State-of-the-art VLBI imaging: 3C345
1991 ◽
Vol 131
◽
pp. 354-357
Keyword(s):
AbstractMost VLBI images have low dynamic range because they are limited by instrumental effects such as calibration errors and poor u, v-coverage. We outline the method used to make a new image of the bright quasar 3C345 which has very high dynamic range (peak-to-noise of 5000:1) and which is limited by the thermal noise, not instrumental errors. Both the Caltech VLBI package and the NRAO AIPS package were required to manipulate the data.
2018 ◽
Vol 30
(6)
◽
pp. 1015
Keyword(s):
2019 ◽
Vol 34
(07)
◽
pp. 2059025
Keyword(s):
Keyword(s):
1998 ◽
Vol 45
(3)
◽
pp. 724-727
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2018 ◽
Vol 2018
(5)
◽
pp. 311-1-311-8
◽
2009 ◽
Vol 28
(8)
◽
pp. 2343-2367
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Keyword(s):
Keyword(s):