Collisional Plasma Models with APEC/APED: Emission Line Diagnostics of Hydrogen-like and Helium-like Ions

Abstract

New X-ray observatories (Chandra and XMM-Newton) are providing a wealth of high-resolution X-ray spectra in which hydrogen- and helium-like ions are usually strong features. We present results from a new collisional-radiative plasma code, the Astrophysical Plasma Emission Code (APEC), which uses atomic data in the companion Astrophysical Plasma Emission Database (APED) to calculate spectral models for hot plasmas. APED contains the requisite atomic data such as collisional and radiative rates, recombination cross sections, dielectronic recombination rates, and satellite line wavelengths. We compare the APEC results to other plasma codes for hydrogen- and helium-like diagnostics, and test the sensitivity of our results to the number of levels included in the models. We find that dielectronic recombination with hydrogen-like ions into high (n=6-10) principal quantum numbers affects some helium-like line ratios from low-lying (n=2) transitions.

5 pages, 6 figures, accepted by ApJ Letters

References in corpus (4)

• Ionization balance for optically thin plasmas: rate coefficients for all atoms and ions of the elements H to Ni
• X-ray photoionized plasma diagnostics with Helium-like ions. Application to Warm Absorber-Emitter in Active Galactic Nuclei
• Recombination spectra of Helium-Like Ions
• Resonant Scattering of Emission Lines in Coronal Loops: Effects on Image Morphology and Line Ratios

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• Deep XMM and Chandra observations of ClJ1226.9+3332: A detailed X-ray mass analysis of a z=0.89 galaxy cluster
• Three-dimensional modeling of the asymmetric blast wave from the 2006 outburst of RS Ophiuchi: Early X-ray emission
• Jets, accretion, coronae and all that: The enigmatic X-rays from the Herbig star HD 163296
• An Analytic Model of the Physical Properties of Galaxy Clusters
• Multi-frequency imaging of the galaxy cluster Abell 2163 using the Sunyaev-Zel'dovich Effect
• No hydrogen exosphere detected around the super-Earth HD97658 b
• Measuring turbulence and gas motions in galaxy clusters via synthetic Athena X-IFU observations
• From Radio to X-ray: The Quiescent Atmosphere of the dMe Flare Star EV Lacertae
• Bursting SN 1996cr's Bubble: Hydrodynamic and X-ray Modeling of its Circumstellar Medium
• Fast and Furious: Shock Heated Gas as the Origin of Spatially Resolved Hard X-ray Emission in the Central 5 kpc of the Galaxy Merger NGC 6240
• Supermassive Black Hole Winds in X-rays -- SUBWAYS. I. Ultra-fast outflows in QSOs beyond the local Universe
• Large X-ray Flares on Stars Detected with MAXI/GSC: A Universal Correlation between the Duration of a Flare and its X-ray Luminosity
• X-ray Spectroscopy of the Core of the Perseus Cluster with Suzaku: Elemental Abundances in the Intracluster Medium
• High Resolution XMM-Newton Spectroscopy of the Cooling Flow Cluster A3112
• Probing the Outskirts of the Early Stage Galaxy Cluster Merger A1750
• Forecasts on dark energy from the X-ray cluster survey with eROSITA: constraints from counts and clustering
• The XUV environments of exoplanets from Jupiter-size to super-Earth
• Radio footprints of a minor merger in the Shapley Supercluster: From supercluster down to galactic scales
• A Chandra X-ray detection of the L dwarf binary Kelu-1: Simultaneous Chandra and Very Large Array observations
• The Coronal X-ray Spectrum of the Multiple Weak-Lined T Tauri Star System HD 98800
• A wide angle tail radio galaxy in the COSMOS field: evidence for cluster formation
• The abundance pattern of O, Mg, Si and Fe in the intracluster medium of the Centaurus cluster observed with XMM-Newton
• A Chandra ACIS Study of the Young Star Cluster Trumpler 15 in Carina and Correlation with Near-infrared Sources
• X-ray detection of a nova in the fireball phase
• EAGLE and Illustris-TNG predictions for resolved eROSITA X-ray observations of the circumgalactic medium around normal galaxies
• Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
• Enriching the hot circumgalactic medium
• X-ray Emission from Strongly Asymmetric Circumstellar Material in the Remnant of Kepler's Supernova
• Evolutionary Status of SNR 1987A at the Age of Eighteen
• On the thermodynamic self-similarity of the nearest, most relaxed, giant ellipticals
• Simultaneous Multiwavelength Observations of Magnetic Activity in Ultracool Dwarfs. IV. The Active, Young Binary NLTT 33370 AB (=2MASS J13142039+1320011)
• Questioning a 3.5 keV dark matter emission line
• X-ray emission from massive stars in Cyg OB2
• A Far-Ultraviolet Spectroscopic Survey of Luminous Cool Stars
• Evolution of X-ray cavities
• The isolated elliptical NGC 4555 observed with Chandra
• An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l=120 and l=240
• X-ray Emission from an Asymmetric Blast Wave and a Massive White Dwarf in the Gamma-ray Emitting Nova V407 Cyg
• Chandra Observations of the Eagle Nebula. I. Embedded Young Stellar Objects near the Pillars of Creation
• The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles
• XMM-Newton X-ray study of early type stars in the Carina OB1 association
• The WIRCAM Deep Infrared Cluster Survey I: Groups and Clusters at z > 1.1
• An XMM-Newton Observation of the Local Bubble Using a Shadowing Filament in the Southern Galactic Hemisphere
• Growing a `Cosmic Beast': Observations and Simulations of MACS J0717.5+3745
• Star Formation Suppression Due to Jet Feedback in Radio Galaxies with Shocked Warm Molecular Gas
• Deep Chandra observation and numerical studies of the nearest cluster cold front in the sky
• A Giant Metrewave Radio Telescope/Chandra view of IRAS 09104+4109: A type 2 QSO in a cooling flow
• Testing EUV/X-ray Atomic Data for the Solar Dynamics Observatory
• High resolution X-ray spectroscopy of the multiphase interstellar medium toward Cyg X-2
• On the Importance of the Interclump Medium for Superionization: O VI Formation in the Wind of Zeta Pup
• Chandra Measurements of a Complete Sample of X-ray Luminous Galaxy Clusters: the Gas Mass Fraction
• Chandra Observations of MBM12 and Models of the Local Bubble
• Chandra LETG Observations of Supernova Remnant 1987A
• The gravitational field of X-COP galaxy clusters
• X-ray Spectral Study of the extended emission,'the Cap', located 11.6 kpc above the disk of M82
• Simultaneous X-ray and optical spectroscopy of the Oef supergiant lambda Cep
• Suzaku observations of Abell 1835 outskirts: Deviation from hydrostatic equilibrium
• High-Resolution Chandra X-ray Imaging and Spectroscopy of the Sigma Orionis Cluster
• Chandra X-ray spectroscopy of the very early O supergiant HD 93129A: constraints on wind shocks and the mass-loss rate
• Detection of a giant flare displaying quasi-periodic pulsations from a pre-main sequence M star with NGTS
• The corona and companion of CoRoT-2A. Insights from X-rays and optical spectroscopy
• Suzaku Observations of the North Polar Spur: Evidence for Nitrogen Enhancement
• X-ray properties of the Youngest Radio Sources and their Environments
• The MUSIC of Galaxy Clusters II: X-ray global properties and scaling relations
• Not that long time ago in the nearest galaxy: 3D slice of molecular gas revealed by a 110 years old flare of Sgr A*
• YSO accretion shocks: magnetic, chromospheric or stochastic flow effects can suppress fluctuations of X-ray emission
• Spherically Averaging Ellipsoidal Galaxy Clusters in X-Ray and Sunyaev-Zel'dovich Studies: II. Biases
• From X-ray dips to eclipse: Witnessing disk reformation in the recurrent nova USco
• Chandra and XMM-Newton Observations of the Abell 3391/Abell 3395 Intercluster Filament
• X-ray Doppler Imaging of 44i Boo with Chandra
• X-Ray Emitting Ejecta of Supernova Remnant N132D
• Suzaku observations of the Hydra A cluster out to the virial radius
• Iron in X-COP: tracing enrichment in cluster outskirts with high accuracy abundance profiles
• AWM 4 - an isothermal cluster observed with XMM-Newton
• Radiative accretion shocks along nonuniform stellar magnetic fields in classical T Tauri stars
• Altair - the 'hottest' magnetically active star in X-rays
• X-ray and IR Point Source Identification and Characteristics in the Embedded, Massive Star-Forming Region RCW 108
• Constraints on turbulent velocity broadening for a sample of clusters, groups and elliptical galaxies using XMM-Newton
• GK Per and EX Hya: Intermediate polars with small magnetospheres
• A Search for a keV Signature of Radiatively Decaying Dark Matter with Suzaku XIS Observations of the X-ray Diffuse Background
• The Transparency of Solar Coronal Active Regions
• The Young Binary DQ Tau: A Hunt For X-ray Emission From Colliding Magnetospheres
• Shock Speed, Cosmic Ray Pressure, and Gas Temperature in the Cygnus Loop
• X-ray spectra of the Fe-L complex
• Linear Structures in the Core of the Coma Cluster of Galaxies
• Jet-ISM Interaction in the Radio Galaxy 3C293: Jet-driven Shocks Heat ISM to Power X-ray and Molecular H2 emission
• The Growth and Enrichment of the Intragroup Gas
• An X-Ray Face-on View of the Sgr B Molecular Clouds Observed with Suzaku
• The Chandra ACIS Survey of M33 (ChASeM33): The final source catalog
• Simulating the Fermi Bubbles as Forward Shocks Driven by AGN Jets
• Deep Chandra observations of the stripped galaxy group falling into Abell 2142
• The metal content of the hot atmospheres of galaxy groups
• What Do the Hitomi Observations Tell Us About the Turbulent Velocities in the Perseus Cluster? Probing the Velocity Field with Mock Observations
• Pressure profiles and mass estimates using high-resolution Sunyaev-Zel'dovich effect observations of Zwicky 3146 with MUSTANG-2
• Resonant scattering in the Perseus Cluster: spectral model for constraining gas motions with Astro-H
• A Deep X-ray View of the Hot Halo in the Edge-on Spiral Galaxy NGC 891
• Properties of Cosmological Filaments extracted from Eulerian Simulations
• Chandra spectroscopy of the hot star beta Crucis and the discovery of a pre-main-sequence companion
• Metal Abundances in the Cool-Cores of Galaxy Clusters
• A textbook example of ram-pressure stripping in the Hydra A/A780 cluster
• Evidence for a neutral iron line generated by MeV protons from supernova remnants interacting with molecular clouds
• On the Anomalous Temperature Distribution of the Intergalactic Medium in the NGC 3411 Group of Galaxies
• The Nature of the Stable Soft X-ray Emissions in Several Types of Active Galactic Nuclei Observed by Suzaku
• Characterizing hydrostatic mass bias with Mock-X
• Modeling UV and X-Ray Emission in a Post-CME Current Sheet
• Detecting shocked intergalactic gas with X-ray and radio observations
• Discovery of Gas Bulk Motion in the Galaxy Cluster Abell 2256 with Suzaku
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• The Properties of the Galactic Hot Gaseous Halo from X-ray Emission
• A new paradigm for the X-ray emission of O stars from XMM-Newton observations of the O9.7 supergiant zeta Orionis
• A multi-wavelength view of cooling vs. AGN heating in the X-ray luminous cool-core of Abell 3581
• A Strong Merger Shock in Abell 665
• Numerical Simulations of Supernova Remnant Evolution in a Cloudy Interstellar Medium
• Predicting Merger-Induced Gas Motions in Lambda-CDM Galaxy Clusters
• Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
• Unraveling the Origin of Overionized Plasma in the Galactic Supernova Remnant W49B
• The split in the ancient cold front in the Perseus cluster
• The effects of galaxy shape and rotation on the X-ray haloes of early-type galaxies - II. Numerical simulations
• The galaxy group NGC 507: newly detected AGN remnant plasma transported by sloshing
• Active Galactic Nuclei Feedback in an Elliptical Galaxy with the Most Updated AGN Physics (II): High-Angular Momentum Case
• Heating in an Extended Accretion Disk Corona along the Z-Pattern in Cyg X-2
• Studying the merging cluster Abell 3266 with eROSITA
• G11.2-0.3: The Young Remnant of a Stripped-Envelope Supernova
• An X-ray Imaging Study of the Stellar Population in RCW49
• APO & SMARTS flare star campaign observations I. Blue wing asymmetries in chromospheric lines during mid M dwarf flares from simultaneous spectroscopic and photometric observation data
• Observational Constraints on Superbubble X-ray Energy Budgets
• Chandra X-ray Grating Spectrometry of Eta Carinae near X-ray Minimum: I. Variability of the Sulfur and Silicon Emission Lines
• Suzaku Observation of HESS J1825-137: Discovery of Largely-Extended X-rays near from PSR J1826-1334
• A detailed X-ray investigation of ζ Puppis III. A spectral analysis of the whole RGS spectrum
• Simultaneous Multiwavelength Flare Observations of EV Lacertae
• A Chandra Study of the Rosette Star-Forming Complex. II. Clusters in the Rosette Molecular Cloud
• Resonant scattering of X-ray emission lines in the hot intergalactic medium
• The EUVE point of view of AD Leo
• X-ray and Optical Correlation of Type I Seyfert NGC 3516 Studied with Suzaku and Japanese Ground-Based Telescopes
• Bias from gas inhomogeneities in the pressure profiles as measured from X-ray and SZ observations
• Extended X-ray Emission in the HI Cavity of NGC 4151: Galaxy-scale AGN Feedback?
