J/MNRAS/479/111     AST3-1 Point Source Catalogue                   (Ma+, 2018)

The first release of the AST3-1 Point Source Catalogue from Dome A, Antarctica. Ma B., Shang Z., Hu Y., Hu K., Liu Q., Ashley M.C.B., Cui X., Du F., Fan D., Feng L., Huang F., Gu B., He B., Ji T., Li X., Li Z., Liu H., Tian Q., Tao C., Wang D., Wang L., Wang S., Wang X., Wei P., Wu J., Xu L., Yang S., Yang M., Yang Y., Yu C., Yuan X., Zhou H., Zhang H., Zhang X., Zhang Y., Zhao C., Zhou J., Zhu Z.-H. <Mon. Not. R. Astron. Soc., 479, 111-120 (2018)> =2018MNRAS.479..111M 2018MNRAS.479..111M (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Photometry Keywords: methods: data analysis - methods: observational - techniques: image processing - techniques: photometric - catalogues - surveys Abstract: The three Antarctic Survey Telescopes (AST3) aim to carry out time-domain imaging survey at Dome A, Antarctica. The first of the three telescopes (AST3-1) was successfully deployed in 2012 January. AST3-1 is a 500mm aperture modified Schmidt telescope with a 680mm diameter primary mirror. AST3-1 is equipped with a SDSS i filter and a 10kx10k frame transfer CCD camera, reduced to 5kx10k by electronic shuttering, resulting in a 4.3deg2 field of view. To verify the capability of AST3-1 for a variety of science goals, extensive commissioning was carried out between 2012 March and May. The commissioning included a survey covering 2000deg2 as well as the entire Large and Small Magellanic Clouds. Frequent repeated images were made of the centre of the Large Magellanic Cloud, a selected exoplanet transit field, and fields including some Wolf-Rayet stars. Here, we present the data reduction and photometric measurements of the point sources observed by AST3-1. We have achieved a survey depth of 19.3mag in 60s exposures with 5mmag precision in the light curves of bright stars. The facility achieves sub-mmag photometric precision under stable survey conditions, approaching its photon noise limit. These results demonstrate that AST3-1 at Dome A is extraordinarily competitive in time-domain astronomy, including both quick searches for faint transients and the detection of tiny transit signals. Description: We present the first data release, DR1, of the photometric data from the AST3-1 commissioning surveys. DR1 consists of 14 000 scientific images, 16 million sources bright than i∼19 with photometry and astrometry, and 2 million light curves. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file lmc_smc.dat 69 3396185 AST3-1 DR1 LMC/SCM sources snsurvey.dat 72 12768876 AST3-1 DR1 SN sources -------------------------------------------------------------------------------- See also: https://nadc.china-vo.org/data : AST3-1 DR1 home page Byte-by-byte Description of file: lmc_smc.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 I8 --- ID [30000001/33396185] Source index 10- 30 F21.17 deg RAdeg ?=- Right ascension (J2000) 32- 51 F20.16 deg DEdeg ?=- Declination (J2000) 53- 59 F7.4 mag imag ?=- Mean i magnitude 61- 66 F6.4 mag e_imag ?=- Standard deviation of i magnitude 68- 69 I2 --- o_imag ?=- Number of observations -------------------------------------------------------------------------------- Byte-by-byte Description of file: snsurvey.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 I8 --- ID [10000001/22768934] Source index 10- 33 F24.20 deg RAdeg ?=- Right ascension (J2000) 35- 54 F20.16 deg DEdeg ?=- Declination (J2000) 56- 62 F7.4 mag imag ?=- Mean i magnitude 64- 69 F6.4 mag e_imag ?=- Standard deviation of i magnitude 71- 72 I2 --- o_imag ?=- Number of observations -------------------------------------------------------------------------------- History: Copied at https://nadc.china-vo.org/data/
(End) Patricia Vannier [CDS] 24-Feb-2022
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