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Nachrichten, Termine, Experten
Nachrichten, Termine, Experten
The National Astronomical Research Institute of Thailand (NARIT), in collaboration with the Max Planck Institute for Radio Astronomy (MPIfR), has achieved the historic first detection of astronomical radio signals using Very Long Baseline Interferometry (VLBI) with the 40-m Thai National Radio Telescope (TNRT). The experiment, performed together with the Effelsberg 100-m radio telescope in Germany, marks the first ever VLBI signal detection made in Thailand.
Very Long Baseline Interferometry (VLBI) refers to multiple radio telescopes located far away from each other, sometimes even on different continents, and working together to produce detailed images. VLBI is an extremely challenging observing mode in which the signals recorded by each telescope must be precisely aligned and added together. Doing this successfully combines the two telescopes into one giant virtual telescope with a resolving power (ability to see extremely small things far away) that is many thousands of times better than that of the individual telescopes.
The successful VLBI observations with the TNRT and the Effelsberg radio telescopes were conducted in the 1.658-1.674 GHz frequency range on May 16, 2024, UTC 14:00-17:00. The distance between these telescopes is approximately 8,500 km, resulting in a 4.4 milliarcsecond resolution, more than 13,000 times better than the human eye. If the human eye was capable of such a resolution, you would be able to see the centre circle of a football pitch on the moon.
During the experiment, the team observed four extra-galactic radio galaxies and quasars: OJ287, 3C273, M87 (Virgo A) and J2005+7752, which are bright continuum astronomical objects in radio wavelengths. The observation data were recorded in a cutting-edge digital processing and recording system: the Effelsberg Direct Digitization (EDD) system, which is part of the Universal Software Backend (USB) developed by MPIfR. All the members of the team that made this achievement possible are listed in the Background Information section.
Through electronic data transfer from Thai National Radio Astronomy Observatory (TNRO) to MPIfR and signal processing to achieve an aperture synthesis with a VLBI data correlator at MPIfR, detections of VLBI radio correlated signals (so-called “fringes”) were finally achieved in all the observed objects. The detected signals presented correlated amplitudes with signal-to-noise ratios that are equivalent to the expectations.
Dr. Gundolf Wieching, Division Head of Electronic Department in MPIfR, states “It has been an honour to follow the journey of the excellent NARIT team to the first VLBI observations in Thailand. This is a significant milestone, only possible with the great NARIT team, and shows the potential of the superb TNRT telescope for future science.”
Dr. Koichiro Sugiyama, Chief Scientist of TNRO in NARIT, states “We are really honoured to welcome this historical moment of the 1st VLBI signal detection of the 40-m TNRT together with excellent team of MPIfR. This is the dawn of radio astronomy with VLBI technique in Thailand. Based on this great successful, we look forward to accelerate and strengthen research collaboration with the world-wide radio astronomy community through VLBI observations.”
This successful experiment is the essential first step towards expanding research fields and opportunities with the 40-m TNRT through world-wide collaboration with VLBI networks, such as the European VLBI Network, Very Long Baseline Array, East Asia VLBI Network, Australian Long Baseline Array, Asia Pacific Telescope, Global VLBI Array, and many more. This also provides a solid foundation to establish a national VLBI array in Thailand, the so-called TVA, and a next regional VLBI network in South-East Asia, so-celled SEAVN in collaboration with Indonesia, Malaysia, Vietnam, etc. in the near future.
These achievements are the result of a long-term collaboration between NARIT and MPIfR since 2012, leading to an agreement in 2018 for the development of state-of-the-art L- and K-band receivers with direct digitisation and the development of a generic astronomical software backend for TNRT.
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Background Information:
The signing of the MoU between NARIT and MPIfR took place in 2012, including Assoc. Prof. Boonrucksar Soonthornthum, Founding Director of NARIT; Prof. Karl Menten, Managing Director of MPIfR and Director of the Research Department Millimeter and Submillimeter Astronomy; Prof. Michael Kramer, Director of the Research Department Fundamental Physics in Radio Astronomy. The 2018 Annex Signing Ceremony included Dr. Ewan Barr, Group Leader Electronics, Software Development; Dr. Gundolf Wieching, Division Head of Electronic Department; Prof. Michael Kramer and Prof. Anton Zensus, Managing Director and Director of the Research Department Radio Astronomy/VLBI, all from MPIfR, and also Dr. Saran Poshyachinda, Executive Director of NARIT; Dr. Suvit Maesincee, Minister of Science and Technology of Thailand; Dr. Manop Sittidech, Minister Counsellor (Science and Technology).
Members of the task force achieving this VLBI first signal detection include Gundolf Wieching, Ewan Barr, Niclas Esser, Uwe Bach, Jan Wagner, Jason Wu, Jompoj Wongphechauxsorn (all from MPIfR), and Koichiro Sugiyama, Spiro Sarris, Teep Chairin Nobuyuki Sakai, Naphat Yawilerng, Nikom Prasert, Prachayapan Jiraya, Pathit Chatuphot, Haseng Sani (all from NARIT).
Dr. Gundolf Wieching
Max-Planck-Institut für Radioastronomie, Bonn.
Fon: +49 228 525-175
E-mail: wieching@mpifr-bonn.mpg.de
Dr. Ewan Barr
Max-Planck-Institut für Radioastronomie, Bonn.
Fon: +49 228 525-535
E-mail: ebarr@mpifr-bonn.mpg.de
Dr. Uwe Bach
Max-Planck-Institut für Radioastronomie, Bonn.
Fon: +49 2257 301-168
E-mail: ubach@mpifr-bonn.mpg.de
https://www.mpifr-bonn.mpg.de/8618635/tnrt-fringes.-may2024
Radio telescopes used in this VLBI experiment: Right, the 40-m TNRT and left, the Effelsberg 100-m r ...
TNRO/NARIT (40-m TNRT telescope); Norbert Tacken/MPIfR (Effelsberg telescope)
VLBI fringe between 40-m TNRT und 100-m Effelsberg. Left: fringe signal detected in OJ287, the brigh ...
TNRO
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