• Resonance scattering, absorption and off-centre abundance peaks in clusters of galaxies
• Outer jet X-ray and radio emission in R Aquarii: 1999.8 to 2004.0
• Separating the X-Ray Emissions of UV Ceti A and B with Chandra
• The X-ray puzzle of the L1551 IRS 5 jet
• Storm in a Teacup: X-ray view of an obscured quasar and superbubble
• The stellar contents and star formation in the NGC 7538 region
• The effects of X-ray absorption variability in NGC 4395
• Probing Final Stages of Stellar Evolution with X-Ray Observations of SN 2013ej
• The Enrichment of the Intracluster Medium
• An azimuthally resolved study of the cold front in Abell 3667
• Polarization and long-term variability of Sgr A* X-ray echo
• Close-up view of an ongoing merger between the NGC 4839 group and the Coma cluster - a post-merger scenario
• The cosmological analysis of X-ray cluster surveys: I- A new method for interpreting number counts
• Spectral and Timing Nature of the Symbiotic X-ray Binary 4U 1954+319: The Slowest Rotating Neutron Star in an X-ray Binary System
• A multi-wavelength study of the young star V1118 Orionis in outburst
• Suppression of X-rays from radiative shocks by their thin-shell instability
• AGN/starburst connection in action: the half million second RGS spectrum of NGC1365
• Grid of pseudo-2D chemistry models for tidally locked exoplanets -- II. The role of photochemistry
• MOVES III. Simultaneous X-ray and ultraviolet observations unveiling the variable environment of the hot Jupiter HD 189733b
• Athena X-IFU synthetic observations of galaxy clusters to probe the chemical enrichment of the Universe
• Wavelength Measurements of K Transitions of Oxygen, Neon, and Magnesium with X-ray Absorption Lines
• Chandra Survey of Nearby Highly Inclined Disc Galaxies - III: Comparison with Hydrodynamical Simulations of Circumgalactic Coronae
• A NuSTAR observation of the center of the Coma Cluster
• Long-Lasting X-Ray Emission from Type IIb Supernova 2011dh and Mass-Loss History of The Yellow Supergiant Progenitor
• Mass accretion to young stars triggered by flaring activity in circumstellar disks
• Chandra Observations of the Pleiades Open Cluster: X-ray Emission from Late-B to Early-F Type Binaries
• The weak neutral Fe fluorescence line and long-term X-ray evolution of the Compton-thick AGN in NGC 7674
• SN 2005ip: A Luminous Type IIn Supernova Emerging from a Dense Circumstellar Medium as Revealed by X-Ray Observations
• Planck intermediate results. XL. The Sunyaev-Zeldovich signal from the Virgo cluster
• Fundamental Reference AGN Monitoring Experiment (FRAMEx) I: Jumping Out of the Plane with the VLBA
• Deep Chandra study of the truncated cool core of the Ophiuchus cluster
• Coronal properties of G-type stars in different evolutionary phases
• The stellar content of the XMM-Newton Bright Serendipitous Survey
• XMM-Newton study of 30 Dor C and a newly identified MCSNR J0536-6913 in the Large Magellanic Cloud
• Glimpses of the past activity of Sgr A* inferred from X-ray echoes in Sgr C
• A multi-wavelength look at the young plerionic supernova remnant 0540-69.3
• Cluster X-ray luminosity-temperature relation at z>~1.5
• Simultaneous Kepler/K2 and XMM-Netwon observations of superflares in the Pleiades
• Discrepant Mass Estimates in the Cluster of Galaxies Abell 1689
• An X-ray Selected Galaxy Cluster in the Lockman Hole at Redshift 1.753
• A Deep Chandra Observation of the Oxygen-Rich Supernova Remnant 0540-69.3 in the Large Magellanic Cloud
• Super-virial temperature or Neon overabundance?: Suzaku observations of the Milky Way circumgalactic Medium
• X-ray and UV emission from the recurrent nova RS Ophiuchi in quiescence: Signatures of accretion and shocked gas
• The dark haloes of early-type galaxies in low-density environments: XMM-Newton and Chandra observations of NGC 57, NGC 7796 and IC 1531
• Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
• Evidences of the supercritical disc funnel radiation in X-ray spectra of SS 433
• Testing Secondary Models for the Origin of Radio Mini-Halos in Galaxy Clusters
• Revealing O VII from stacked X-ray grating spectra of clusters, groups and elliptical galaxies
• Evidence for Black Hole Growth in Local Analogs to Lyman Break Galaxies
• The Exceptional Soft X-ray Halo of the Galaxy Merger NGC 6240
• Swift X-ray and UV monitoring of the Classical Nova V458 Vul (Nova Vul 2007)
• Global Distribution of Fe K alpha Lines in the Galactic Center Region Observed with the Suzaku Satellite
• Resonant scattering in galaxy clusters for anisotropic gas motions on various spatial scales
• An Assessment of the Fe XVIII and Fe XIX Line Ratios from the Chandra Grating Observations of Capella
• The K2-3 system revisited: testing photoevaporation and core-powered mass loss with three small planets spanning the radius valley
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
• New Measurement Resolves Key Astrophysical Fe XVII Oscillator Strength Problem
• XMM-Newton observations of the diffuse X-ray emission in the starburst galaxy NGC 253
• The XXL survey: XLVI. Forward cosmological analysis of the C1 cluster sample
• Elemental Abundances in the Possible Type Ia Supernova Remnant G344.7-0.1
• Broad Band X-Ray Spectra of Two Low-luminosity Active Galactic Nuclei NGC 1566 and NGC 4941
• X-Ray Spectral Variability During an Outburst in V1118 Ori
• Observations of X-ray oscillations in XI Boo: Evidence of a fast kink mode in the stellar loops
• Chandra Measurements of a Complete Sample of X-ray Luminous Galaxy Clusters: The Luminosity-Mass Relation
• CHEERS Results from NGC 3393, III: Chandra X-ray Spectroscopy of the Narrow Line Region
• X-ray Variability in the Young Massive Triple theta2 Ori A
• Widespread Detection of Two Components in the Hot Circumgalactic Medium of the Milky Way
• Cold Fronts and Shocks Formed by Gas Streams in Galaxy Clusters
• Chandra X-ray observations of Abell 1835 to the virial radius
• Capella Corona Revisited: A Combined View from \textit{XMM-Newton} RGS, \textit{Chandra} HETGS, and LETGS
• Elemental Abundances in the X-Ray Gas of Early-Type Galaxies with XMM and Chandra Observations
• XMM-Newton observation of the ULIRG NGC 6240: The physical nature of the complex Fe K line emission
• The Structure of the Star-forming Cluster RCW 38
• Probabilistic classification of X-ray sources applied to Swift-XRT and XMM-Newton catalogs
• The imprints of AGN feedback within a supermassive black hole's sphere of influence
• A new type of X-ray pulsar
• Suzaku Observations of Heavily Obscured (Compton-thick) Active Galactic Nuclei selected by Swift/BAT Hard X-ray Survey
• AE Aurigae: first detection of non-thermal X-ray emission from a bow shock produced by a runaway star
• A New Compton-thick AGN in our Cosmic Backyard: Unveiling the Buried Nucleus in NGC 1448 with NuSTAR
• Discovery of Recombining Plasma in the Supernova Remnant 3C 391
• The Coronae of AB Dor and V471 Tau: Primordial angular momentum vs tidal spin-up
• X-Ray Grating Observations of Recurrent Nova T Pyxidis During The 2011 Outburst
• X-ray Spectroscopy of the Contact Binary VW Cephei
• Accretion onto the Companion of Eta Carinae During the Spectroscopic Event: II. X-Ray Emission Cycle
• High-resolution X-ray spectroscopy reveals the special nature of Wolf-Rayet star winds
• Ni abundance in the core of the Perseus Cluster: an answer to the significance of resonant scattering
• The X-Ray Spectrum of a Planetary Nebula at High Resolution: Chandra Gratings Spectroscopy of BD+30 3639
• A Chandra Study of the Rosette Star-Forming Complex. III. The NGC 2237 Cluster and the Region's Star Formation History
• The Massive Star Forming Region Cygnus OB2. I. Chandra catalogue of association members
• Detection of X-ray Resonance Scattering in Active Stellar Coronae
• Broadband Multi-wavelength Properties of M87 during the 2018 EHT Campaign including a Very High Energy Flaring Episode
• Oxygen Abundances in the Milky Way Using X-ray Absorption Measurements Towards Galaxy Clusters
• Galactic Outflows, Star Formation Histories, and Timescales in Starburst Dwarf Galaxies from STARBIRDS
• Modeling broadband X-ray absorption of massive star winds
• A Puzzling Merger in A3266: the Hydrodynamic Picture from XMM-Newton
• X-rays observations of a super-Chandrasekhar object reveal an ONeMg and a CO white dwarf merger product embedded in a putative SN Iax remnant
• Fe Ka line emission from the Arches cluster region - evidence for ongoing particle bombardment?
• Characterisation of the upper atmospheres of HAT-P-32 b, WASP-69 b, GJ 1214 b, and WASP-76 b through their He I triplet absorption
• The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies
• Apparent high metallicity in 3-4 keV galaxy clusters: the inverse iron-bias in action in the case of the merging cluster Abell 2028
• Inside a Beehive: the Multiple Merging Processes in the Galaxy Cluster Abell 2142
• NuSTAR J033202-2746.8: direct constraints on the Compton reflection in a heavily obscured quasar at z~2
• Evidence for a Truncated Accretion Disc in the Low Luminosity Seyfert Galaxy, NGC 7213?
