The eROSITA X-ray telescope on SRG

Abstract

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 commissioning of the instrument and a subsequent calibration and performance verification phase, eROSITA started a survey of the entire sky on December 13, 2019. By the end of 2023, eight complete scans of the celestial sphere will have been performed, each lasting six months. At the end of this program, the eROSITA all-sky survey in the soft X-ray band (0.2--2.3\,keV) will be about 25 times more sensitive than the ROSAT All-Sky Survey, while in the hard band (2.3--8\,keV) it will provide the first ever true imaging survey of the sky. The eROSITA design driving science is the detection of large samples of galaxy clusters up to redshifts $z>1$ in order to study the large-scale structure of the universe and test cosmological models including Dark Energy. In addition, eROSITA is expected to yield a sample of a few million AGNs, including obscured objects, revolutionizing our view of the evolution of supermassive black holes. The survey will also provide new insights into a wide range of astrophysical phenomena, including X-ray binaries, active stars, and diffuse emission within the Galaxy. Results from early observations, some of which are presented here, confirm that the performance of the instrument is able to fulfil its scientific promise. With this paper, we aim to give a concise description of the instrument, its performance as measured on ground, its operation in space, and also the first results from in-orbit measurements.

arXiv comment16 pages, 19 figures, accepted by Astronomy & Astrophysics

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• Cosmological simulations of galaxy clusters
• Outskirts of Galaxy Clusters
• Chandra Observes the End of an Era SN 1987A
• Active Galactic Nuclei and their Large-scale Structure: an eROSITA mock catalogue
• Constraining galaxy cluster temperatures and redshifts with eROSITA survey data
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
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• eROSITA Final Equatorial-Depth Survey (eFEDS): eFEDS X-ray view of WERGS Radio Galaxies selected by the Subaru/HSC and VLA/FIRST survey
• The Luminosity Phase Space of Galactic and Extragalactic X-ray Transients Out to Intermediate Redshifts
• A global view of shocked plasma in the supernova remnant Puppis A provided by SRG/eROSITA
• The corona -- chromosphere connection studied with simultaneous eROSITA and TIGRE observations
• New Active Galactic Nuclei Detected by the ART-XC and eROSITA Telescopes Onboard the SRG Observatory during an All-Sky X-ray Survey
• On the patchy appearance of the circum-Galactic medium and the influence of foreground absorption
• X-ray Binaries in External Galaxies
• Measuring the X-ray luminosities of DESI groups from eROSITA Final Equatorial-Depth Survey: I. X-ray luminosity -- halo mass scaling relation
• X-ray and ultraviolet observations of the eclipsing cataclysmic variables OV Bootis and SDSS J103533.02+055158.3 with degenerate donors
• X-raying the Sco-Cen OB association: The low-mass stellar population revealed by eROSITA
• Representation Learning for Time-Domain High-Energy Astrophysics: Discovery of Extragalactic Fast X-ray Transient XRT 200515
• SRG/eROSITA discovery of 164 s pulsations from the SMC Be/X-ray binary XMMU J010429.4-723136
• G189.6+03.3: the first complete X-ray view provided by SRG/eROSITA
• Weakened Magnetic Braking Signals the Collapse of the Global Stellar Dynamo
• The Average Soft X-ray Spectra of eROSITA Active Galactic Nuclei
• Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe
• X-ray panorama of the SS433/W50 complex by SRG/eROSITA
• Unveiling the origin of XMM-Newton soft proton flares: I. Design and validation of a response matrix for proton spectral analysis
• eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS2
• The perils of stacking optically selected groups in eROSITA data. The Magneticum perspective
• The XMM Cluster Survey: Exploring scaling relations and completeness of the Dark Energy Survey Year 3 redMaPPer cluster catalogue
• Morphological Evidence for the eROSITA Bubbles Being Giant and Distant Structures
• Radial X-ray profiles of simulated galaxies: Contributions from hot gas and XRBs
• SRG/eROSITA-triggered XMM-Newton observations of three Be/X-ray binaries in the LMC: Discovery of X-ray pulsations
