Veranstaltungen am Institut und mit Beteiligung des MPE

8752 1558092495

The Dark Matter mass function with strong gravitational lensing

Institute Seminar
5824 1558092896

"Meet the speaker''

Münchener Physik Kolloquium
We invite you to a student-only discussion-round with the speaker before his Munich Physics Colloquium talk. Be curious and feel free to ask any question. [mehr]
5401 1558092855

Optimized quantum photonics

Münchener Physik Kolloquium
7607 1558095417

AGN demography with JWST and ALMA

ESO Lunch Talk
18632 1558093272

Parker Solar Probe: Initial observations and future perspectives

IPP Seminar
7833 1558093369

Imaging Black Holes with the Event Horizon Telescope

MPP Colloquium
5828 1558095381

We're going to the Moon. I'll bring the Lego

ESO Special Talk
18787 1558095363

We're going to the Moon. I'll bring the Lego

ESO Special Talk
18788 1558095627

We're going to the Moon. I'll bring the Lego

ESO Special Talk
18789 1558095328

We're going to the Moon. I'll bring the Lego

ESO Special Talk
12462 1558095312

Stellar Models: Current Status, Main Problems and Future Directions

Stellar Coffee and Planetary Tea
1138 1557736631

Bayesian population studies of short gamma-ray bursts

Bayes Forum - Talk
Inferring the number, rate and intrinsic properties of short gamma-ray bursts has been a long studied problem in the field. As it is closely related to the number of GW events expected for neutron star mergers, the topic has begun to be discussed int he literature again. However, the utilized techniques for GRBs still rely on improper statistical modeling V/Vmax estimators and in many cases, methods made for humor alone. I will discuss the use of Bayesian hierarchical models to infer population and object level parameters of inhomogeneous-Poisson process distributed populations. Techniques to handle high-dimensional selections effects will be introduced. The methodology will then be applied to sGRB population data with the aim of understand how many of these objects there are, where they are in the Universe and what are their properties under given modeling assumptions. The methodology is general, thus extensions to other populations can be made easily. [mehr]
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