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The new generation radio interferometer

Transactions of IAA RAS, issue 24, 70–74 (2012)

Keywords: VLBI interferometer, Active Galactic Nuclei, cosmology, effective area, sensitivity.

Abstract

To investigate the physical conditions in Active Galactic Nuclei (AGNs), and for cosmological studies we suggest to create a giant VLBI interferometer with the baseline > 5000 km on the basis of square kilometer phased arrays. It is shown that this interferometer will have the sensitivity ~ 1 mJy at a frequency 100 MHz. The interferometer on the basis of diffraction arrays will have the multi-beam interferometer diagram to overlap the whole half sphere of the sky.

Citation

Text

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RIS

V. S. Artyukh. The new generation radio interferometer // Transactions of IAA RAS. — 2012. — Issue 24. — P. 70–74.

@article{artyukh2012,
  abstract = {To investigate the physical conditions in Active Galactic Nuclei (AGNs), and for cosmological studies we suggest to create a giant VLBI interferometer with the baseline > 5000 km on the basis of square kilometer phased arrays. It is shown that this interferometer will have the sensitivity ~ 1 mJy at a frequency 100 MHz. The interferometer on the basis of diffraction arrays will have the multi-beam interferometer diagram to overlap the whole half sphere of the sky.},
  author = {V.~S. Artyukh},
  issue = {24},
  journal = {Transactions of IAA RAS},
  keyword = {VLBI interferometer, Active Galactic Nuclei, cosmology, effective area, sensitivity},
  pages = {70--74},
  title = {The new generation radio interferometer},
  url = {http://iaaras.ru/en/library/paper/827/},
  year = {2012}
}

TY  - JOUR
TI  - The new generation radio interferometer
AU  - Artyukh, V. S.
PY  - 2012
T2  - Transactions of IAA RAS
IS  - 24
SP  - 70
AB  - To investigate the physical conditions in Active Galactic Nuclei
(AGNs), and for cosmological studies we suggest to create a giant
VLBI interferometer with the baseline > 5000 km on the basis of
square kilometer phased arrays. It is shown that this interferometer
will have the sensitivity ~ 1 mJy at a frequency 100 MHz. The
interferometer on the basis of diffraction arrays will have the
multi-beam interferometer diagram to overlap the whole half sphere of
the sky.
UR  - http://iaaras.ru/en/library/paper/827/
ER  -