• Discovery of non-equilibrium ionization plasma associated with the North Polar Spur and Loop I
• The Hot Interstellar Medium
• The black widow pulsar J1641+8049 in the optical, radio and X-rays
• Prospect of Detecting X-Ray Halos Around Middle-Aged Pulsars with eROSITA
• A major galaxy cluster merger caught by eROSITA: weak lensing mass distribution and kinematic description
• eROSITA narrowband maps at the energies of soft X-ray emission lines
• The Extragalactic Serendipitous Swift Survey (ExSeSS) -- I. Survey definition and measurements of the X-ray number counts
• A test of the evolution of gas depletion factor in galaxy clusters using strong gravitational lensing systems
• A multi-wavelength view of the multiple activity cycles of $\epsilon$~Eridani
• Simultaneous X-ray and optical variability of M dwarfs observed with eROSITA and TESS
• X-ray counterpart detection and gamma-ray analysis of the SNR G279.0+01.1 with eROSITA and Fermi-LAT
• A Newborn AGN in a Starforming Galaxy
• eROSITA X-ray Analysis of the PeVatron Candidate Westerlund 1
• The XMM Cluster Survey: An independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies
• The intrinsic X-ray luminosity distribution of an optically-selected SDSS quasar population
• The Success of Optical Variability in Uncovering AGNs in Low-stellar Mass Galaxies
• The first detection of cosmic-ray excited H${}_2$ in interstellar space
• The warm-hot intergalactic medium in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters
• Wide-field X-ray observations of the supernova remnant Puppis A with the SRG/ART-XC telescope
• J1832.4-1627, the first eclipsing stream-fed intermediate polar
• The Atacama Cosmology Telescope: Flux Upper Limits from a Targeted Search for Extragalactic Transients
• Characterising X-ray variability in light curves with complex sampling patterns: application to the eROSITA south ecliptic pole survey
• Gaia GraL: Gaia DR2 Gravitational Lens Systems. VII. XMM-Newton Observations of Lensed Quasars
• Is the X-ray bright z = 5.5 quasar SRGE J170245.3+130104 a blazar?
• Transitions in magnetic behavior at the substellar boundary
• Cosmic-Ray-Related Signals from Detectors in Space: the Spitzer/IRAC Si:As IBC Devices
• Pulsar Wind Nebulae
• Is planetary inward migration responsible for GJ 504's fast rotation and bright X-ray luminosity? New constraints from eROSITA
• Detection of disk-jet co-precession in a tidal disruption event
• The SRG/eROSITA all-sky survey: View of the Fornax galaxy cluster
• Broadband study and the discovery of pulsations from the Be/X-ray binary eRASSU J052914.9-662446 in the Large Magellanic Cloud
• Discovery of a ~30-Year-Duration Post-Nova Pulsating Supersoft Source in the Large Magellanic Cloud
• SRG/ART-XC, Swift, NICER and NuSTAR study of different states of the transient X-ray pulsar MAXI J0903-531
• Dissociation of dark matter and gas in cosmic large-scale structure
• An 85-s X-ray quasi-periodicity after a stellar tidal disruption by a candidate intermediate-mass black hole
• Study of X-ray emission from the S147 nebula with SRG/eROSITA: X-ray imaging, spectral characterization, and a multiwavelength picture
• Strong lensing of tidal disruption events: Detection rates in imaging surveys
• The high-energy environment of the heavy sub-Earth GJ 367 b indicates likely complete evaporation of its atmosphere
• Searching for cold gas traced by MgII quasar absorbers in massive X-ray-selected galaxy clusters
• The first X-ray look at SMSS J114447.77-430859.3: the most luminous quasar in the last 9 Gyr
• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• Central radio galaxies in galaxy clusters: Joint surveys by eROSITA and ASKAP
• First eROSITA-TESS results for M dwarfs: Mass dependence of the X-ray activity rotation relation and an assessment of sensitivity limits
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• The SRG/eROSITA All-Sky Survey: Large-scale view of the Centaurus cluster
• SRG/ART-XC Galactic Plane Survey near Galactic Longitude $l\simeq 20^{\circ }$: Catalog of Sources
• Discovery of the Goat Horn complex: a $\sim 1000$ deg${}^2$ diffuse X-ray source connected to radio loop XII
• Optical polarization of stellar-fed active and quiescent supermassive black holes
• Cosmological Inference with Cosmic Voids and Neural Network Emulators
