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The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite began surveying the sky in December 2019, with the aim of producing all-sky X-ray source lists and sky maps of an unprecedented depth. Here we present catalogues…

High Energy Astrophysical Phenomena · Physics 2024-01-31 A. Merloni , G. Lamer , T. Liu , M. E. Ramos-Ceja , H. Brunner , E. Bulbul , K. Dennerl , V. Doroshenko , M. J. Freyberg , S. Friedrich , E. Gatuzz , A. Georgakakis , F. Haberl , Z. Igo , I. Kreykenbohm , A. Liu , C. Maitra , A. Malyali , M. G. F. Mayer , K. Nandra , P. Predehl , J. Robrade , M. Salvato , J. S. Sanders , I. Stewart , D. Tubín-Arenas , P. Weber , J. Wilms , R. Arcodia , E. Artis , J. Aschersleben , A. Avakyan , C. Aydar , Y. E. Bahar , F. Balzer , W. Becker , K. Berger , T. Boller , W. Bornemann , M. Brüggen , M. Brusa , J. Buchner , V. Burwitz , F. Camilloni , N. Clerc , J. Comparat , D. Coutinho , S. Czesla , S. M. Dannhauer , L. Dauner , T. Dauser , J. Dietl , K. Dolag , T. Dwelly , K. Egg , E. Ehl , S. Freund , P. Friedrich , R. Gaida , C. Garrel , V. Ghirardini , A. Gokus , G. Grünwald , S. Grandis , I. Grotova , D. Gruen , A. Gueguen , S. Hämmerich , N. Hamaus , G. Hasinger , K. Haubner , D. Homan , J. Ider Chitham , W. M. Joseph , A. Joyce , O. König , D. M. Kaltenbrunner , A. Khokhriakova , W. Kink , C. Kirsch , M. Kluge , J. Knies , S. Krippendorf , M. Krumpe , J. Kurpas , P. Li , Z. Liu , N. Locatelli , M. Lorenz , S. Müller , E. Magaudda , C. Mannes , H. McCall , N. Meidinger , M. Michailidis , K. Migkas , D. Muñoz-Giraldo , B. Musiimenta , N. T. Nguyen-Dang , Q. Ni , A. Olechowska , N. Ota , F. Pacaud , T. Pasini , E. Perinati , A. M. Pires , C. Pommranz , G. Ponti , K. Poppenhaeger , G. Pühlhofer , A. Rau , M. Reh , T. H. Reiprich , W. Roster , S. Saeedi , A. Santangelo , M. Sasaki , J. Schmitt , P. C. Schneider , T. Schrabback , N. Schuster , A. Schwope , R. Seppi , M. M. Serim , S. Shreeram , E. Sokolova-Lapa , H. Starck , B. Stelzer , J. Stierhof , V. Suleimanov , C. Tenzer , I. Traulsen , J. Trümper , K. Tsuge , T. Urrutia , A. Veronica , S. G. H. Waddell , R. Willer , J. Wolf , M. C. H. Yeung , A. Zainab , F. Zangrandi , X. Zhang , Y. Zhang , X. Zheng

The eROSITA X-ray telescope on board the Spectrum-Roentgen-Gamma (SRG) spacecraft observed the field of the UKIDSS Ultra-Deep Survey (UDS) in August-September 2019, during its flight to Sun-Earth L2 point. The resulting eROSITA UDS (or…

High Energy Astrophysical Phenomena · Physics 2024-01-22 R. Krivonos , M. Gilfanov , P. Medvedev , S. Sazonov , R. Sunyaev

The eROSITA instrument aboard the Spectrum Roentgen Gamma (SRG) satellite has performed its first all-sky survey between December 2019 and June 2020. This paper presents the resulting hard X-ray (2.3-5 keV) sample, the first created from an…

High Energy Astrophysical Phenomena · Physics 2026-02-11 Sophia G. H. Waddell , J. Buchner , K. Nandra , M. Salvato , A. Merloni , I. Gauger , Th. Boller , R. Seppi , J. Wolf , T. Liu , M. Brusa , J. Comparat , T. Dwelly , Z. Igo , B. Musiimenta

Context. The eROSITA X-ray telescope on board the Spectrum-Roentgen-Gamma (SRG) observatory combines a large field of view and collecting area in the energy range $\sim$0.2 to $\sim$8.0 keV with the capability to perform uniform scanning…

By June of 2020, the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum Roentgen Gamma observatory had completed its first of the planned eight X-ray all-sky survey (eRASS1). The large effective area of…

eROSITA is the soft X-ray instrument aboard the Spectrum Roentgen Gamma (SRG) satellite that is most sensitive in the energy range between 0.2 and 2.3 keV. Between December 2019 and December 2021, eROSITA completed four all-sky surveys…

