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GMVA observed proposals for the 40m telescope in 2022
Year stands for the year when the proposal was submitted. Session stands for the observing session. Proposals are usually observed 9 months after submission and they may be splitted and observed in several sessions.
Proposal ID |
Proposal Code |
Year |
Session |
PI |
Title |
20B-145 |
MM018 |
2020 |
2022A |
MacDonald |
Disorder vs. Order: Discerning the nature
of the magnetic field in PKS 1510-089 |
20B-204 |
MK015 |
2020 |
2022A |
Kim |
First subparsec-scale imaging of the
new TeV gamma-ray radio galaxy 3C 264 |
20B-220 |
ML010 |
2020 |
2022A |
Lu |
Jet Meets Black Hole in M87: Breaking New Ground with GMVA+ALMA |
20B-269 |
MI003 |
2020 |
2022A |
Issaoun |
Sharpening the Source Model for Sgr A* with GMVA+ALMA |
21A-209 |
MP002 |
2021 |
2021B, 2022A |
Paraschos |
Where is the black hole in 3C84 located? |
21A-233 |
MB016 |
2021 |
2021B, 2022A |
Baczko |
Resolving the twin-jet base in NGC 1052 |
21B-078 |
MP003 |
2021 |
2022A |
Park |
Is shear acceleration at work in the jets of NGC 315?
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21B-162 |
MG009 |
2021 |
2022A |
Gomez |
Imaging massive binary black hole candidate OJ287 with the GMVA+ALMA
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21B-164 |
MT002 |
2021 |
2021B, 2022A |
Traianou |
Moving and stationary shocks interaction
after a gamma-ray flare in TXS2013+370
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22A-361 |
MR013 |
2021 |
2022B |
Roesch |
GMVA Highest-Resolution Imaging of Radio Flaring Doppler-Crisis Blazars |
22A-410 |
MK021 |
2021 |
2022A |
Koyama |
Resolving the jet collimation region in TeV blazar Mrk 501 |
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