Explanation:

Fast Radio Burst (FRB)

• The first FRB was discovered in 2007, since when scientists have been working towards finding the source of their origin. 
• The FRBs are bright bursts of radio waves (radio waves can be produced by astronomical objects with changing magnetic fields) whose durations lie in the millisecond-scale, because of which it is difficult to detect them and determine their position in the sky.
• FRB detected recently:
• The source of the FRB detected recently in the Milky Way is a very powerful magnetic neutron star, referred to as a magnetar, called SGR 1935+2154 or SGR 1935.
• The FRB was part of one of the magnetar’s most prolific flare-ups, with the X-ray bursts lasting less than a second. 
• The radio burst, on the other hand, lasted for a thousandth of a second and was thousands of times brighter than any other radio emissions from magnetars seen in the Milky Way previously. 
• It is possible that the FRB-associated burst was exceptional because it likely occurred at or close to the magnetar’s magnetic pole.

Hence both statements are correct.