Milliarcsecond Localization of the Repeating FRB 20201124A
Artikel i vetenskaplig tidskrift, 2022
Very long baseline interferometric (VLBI) localizations of repeating fast radio bursts (FRBs) have demonstrated a diversity of local environments: from nearby star-forming regions to globular clusters. Here we report the VLBI localization of FRB 20201124A using an ad hoc array of dishes that also participate in the European VLBI Network (EVN). In our campaign, we detected 18 bursts from FRB 20201124A at two separate epochs. By combining the visibilities from both epochs, we were able to localize FRB 20201124A with a 1 sigma uncertainty of 2.7 mas. We use the relatively large burst sample to investigate astrometric accuracy and find that for greater than or similar to 20 baselines (greater than or similar to 7 dishes) we can robustly reach milliarcsecond precision even using single-burst data sets. Subarcsecond precision is still possible for single bursts, even when only similar to 6 baselines (four dishes) are available. In such cases, the limited uv coverage for individual bursts results in very high side-lobe levels. Thus, in addition to the peak position from the dirty map, we also explore smoothing the structure in the dirty map by fitting Gaussian functions to the fringe pattern in order to constrain individual burst positions, which we find to be more reliable. Our VLBI work places FRB 20201124A 710 +/- 30 mas (1 sigma uncertainty) from the optical center of the host galaxy, consistent with originating from within the recently discovered extended radio structure associated with star formation in the host galaxy. Future high-resolution optical observations, e.g., with Hubble Space Telescope, can determine the proximity of FRB 20201124A's position to nearby knots of star formation.
Författare
K. Nimmo
Netherlands Institute for Radio Astronomy (ASTRON)
Universiteit Van Amsterdam
D. M. Hewitt
Universiteit Van Amsterdam
J. W. T. Hessels
Netherlands Institute for Radio Astronomy (ASTRON)
Universiteit Van Amsterdam
Franz Kirsten
Netherlands Institute for Radio Astronomy (ASTRON)
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
B. Marcote
Joint Institute for VLBI in Europe (JIVE)
U. Bach
Max-Planck-Gesellschaft
R. Blaauw
Netherlands Institute for Radio Astronomy (ASTRON)
M. Burgay
INAF Osservatorio Astronomico di Cagliari
A. Corongiu
INAF Osservatorio Astronomico di Cagliari
R. Feiler
Uniwersytet Mikolaja Kopernika
M. P. Gawronski
Uniwersytet Mikolaja Kopernika
M. Giroletti
Istituto nazionale di astrofisica (INAF)
R. Karuppusamy
Max-Planck-Gesellschaft
A. Keimpema
Joint Institute for VLBI in Europe (JIVE)
M. A. Kharinov
Russian Academy of Sciences
Michael Lindqvist
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
G. Maccaferri
Istituto nazionale di astrofisica (INAF)
A. Melnikov
Russian Academy of Sciences
A. Mikhailov
Russian Academy of Sciences
O. S. Ould-Boukattine
Universiteit Van Amsterdam
Z. Paragi
Joint Institute for VLBI in Europe (JIVE)
M. Pilia
INAF Osservatorio Astronomico di Cagliari
A. Possenti
INAF Osservatorio Astronomico di Cagliari
M. P. Snelders
Universiteit Van Amsterdam
G. Surcis
INAF Osservatorio Astronomico di Cagliari
M. Trudu
INAF Osservatorio Astronomico di Cagliari
T. Venturi
Istituto nazionale di astrofisica (INAF)
Wouter Vlemmings
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
N. Wang
Chinese Academy of Sciences
Jun Yang
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
J. Yuan
Chinese Academy of Sciences
Astrophysical Journal Letters
2041-8205 (ISSN) 2041-8213 (eISSN)
Vol. 927 1 L3Ämneskategorier
Astronomi, astrofysik och kosmologi
Annan fysik
Multidisciplinär geovetenskap
DOI
10.3847/2041-8213/ac540f