Supermassive black hole 4C+35.28
Object 4C+35.28, also known RFC J1215+3448, 1213+350, 6C~1213+3504 with position
12:15:55.598593 ± 0.000003 in right ascension and +34:48:15.19900 ± 0.000055
declination at a distance of 5530 Mpc (redshift 0.857 ± 0.001) hosts two components
at separation 37 mas or 290 parsec. Most likely these are two supermassive black
holes.
Properties of 4C+35.28
Properties of 4C+25.28
High resolution radio images of 4C+35.28 synthesized with VLBI
Explanation:
- radplot means dependence of calibrated flux density on projection
of the baseline vector expressed in wavelengths
averaged over all spectral channels of a given intermediate
frequency.
- uva data means a priori calibrated visibilities.
- uvs data means a self-calibrated visibilities averaged over
all spectral channels of a given intermediate frequency
as the output of hybrid image synthesis process.
Low resolution radio images of 4C+35.28 VLBI
Source code used for processing 4C+35.28 data
Source code used for processing 4C+35.28 data.
Low resolution radio images of 4C+35.28 VLBI
List of 87 VLBA projects that target imaging dual-AGNs of bSMBH_VLBI_projects.txt
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Responsible NASA official: Leonid Petrov
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Last update: 2026.03.28_23:35:13
UTC