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.

Telescope Success

JWST

Darko Donevski and Giuliano Lorenzon from the Astrophysics Department BP4 - National Centre for Nuclear Research have been awarded, as co-investigators, 13 hours of time on the largest space instrument - James Webb Space Telescope (JWST). They participated in the highly competitive Cycle 4 JWST proposal competition, which received a total of 2377 submissions. The project, led by Prof. A. Man (UBC Vancouver), aims to obtain the deepest-ever mid-infrared spectroscopy of a brightest cluster galaxy at z = 0.4. Darko and Giuliano will contribute to interpreting the interplay between warm and cold dust emission in this exceptional system, which harbours one of the most extended reservoirs of dust and gas observed to date.

Grant Success

NAWA Bekker

Congratulations to Margherita Grespan, a PhD candidate from the Astrophysics Department, who has been awarded the Bekker NAWA Fellowship! Over the next two years, she will join Oxford University’s Department of Physics to conduct research on anomaly detection in astronomical surveys, leveraging advanced machine learning techniques, including active learning. Her work will focus on uncovering rare phenomena, such as strong gravitational lenses, within the vast datasets produced by new-generation telescopes such as Euclid and Vera C. Rubin.

Also congratulations to Dr. Darko Donevski, who also received a Bekker NAWA Fellowship. Over the next 18 months, Dr. Darko Donevski will be conducting visiting research with the Astrophysics Group at SISSA (Trieste, Italy). He will lead a project exploring dust re-formation in galaxies that undergo strong outflows of gas. The project will combine theoretical approaches with cutting-edge data from the James Webb and Euclid space telescopes, as well as data from large ground-based observatories such as JCMT, ALMA and NOEMA, where Dr. Darko Donevski serves as PI or co-PI.

NCN OPUS

Congratulations to Kasia Małek, who received the OPUS 27 grant! The project is of course focused on dust: "DUSTiny: dust influence on galaxy properties in new generation surveys." (CLICK HERE for more info) Soon, we will open the call for a postdoc and a PhD; stay tuned!

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 over the last year or so.

Latest News

POLAR-2 at the POLSA conference

W dniach 23-24 listopada odbędzie się konferencja „O Lemie i kosmosie” organizowana przez Polską Agencję Kosmiczną POLSA.  Dr Adam Zadrożny oraz mgr inż. Dominik Rybka – naukowcy z Narodowego Centrum Badań Jądrowych, będą mówić na niej o międzynarodowym projekcie POLAR-2 i polskim wkładzie w tę misję.

Ilustracja wielkości i rodzajów obiektów obserwowanych przez konsorcjum LVK

LIGO and Virgo extend the catalog of gravitational waves

In the data from the third observatory campaign of Advanced-LIGO and Advanced-Virgo observatories (from November 2019 to March 2020), another 35 sources of gravitational waves were found, thus extending their list to 90 objects. 32 sources come from the merger of two black holes, and 3 from the merger of the black hole system with a neutron star.  Scientists from the NCBJ Astrophysics Department are participating in the work of the LVK consortium.

plakat dnia ciemnej materii

Dark Matter Day

Serdecznie zapraszamy do wzięcia udziału w tegorocznym spotkaniu online, które odbędzie się 28 października i wysłuchania wykładów popularnonaukowych na temat ciemnej materii przygotowanych m. in. przez pracowników NCBJ.

Mapa nieba z zaznaczonymi obszarami objętymi w ramach katalogu HELP

HELP – a modern and standardized catalog of extra-galactic objects

An international team of scientists has provided scientists and enthusiasts with the most complete catalog of extragalactic objects to date, covering an area of ​​over 3% of the full angle of the sky’s solid and containing 170 million sources. The modeling of their energy spectra was the responsibility of Ph. D. Katarzyna Małek from the NCBJ Astrophysics Department.

Laureaci Nagród Dyrektora DBP

Awards of the DBP Director were awarded

The Committee of the Director of the Fundamental Research Department Award has announced the list of this year's winners. For scientific achievements in 2020, equal prizes were awarded to: professor Lech Szymanowski, Dr. hab. Paweł Bielewicz and Dr. Artur Ukleja. Dr. Anna Durkalec received the award for popularizing activities. Congratulations to the winners!

Zdjęcie przedstawia najgłębszy obraz LOFAR-a, jaki kiedykolwiek wykonano, w rejonie nieba zwanym "Elais-N1".

Obrazy radiowe młodego Wszechświata

Międzynarodowy zespół astronomów, w którego składzie znajdują się także naukowcy z Polski, opublikował w czasopiśmie "Astronomy and Astrophysics" najdokładniejszą w historii mapę Wszechświata w zakresie niskich częstotliwości radiowych. Mapę stworzono dzięki europejskiej sieci odbiorników LOFAR. Naukowcy wykryli m.in. słabe poświaty radiowe od gwiazd, które eksplodowały jako supernowe w dziesiątkach tysięcy galaktyk.