High Energy Astrophysical Phenomena · Physics 2025-01-09 S. Friedrich , C. Maitra , K. Dennerl , A. Schwope , K. Werner , B. Stelzer

eROSITA, launched on 13 July 2019, will be completing the first all-sky survey in the soft and medium X-ray band in nearly three decades. This 4-year survey, finishing in late 2023, will present a rich legacy for the entire astrophysics…

The eROSITA X-ray telescope on board the Spectrum-Roentgen-Gamma (SRG) satellite has started to detect new X-ray sources over the full sky at an unprecedented rate. Understanding the performance and selection function of the source…

eROSITA is the primary instrument on the Russian SRG mission. In the first four years of scientific operation after its launch, foreseen for 2014, it will perform a deep survey of the entire X-ray sky. In the soft X-ray band (0.5-2 keV),…

With its first All-Sky Survey (eRASS1), the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum-Roentgen-Gamma (SRG) mission has offered an unprecedented, comprehensive view of the variable X-ray sky.…

High Energy Astrophysical Phenomena · Physics 2025-08-06 Th. Boller , M. Salvato , J. Buchner , M. Freyberg , F. Haberl , C. Maitra , A. Schwope , J. Robrade , S. Rukdee , A. Rau , I. Grotova , S. Waddell , Q. Ni , M. Krumpe , A. Georgakakis , A. Merloni , K. Nandra

The soft X-ray telescope on board the Spectrum-Roentgen-Gamma (SRG) mission, eROSITA (extended ROentgen Survey with an Imaging Telescope Array), has produced the largest sample to date of galaxy groups and clusters detected via their…

eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the primary instrument on the Spectrum-Roentgen-Gamma (SRG) mission, which was successfully launched on July 13, 2019, from the Baikonour cosmodrome. After the…

We present the first look at the spectral and timing analysis of Narrow-Line Seyfert 1 Galaxies (NLS1s) with the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum-Roentgen-Gamma (SRG) mission. The…

High Energy Astrophysical Phenomena · Physics 2023-01-04 G. Grünwald , Th. Boller , S. Rakshit , J. Buchner , T. Dauser , M. Freyberg , T. Liu , M. Salvato , A. Schichtel

The first eROSITA all-sky survey (eRASS1) performed on board the Spectrum-Roentgen-Gamma mission (SRG) provides more than 900,000 X-ray sources in the 0.2 - 2.3 keV band located in the western hemisphere. We present identifications of the…

Solar and Stellar Astrophysics · Physics 2024-01-31 S. Freund , S. Czesla , P. Predehl , J. Robrade , M. Salvato , P. C. Schneider , H. Starck , J. Wolf , J. H. M. M. Schmitt

X-ray surveys are well suited to detect, identify and study young stars based on their high levels of magnetic activity and thus X-ray brightness. The eROSITA instrument onboard the Spectrum-Roentgen-Gamma (SRG) satellite will perform an…

Solar and Stellar Astrophysics · Physics 2016-02-03 Jan Robrade

The first SRG/eROSITA all-sky X-ray survey, eRASS1, resulted in a catalogue of over twelve thousand optically-confirmed galaxy groups and clusters in the western Galactic hemisphere. Using the eROSITA images of these objects, we measure and…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-19 J. S. Sanders , Y. E. Bahar , E. Bulbul , V. Ghirardini , A. Liu , N. Clerc , M. E. Ramos-Ceja , T. H. Reiprich , F. Balzer , J. Comparat , M. Kluge , F. Pacaud , X. Zhang

The 140 square degree Final Equatorial-Depth Survey (eFEDS) field, observed with the extended ROentgen Survey with an Imaging Telescope Array (eROSITA) aboard the Spectrum-Roentgen-Gamma (SRG) mission, provides a first look at the variable…

High Energy Astrophysical Phenomena · Physics 2022-05-18 Th. Boller , J. H. M. M. Schmitt , J. Buchner , M. Freyberg , A. Georgakakis , T. Liu , J. Robrade , A. Merloni , K. Nandra , A. Malyali , M. Krumpe , M. Salvato , T. Dwelly

Context: After the successful launch of the Spectrum-Roentgen-Gamma (SRG) mission in July 2019, eROSITA, the soft X-ray instrument aboard SRG, performed scanning observations of a large contiguous field, namely the eROSITA Final Equatorial…

We present the results of the first X-ray all-sky survey (eRASS1) performed by the eROSITA instrument onboard the Spectrum-Roentgen-Gamma (SRG) mission on X-ray emitting red giants and supergiants. Focussing on stars positioned at high…

Solar and Stellar Astrophysics · Physics 2024-07-31 J. H. M. M. Schmitt , M. Hünsch , P. C. Schneider , S. Freund , S. Czesla , J. Robrade , A. Schwope

Characterising galaxy cluster populations from catalog of sources selected in astronomical surveys requires knowledge of sample incompleteness, known as selection function. The first All-Sky Survey (eRASS1) by eROSITA onboard Spectrum…

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