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Status of the Thai 40-m Radio Telescope
Published online by Cambridge University Press: 04 June 2018
Abstract
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Since the first light of the 2.4-m Thai National Telescope in 2013, Thailand foresees another great leap forward in astronomy. A project known as “Radio Astronomy Network and Geodesy for Development” (RANGD) by National Astronomical Research Institute of Thailand (NARIT) has been approved for year 2017-2021. A 40-m radio telescope has been planned to operate up to 115-GHz observation with prime-focus capability for low frequency and phased array feed receivers. The telescope’s first light is expected in late 2019 with a cryogenics K-band and L-band receivers. RFI environment at the site has been investigated and shown to be at reasonable level. A 13-m VGOS telescope is also included for geodetic applications. Early single-dish science will focus on time domain observations, such as pulsars and transients, outbursts and variability of maser and AGN sources.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 13 , Symposium S337: Pulsar Astrophysics the Next Fifty Years , September 2017 , pp. 346 - 347
- Copyright
- Copyright © International Astronomical Union 2018
References
López Fernández, J. A., Gómez González, J., & Barcía Cáncio, A., 2006, Lecture Notes and Essays in Astrophysics, 2, 257LGoogle Scholar
Jaroenjittichai, J., Bandudej, K., Kempet, P., Punyawarin, S., Singwong, D., Somboonpon, P., Poshyachinda, S., & Kramer, B. H. 2017, Journal of Physics: Conference Series, 901, 1, p.12062Google Scholar
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