© JWTH/ASTRON
This year's students, Anouk, Ramon, Rico, and Sjoerd, analyzed 12 LOFAR pulsar observations in order to blindly discover the pulsar's rotational period and dispersion measure; refine their parameter estimation and then track the changes of the rotational period with time; and then finally use this information to model the pulsar's binary orbit and the properties of the eclipsing gas in this system.
As part of the project, the students also write-up a report on their findings and present them to their peers in Amsterdam.