Limiting magnitudes and night sky brightness at the Langkawi National Observatory based on observations of standard stars

2017 International Conference on Space Science and Communication

物理学;无线电电子学

Ngeow, C.-C.^1 ; Luo, S.-C.^1

Graduate Institute of Astronomy, National Central University, Jhongli

32001, Taiwan^1

关键词: CCD images;    Exposure-time;    Night time;    Photometric calibration;    Point sources;    Transformation equationss;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/852/1/012002/pdf
DOI  :  10.1088/1742-6596/852/1/012002

来源: IOP

【 摘 要 】

We present the estimation of limiting magnitudes and night sky brightness at the Langkawi National Observatory with observations of selected standard stars. We first derived the transformation equations using the standard stars in our CCD images, followed by photometric calibration of the 2MASS point sources located in these images. Based on the calibrated magnitudes, we estimated a limiting magnitude of V=16.6±0.1 mag can be reached with a 60 second exposure time. For the night sky brightness, our measurements give Vsky=19.0±0.1 mag arc-second-2at the zenith direction. Our results can be used for planning the night time observations at the Langkawi National Observatory.