Spektr-RG

It was not a joke: on the first day of the month the number of energetic solar protons near the Lagrange point L2 increased significantly to around 14 counts per second. This was almost 7 times higher than usual background, registered by ART-XC detectors, and the most prominent rise in 5 years of monitoring Sun's activity.

The team of astrophysicists from IKI and other organizations used X-ray data collected by SRG/eROSITA telescope onboard Spektr-RG observatory to look into the hot interior of the S147/Spaghetti nebula and explain its unusual properties.

On December 25, 2024, delegation of cosmonauts and specialists from Yu. A. Gagarin Research & Test Cosmonaut Training Center visited IKI.

In 2024, IKI scientists and their colleagues completed the analysis of the data from the Milky Way central region deep survey and the first five all-sky surveys (2019–2022) made by Mikhail Pavlinsky ART-XC telescope onboard Spektr-RG X-ray observatory.

Marcel Grossmann institutional award for the Spektrum-Roentgen-Gamma (SRG) mission was presented to IKI at the opening of the "High-Energy Astrophysics Today and Tomorrow" conference on December 23, 2024

New model developed by IKI astrophysicists and their colleagues and based on the data of SRG/eROSITA X-ray telescope, links the bright structure seen in our Galaxy to bubbles of hot gas that emerge from star-formation regions like smoke from the chimney.

The Prime Minister of Russia, Mikhail Mishustin presented Government science and technology awards on November 27, 2024.

Academician Gennady Krasnikov, president of the Russian Academy of Sciences, visited IKI in praise of the 5th anniversary of Spektr-RG launch.