Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-09T19:44:31.091Z Has data issue: false hasContentIssue false

Status of the Thai 40-m Radio Telescope

Published online by Cambridge University Press:  04 June 2018

Phrudth Jaroenjittichai*
Affiliation:
National Astronomical Research Institute of Thailand, 260 Moo 4, Donkaew, Maerim, Chiangmai, 50180, Thailand email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
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