Seminarium Zakładu Astrofizyki

The rapidly rotating neutron stars can be source of gravitational waves. I will present the methods used to find almost monochromatic signals detected by ground-base gravitation waves detectors.

The pipeline F-statistics used by our group, and pipelines other groups. The talk will describe a present stage and what to expect in close future.

Microlensing has become a powerful method to detect extrasolar planets beyond the snowline and free-floating planets. In this talk, I will first discuss the basic concepts of gravitational microlensing, then review some of the recent progress and finally discuss the future outlook.