• Cosmology and Astrophysics with the Diffuse eRASS1 X-ray Angular Power Spectrum
• G321.3-3.9: A new supernova remnant observed with multi-band radio data and in the SRG/eROSITA All-Sky Surveys
• New Active Galactic Nuclei Detected by the ART-XC and eROSITA Telescopes during the First Five SRG All-Sky X-ray Surveys
• X-ray variability of the triplet star system LTT1445 and evaporation history of the exoplanets around its A component
• Magnetic braking below the cataclysmic variable period gap and the observed dearth of period bouncers
• The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
• The Composite Spectral Energy Distribution of Quasars is Surprisingly Universal Since Cosmic Noon
• A Novel Method for Estimating the Ambient Medium Density Around Distant Radio Sources from Their Observed Radio Spectra
• Discovery of the lensed quasar eRASS1 J050129.5-073309 with $\text{SRG}/$eROSITA and $Gaia$
• The stellar activity-rotation-age relationship under the lens of asteroseismology
• Machine learning applications for the study of AGN physical properties using photometric observations
• Serendipitous discovery of the magnetic cataclysmic variable SRGE J075818-612027
• Nature of 4FGL J1838.2+3223: a flaring `spider' pulsar candidate
• Scaling relations of clusters and groups, and their evolution
• A new look at the extragalactic Very High Energy sky: searching for TeV-emitting candidates among the X-ray bright, non-Fermi detected blazar population
• On the origin of the $10^7$ K hot emitting gas in the Circumgalactic medium of the Milky Way
• Correlation Analysis of Decaying Sterile Neutrino Dark Matter in the Context of the SRG Mission
• X-ray selected broad absorption line quasars in SDSS-V: BALs and non-BALs span the same range of X-ray properties
• Searching for stellar cycles on low mass stars using TESS data
• Measuring the ICM velocity structure within the A3266 galaxy cluster
• The eROSITA extragalactic CalPV serendipitous catalog
• The First SRG/eROSITA All-Sky Survey. Characterization of clusters of galaxies misclassified in the eRASS1 point source catalog
• Robust detection of hot intragroup medium in optically selected, poor galaxy groups by eROSITA
• Millinovae: A New Class of Transient Supersoft X-ray Sources without a Classical Nova Eruption
• Characterisation of the X-ray point source variability in the eROSITA south ecliptic pole field
• Probing the physical properties of the IGM using SRG/eROSITA spectra from blazars
• Filters for X-ray detectors on Space missions
• Supernova remnant candidates identified using MWA Galactic Plane Monitoring over 285deg < l < 70deg and |b| < 16deg
• AMICO galaxy clusters in KiDS-1000: cosmological sample
• The eROSITA view on the halo mass-temperature relation: From low-mass groups to massive clusters
• The SRG/eROSITA All-Sky Survey: Exploring halo assembly bias with X-ray selected superclusters
• Modelling the selection of galaxy groups with end to end simulations
• Winds of change: the nuclear and galaxy-scale outflows and the X-ray variability of 2MASS 0918+2117
• SRGe J194401.8+284452 -- an X-ray Cataclysmic Variable in the Field of the Gamma-Ray Source 4FGL J1943.9+2841
• Introducing the Descriptive Parametric Model: Gaseous Profiles for Galaxies, Groups, and Clusters
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• SRGe2149+6736 -- the new candidate to AM~Her type variables discovered by eROSITA telescope on "Spectrum--Roentgen--Gamma" orbital observatory
• Cluster outskirts and their connection to the cosmic web
• eROSITA-RU Tidal Disruption Events with Keck-I/LRIS: Sample Selection, Optical Properties, and Host Galaxy Demographics
• Satellite Content and Halo Mass of Galaxy Clusters: Comparison between Red-Sequence and Halo-based Optical Cluster Finders
• X-Ray Redshifts of Obscured Chandra Source Catalog AGN
• Identifying interesting planetary systems for future X-ray observations
• Multi-messenger connection in high-energy neutrino astronomy
• The first evidence of tidally induced activity in a brown dwarf-M dwarf pair: A Chandra study of the NLTT 41135/41136 system
• The luminosity function of TDEs from fallback-powered emission: implications for the black hole mass function
• A new understanding of the Gemini-Monoceros X-ray enhancement from discoveries with eROSITA
• Is the high-energy environment of K2-18b special?
