The Fast World Radio Telescope (FAST) Cosmic Source Survey is an ongoing project that uses the FAST radio telescope in China to study the distribution and properties of active galactic nuclei (AGN) in the local universe.
AGN are powered by supermassive black holes at the center of galaxies. They are some of the most powerful objects in the universe and are thought to play a role in regulating the growth and evolution of galaxies.
The FAST Cosmic Source Survey is studying a large sample of AGN in the local universe in order to better understand their properties and how they interact with their host galaxies. The survey will also help to identify new AGN candidates for further study.
The FAST radio telescope is the world’s largest and most sensitive radio telescope. It is located in Guizhou Province in south-western China. The FAST Cosmic Source Survey is the first major project to use the telescope.
The FAST Cosmic Source Survey is a collaboration between the National Astronomical Observatories of China (NAOC) and the University of Science and Technology of China (USTC). The project is funded by the National Basic Research Program of China (973 Program) and the National Science Foundation of China.
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What has the FAST telescope found?
The FAST telescope is a new and powerful telescope that has been recently built in China. It is the largest telescope in the world, and it has been used to find many interesting objects in space.
One of the first things that the FAST telescope found was a new type of star. This star is called a red supergiant, and it is much larger than other types of stars. The FAST telescope was also able to find a number of new galaxies. These galaxies are very distant, and they are some of the most distant galaxies that have ever been found.
The FAST telescope has also been used to study black holes. One of the most interesting things that has been found is that black holes can come in different sizes. Some black holes are very small, while others are very large. The FAST telescope has also been used to study the atmosphere of planets outside of our own solar system.
Overall, the FAST telescope has been very successful in finding new objects and learning more about them. It is clear that this telescope will continue to be a valuable tool for scientists in the future.
How does the FAST radio telescope work?
The FAST radio telescope (FAST), also known as the Five hundred meter Aperture Spherical Telescope, is a large radio telescope located in Guizhou province, China. Construction of the telescope began in March 2011 and was completed in September 2016. The telescope is the largest and most sensitive radio telescope in the world, with a diameter of 500 meters.
The FAST radio telescope is used for a variety of purposes, including astronomy, atmospheric science, and earth science. It is used to study objects in space, such as galaxies and black holes, and to study the Earth’s atmosphere and climate. The telescope is also used to study communication and navigation systems, and to search for signs of extraterrestrial life.
The FAST radio telescope is made up of 4,450 panels that together form a spherical mirror. The panels are made of metal and are supported by a steel frame. The telescope is mounted on a platform that can rotate to aim the telescope at different objects in the sky.
The FAST radio telescope is powered by a 12,000 kilowatt generator. The telescope is cooled by a liquid nitrogen system that circulates liquid nitrogen through the panels to keep them cool.
The FAST radio telescope is a very large and sensitive instrument. It is able to detect very weak signals from space that are not detectable by other radio telescopes. The telescope is also able to detect signals from a wide range of frequencies, from 0.1 to 80 GHz.
Where is the most powerful radio telescope?
The most powerful radio telescope is located at the Arecibo Observatory in Puerto Rico. The telescope is 305 meters in diameter and has a collecting area of 18,000 square meters. It is used for a variety of research, including the study of pulsars, quasars, and the interstellar medium.
Where is the FAST radio telescope?
The Fast Radio Telescope (FAST), located in the Dawodang depression in the Guizhou Province of China, is the world’s largest and most sensitive radio telescope. It is also the most expensive, having cost 1.2 billion yuan (US$180 million) to build.
The FAST telescope is made up of 4,450 panels, each of which is made up of 11 antennas. The antennas are arranged in a Y-shape, with each arm of the Y measuring about 500 meters long. The telescope can scan the entire sky in just five minutes.
The FAST telescope is used to study pulsars, quasars, and other objects in space. It is also being used to study the distribution of dark matter and dark energy in the universe.
What is the biggest antenna in the world?
The biggest antenna in the world is the Arecibo Observatory, which is located in Puerto Rico. It is also the largest single-dish radio telescope in the world, with a diameter of 305 meters. The observatory was constructed in the early 1960s, and it has been used for a variety of research projects over the years.
Where is the world’s biggest satellite dish?
The world’s biggest satellite dish is located in China. It is known as the Beijing Earth Station and has a diameter of 45 meters. It is used to receive satellite transmissions from all over the world.
How far can a radio telescope see?
Radio telescopes are used to detect and study radio waves from space. They are different from optical telescopes, which detect and study visible light. Radio waves are much longer than visible light waves, and can travel through much more of the universe than visible light.
Radio telescopes can see much further than optical telescopes. They can detect radio waves from objects that are billions of light-years away. This is because the universe is expanding, and the further away an object is, the faster it is moving away from us. The expansion of the universe stretches the radio waves from these objects, making them longer and easier to detect.
Radio telescopes can also see objects that are hidden behind thick clouds of gas and dust. Optical telescopes can’t see through these clouds, but radio telescopes can. This is because radio waves can pass through these clouds more easily than visible light waves.
Despite their great distance, radio telescopes don’t always see objects in great detail. This is because the strength of the radio waves that they detect decreases the further away the object is. This means that the further away an object is, the less information we have about it.