• The hot circumgalactic medium in the eROSITA All-Sky Survey II. Scaling relations between X-ray luminosity and galaxies' mass
• The Chemical Evolution of Galaxy Clusters: Dissecting the Iron Mass Budget of the Intracluster Medium
• Core-collapse supernova enrichment in the core of the Virgo Cluster
• Shocking Features in the Merging Galaxy Cluster RXJ0334.2-0111
• Understanding the X-ray Flaring from Eta Car
• XMM-Newton observations of the Galactic Centre Region - I: The distribution of low-luminosity X-ray sources
• Sloshing cold fronts in galaxy groups and their perturbing disk galaxies: an X-ray, Optical and Radio Case Study
• Activity and rotation of the X-ray emitting Kepler stars
• Suzaku Spectroscopy Study of Hard X-Ray Emission in the Arches Cluster
• Chandra and XMM-Newton X-ray observations of AWM 7 - I: Investigating X-ray surface brightness fluctuations
• XMM-Newton Witness of M86 X-ray Metamorphosis
• A2163: Merger events in the hottest Abell galaxy cluster II. Subcluster accretion with galaxy-gas separation
• Multiwavelength observations of V407 Lupi (ASASSN-16kt) --- a very fast nova erupting in an intermediate polar
• Searching for the 3.5 keV Line in the Stacked Suzaku Observations of Galaxy Clusters
• XMM-Newton spectroscopy of the metal depleted T Tauri star TWA 5
• Testing the galaxy cluster mass-observable relations at z = 1 with XMM-Newton and Chandra observations of XLSSJ022403.9-041328
• X-Ray Flaring on the dMe Star, Ross 154
• Stability of Cool Cores During Galaxy Cluster Growth: A Joint $Chandra$/SPT Analysis of 67 Galaxy Clusters Along a Common Evolutionary Track Spanning 9 Gyr
• The MUSCLES Extension for Atmospheric and Transmission Spectroscopy: UV and X-ray Host-star Observations for JWST ERS & GTO Targets
• Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters
• On the X-ray and optical properties of the Be star HD 110432: a very hard-thermal X-ray emitter
• The XMM-Newton view of NGC 6251
• Establishing the X-ray Source Detection Strategy for eROSITA with Simulations
• X-ray properties expected from AGN feedback in elliptical galaxies
• Inside the core of a young massive star cluster: 3D MHD simulations
• A Compton thick AGN in the barred spiral NGC 4785
• Arithmetic with X-ray images of galaxy clusters: effective equation of state for small-scale perturbations in the ICM
• Investigating the X-ray emission from the massive WR+O binary WR 22 using 3D hydrodynamical models
• Chandra/HETGS Observations of the Capella System: the Primary as a Dominating X-ray Source
• A joint XMM-NuSTAR observation of the galaxy cluster Abell 523: constraints on Inverse Compton emission
• Variegate galaxy cluster gas content: Mean fraction, scatter, selection effects and covariance with X-ray luminosity
• Dark matter line emission constraints from NuSTAR observations of the Bullet Cluster
• The effect of feedback on the emission properties of the Warm-Hot Intergalactic Medium
• Finding Fossil Groups: Optical Identification and X-ray Confirmation
• Sub-galactic scaling relations between X-ray luminosity, star-formation rate, and stellar mass
• Fe IX Calculations for the Solar Dynamics Observatory
• Tracing High-Energy Radiation from T Tauri Stars Using Mid-Infrared Neon Emission from Disks
• Polarization of X-ray lines from galaxy clusters and elliptical galaxies - a way to measure tangential component of gas velocity
• Simulating Astro-H Observations of Sloshing Gas Motions in the Cores of Galaxy Clusters
• Constraining SIDM with halo shapes: revisited predictions from realistic simulations of early-type galaxies
• WD 1145+017: Optical Activity During 2016-2017 and Limits on the X-Ray Flux
• The XXL survey XXXV. The role of cluster mass in AGN activity
• The X-ray catalog of spectroscopically identified Galactic O stars: Investigating the dependence of X-ray luminosity on stellar and wind parameters
• X-ray and SZ constraints on the properties of hot CGM
• X-ray, UV and optical analysis of supergiants: $\epsilon$ Ori
• A critical assessment of the metal content of the ICM
• NuSTAR observations of the powerful radio-galaxy Cygnus A
• A Pilot Deep Survey for X-Ray Emission from fuvAGB Stars
• AGN activity and the misaligned hot ISM in the compact radio elliptical NGC4278
• The Complicated Evolution of the ACIS Contamination Layer over the Mission Life of the Chandra X-ray Observatory
• Multiwavelength observations of a giant flare on CN Leonis III. Temporal evolution of coronal properties
• Simulation tests of galaxy cluster constraints on chameleon gravity
• X-ray emission from Planetary Nebulae. I. Spherically symmetric numerical simulations
• A Study of High-redshift AGN Feedback in SZ Cluster Samples
• Stellar Coronae, Solar Flares: a Detailed Comparison of sigma Gem, HR 1099, and the Sun in High-resolution X-rays
• No Transition Disk? Infrared Excess, PAH, H2, and X-rays from the Weak-Lined T Tauri Star DoAr 21
• The X-ray luminosity-temperature relation of a complete sample of low-mass galaxy clusters
• Multiwavelength Signatures of Magnetic Activity from Young Stellar Objects in the LkH\alpha101 Cluster
• Two Distinct-Absorption X-Ray Components from Type IIn Supernovae: Evidence for Asphericity in the Circumstellar Medium
• The Role of Diffusive Shock Acceleration on Nonequilibrium Ionization in Supernova Remnant Shocks II: Emitted Spectra
• Numerical simulations of supernova remnants in turbulent molecular clouds
• X-ray-inferred kinematics of the core ICM in Perseus-like clusters: Insights from the TNG-Cluster simulation
• The RS CVn type star GT Mus shows most energetic X-ray flares throughout the 2010s
• Optical and X-ray studies of chromospherically active stars : FR Cancri, HD 95559 and LO Pegasi
• A multi-wavelength study of Supernova Remnants in six nearby galaxies. I: Detection of new X-ray selected Supernova Remnants with Chandra
• X-ray emission from cosmic web filaments in SRG/eROSITA data
• Results from DROXO. III. Observation, source list and X-ray properties of sources detected in the "Deep Rho Ophiuchi XMM-Newton Observation"
• Element abundances in X-ray emitting plasmas in stars
• The progenitor of SN 2011ja: Clues from circumstellar interaction
• An XMM-Newton observation of the galaxy group MKW 4
• Neon and oxygen in low activity stars: towards a coronal unification with the Sun
• Feedback, scatter and structure in the core of the PKS 0745-191 galaxy cluster
• Helium absorption in exoplanet atmospheres is connected to stellar coronal abundances
• Testing the companion hypothesis for the origin of the X-ray emission from intermediate-mass main-sequence stars
• Redshifted X-rays from the material accreting onto TW Hya: evidence of a low-latitude accretion spot
• The Entire Virial Radius of the Fossil Cluster RXJ1159+5531: I. Gas Properties
• The Mysterious Merger of NGC6868 and NGC6861 in the Telescopium Group
• The Radial Velocity and Mass of the White Dwarf of EX Hydrae Measured with Chandra
• Mixed-Morphology Supernova Remnants in X-rays: Isothermal Plasma in HB21 and Probable Oxygen-Rich Ejecta in CTB 1
• Discovery of a very young high-mass X-ray binary associated with the supernova remnant MCSNRJ0513-6724 in the LMC
• A Chandra Survey of Supermassive Black Holes with Dynamical Mass Measurements
• Inhomogeneous Metal Distribution in the Intra-Cluster Medium
• The warm-hot circumgalactic medium of the Milky Way as seen by eROSITA
• A Deep Chandra Observation of the AGN Outburst and Merger in Hickson Compact Group 62
• CHEX-MATE: Robust reconstruction of temperature profiles in galaxy clusters with XMM-Newton
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• Multi-wavelength campaign on NGC7469 I. The rich 640 ks RGS spectrum
• Pressure profiles of distant galaxy clusters in the Planck catalog
• The X-ray activity-rotation relation of T Tauri stars in Taurus-Auriga
• OI Fluorescent Line Contamination in Soft X-Ray Diffuse Background Obtained with Suzaku/XIS
• Modelling the thermal X-ray emission around the Galactic Centre from colliding Wolf-Rayet winds
• X-ray spectra of the Fe-L complex II: atomic data constraints from EBIT experiment and X-ray grating observations of Capella
• Chandra high resolution spectroscopy of the circumnuclear matter in the Broad Line Radio Galaxy 3C445
• Suzaku spectra of a Type II Supernova Remnant Kes 79
• SRG/eROSITA X-ray shadowing study of giant molecular clouds
• XMM-Newton spectral properties of the Ultraluminous IRAS Galaxy Mrk 273
• NuSTAR measurement of the cosmic X-ray background in the 3-20 keV energy band
• IC 3639 - A new bona fide Compton thick AGN unveiled by NuSTAR
• Uniform Contribution of Supernova Explosions to the Chemical Enrichment of Abell 3112 out to R200
• Suzaku Metal Abundance Patterns in the Outflow Region of M82 and the Importance of Charge Exchange
• The Effects of Clumps in Explaining X-ray Emission Lines from Hot Stars
• Chemical abundances in Sgr A East: evidence for a Type Iax supernova remnant
• Suzaku Observations of HESS J1616-508: Evidence for a Dark Particle Accelerator
• Simulations of Mixed Morphology Supernova Remnants With Anisotropic Thermal Conduction
• X-Ray Determination of the Variable Rate of Mass Accretion onto TW Hydrae
• Expansion of Kes 73, a Shell Supernova Remnant Containing a Magnetar
• Stellar X-ray sources in the Chandra COSMOS survey
• Origin of asymmetries in X-ray emission lines from the blast wave of the 2014 outburst of nova V745 Sco
• The bow shock, cold fronts and disintegrating cool core in the merging galaxy group RXJ0751.3+5012
• A Hard X-ray Study of the Normal Star-Forming Galaxy M83 with NuSTAR
• Suzaku Spectroscopy of the Extended X-Ray Emission in M17
• Chandra Observations of SNR RCW 103
• Probing multiphase gas in local massive elliptical galaxies via multiwavelength observations
• Connection between planetary He I $\lambda$10830 Å absorption and extreme-ultraviolet emission of planet-host stars
• Detailed X-Ray Mapping of the Shocked Ejecta and Circumstellar Medium in the Galactic Core-Collapse Supernova Remnant G292.0+1.8
• The CHIANTI atomic database
• Mass-Metallicity Relation from Cosmological Hydrodynamical Simulations and X-ray Observations of Galaxy Groups and Clusters
• Chandra High Energy Transmission Gratings Spectra of V3890 Sgr
• Chemical enrichment of the complex hot ISM of the Antennae galaxies: I. Spatial and spectral analysis of the diffuse X-ray emission
• X-ray optical depth diagnostics of T Tauri accretion shocks
• Diffuse coronae in cosmological simulations of Milky Way-sized galaxies
• Dielectronic Recombination of Argon-Like Ions
• X-ray analysis of JWST's first galaxy cluster lens SMACS J0723.3-7327
• X-ray spectroscopy of the unsteady quiescent corona of AD Leo with Chandra
• X-ray Observations of the Supernova Remnant CTB 87 (G74.9+1.2): An Evolved Pulsar Wind Nebula
• Evolution of X-ray Activity in <25 Myr Old Pre-Main Sequence Stars
• Chandra X-Ray Study of Galactic Supernova Remnant G299.2-2.9
• Suzaku monitoring of the Wolf-Rayet binary WR140 around periastron passage: An approach for quantifying the wind parameters
• Detection of a pair of prominent X-ray cavities in Abell 3847
• XMM-Newton observation of MV Lyr and the sandwiched model confirmation
• Clumping and X-Rays in cooler B supergiant stars
• On the origin of central abundance drops in the intracluster medium of galaxy groups and clusters
• $NuSTAR$ Observations of Four Nearby X-ray Faint AGN: Low Luminosity or Heavy Obscuration?