• The Curious Case of the "Heartworm" Nebula
• Spatially resolved X-ray spectra of the Galactic SNR G18.95-1.1: SRG/eROSITA view
• Constraints on the parameters of keV-scale mass annihilating Dark Matter obtained with SRG/ART-XC observations
• Three young planets around the K-dwarf K2-198: High-energy environment, evaporation history and expected future
• Predicting the Non-Thermal Pressure in Galaxy Clusters
• Hunting isolated neutron stars with proper motions from wide-area optical surveys
• Ionised AGN outflows in the Goldfish galaxy -- The illuminating and interacting red quasar eFEDSJ091157.4+014327 at z $\sim$ 0.6
• Average energy of the X-ray spectrum as a model-independent proxy for the mass of galaxy clusters
• Discovery of the magnetic cataclysmic variable XMM J152737.4-205305.9 with a deep eclipse-like feature
• Observability of HOFNARs with SRG/eROSITA
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• HD 34736: An intensely magnetised double-lined spectroscopic binary with rapidly-rotating chemically peculiar B-type components
• The eROSITA DR1 variability catalogue
• Optical Identification and Spectroscopic Redshift Measurements of 216 Galaxy Clusters from the SRG/eROSITA All-Sky Survey
• Revisiting the X-ray-to-UV relation of Quasars in the era of all-sky surveys
• The Cosmological analysis of X-ray cluster surveys VII. Bypassing scaling relations with Lagrangian Deep Learning and Simulation-based inference
• The SRG/eROSITA all-sky survey: Hard X-ray selected Active Galactic Nuclei
• First characterization of a new High Mass X-ray Binary in LMC eRASSU J050810.4$-$660653 with SRG/ART-XC, NuSTAR and Swift
• SRG/eROSITA 3D mapping of the ISM using X-ray absorption spectroscopy
• The SRG/eROSITA all-sky survey: Constraints on Ultra-light Axion Dark Matter through Galaxy Cluster Number Counts
• BASS XLV: Quantifying AGN Selection Effects in the Chandra COSMOS-Legacy Survey with BASS
• Accretion Flares from Stellar Collisions in Galactic Nuclei
• Exploring the X-ray-radio connection for AGN via measurements of the multi-dimensional luminosity function
• Searching for Particle Dark Matter with eROSITA Early Data
• Galactic bars and active galactic nucleus fuelling in the second half of cosmic history
• An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
• SRG/eROSITA Survey in the Lockman Hole: Classification of X-ray Sources
• Rapid onset of a Comptonisation zone in the repeating tidal disruption event XMMSL2 J140446.9-251135
• Unveiling the soft X-ray source population towards the inner Galactic disk with XMM-Newton
• The average X-ray spectrum of the volume-complete M-, F-, G-, and K-type star sample within 10 pc of the Sun
• The FLAMINGO simulations data release
• Robust AGN and host-galaxy decomposition in optical spectral fitting
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• Search for pre-burst emission from binary neutron star mergers with Spectrum-Roentgen-Gamma
• On the Robustness of Cluster Clustering Covariance Calibration
• A new quasar strongly-lensed candidate by the galaxy cluster WHJ0400-27 with a $18^{\prime \prime }$ image-separation
• Cataclysmic Variable Candidates Identified in eROSITA-DE DR1,XMM-Newton, Swift, and ROSAT Catalogs
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• Searching for supermassive black holes binaries within SRG/eROSITA-De I: Properties of the X-ray selected candidates
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• Long-term stability of scientific X-ray CMOS detectors
• The X-ray and Radio Loud Fast Blue Optical Transient AT2020mrf: Implications for an Emerging Class of Engine-Driven Massive Star Explosions
• State Space Modelling for detecting and characterising Gravitational Waves afterglows
• Soft X-ray emission from the classical nova AT 2018bej
• A long-lived compact jet in the black hole X-ray binary candidate AT2019wey
• Optical Identification of Galaxy Clusters among SRG/eROSITA X-ray Sources Based on Photometric Redshift Estimates for Galaxies
