 A1 --- DE- Declination sign (J2000) 15- 16 I2 deg DEd Declination (J2000) 18- 19 I2 arcmin DEm Declination (J2000) 21- 25 F5.2 arcsec DEs Declination (J2000) 28- 37 F10.4 pix Xpos X position 40- 49 F10.4 pix Ypos Y position 51- 57 F7.4 mag imag SDSS i-band magnitude 59- 66 F8.6 mag e_imag rms uncertainty on imag -------------------------------------------------------------------------------- History: Copied at http://archive.bao.ac.cn/en/cstar
(End) Patricia Vannier [CDS] 07-Aug-2013
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line