Has a Deep Field Picture of the Sky Been Captured with a Radio Telescope?

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SUMMARY

The discussion centers on the capabilities of radio telescopes for capturing deep field images of the sky, comparing the Five-hundred-meter Aperture Spherical Telescope (FAST) and the Square Kilometre Array (SKA). While FAST excels in pulsar detection due to its larger aperture, it is limited in deep sky observations due to its single-location design and zenith restrictions. In contrast, the SKA, with its distributed aperture and long baseline interferometer capabilities, is positioned to achieve significantly higher resolution for deep sky imaging. The challenges of man-made interference and noise floor are also highlighted as critical factors affecting image quality.

PREREQUISITES
  • Understanding of Very Long Baseline Interferometry (VLBI)
  • Familiarity with radio telescope technology, specifically FAST and SKA
  • Knowledge of signal processing techniques for radio astronomy
  • Awareness of the impact of man-made interference on astronomical observations
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  • Research the operational principles of Very Long Baseline Interferometry (VLBI)
  • Explore the capabilities and design of the Square Kilometre Array (SKA)
  • Study the effects of noise floor on radio astronomical imaging
  • Investigate the advancements in signal processing for radio telescopes
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Astronomers, astrophysicists, and researchers in radio astronomy, particularly those focused on deep sky observations and the technological advancements in radio telescope capabilities.

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Has anyone ever taken a "deep field" picture of the sky, like Hubble, but with a radio telescope?
 
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Some of the early radio astronomical survey mapping was done by telescopes like "Big Ear" in the North, or by the Mills Cross in the South.
https://en.wikipedia.org/wiki/Ohio_State_University_Radio_Observatory
https://en.wikipedia.org/wiki/Mills_Cross_Telescope

To get deeper detailed images of smaller areas, requires VLBI, with international collaboration. The construction of detailed radio images, from the VLBI time data, requires intensive numerical processing. An optical image can be accumulated, on an image sensor array, which is a faster parallel process.
 
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Baluncore said:
To get deeper detailed images of smaller areas, requires VLBI, with international collaboration. The construction of detailed radio images, from the VLBI time data, requires intensive numerical processing. An optical image can be accumulated, on an image sensor array, which is a faster parallel process.
All that exists at FAST but all publications I could find from them were pulsars and FRB and again pulsars, i.e. only the sources that were very bright for the telescope. I wonder whether this is for a reason or due to the relatively young age of FAST.
 
fresh_42 said:
All that exists at FAST but all publications I could find from them were pulsars and FRB and again pulsars, i.e. only the sources that were very bright for the telescope.
Deep sky observations require high sensitivity and high resolution. Unfortunately, man-made interference, and nearby bright sources, raise the noise floor of the synthesised images.

The Five-hundred-meter Aperture Spherical radio Telescope (FAST), operating alone, is a single location observatory. Resolution is limited by the 500 metre diameter. FAST finds more pulsars because it has a larger aperture area, and therefore has higher sensitivity than earlier observatories. It can make point measurements, where the signal is the sum of all the beam energy. That is suited to strong signals, or pulsar observations, not deep sky.
https://en.wikipedia.org/wiki/Five-hundred-meter_Aperture_Spherical_Telescope

The Square Kilometre Array (SKA) has a distributed aperture, so should have over 1000 times the resolution of FAR, since SKA is designed to operate as a long baseline interferometer. That would be more suited to deep sky observations, if you can find and fund the computer time.
https://en.wikipedia.org/wiki/Square_Kilometre_Array

FAST is located at about 26° North, and zenith limited, so is restricted to the northern sky. It is not as steerable as the elements of the SKA.
The SKA is based in Africa and Australia, with many more steerable elements. It is better positioned to observe the southern sky with the best view of the Milky Way.
 
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Thank you. That is just what I was looking for.
 
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