• Discovery of a magnetar candidate X-ray pulsar in the Large Magellanic Cloud
• Mock X-ray observations of hot gas with L-Galaxies semi-analytic models of galaxy formation
• An Analytic, Fully Relativistic Framework for Tidal Disruption Event Streams in Schwarzschild Geometry
• Discovery of a new supergiant fast X-ray transient MAXI J0709-159 associated with the Be star LY CMa
• X-ray Spectral Variability as Probe of Multimessenger Emission in Blazar 5BZB J0630-24064
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• Precursors in tidal disruption events: repeating, fast, and AGN-hosted TDEs
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• The X-ray$-$UV Luminosity Relation of eROSITA Quasars
• Determination of the Solar System contribution to the soft X-ray sky
• Formation of A Nuclear Star Cluster Through A Merger Event In The Low Surface Brightness Galaxy AGC 223218
• Source identification for the Swift-BAT 150-month hard X-ray catalog using soft X-ray observations
• INTEGRAL, eROSITA and Voyager Constraints on Light Bosonic Dark Matter: ALPs, Dark Photons, Scalars, $B-L$ and $L_i-L_j$ Vectors
• Perseus cluster in its X-ray entirety with SRG/eROSITA. Merger and Radio-Uroboroses
• Studying the multi-phase interstellar medium in the Large Magellanic Cloud with SRG/eROSITA -- I. Analysis of diffuse X-ray emission
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• A comprehensive search for high-velocity X-ray sources: New compact object binary candidates in the Gaia era
• Bayesian Multi-wavelength Imaging of the LMC SN1987A with SRG/eROSITA
• DarsakX: A Python Package for Designing and Analyzing Imaging Performance of X-ray Telescopes
• Tidal disruption events as the origin of the eROSITA and Fermi bubbles
• UGPS J194310+183851: an Unusual Optical and X-ray Faint Cataclysmic Variable?
• DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
• Wind-mediated Eddington-limited emission in a $10^4{M}_{\odot }$ Black Hole Tidal Disruption Event
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray stacking analysis of Subaru's optically selected clusters spanning low richness regime
• X-ray flux -- mass relation for $z\gtrsim 0.7$ galaxy clusters
• Possible evidence for extended X-ray emission surrounding PSR B0656+14 with eROSITA
• A systematic study of AGN feedback in a disk galaxy using MACER II: predictions of X-ray surface brightness profiles and comparison with eROSITA observations
• Contaminating Electromagnetic Transients in LISA Gravitational Wave Localization Volumes. I: The Intrinsic Rates
• SRG/ART-XC all-sky X-ray survey: Catalog of sources detected during the first year
• New Active Galactic Nuclei Detected by the ART-XC and eROSITA Telescopes during the First Five SRG All-Sky X-ray Surveys. Part 2
• A Tidal Disruption Event from an Intermediate-mass Black Hole Revealed by Comprehensive Multi-wavelength Observations
• Tracing X-ray and HI absorption in peaked spectrum sources
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Detectability of Supernova Remnants with the Southern Wide-field Gamma-ray Observatory
• A look at the high energy aspects of the supernova remnant G309.8+00.0 with eROSITA and Fermi-LAT
• eROSITA-selection of new period-bounce Cataclysmic Variables: First follow-up confirmation using TESS and SDSS
• Unveiling the nature of the unidentified gamma-ray sources 4FGL J1908.6+0915e, HESS J1907+089/HOTS J1907+091, and 3HWC J1907+085 in the sky region of the magnetar SGR 1900+14
• Merger of massive galaxy cluster CL0238.3+2005 at z~0.4: just after pericenter passage?
• Searching for Axion-Like Particles with X-ray Observations of Alpha Centauri
• Nearby Young Stars and Young Moving Groups
• An Asymmetrical Model for High Energy Radiation of Cassiopeia A
• The X-ray statistical properties of dust-obscured galaxies detected by eROSITA
• Detection of Anisotropies in the Circumgalactic Medium of Disk Galaxies: Supermassive Black Hole Activity or Star Formation-driven Outflows?