• XMM-Newton observation of the young open cluster Blanco 1. I. X-ray spectroscopy and photometry
• XMM-Newton monitoring of the close pre-main-sequence binary AK Sco. Evidence of tide driven filling of the inner gap in the circumbinary disk
• Suzaku Observations of Metal Distributions in the Intracluster Medium of the Centaurus Cluster
• The Circum-Galactic Medium of MASsive Spirals I: Overview and a Case Study of NGC 5908
• The 2019 eruption of recurrent nova V3890 Sgr: observations by Swift, NICER and SMARTS
• An X-ray view of WLRGs/LINERs
• FUV and X-ray Observations of the Reverse Shock in the SMC SNR 1E 0102.2-7219
• NuSTAR Observations of AGN with Low Observed X-ray to [OIII] Luminosity Ratios: Heavily Obscured AGN or Turned-Off AGN?
• The effects of stellar dynamics on the X-ray emission of flat early-type galaxies
• Simulations of cosmic rays in large-scale structures: numerical and physical effects
• Detailed diagnostics of an X-ray flare in the single giant HR 9024
• Metal-mass-to-light ratios of the Perseus cluster out to the virial radius
• XMM-Newton and Suzaku X-ray Shadowing Measurements of the Solar Wind Charge Exchange, Local Bubble, and Galactic Halo Emission
• Evidence for a merger induced shock wave in ZwCl\,0008.8+5215 with {\it Chandra} and {\it Suzaku}
• The Atacama Cosmology Telescope: High-Resolution Sunyaev-Zel'dovich Array Observations of ACT SZE-selected Clusters from the Equatorial Strip
• Chandra's Discovery of Activity in the Quiescent Nuclear Black Hole of NGC 821
• Infrared and X-Ray Evidence of an AGN in the NGC 3256 Southern Nucleus
• On X-ray Optical Depth in the Coronae of Active Stars
• Multi-epoch analysis of the X-ray spectrum of the active galactic nucleus in NGC 5506
• A Chandra Observation of the Nearby Sculptor Group Sd Galaxy NGC 7793
• CSI 2264: Simultaneous optical and X-ray variability in pre-Main Sequence stars. I: Time resolved X-ray spectral analysis during optical dips and accretion bursts in stars with disks
• The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
• Modeling the mixed-morphology supernova remnant IC 443. Origin of its complex morphology and X-ray emission
• NuSTAR and Swift observations of the fast rotating magnetized white dwarf AE Aquarii
• Separating Thermal and Non-Thermal X-Rays in Supernova Remnants II: Spatially Resolved Fits to SN1006 AD
• Cavities, shocks and a cold front around 3C 320
• A test for the theory of colliding winds: the periastron passage of 9 Sagittarii I. X-ray and optical spectroscopy
• X-raying hot plasma in solar active regions with the SphinX spectrometer
• Chandra Observation of Abell 2065: An Unequal Mass Merger?
• The Great Flare of 2021 November 19 on AD Leo. Simultaneous XMM-Newton and TESS observations
• Studying the Warm-Hot Intergalactic Medium in Emission
• Accretion onto the Companion of Eta Carinae During the Spectroscopic Event: III. the He II 4686 Line
• Digging for red nuggets: discovery of hot halos surrounding massive, compact, relic galaxies
• X-ray to NIR emission from AA Tauri during the dim state - Occultation of the inner disk and gas-to-dust ratio of the absorber
• X-Ray and Infrared Observations of Embedded Young Stars in L1630
• The evolution of the warm absorber reveals a shocked outflow in the narrow line Seyfert 1 galaxy IRAS 17020+4544
• Suzaku Observations of Thermal and Non-Thermal X-Ray Emission from the Middle-Aged Supernova Remnant G156.2+5.7
• Some Like it Hot: The X-Ray Emission of The Giant Star YY Mensae
• Search for gas bulk motions in eight nearby clusters of galaxies with Suzaku
• Resolving the Inner Arcsecond of the RY Tau Jet With HST
• Probing Wolf-Rayet Winds: Chandra/HETG X-Ray Spectra of WR 6
• A search for active galactic nuclei in low-mass compact galaxies
• XMM-Newton view of the N 206 superbubble in the Large Magellanic Cloud
• Hard X-rays from Ultra-Compact HII Regions in W49A
• Dark matter-baryons separation at the lowest mass scale: the Bullet Group
• X-ray emission from the double-binary OB-star system QZ Car (HD 93206)
• Suzaku Observations of Iron K-lines from the Intracluster Medium of the Coma Cluster
• High-resolution X-ray spectroscopy of the stellar wind in Vela X-1 during a flare
• Impact of supernova and cosmic-ray driving on the surface brightness of the galactic halo in soft X-rays
• An XMM-Newton study of the RGH 80 galaxy group
• Chandra/ACIS-I study of the X-ray properties of the NGC 6611 and M16 stellar population
• Metal distributions out to 0.5 r180 in the intracluster medium of four galaxy groups observed with Suzaku
• A multi-wavelength study of SXP 1062, the long period X-ray pulsar associated with a supernova remnant
• The XXL Survey VII: A supercluster of galaxies at z=0.43
• X-Ray emission from SN 2004dj: A Tale of Two Shocks
• Reconstruction of Radio Relics and X-ray Tails in an Off-axis Cluster Merger: Hydrodynamical Simulations of A115
• A deep Chandra observation of the poor cluster AWM 4 - I. Properties of the central radio galaxy and its effects on the intracluster medium
• Is the Cygnus Superbubble a Hypernova Remnant?
• Galaxy Clusters at z>=1: Gas Constraints from the Sunyaev-Zel'dovich Array
• New deep XMM-Newton observations to the west of the sigma Orionis cluster
• CHEX-MATE: Characterization of the intra-cluster medium temperature distribution
• Building a cluster: shocks, cavities, and cooling filaments in the group-group merger NGC 6338
• Using Multiwavelength Variability to Explore the Connection between X-ray Emission, the Far-Ultraviolet H2 Bump, and Accretion in T Tauri Stars
• Suzaku observations of the type 2 QSO in the central galaxy of the Phoenix cluster
• An X-ray survey of low-mass stars in Trumpler 16 with Chandra
• Jet-related Excitation of the [CII] Emission in the Active Galaxy NGC 4258 with SOFIA
• Beyond XSPEC: Towards Highly Configurable Analysis
• Extremely Dense Cores associated with Chandra Sources in Ophiuchus A: Forming Brown Dwarfs Unveiled?
• The origin of the chemical elements in cluster cores
• A study of X-ray emission of galaxies hosting molecular outflows (MOX sample)
• Phase-resolved XMM-Newton and swift observations of WR 25
• The complementary roles of feedback and mergers in building the gaseous halo and the X-ray corona of Milky Way-sized galaxies
• Nature of Compton-thick Active Galactic Nuclei in "Non-merging'' Luminous Infrared Galaxies UGC 2608 and NGC 5135 Revealed with Broadband X-ray Spectroscopy
• Anomalous X-ray line ratios in the cTTS TW Hya
• Doppler imaging an X-ray flare on the ultrafast rotator BO Mic - A contemporaneous multiwavelength study using XMM-Newton and VLT
• Diffraction-limited Subaru imaging of M82: sharp mid-infrared view of the starburst core
• Connecting turbulent velocities and magnetic fields in galaxy cluster simulations with active galactic nuclei jets
• Discovery of a pre-merger shock in an intercluster filament in Abell 98
• YSOVAR: Mid-infrared Variability Among YSOs in the Star Formation Region GGD 12-15
• Constraining hydrostatic mass bias of galaxy clusters with high-resolution X-ray spectroscopy
• Suzaku Observation of 30Dor C: A Supernova Remnant with the Largest Non-Thermal Shell
• Separating the BL Lac and Cluster X-ray Emissions in Abell 689 with Chandra
• Embedded Spiral Patterns in the Cool Core of the Massive Cluster of Galaxies Abell 1835
• Decomposition of galactic X-ray emission with Phox: Contributions from hot gas and XRBs
• The hot circumgalactic medium of the Milky-Way: new insights from XMM-Newton observations
• The Massively Accreting Cluster A2029
• Star Formation in the Outer Galaxy: Coronal Properties of NGC 1893
• Investigation of coronal properties of X-ray bright G-dwarf stars based on the solar surface magnetic field -- corona relation
• A MUSE view of the massive merging galaxy cluster ACT-CL J0102-4915 (El Gordo) at z = 0.87: robust strong lensing model and data release
• X-ray spectroscopy in the microcalorimeter era I: Effects of Fe XXIV Resonance Auger Destruction on Fe XXV K$\alpha$ spectra
• The enigmatic young brown dwarf binary FU Tau: accretion and activity
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• Chemical and physical parameters from X-ray high resolution spectra of the Galactic nova V959 Mon
• Detection of X-rays from the jet-driving Symbiotic Star MWC 560
• A Chandra View of the Normal SO Galaxy NGC 1332: II: Solar Abundances in the Hot Gas and Implications for SN Enrichment
• Nitrogen abundance in the X-ray halos of clusters and groups of galaxies
• X-ray spectroscopy of the hot has in the M31 bulge
• HFPK 334: An unusual Supernova Remnant in the Small Magellanic Cloud
• Frontier Fields Clusters: Deep Chandra Observations of the Complex Merger MACS J1149.6+2223
• An outburst scenario for the X-ray spectral variability in 3C 111
• Beyond the Ultra-deep Frontier Fields And Legacy Observations (BUFFALO): a high-resolution strong + weak-lensing view of Abell 370
• A Massive Cluster at z = 0.288 Caught in the Process of Formation: The Case of Abell 959
• The origin of X-ray coronae around simulated disc galaxies
• PALOMA: A Magnetic CV between Polars and Intermediate Polars
• Chandra ACIS Survey of M33 (ChASeM33): The enigmatic X-ray emission from IC131
• The Chandra Local Volume Survey: The X-ray Point Source Catalog of NGC 300
• Observation of the new emission line at ~3.5 keV in X-ray spectra of galaxies and galaxy clusters
• Intriguing X-ray and optical variations of the gamma Cas analog HD45314
• Multi-wavelength scaling relations in galaxy groups: a detailed comparison of GAMA and KiDS observations to BAHAMAS simulations
• The role of the artificial conductivity in SPH simulations of galaxy clusters: effects on the ICM properties
• Probing atmospheric escape through metastable He I triplet lines in 15 exoplanets observed with SPIRou
• Discovery of an extended X-ray jet in AP Librae
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• The Peculiar Multi-Wavelength Evolution Of V1535 Sco
• An Unexpected Discovery in the Rich Open Cluster NGC 6819 Using XMM-Newton
• The polyhedral nature of LINERs: An XMM-Newton view of LINERs in radio galaxies
• Universal transition diagram from dormant to actively accreting supermassive black holes
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• Searching for Diffuse Nonthermal X-Rays from the Superbubbles N11 and N51D in the Large Magellanic Cloud
• Projection effects in galaxy cluster samples: insights from X-ray redshifts
