A5022000679- Radio Astronomy Observations and Technology
- Astrophysics and Cosmic Phenomena
- Geophysics and Gravity Measurements
- Astronomical Observations and Instrumentation
- Superconducting and THz Device Technology
- Gamma-ray bursts and supernovae
- Adaptive optics and wavefront sensing
- Satellite Communication Systems
- GNSS positioning and interference
- Astronomy and Astrophysical Research
- Galaxies: Formation, Evolution, Phenomena
- Scientific Research and Discoveries
- Internet of Things and Social Network Interactions
- Precipitation Measurement and Analysis
- Optical Systems and Laser Technology
- Telecommunications and Broadcasting Technologies
- Wireless Sensor Networks and IoT
- Particle Detector Development and Performance
Instituto Argentino de Radioastronomía
2000-2021
Consejo Nacional de Investigaciones Científicas y Técnicas
2016
Authorised Association Consortium
2013
We present the final data release of high sensitivity λ 21-cm neutral hydrogen survey sky south . A total 50 980 positions lying on a galactic coordinate grid with points spaced by () = (05/cos b, 05) were observed 30-m dish Instituto Argentino de Radioastronomía (IAR). The angular resolution is HPBW 05 and velocity coverage spans interval -450 to +400 (LSR). 1.27 rms noise entire database 0.07 K. are corrected for stray radiation converted brightness temperatures.
This paper reports on a high sensitivity λ 21-cm neutral hydrogen survey of the sky south -25°. A total 50980 positions lying galactic coordinate grid with points spaced by ( l, b) = (05/cos b, 05), were observed 30 m dish Instituto Argentino de Radioastronomía (IAR). The angular resolution is HPBW 30', and velocity coverage spans interval -450 to +400 (LSR). 1.27 final rms noise entire database ~ 0.07 K. brightness temperature scale accurate 5%.
We describe the equipment, observational method and reduction procedure of an absolutely calibrated radio continuum survey South Celestial Hemisphere at a frequency 1420 MHz. These observations cover area for declinations less than . The sensitivity is about 50 mK TB (full beam brightness) angular resolution (HPBW) , which matches existing northern sky same frequency.
We present briefly the LLAMA sub-mm radiotelescope, a joint project of Argentina and Brazil, being mounted in Andes, Argentina, at 4800 m altitude. Here we focus on activities that are going mostly under responsibility like high frequency receivers, parts back-end electronics, optical system telescope to bring radiation equipment needed for integration verification phase (optical holography) computation system.The main scientific applications planned dscribed. also report program with BRICS...
The Cherenkov Telescopes Array (CTA) is planned to be an Observatory for very high energy gamma ray astronomy and will consist of several tens telescopes which account a reflective surface more than 10000 m$^2$. mirrors these formed by set facets. Different technological solutions, fast cost efficient production light-weight mirror facets are under test inside the CTA Consortium. Most them involve composite structures whose behavior real observing conditions not yet fully tested. An outdoor...