• Tidal star-planet interaction and its observed impact on stellar activity in planet-hosting wide binary systems
• Cross-correlations between X-ray clusters and the general galaxy population
• A census of Dark Energy Survey Year 3 redMaPPer galaxy clusters in a high exposure eROSITA All Sky Survey region
• Superflare on a rapidly-rotating solar-type star captured in X-rays
• NuSTAR discovery of the hard X-ray emission and a wide-band X-ray spectrum from the Pictor A western hot spot
• X-ray spectral fitting with Monte Carlo Dropout Neural Networks
• Predictions for the X-ray circumgalactic medium of edge-on discs and spheroids
• A detailed study on spectroscopic performance of SOI pixel detector with a pinned depleted diode structure for X-ray astronomy
• On the nature of the 2.4 hr-period eclipsing cataclysmic variable W2 in 47 Tuc
• Multiwavelength study of 1eRASS J085039.9-421151 with eROSITA NuSTAR and X-shooter
• Identification of high-redshift X-ray active galactic nuclei in the 4XMM-DR11 serendipitous catalogue using DES data: Comparative analysis with optically-selected QSOs
• Chemical enrichment of ICM within the A3266 cluster I: radial profiles
• An expanded ultraluminous X-ray source catalogue
• Planetary Nebulae in the eROSITA eRASS1 catalog
• Probing AGN duty cycle and cluster-driven morphology in a giant episodic radio galaxy
• Testing the correlation between bending angle and polarization properties of bent radio galaxies
• Identification of radio and gamma-ray pulsars in X-rays using data from the SRG/eROSITA all-sky survey
• X-ray Properties of the Luminous Quasar PG 1634+706 at z = 1.337 from SRG and XMM-Newton Data
• Confirmation of SRGt 062340.2-265751 as a nova-like cataclysmic variable with a possible magnetic nature
• Galactic X-ray Transients in the First eROSITA All Sky Survey
• Ultraluminous X-ray sources in the first eROSITA survey I. Candidate catalogs
• Study of Massive OBA Stars with X-ray Emission
• LOFAR detection of faint radio emission from the supernova remnant SRGeJ0023+3625=G116.6-26.1: probing the Milky Way synchrotron halo
• Nature of 4FGL J2249.4+6229: Evidence for a redback system with a cool companion and low X-ray and $\gamma$-ray luminosities
• Losing a minute every two years: SRG X-ray view on the rapidly accelerating X-ray pulsar SXP1323
• Constraining the synchrotron peak and estimating the VHE brightness of a sample of extreme high synchrotron peak blazars
• AT2024lhc and AT2024kmq in the landscape of featureless tidal disruption events
• Intracluster Medium Fluctuations on Scales up to 1 Mpc: A Combined eROSITA and SPT/Planck Analysis of Abell 3266
• High Energy Emission from the Galactic Center
• Probing habitable regions with SRG/eROSITA
• The SRG/eROSITA all-sky survey: The morphologies of clusters of galaxies: II. The intrinsic distributions of morphological parameters
• Rate of Repeating Tidal Disruption Events with 5--19 years interval
• First studies of the diffuse X-ray emission in the Large Magellanic Cloud with eROSITA
• The ROSAT Raster Survey in the North-Ecliptic Pole Field: X-ray Catalogue and Optical Identifications
• SRG/eROSITA-SDSS view on the relation between X-ray and UV emission for quasars
• A Study of Cataclysmic Variables from the eFEDS Survey
• The Sun as an X-ray star V.: A new method to retrieve coronal filling factors
• Extracting latent representations from X-ray spectra. Classification, regression, and accretion signatures of Chandra sources
• The SRG/eROSITA All-Sky Survey $J$-Band Follow-Up Observations for Selected High-Redshift Galaxy Cluster Candidates
• Old Galactic novae in the eROSITA All Sky Survey
• XMM-Newton follow-up of two eROSITA X-ray binary candidates
• A test of MOND and Emergent Gravity with SMACS J0723.3-7327 using eROSITA observations
• A Multi-Mission Catalogue of Ultraluminous X-ray Source Candidates
• DUCA: Dynamic Universe Cosmological Analysis. II. The impact of clustering dark energy on the halo mass function