| NCBJ

Future Opportunities of Lignin derived Advanced Materials

https://meet.goto.com/NCBJmeetings/nomaten-seminar

30 Apr, 2024 - 30 Apr, 2024

Seria: NOMATEN Online Seminar Prelegent: Dr. Maurice Collins, University of Limerick, Ireland Data: April 30th, 2024

Akcelerator AQURE FLASH (RT). Źródło: NCBJ

Accelerator in search of new cancer therapies

24-04-2024

The FLASH therapy may be a promising method of destroying tumours while better preserving healthy cells. An accelerator built at the NCBJ is already supporting research into this treatment modality at the Wielkopolska Oncology Centre.

Apr

2024

Professor | BP2

Termin zbierania ofert: 17-05-2024

The Theoretical Physics Division opens the competition for the position of professor.

Exploring the Low Surface Brightness Galaxies in Abell 194 with Transfer Learning

room 207, Pasteura 7 / https://www.gotomeet.me/NCBJmeetings/phd-seminar / https://events.ncbj.gov.pl/e/Seminar_23_24

25 Apr, 2024 - 25 Apr, 2024

Seria: Seminarium Szkoły Doktorskiej NCBJ Prelegent: Hareesh Thuruthipilly (Szkoła Doktorska NCBJ) Data: Thursday, 25 April 2024, 9:15

Konkurs MAPS - wielostronna współpraca badawcza pomiędzy Bułgarią, Chorwacją, Węgrami, Polską, Rumunią i Szwajcarią

Finansowanie: Inne

14 Apr, 2024 - 01 Jul, 2024

The Swiss National Science Foundation (SNSF) announced the MAPS (Multilateral Academic Projects) call for multilateral research projects implemented by scientists from Switzerland in collaboration with teams from Poland, Bulgaria, Croatia, Hungary and Romania. Applications can be submitted until the end of June 2024. Polish teams in the MAPS call for proposals will be financed from the Swiss-Polish Cooperation Programme, which is part of the second Swiss financial support for selected EU member states.

Ten krajobraz "gór" i "dolin" usianych gwiazdami to w rzeczywistości krawędź pobliskiego, młodego regionu gwiazdotwórczego o nazwie NGC 3324 w Mgławicy Carina. Uchwycony w świetle podczerwonym przez Kosmiczny Teleskop Jamesa Webba, obraz ten po raz pierwszy ujawnia niewidoczne wcześniej obszary narodzin gwiazd. Źródło: NASA, ESA, CSA, STScI

Can dust evaporate in harsh interstellar environments?

24-04-2024

Dust represents an important component of the interstellar medium of galaxies and is involved in various physical processes. As a consequence, it is crucial to understand the factors that influence its formation and destruction. In a recent study, a team of scientists led by dr Ambra Nanni of the NCBJ’s Astrophysics Division analysed the effect of photo-evaporation on the survival of dust in the interstellar medium of galaxies.

Dwarf galaxies in deep-wide surveys: a new frontier in the study of galaxy evolution

ul. Pasteura 7, sala 404 / https://meet.goto.com/NCBJmeetings/seminarium-astrofizyczne

23 Apr, 2024 - 23 Apr, 2024

Seria: Seminarium Astrofizyczne Prelegent: Sugata Kaviraj (Centre for Astrophysics Research, University of Hertfordshire, UK) Data: wtorek 23.04.2024 godz. 12:30

EagleEye - pierwszy zaprojektowany i zbudowany w Polsce satelita o masie powyżej 50 kg. W tym roku satelita zostanie wyniesiony na orbitę okołoziemską. Źródło: Creotech Instruments S.A.

Will the electronics in EagleEye survive the space mission? NCBJ scientists conducted radiation tests of microsatellite systems

19-04-2024

Electronic systems that are part of space missions are exposed to ionising radiation, which can cause errors or even permanent damage to the entire system. For this reason, it is important to select components with adequate radiation resistance. In NCBJ, tests were carried out on systems to be used in the Polish EagleEye microsatellite.

Efficient data analysis and fatigue life prediction using nCode software

sala 172, bud. 39 (Cyfronet, III piętro) / https://www.gotomeet.me/NCBJmeetings/uz3-and-phd4gen-seminars

23 Apr, 2024 - 23 Apr, 2024

Seria: Seminarium Zakładu Energetyki Jądrowej i Analiz Środowiska (UZ3) Prelegent: Dipl.-Ing. Thomas Kemmerich HBK Data: 23.04.2024, godz. 11:30

Investigating the Redshift Evolution of Lensing Galaxy Density Slope via Model-Independent Distance Ratios