• A Multi-Wavelength Mass Analysis of RCS2 J232727.6-020437, a ~3x10${}^{15}$M${}_{\odot }$ Galaxy Cluster at z=0.7
• High-resolution X-ray Spectra Of The Symbiotic Star SS73 17
• Plasma-screening effects in the atrophysically relevant He-like and Li-like Mg and Fe ions
• Spectral Implications of Atomic Uncertainties in Optically-thin Hot Plasmas
• A Chandra Study of the Radio Galaxy NGC 326: Wings, Outburst History, and AGN Feedback
• HRC-I/Chandra X-ray observations towards sigma Orionis
• Dynamics of X-Ray-Emitting Ejecta in the Oxygen-Rich Supernova Remnant Puppis A Revealed by the XMM-Newton RGS
• X-ray emission from the giant magnetosphere of the magnetic O-type star NGC 1624-2
• An Environmental Study of the Ultraluminous X-ray Source Population in Early-type Galaxies
• Cutoff in the hard X-ray spectra of the ultraluminous X-ray sources HoIX X-1 and M82 X-1
• The corona and upper transition region of epsilon Eridani
• A new superwind galaxy: XMM-Newton observations of NGC 6810
• X-ray Irradiation of the LkCa 15 Protoplanetary Disk
• The Chandra ACIS Survey of M33 (ChASeM33): Investigating the Hot Ionized Medium in NGC604
• Hot Grain Dynamics by Electric Charging and Magnetic Trapping in Debris Disks
• A High Spectral Resolution Study of the Soft X-ray Background with the X-ray Quantum Calorimeter
• Unveiling the merger dynamics of the most massive MaDCoWS cluster at $z=1.2$ from a multi-wavelength mapping of its intracluster medium properties
• Suzaku and XMM-Newton Observations of the Fornax cluster: Temperature and Metallicity Distribution
• Flare X-ray observations of AB Dor: evidence for Stellar Coronal Opacity
• X-ray Spectroscopy of Clusters of Galaxies
• The SRG/eROSITA diffuse soft X-ray background. I. The local hot bubble in the western Galactic hemisphere
• A Supernova-driven, Magnetically-collimated Outflow as the Origin of the Galactic Center Radio Bubbles
• High energy emission component, population, and contribution to the extragalactic gamma-ray background of gamma-ray emitting radio galaxies
• Burn Out or Fade Away? On the X-ray and Magnetic Death of Intermediate Mass Stars
• Photospheric and coronal abundances in solar-type stars: the peculiar case of Tau Bootis
• HD45314: a new gamma Cas analog among Oe stars
• Modelling the Central Constant Emission X-ray component of eta Carinae
• The interstellar medium and the massive stellar content toward the SNR G18.1-0.1 and neighboring HII regions
• Hydrogen Column Density Variability in a Sample of Local Compton-Thin AGN
• Swift and XMM-Newton observations of an RS CVn type eclipsing binary SZ Psc: Superflare and coronal properties
• Effects of Multiphase Gas and Projection on X-ray Observables in Simulated Galaxy Clusters as Seen by eROSITA
• Suzaku X-ray Observations of the Nearest Non-Cool Core Cluster, Antlia: Dynamically Young but with Remarkably Relaxed Outskirts
• The Factory and the Beehive. IV. A Comprehensive Study of the Rotation X-ray Activity Relation in Praesepe and the Hyades
• Ionization of HeII in star-forming galaxies by X-rays from cluster winds and superbubbles
• The X-ray coronae of the two brightest galaxies in the Coma cluster
• Suzaku Detection of Super-hard X-ray Emission from the Classical Nova V2491 Cygni
• X-ray Emission from Young Stellar Objects in the εChamaeleontis Group: the Herbig Ae Star HD 104237 and Associated Low-Mass Stars
• X-ray ejecta kinematics of the Galactic core-collapse supernova remnant G292.0+1.8
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Search for Thermal X-ray Features from the Crab nebula with Hitomi Soft X-ray Spectrometer
• X-ray and EUV spectroscopy of various astrophysical and laboratory plasmas -- Collisional, photoionization and charge-exchange plasmas
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• The spectroscopically confirmed huge cosmic structure at z=0.55
• The History of Metal Enrichment Traced by X-ray Observations of High Redshift Galaxy Clusters
• A New Calculation of Ne IX Line Diagnostics
• X-ray properties of the white dwarf pulsar eRASSU J191213.9-441044
• Evidence for magnetic activity at starbirth: a powerful X-ray flare from the Class 0 protostar HOPS 383
• Investigating the hard X-ray emission from the hottest Abell cluster A2163 with Suzaku
• An X-ray and Radio Study of the Hubble Frontier Field Cluster Abell S1063
• The Importance of XUV Radiation as a Solution to the P V Mass Loss Rate Discrepancy in O-Stars
• Simulation view of galaxy clusters with low X-ray surface brightness
• Merging cold front and AGN feedback in the peculiar galaxy cluster Abell 2626
• AGN Feedback in galaxy groups: a detailed study of X-ray features and diffuse radio emission in IC1262
• Global modelling of X-ray spectra produced in O-type star winds
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray properties of Subaru optically-selected clusters
• The X-ray emission of gamma Cassiopeiae during the 2020-2021 disc eruption
• Testing a generalized cubic Galileon gravity model with the Coma Cluster
• SRGA J181414.6-225604: A new Galactic symbiotic X-ray binary outburst triggered by an intense mass loss episode of a heavily obscured Mira variable
• Intracluster medium of the merging cluster Abell 3395
• The X-ray Properties of Weak Lensing Selected Galaxy Clusters
• The Hot Interstellar Medium of the Interacting Galaxy NGC 4490
• Exploring the hot gaseous halo around an extremely massive and relativistic jet launching spiral galaxy with XMM-Newton
• Spatial Distribution of Metals in the ICM: Evolution of the Iron Excess in Relaxed Galaxy Clusters
• X-ray Point Source Populations Constituting the Galactic Ridge X-ray Emission
• The diffuse soft excess emission in the Coma cluster from the ROSAT All-Sky Survey
• Broadband X-ray Spectral Analysis of the Double-Nucleus Luminous Infrared Galaxy Mrk 463
• Suzaku Observation Adjacent to the South End of the Radio Arc
• Coronal X-Ray Emission from Nearby, Low-Mass, Exoplanet Host Stars Observed by the MUSCLES and Mega-MUSCLES HST Treasury Survey Projects
• Detection of non-thermal X-ray emission in the lobes and jets of Cygnus A
• Suzaku Observations of the X-ray Brightest Fossil Group ESO 3060170
• On The Road To More Realistic Galaxy Cluster Simulations: The Effects of Radiative Cooling and Thermal Feedback Prescriptions on the Observational Properties of Simulated Galaxy Clusters
• Competitive X-ray and Optical Cooling in the Collisionless Shocks of WR 140
• A detailed look at the thermal and non-thermal X-ray emission from the Vela supernova remnant with SRG/eROSITA
• Effect of the Metallicity on the X-ray Emission from the Warm-Hot Intergalactic Medium
• X-ray and optical spectroscopy of the massive young open cluster IC1805
• The high resolution X-ray spectrum of SNR 0506-68 using XMM-Newton
• Extended X-ray emission in PKS 1718$-$649
• Determining The Galactic Halo's Emission Measure from UV and X-ray Observations
• Testing the cooling flow model in the intermediate polar EX Hydrae
• Diffuse Thermal X-Ray Emission in the Core of the Young Massive Cluster Westerlund 1
• Suzaku Reveals Helium-burning Products in the X-ray Emitting Planetary Nebula BD+303639
• Asymmetries of Heavy Elements in the Young Supernova Remnant Cassiopeia A
• Suzaku X-Ray Spectroscopy of a Peculiar Hot Star in the Galactic Center Region
• The shared evaporation history of three sub-Neptunes spanning the radius-period valley of a Hyades star
• X-ray Constraints on Galaxy-Gas-Jet Interactions in the Dumbbell Galaxies NGC4782 and NGC4783 in the LGG316 Group
• A Fundamental Plane Relation for the X-Ray Gas in Normal Elliptical Galaxies
• Identification of a Jet-Driven Supernova Remnant in the Small Magellanic Cloud: Possible Evidence for the Enhancement of Bipolar Explosions at Low Metallicity
• X-ray Emission from the Taffy (VV254) Galaxies and Bridge
• X-Ray Emission from Planetary Nebulae Calculated by 1D Spherical Numerical Simulations
• The Stellar Population And Origin Of The Mysterious High-Latitude Star Forming Cloud CG 12
• Observations of asymmetric velocity fields and gas cooling in the NGC 4636 galaxy group X-ray halo
• Reflection-dominated nuclear X-ray emission in the early-type galaxy ESO 565--G019
• Search for WHIM around A2744 using Suzaku
• Discovery of recombining plasma inside the extended gamma-ray supernova remnant HB9
• Merger Hydrodynamics of the Luminous Cluster RXJ1347.5-1145
• The Norma Arm Region Chandra Survey: X-ray Populations in the Spiral Arms
• Gas Density Perturbations in Cool Cores of CLASH Galaxy Clusters
• Dissecting the X-ray Emission in the Young Planetary Nebula NGC 7027
• X-ray spectral and timing characteristics of the stars in the young open cluster IC 2391
• The XUV irradiation and likely atmospheric escape of the super-Earth $\pi$ Men c
• Evolution of X-ray spectra and light curves of V1494 Aquilae
• Suzaku study of gas properties along filaments of A2744
• A Detailed Archival CHANDRA Study of the Young Core-Collapse Supernova Remnant 1E 0102.2-7219 in the Small Magellanic Cloud
• The prototypical major cluster merger Abell 754. I. Calibration of MeerKAT data and radio/X-ray spectral mapping of the cluster
• The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
• The large-scale magnetic field of the eccentric pre-main-sequence binary system V1878 Ori
• X-Ray Spectroscopy of the Classical Nova V458 Vulpeculae with Suzaku
• X-ray emission from hydrodynamical simulations in non-LTE wind models
• The Structure of the Young Star Cluster NGC 6231. I. Stellar Population
• Asymmetric eROSITA bubbles as the evidence of a circumgalactic medium wind
• X-raying the AU Microscopii debris disk
• The XMM Cluster Survey analysis of the SDSS DR8 redMaPPer Catalogue: Implications for scatter, selection bias, and isotropy in cluster scaling relations
• X-ray spectroscopy of the starburst feedback in 30 Doradus
• How do atomic code uncertainties affect abundance measurements in the intracluster medium?
• Discovery of X-ray flaring activity in the Arches cluster
• Observational signatures of past mass-exchange episodes in massive binaries: The case of LSS 3074
• Solar Wind Charge Exchange contribution to the ROSAT All Sky Survey Maps
• The Chandra/HETG view of NGC 1365 in a Compton-thick state
• An Analysis of the Broadband (22-3900 MHz) Radio Spectrum of HB3 (G132.7+1.3): The Detection of Thermal Radio Emission from an Evolved Supernova Remnant?
