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A Deep VLA Search for a Persistent Radio Counterpart to the One-off FRB 20250316A

Tao An, Ailing Wang, Yu-Chen Huang et al., 2025. The Astrophysical Journal Letters 991(1), L20.

FRB 20250316A, detected by CHIME on 16 March 2025 at about 40 Mpc with a fluence of 1.7 kJy ms, has no persistent radio source to a 3-sigma limit of 8.4 microjansky at 15 GHz, more than three orders of magnitude below the compact sources around well-studied repeaters.

MYS0CVCM6RE3JKJ · mystery · click to copyMFast radio bursts and the origin of the one-off burstsArticledoi: 10.3847/2041-8213/ae0324Checked against the original0

What it's used for here

The deepest persistent-source limit for a non-repeater; disfavours bright magnetar nebulae for it.

Cited by on this site 4 records

Cite it

An, T., Wang, A., Huang, Y. C., Feng, J. P., & et al. (2025). A Deep VLA Search for a Persistent Radio Counterpart to the One-off FRB 20250316A. The Astrophysical Journal Letters 991(1), L20. https://doi.org/10.3847/2041-8213/ae0324
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