Our Research

The fourth division (BP4) of The Fundamental Research Department (Departament Badań Podstawowych) deals with research in astrophysics and astronomy, mainly their observational aspects. The BP4 division is located in Warsaw at 7 Pasteura street.

The research conducted at the Astrophysics Laboratory includes:

  • Cosmology: CMB, large structures of the Universe, dark matter, non-standard cosmology and gravitational lensing
  • Gravitational waves: Multi-messenger astronomy, new tools for cosmology
  • Physics of galaxies: Formation and evolution of galaxies, AGN, quasars and gamma-ray burst
  • Interstellar medium: Star formation, neutron stars and white dwarfs
Check our Research Fields page for more information.


The BP4 division is also involved in several international projects. Check our Scientific Projects page for more information.

 

Seminars

Upcoming seminars for all of NCBJ can be found here.

The seminar archive for NCBJ can be found here.

 

Latest News

Scroll down for the latest news about the research done by our division or click here.

Conference Participation

BP4 participate in may national and intersectional conferences. We share our cutting edge research and enthusiasm with other astronomers across the world. Below are pictures from our trips across the globe.

Latest News

Soczewkowane obrazy rozbłysku gamma mogą dochodzić do obserwatora po drogach o różnej długości (A, B). Jeśli fotony o różnych energiach podróżują z tą samą prędkością, opóźnienia między tymi samymi zmianami w wyglądzie obrazów A' i B' nie będą zależały od energii fotonów. Jeśli dla fotonów o większych energiach opóźnienie się zmieni, będzie to świadczyło, że poruszają się one z nieco inną prędkością niż fotony o mniejszych energiach. (Źródło: NCBJ)

Wyścigi fotonów pod lupą grawitacji

Fotony przemierzają Wszechświat z niezmienną prędkością. Tylko czy zawsze wszystkie z tą samą? Aby sprawdzić, czy potencjalne efekty kwantowej grawitacji nie wpływają na prędkości fotonów o bardzo dużych energiach, polsko-chiński zespół naukowców zaprzągł do pracy dwa spektakularne zjawiska kosmiczne: soczewki grawitacyjne i wybuchy promieniowania gamma.

Przykłady silnych soczewek grawitacyjnych sfotografowanych przez teleskop Hubble'a. W lewym dolnym roku wyraźny pierścień Einsteina. (Źródła: Hubble/NASA/ESA)

Artificial intelligence will track down gravity lenses

Images of distant galaxies, distorted by powerful gravitational lenses, are visually the most out-of-the-box phenomena photographed by telescopes. Their automatic detection is difficult for many reasons. During the international workshop in Warsaw, dedicated to machine learning, NCBJ scientists demonstrated theoretical models and software that deal with this task with high efficiency and reliability.

dr William James Pearson

Dr. William Pearson receives the scholarship for outstanding young scientists

"My work so far was focused on the formation and evolution of galaxies using modern machine learning methods" - explains Dr. William James Pearson of the NCBJ Astrophysics Division. Dr. Pearson received one of this year's scholarships from the Minister of Education and Science for outstanding young scientists demonstrating significant achievements in scientific activity.

Uroczystość wręczenia nagród Dyrektora DBP NCBJ za rok 2021

Awards of the Director of DBP NCBJ for scientific achievements in 2021

On June 27, the Awards of the Director of the Fundamental Research Department of NCBJ were presented for scientific achievements and popularizing activities for 2021. This year, the following were awarded: PhD. Varvara Batozskaya from the Department of High Energy Physics, prof. Marek Biesiada from the Department of Astrophysics, professors Michał Kowal and Janusz Skalski from the Department of Theoretical Physics and prof. Katarzyna Małek from the Department of Astrophysics for achievements in the area of ​​popularization.

How heavy can a graviton be?

Scientists are trying to determine the properties of the graviton – the hypothetical particle that carries the gravitational force. In a study published in the Journal of High Energy Astrophysics, based on the analysis of 12 galaxy clusters, prof. Marek Biesiada and his colleagues presented a new limit on the mass of graviton. It is seven orders of magnitude stronger than the limitations of observing gravitational waves.

Wizja artystyczna układu podwójnego składającego się z gwiazdy neutronowej i gwiazdy o masie mniejszej niż masa Słońca.

Influence of gravitational darkening on the spectrum of rotating objects

Exotic, rapidly rotating objects are of interest to astrophysicists. Polish astronomers are trying to obtain information about the physical conditions inside fast-rotating neutron stars. In a work published in The Astronomical Journal, they enriched the analysis with effects resulting from the phenomenon of gravitational darkening.