• A Coordinated X-ray and Optical Campaign of the Nearby Massive Binary $\delta$ Orionis Aa: II. X-ray Variability
• X-ray flares on the UV Ceti-type star CC Eridani: a "peculiar" time-evolution of spectral parameters
• Molecules in the transition disk orbiting T Cha
• An XMM-Newton view of the merging activity in the Centaurus cluster
• A Survey of High Contrast Stellar Flares Observed by Chandra
• X-ray source population study of the starburst galaxy M83 with XMM-Newton
• X-ray absorption variability in NGC 4507
• A Systematic Comparison of Galaxy Cluster Temperatures Measured with NuSTAR and Chandra
• The eROSITA Final Equatorial-Depth Survey (eFEDS): A complete census of X-ray properties of Subaru Hyper Suprime-Cam weak lensing shear-selected clusters in the eFEDS footprint
• Narrow Radiative Recombination Continua: A Signature of Ions Crossing the Contact Discontinuity of Astrophysical Shocks
• Detecting Intracluster Gas Motion in Galaxy Clusters: Mock Astro-E2 Observations
• Decoding X-ray observations from centres of galaxy clusters using MCMC
• An Ejecta Kinematics Study of Kepler's Supernova Remnant with High-Resolution $Chandra$ HETG Spectroscopy
• New Insights into SNR Evolution Revealed by the Discovery of Recombining Plasmas
• The Effect of Helium Sedimentation on Galaxy Cluster Masses and Scaling Relations
• X-ray and Near-infrared Studies of a Star-forming Cloud; L1448
• The dynamical state of Abell 2399: a bullet-like cluster
• Checking Potassium origin of new emission line at 3.5 keV with K XIX line complex at 3.7 keV
• Suzaku Detection of Diffuse Hard X-Ray Emission outside Vela X
• X-Ray Superflares on CC Eri
• The complex circumnuclear environment of the broad-line radio galaxy 3C 390.3 revealed by Chandra HETG
• Testing Emergent Gravity on Galaxy Cluster Scales
• Years Delayed X-ray Afterglows of TDEs Originated from Wind-Torus Interactions
• A Chandra Study of Radial Temperature Profiles of the Intra-Cluster Medium in 50 Galaxy Clusters
• A multi-epoch X-ray study of the nearby Seyfert 2 galaxy NGC 7479: Linking column density variability to the torus geometry
• Chandra Imaging and Spectroscopy of the Eastern XA Region of the Cygnus Loop Supernova Remnant
• X-ray Diagnostics of Thermal Conditions of the Hot Plasmas in the Centaurus Cluster
• Low X-ray surface brightness clusters: Implications on the scatter of the $M-T$ and $L-T$ relations
• Optical and X-ray luminosity of expanding nebulae around ultraluminous X-ray sources
• X-ray/H$\alpha$ scaling relationships in stellar flares
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• X-ray spectra of the Fe-L complex III: systematic uncertainties in the atomic data
• Revealing the "missing" low-mass stars in the S254-S258 star forming region by deep X-ray imaging
• Gas sloshing and cold fronts in pre-merging galaxy cluster Abell 98
• Multiwavelength study of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field
• Origins of the 1/4 keV Soft X-Ray Background
• FUV line emission, gas kinematics, and discovery of [Fe XXI] $\lambda$1354.1 in the sightline towards a filament in M87
• A New Sample of Obscured AGNs Selected from the XMM-Newton and AKARI Surveys
• X-Ray Emission by A Shocked Fast Wind from the Central Stars of Planetary Nebulae
• X-ray Signatures of Non-Equilibrium Ionization Effects in Galaxy Cluster Accretion Shock Regions
• disnht: modeling X-ray absorption from distributed column densities
• Revealing a Highly-Dynamic Cluster Core in Abell 1664 with Chandra
• Multi-frequency study of DEM L299 in the Large Magellanic Cloud
• Gas absorption and dust extinction towards the Orion Nebula Cluster
• Inverse-Compton Emission from Clusters of Galaxies: Predictions for ASTRO-H
• Deep XMM-Newton observation of the Eta Chamaleontis cluster
• Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
• An X-ray and SZ bright diffuse source toward M31: a Local Hot Bridge
• Deep Chandra observations of diffuse hot plasma in M83
• LO Peg: surface differential rotation, flares, and spot-topographic evolution
• The advection-dominated accretion flow+thin accretion disk model for two low-luminosity active galactic nuclei: M81 and NGC4579
• A confined dynamo: magnetic activity of the K-dwarf component in the pre-cataclysmic binary system V471 Tauri
• A Grid of Core-Collapse Supernova Remnant Models I: The Effect of Wind-Driven Mass-Loss
• Formation of X-ray emitting stationary shocks in magnetized protostellar jets
• The first all-sky survey of star-forming galaxies with eROSITA: Scaling relations and a population of X-ray luminous starbursts
• X-Ray observations of a subhalo associated with the NGC 4839 group infalling toward the Coma cluster
• X-Ray Studies of the Abell 3158 Galaxy Cluster with eROSITA
• Chandra observations of dying radio sources in galaxy clusters
• Hydrodynamical simulations of the jet in the symbiotic star MWC 560 III. Application to X-ray jets in symbiotic stars
• RAiSE X: searching for radio galaxies in X-ray surveys
• Hydrostatic Mass Profiles of Galaxy Clusters in the eROSITA Survey
• X-ray emission from a brown dwarf in the Pleiades
• X-ray Emission and Corona of the Young Intermediate Mass Binary ${\theta }^1$ Ori E
• Thermal X-ray iron line emission from the advection dominated accretion flow in the galactic binary GX 339-4
• The Chandra view of the Largest Quasar Lens SDSS J1029+2623
• Low energy range dielectronic recombination of Fluorine-like Fe17+ at the CSRm
• X-ray emission from star cluster winds in starburst galaxies
• SNR 0104-72.3: A remnant of Type Ia Supernova in a Star-forming region?
• Laboratory evidence for asymmetric accretion structure upon slanted matter impact in young stars
• CTIO, ROSAT HRI and Chandra ACIS Observations of the Archetypical Mixed-Morphology Supernova Remnant W28 (G6.4-0.1)
• Pairs of Giant Shock Waves (N-Waves) in Merging Galaxy Clusters
• Searching for the pulsar in G18.95-1.1: Discovery of an X-ray point source and associated synchrotron nebula with Chandra
• A Deep Chandra View of the NGC 404 Central Engine
• Hot Interstellar Gas and Stellar Energy Feedback in the Antennae Galaxies
• Diffuse X-ray emission from the superbubbles N 70 and N 185 in the Large Magellanic Cloud
• On the binary nature of massive blue hypergiants: high-resolution X-ray spectroscopy suggests that Cyg OB2 12 is a colliding wind binary
• X-ray spectroscopy of galaxy clusters: beyond the CIE modeling
• Discovery of large-scale diffuse radio emission and of a new galaxy cluster in the surroundings of MACSJ0520.7-1328
• The Exceptional X-ray Evolution of SN1996cr in High Resolution
• Feeding and feedback in the powerful radio galaxy 3C 120
• SRG/eROSITA and XMM-Newton observations of Vela Jr
• LOFAR Detection of a Low-Power Radio Halo in the Galaxy Cluster Abell 990
• Abundance Patterns in the Interstellar Medium of the S0 Galaxy NGC 1316 (Fornax A) Revealed with Suzaku
• Evidence for Resonance Line Scattering in the Suzaku X-ray Spectrum of the Cygnus Loop
• XMM-Newton survey of two Upper Scorpius regions
• Are the Effects of Structure Formation Seen in the Central Metallicity of Galaxy Clusters?
• A Deep Chandra Observation of Oxygen-Rich Supernova Remnant B0049-73.6 in the Small Magellanic Cloud
• Soft X-ray Spectroscopy of the Cygnus Loop Supernova Remnant
• Impact of thermal diffusion and other abundance anomalies on cosmological uses of galaxy clusters
• Hydrostatic gas distributions: global estimates of temperature and abundance
• Stellar kinematics of X-ray bright massive elliptical galaxies
• Signatures of multiple episodes of AGN activity in the core of Abell 1795
• Outstanding X-ray emission from the stellar radio pulsar CU Virginis
• The unusual morphology of the intragroup medium in NGC 5171
• Neutral iron line in the supernova remnant IC 443 and implications for MeV cosmic rays
• A Search For X-ray Emission From Colliding Magnetospheres In Young Eccentric Stellar Binaries
• Constraining density and metallicity of the Milky Way's hot gas halo from O VII spectra and ram-pressure stripping
• Suzaku Observations of the Merging Cluster Abell 85: Temperature Map and Impact Direction
• The Solar-Cycle Temporal Variation of the Solar Wind Charge Exchange X-ray Lines
• Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
• Long-term soft and hard X-ray investigation of the colliding wind WN+O binary WR 25
• First Study of the Supernova Remnant Population in the Large Magellanic Cloud with eROSITA
• EBIT Observation of Ar Dielectronic Recombination Lines Near the Unknown Faint X-Ray Feature Found in the Stacked Spectrum of Galaxy Clusters
• A Galaxy Merger Scenario for the NGC 1550 Galaxy from Metal Distributions in the X-ray Emitting Plasma
• The nature of the high Galactic latitude O-star HD93521: new results from X-ray and optical spectroscopy
• Early multiwavelength analysis of the recurrent nova V745 Sco
• Distribution of Si, Fe, and Ni in the Intracluster Medium of the Coma Cluster
• Recovering Swift-XRT energy resolution through CCD charge trap mapping
• A Large X-ray Flare from a Single Weak-lined T Tauri Star TWA-7 Detected with MAXI GSC
• Long-term X-ray Variability of the Symbiotic System RT Cru based on Chandra Spectroscopy
• Spatially Resolved X-ray Study of Supernova Remnant G306.3$-$0.9 with Unusually High Calcium Abundance
• The WARPS Survey. VIII. Evolution of the Galaxy Cluster X-ray Luminosity Function
• The nature of the broadband X-ray variability in the dwarf Seyfert galaxy NGC 4395
• Multi-wavelength analysis of the Galactic supernova remnant MSH 11-61A
• An X-ray spectroscopic search for dark matter and unidentified line signatures in the Perseus cluster with Hitomi
• Suzaku observations of a shock front tracing the western edge of the giant radio halo in the Coma Cluster
• A Spatially Resolved Study of X-ray Properties in Superbubble 30 Dor C with $XMM-Newton$
• The corona of GJ 1151 in the context of star-planet interaction
• XMM-Newton observation of the interacting galaxies NGC1512 and NGC1510
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Asymmetry in The Observed Metal-Rich Ejecta of Galactic Type Ia Supernova Remnant G299.2-2.9
• Merger Signatures in the Galaxy Cluster Abell 98
• An XMM-Newton Study of the Coronae of ${\sigma }^2$ Coronae Borealis
• On the Observability of Recurrent Nova Super-Remnants
• Abundance Patterns in the Interstellar Medium of Early-type Galaxies Observed with Suzaku
• Neural network-based preprocessing to estimate the parameters of the X-ray emission of a single-temperature thermal plasma
• Suzaku Follow-up of Heavily Obscured Active Galactic Nuclei Detected in Swift/BAT Survey: NGC 1106, UGC 03752, and NGC 2788A
• Exploring the supernova remnant G308.4-1.4
• Recombining Plasma & Gamma-ray Emission in the Mixed-morphology Supernova Remnant 3C 400.2
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• The soft X-ray background with Suzaku: I. Milky Way halo
• An XMM-Newton Study of the Mixed-Morphology Supernova Remnant G346.6-0.2
• A cluster pair : A3532 and A3530
• Soft X-ray emission from warm gas in IllustrisTNG circum-cluster environments
• Suzaku Observations of the Cluster Outskirts and Intercluster Filament in the Triple Merger Cluster Abell 98
• Chandra follow up of the Hectospec Cluster Survey: Comparison of Caustic and Hydrostatic Masses and Constraints on the Hydrostatic Bias
• Fluorescent Fe K line emission of gamma Cas stars I. Do gamma Cas stars host propelling neutron stars?
• Reconstructing the projected gravitational potential of Abell 1689 from X-ray measurements
• The eROSITA Final Equatorial Depth Survey (eFEDS): the hard X-ray selected sample
• Coronae of Stars with Super Solar Elemental Abundances
• Suzaku Detection of Thermal X-Ray Emission Associated with the Western Radio Lobe of Fornax A
• Characterizing the X-ray Emission of Intermediate-Mass Pre-Main-Sequence Stars
• Constraints on precipitation-limited hot halos from massive galaxies to galaxy clusters
• A weak lensing analysis of the PLCK G100.2-30.4 cluster
• SNR 0453-68.5: An Asymmetric Remnant and its Plerion in the Large Magellanic Cloud
• The cooling, mass and radius of the neutron star in EXO 0748-676 in quiescence with XMM-Newton
• Systematic Perturbations of the Thermodynamic Properties in Cool Cores of HIFLUGCS Galaxy Clusters
• Suzaku observations of the low surface brightness cluster A76
• The Galaxy Cluster 'Pypeline' for X-ray Temperature Maps: ClusterPyXT
• A comprehensive study of NGC 2023 with XMM-Newton and Spitzer
• Chandra Observation of Abell 1142: A Cool-Core Cluster Lacking a Central Brightest Cluster Galaxy?
