Spektr-RG

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.

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.

On July 13, 2019, Proton rocket launcher with DM-03 booster blasted off from Baikonur cosmodrome, carrying Russian X-ray observatory Spektr-RG. Today, we name some — but by no means the only — fascinating results of its work in these five years.

The new catalogue includes more than one and a half thousand objects. Mikhail Pavlinsky ART-XC telescope is one of the two instruments aboard Russian Spektr-RG space observatory, currently working in L2 point.

SN2024ggi, a II-type supernova, was first found on April 11, 2024 by ATLAS project team. It sits in a nearby galaxy NGC3621. Mikhail Pavlinsky ART-XC telescope onboard Spektr-RG observatory was the first to register its X-ray emission.

After the first few days of observations a new X-ray source turned out to be a pulsar in a binary system with a low-mass companion.