• Puzzling X-rays from the new colliding wind binary WR65
• Star formation history of Canis Major OB1 - II. A bimodal X-ray population revealed by XMM-Newton
• X-ray Study of Rekindled Accretion in the Classical Nova V2491 Cygni
• An X-ray study of coronally connected active eclipsing binaries
• Spatially-Resolved Study of Recombining Plasma in W49B Using XMM-Newton
• A Suzaku Study of Ejecta Structure and Origin of Hard X-ray Emission in the Supernova Remnant G156.2+5.7
• Environment from cross-correlations: connecting hot gas and the quenching of galaxies
• A Chandra Study of the Image Power Spectra of 41 Cool Core and Non-Cool Core Galaxy Clusters
• Unveiling the AGN in IC 883: discovery of a parsec-scale radio jet
• Discovery of Extended X-Ray emission from the unidentified TeV source HESS J1614-518 using the Suzaku Satellite
• Multi-frequency study of the newly confirmed supernova remnant MCSNR J0512-6707 in the Large Magellanic Cloud
• Evidence for non-thermal X-ray emission from the double WR colliding-wind binary Apep
• Suzaku Observation of the Fermi Cygnus Cocoon: Search for a Signature of Young Cosmic-Ray Electrons
• X-ray Light Curves and Accretion Disk Structure of EX Hydrae
• The X-ray Ribs Within the Cocoon Shock of Cygnus A
• An XMM-Newton study of active-inactive galaxy pairs
• New Insights with XRISM & Cloudy: A novel Column Density Diagnostic
• Constraints on the winds of hot subdwarf stars from X-ray observations of two sdB binaries with compact companions: CD -30 11223 and PG 1232-136
• Spatial Distribution of Abundance Patterns in the Starburst Galaxy NGC 3079 Revealed with Chandra and Suzaku
• Unveiling the nature of RX J0002+6246 with XMM-Newton
• Electron density diagnostic for hot plasmas in coronal regime by using B-like ions
• Coronal density diagnostics with Si X: CHANDRA/LETGS observations of Procyon, $\alpha$ Cen A$&$B, Capella and $\epsilon$ Eri
• Phase resolved X-ray spectroscopy of HDE228766: Probing the wind of an extreme Of+/WNLha star
• The electron energy-loss rate due to radiative recombination
• The X-ray footprint of the CircumNuclear Disk
• Properties of the circumgalactic medium in simulations compared to observations
• Simulations of the merging cluster of galaxies Cygnus A
• X-ray Spectra from Plasmas with High-Energy Electrons: kappa-distributions and e-e Bremsstrahlung
• Deciphering the Nature of the Pulsar Wind Nebula CTB 87 with XMM-Newton
• A HaloSat Analysis of the Cygnus Superbubble
• The Relative Supernovae Contribution to the Chemical Enrichment History of Abell 1837
• The formation and stability of a cold disc made out of stellar winds in the Galactic Centre
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• Mixing of hot shocked plasma with cold gas in Nova YZ Ret 2020
• AXES-2MRS: A new all-sky catalogue of extended X-ray galaxy groups
• X-ray Emissions from the Jovian System
• The high energy spectrum of Proxima Centauri simultaneously observed at X-ray and FUV wavelengths
• Line-of-sight Elongation and Hydrostatic Mass Bias of the Frontier Fields Galaxy Cluster Abell 370
• The velocity structure of the intracluster medium during a major merger: simulated microcalorimeter observations
• Quest for the upcoming periastron passage of an episodic dust maker and particle accelerating colliding wind binary: WR 125
• Constraining black hole feedback in galaxy clusters from X-ray power spectra
• Nova LMC 2009a as observed with XMM-Newton, compared with other novae
• The Merger Dynamics of the Galaxy Cluster Abell 1775: New Insights from Chandra and XMM-Newton for a Cluster Simultaneously Hosting a WAT and a NAT Radio Sources
• Constraining the Milky Way Mass with Its Hot Gaseous Halo
• Introducing constrained matched filters for improved separation of point sources from galaxy clusters
• Structure of X-ray emitting jets close to the launching site: from embedded to disk-bearing sources
• Suzaku Observations of Low Surface Brightness Cluster Abell 1631
• The long-period massive binary HD~54662 revisited
• X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field
• XMM-Newton X-ray Observations of LkCa 15: A T Tauri Star With a Formative Planetary System
• Broad-band X-ray spectra of anomalous X-ray pulsars and soft $\gamma$-ray repeaters: pulsars in a weak-accretion regime ?
• A Coordinated X-ray and Optical Campaign on the Nearest Massive Eclipsing Binary, Delta Ori Aa: I. Overview of the X-ray Spectrum
• X-ray and Radio Follow-up Observations of High-Redshift Blazar Candidates in the Fermi-LAT Unassociated Source Population
• An XMM-Newton view of the M17 nebula
• Discovery of a Pulsar Wind Nebula Candidate in the Cygnus Loop
• No X-Ray Excess from the HESS J1741-302 Region except a New Intermediate Polar Candidate
• A detailed study of the rise phase of a long duration X-ray flare in the young star TWA 11B
• The Chandra X-ray view of the power sources in Cepheus A
• Chandra Observation of the Cluster of Galaxies MS 0839.9+2938 at z=0.194: the Central Excess Iron and SN Ia Enrichment
• A Deep Look at the T-Type Brown Dwarf Binary $\epsilon$ Indi Bab with Chandra and ATCA
• The Collisional and Photoionized Plasma in the Polarized NLS1 galaxy Mrk 1239
• Chandra X-ray Measurement of Gas-phase Heavy Element Abundances in the Central Parsec of the Galaxy
• SPT-CL J2215-3537: A Massive Starburst at the Center of the Most Distant Relaxed Galaxy Cluster
• The Abundance Pattern of O, Ne, Mg, and Fe in the Interstellar Medium of S0 Galaxy NGC 4382 Observed with Suzaku
• Scaling relations of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program Field
• The NuSTAR and Chandra view of CL 0217+70 and Its Tell-Tale Radio Halo
• Multi-wavelength study of NGC 1365: The obscured active nucleus and off-nuclear compact X-ray sources
• Joint HST, VLT/MUSE and XMM-Newton observations to constrain the mass distribution of the two strong lensing galaxy clusters: MACS J0242.5-2132 & MACS J0949.8+1708
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• The ionised X-ray outflowing torus in ESO 323-G77: low-ionisation clumps confined by homogeneous warm absorbers
• A compact flare eclipsed in the corona of SV Cam
• How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
• XMM-Newton EPIC and OM observation of Nova Centauri 1986 (V842 Cen)
• Measuring the X-ray luminosities of DESI groups from eROSITA Final Equatorial-Depth Survey: I. X-ray luminosity -- halo mass scaling relation
• Charge exchange emission and cold clumps in multi-phase galactic outflows
• Chandra Observations of the field containing HESS J1616-508
• XMM-Newton Observations of the Southeastern Radio Relic in Abell 3667
• Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zel'dovich measurements
• X-ray Spectra and Light Curves of Cooling Novae and a Nova-Like
• Suzaku Observations of the cluster of galaxies Abell 2052
• X-Atlas: An Online Archive of Chandra's Stellar High Energy Transmission Gratings Observations
• Tracing the ejecta structure of SN 1987A: Insights and diagnostics from 3D MHD simulations
• SUZAKU Observation of a New Merging Group of Galaxies at a Filamentary Junction
• Suzaku Analysis of the Supernova Remnant G306.3-0.9 and the Gamma-ray View of Its Neighborhood
• Suzaku Observation of the Metallicity in the Interstellar Medium of NGC 4258
• SWIFT J0503.7-2819: A nearly synchronous intermediate polar below the period gap?
• Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium
• On the nature of EXO 0423.4-0840
• An X-ray high-frequency quasi-periodic oscillation in NGC 1365
• Multiple giant eruptions and X-ray emission in the recoiling AGN/LBV candidate SDSS1133
• G189.6+03.3: the first complete X-ray view provided by SRG/eROSITA
• Variable Hard X-ray Emission from the Candidate Accreting Black Hole in Dwarf Galaxy Henize 2-10
• An X-ray flare from 47 Cas
• Correlation between centre offsets and gas velocity dispersion of galaxy clusters in cosmological simulations
• Global X-Ray Properties of the Vela and Puppis A Supernova Remnants
• The XMM Cluster Survey: Exploring scaling relations and completeness of the Dark Energy Survey Year 3 redMaPPer cluster catalogue
• Observations of a Radio-quiet Solar Preflare
• The XXL Survey: XXXIII. Chandra Constraints on the AGN Contamination of z > 1 XXL Galaxy Clusters
• AstroSat observations of long-duration X-ray superflares on active M-dwarf binary EQ Peg
• Suzaku Constraints on the Soft and Hard Excess Emissions from Abell 2199
• An X-ray upper limit on the presence of a Neutron Star for the Small Magellanic Cloud and Supernova Remnant 1E0102.2-7219
• The Effect of Molecular Cloud Properties on the Kinematics of Stars Formed in the Trifid Region
• Redshift evolution of the 1.4 GHz volume averaged radio luminosity function in clusters of galaxies
• Ion-by-Ion DEM Determination: I. Method
• The Hercules cluster in X-rays with $XMM$-$Newton$ and $Chandra$
• A Chandra Study: Are Dwarf Carbon Stars Spun Up and Rejuvenated by Mass Transfer?
• New radiative loss curve from updates to collisional excitation in the low-density, optically thin plasmas in SPEX
• The origin of an extended X-ray emission apparently associated with the globular cluster 47 Tucanae
• The First Candidate Colliding-Wind Binary in M33
• Testing the rotation versus merger scenario in the galaxy cluster Abell 2107
• XMM-Newton Measurement of the Galactic Halo X-ray Emission using a Compact Shadowing Cloud
• Dynamics of ten clusters of galaxies with substructures
• A WHIM origin for the soft excess emission in the Coma cluster
• The XXL Survey: XLVIII; X-ray follow-up of distant XXL clusters: Masses, scaling relations and AGN contamination
• MACS J0553.4-3342: A young merging galaxy cluster caught through the eyes of Chandra and HST
• Suzaku Spectroscopy of Vela Shrapnel B
• DN Tauri - coronal activity and accretion in a young low-mass CTTS
• X-Raying the Dark Side of Venus - Scatter from Venus Magnetotail?
• The XMM Cluster Survey: An independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies
• Contemporaneous XMM-Newton investigation of a giant X-ray flare and quiescent state from a cool M-class dwarf in the local cavity
• Deep Near-infrared Imaging Observation of the Faint X-ray Point Sources Constituting the Galactic Bulge X-ray Emission
• X-ray Emission from the Exoplanet Hosting LTT 1445 Triple Star System
• A Swift view of X-ray and UV radiation in the planet-forming T-Tauri system PDS 70
• Radial X-ray profiles of simulated galaxies: Contributions from hot gas and XRBs
• Probing the Halo Gas Distribution in the Inner Galaxy with Fermi Bubble Observations
• eROSITA narrowband maps at the energies of soft X-ray emission lines
• Studying galaxy cluster morphological metrics with Mock-X
• NIRPS detection of delayed atmospheric escape from the warm and misaligned Saturn-mass exoplanet WASP-69b
• Computation of the transmitted and polarized scattered fluxes by the exoplanet HD 189733b in X-rays
• Hard X-ray emission from the core of the Perseus cluster and the thermal content of the radio bubbles
• The high-energy environment of the heavy sub-Earth GJ 367 b indicates likely complete evaporation of its atmosphere
• X-ray Variability in the Symbiotic Binary RT Cru: Principal Component Analysis
• Long-term X-ray variation of the colliding wind Wolf-Rayet binary WR 125
• Suzaku Discovery of Twin Thermal Plasma from the Tornado Nebula
• Theoretical X-ray light curves of young SNe II: the example of SN 2013ej
• X-ray line formation in the spectrum of SS 433
• The Young Binary DQ Tau Produces Another X-ray Flare Near Periastron
• X-ray emission in the enigmatic CVSO 30 system
• Exploring the multiphase medium in MKW 08: from the central active galaxy up to cluster scales
• Detection of a Cool, Accretion Shock-Generated X-ray Plasma in EX Lupi During the 2008 Optical Eruption
• X-ray and UV observations of V751 Cyg in an optical high state
• A Novel Machine Learning Approach to Disentangle Multi-Temperature Regions in Galaxy Clusters
• Revisit the Circumnuclear X-ray Emission of NGC 2992 in a Historically Low State
• Spectral Indications of Density Variability in the Corona of AD Leonis
• Multi-band observations of Swift J0840.7-3516: a new transient ultra-compact X-ray binary candidate
• A systematic cross-search for radio/infrared counterparts of XMM-Newton sources
• The Origin of the X-ray Emission from the High-velocity Cloud MS30.7-81.4-118
• Cosmological Simulation of Galaxy Groups and Clusters-II: Studying Different Modes of Feedback through X-ray Observations
• R-matrix electron-impact excitation data for the H- and He-like ions with Z=6-30
• High-temperature behaviour of the helium-like K ALPHA G ratio: the effect of improved recombination rate coefficients for calcium, iron, and nickel
• Discovery of extraordinary X-ray emission from magnetospheric interaction in the unique binary stellar system $\epsilon$ Lupi
• O, Ne, Mg, and Fe Abundances in Hot X-Ray-emitting Halos of Galaxy Clusters, Groups, and Giant Early-type Galaxies with XMM-Newton RGS Spectroscopy
• Dynamical properties and detectability of the magneto-thermal instability in the intracluster medium
• A Suzaku X-ray study of the mixed-morphology supernova remnant Kes 69 and searching for its gamma-ray counterpart
• The Double Galaxy Cluster Abell 2465 III. X-ray and Weak-lensing Observations
• Simulating the pericentre passage of the Galactic centre star S2
• Discovery of X-rays from the old and faint pulsar J1154--6250
• The impact of improved plasma diagnostics on modeling the X-ray Universe
• Growth and disruption in the Lyra complex
• Search for non-thermal X-ray emission in the colliding wind binary Cyg OB2 #8A
• Prospects for IXPE and eXTP polarimetric archaeology of the reflection nebulae in the Galactic center
• X-ray Shadowing Experiments Toward Infrared Dark Clouds
• Prospects for the polarimetric mapping of the Sgr A molecular cloud complex with IXPE
• Characterizing X-ray activity cycles of young solar-like stars with solar observations
• New Clues to the Evolution of Dwarf Carbon Stars From Their Variability and X-ray Emission
• Five new hot-Jupiter transits investigated with Swift-UVOT
• Limits on Leptonic TeV Emission from the Cygnus Cocoon with Swift-XRT
• The XXL Survey LI. Pressure profile and $Y_{\mathrm{SZ}}$-$M$ scaling relation in three low-mass galaxy clusters at $z\sim 1$ observed with NIKA2
• Multiwavelength Observations of the Runaway Binary HD 15137
• X-ray variability of the triplet star system LTT1445 and evaporation history of the exoplanets around its A component
• Discovery of the Goat Horn complex: a $\sim 1000$ deg${}^2$ diffuse X-ray source connected to radio loop XII
• The SRG/eROSITA All-Sky Survey: Large-scale view of the Centaurus cluster
• Chandra observation of Cepheus A: The diffuse emission of HH 168 resolved
• Relativistic reflection within an extended hot plasma geometry
• Fire and Ice in the Whirlpool: Spatially Resolved Scaling Relations between X-ray Emitting Hot Gas and Cold Molecular Gas in M51
• Diving into the magnetosphere of the Of?p star HD108
• Hydrodynamic Evolution of Sgr A East: The Imprint of A Supernova Remnant in the Galactic Center
• New Active Galactic Nuclei Detected by the ART-XC and eROSITA Telescopes during the First Five SRG All-Sky X-ray Surveys
• XMM-Newton study of the Sculptor dwarf spheroidal galaxy
• Chandra observations of nova KT Eridani in outburst
• Multiwavelength Observations of the RV Tauri Variable System U Monocerotis: Long-Term Variability Phenomena That Can Be Explained by Binary Interactions with a Circumbinary Disk
• The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey II. X-ray and optical properties of the cluster sample
• The Active Nucleus of IC4970: A Nearby Example of Merger-Induced Cold-Gas Accretion
• Observational limits on the X-ray emission from the bubble nebula surrounding Ho IX X-1
• A Pre-Merger Stage Galaxy Cluster: Abell 3733
• CHEX-MATE: Multi-probe analysis of Abell 1689
• Tracing the Origins of Hot Halo Gas in Milky Way-Type Galaxies with SMUGGLE
• Discovery of an Outstanding Disk in the cD Galaxy of the Hydra A Cluster
• Spectral and photometric variability of SS 433 observed with XRISM and simultaneous optical and near-infrared telescopes
• First Detection of Ar-K Line Emission from the Cygnus Loop
• X-ray Properties of Low-Mass Pre-Main Sequence Stars in the Orion Trapezium Cluster
• Suzaku Observations of the old pulsar wind nebula candidate HESS J1356-645
• Helium escaping from the atmosphere of a nearby rocky exoplanet orbiting in a habitable zone
• Near-Infrared Spectroscopy of Faint Discrete X-ray Point Sources Constituting the Galactic Ridge X-ray Emission
• X-ray confirmation of the intermediate polar IGR J16547-1916
• A multiwavelength study of the hierarchical triple HD 181068: A test bed for studying star-planet-interaction?
• A new understanding of the Gemini-Monoceros X-ray enhancement from discoveries with eROSITA
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• Suzaku and Fermi view of the supernova remnant 3C 396
• X-ray spectroscopy of Abell S1101 with Chandra, XMM-Newton and ROSAT: band-pass dependence of he temperature profile and soft excess emission
• Modelling the selection of galaxy groups with end to end simulations
• Chandra observation of a cold front in Abell 2554
• Unraveling the nature of a deeply embedded Wolf-Rayet star WR 121a
• Testing the Reliability of X-rays as a Tool for Constraining Mass-loss Rates of Hot Stars
• Why are some galaxy clusters underluminous? The very low concentration of the CL2015 mass profile
• Betelgeuse's Buddy: X-Ray Constraints on the Nature of $\alpha$ Ori B
• Discovery of Diffuse Hard X-Ray Emission from the Vicinity of PSR J1648-4611 with Suzaku
• The Chandra Local Volume Survey: The X-ray Point Source Population of NGC 404
• X-ray Activity Variations and Coronal Abundances of the Star-Planet Interaction candidate HD 179949
• Revisiting the abundance pattern and charge-exchange emission in the M82 centre
• X-Shooting ULLYSES: Massive stars at low metallicity. XIII. Putting the bi-stability jump to the test in the LMC
• Universality of coronal properties in accreting black holes across mass and accretion rate
• Initial state of the recombining plasma in supernova remnant W 28
• The X-ray-Resolved Supernova Remnant S8 in the Dwarf Irregular Galaxy IC 1613
• Detailed X-Ray Line Properties of Theta2 Ori A in Quiescence
• X-ray and UV radiation in the planet-forming T-Tauri system PDS 70. Signs of accretion and coronal activity
• The infalling elliptical galaxy M89: The chemical composition of the AGN disturbed hot atmosphere
• Chandra View of the LINER-type Nucleus in the Radio-Loud Galaxy CGCG 292-057: Ionized Iron Line and Jet-ISM Interactions
• The strongly irradiated planets in Praesepe
• Detection of a radio-filled X-ray cavity within the interstellar medium of NGC 5141
• Reproducibility and monitoring of the instrumental particle background for the X-Ray Integral Field Unit
• Discovery of the magnetic cataclysmic variable XMM J152737.4-205305.9 with a deep eclipse-like feature
• X-ray measurement of the elemental abundances at the outskirts of the Perseus cluster with Suzaku
• Revealing the nature of central emission nebulae in the dwarf galaxy NGC 185
• Turbulence in Simulated Local Cluster Analogs: One-to-one comparisons between SLOW and XRISM/Hitomi
• A Possible Supernova Remnant high above the Galactic Disk
• Strong Evidence for Cosmic Ray-Supported $\sim$L${}^{\ast }$ Galaxy Halos via X-ray \& tSZ Constraints
• Is the high-energy environment of K2-18b special?
• The eROSITA DR1 variability catalogue
• The corona of a fully convective star with a near-polar flare
• A Flaring X-ray Source with an Halpha-bright Counterpart toward the SMC
• X-raying the coronae of HD~155555
• First X-ray dectection of the young variable V1180 Cas
• Buoyancy-driven inflow to a relic cold core: the gas belt in radio galaxy 3C 386
• XRISM view of a stellar flare: High-resolution Fe K spectra of HR 1099, an RS CVn-type star
• Soft X-ray excess of clusters: a thermal filament model, and the strong lensing of background galaxy groups
• Hard X-ray Emission from the NGC 5044 Group
• Soft X-ray emissions of Si IX in Procyon
• Three X-ray Flares Near Primary Eclipse of the RS CVn Binary XY UMa
• Spatially-resolved Chandra Imaging Spectroscopy of the classical/weak-lined T Tauri system V710 Tau
• A novel approach to detect line emission under high background in high-resolution X-ray spectra
• Optical/X-ray/radio view of Abell 1213: A galaxy cluster with anomalous diffuse radio emission
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• Point source contribution to the Diffuse X-ray Background below 1 keV and its effect on our understanding of the circum-galactic medium
• Diffusion of Elements in the Interstellar Medium in Early-Type Galaxies
• An X-ray View of Two Infrared Dark Clouds G034.43+00.24 and G035.39-00.33
• Extragalactic transient candidates in the Second Swift-XRT Point Source catalogue
• Possible non-thermal origin of the hard X-ray emission in the merging galaxy cluster SPT-CL J2031-4037
• The near-infrared companion to HD94660 (=KQ Vel)
• A Swift X-ray view of the SMS4 sample -- II: X-ray properties of 17 bright radio sources
• High resolution X-ray spectra of the compact binary supersoft X-ray source CAL 87
• Mapping the gas thermodynamic properties of the massive cluster merger MOO J1142$+$1527 at z = 1.2
• Searching for rotation in X-COP galaxy clusters
• Relighting the fire in Hickson Compact Group (HCG) 15: magnetised fossil plasma revealed by the SKA Pathfinders & Precursors
• Fluorescent Fe K line emission of gamma Cas stars II. Predictions for magnetic interactions and white-dwarf accretion scenarios
• The NuSTAR View of Perseus: the ICM and a Peculiar Hard Excess
• Observed epochal variations in X-ray lines from the O Supergiant $\zeta$ Puppis do not require substantial changes in the wind mass flux
• Toward mapping turbulence in the intracluster medium III. Constraints on the turbulent power spectrum with Athena/X-IFU
• Harnessing the XMM-Newton data: X-ray spectral modelling of 4XMM-DR11 detections and 4XMM-DR11s sources
• Quokka-based understanding of outflows (QED) -- II. X-ray metallicity gradients as a signature of galactic wind metal loading
• An XMM-Newton look at the strongly variable radio-weak BL Lac Fermi J1544-0639
• Observing gravitational redshift with X-Ray emission in galaxy clusters with Athena X-IFU
• A multi-wavelength approach to classifying transient events in the direction of M31
• Constraints on thermal conductivity in the merging cluster Abell 2146
• Searching for Particle Dark Matter with eROSITA Early Data
• Probing AGN-ISM Feedback through Extended X-ray Emission in ESO 137-G034
• X-ray irradiation of three planets around Hyades star K2-136
• Predicting the X-ray signatures of the imminent T Coronae Borealis outburst through 3D hydrodynamic modeling
• X-ray study of extended emission around M86 observed with Suzaku
• X-ray detection of the substellar twin 2MASS J11011926-7732383 AB
• A Search for a Contribution from Axion-Like Particles to the X-Ray Diffuse Background Utilizing the Earth's Magnetic Field
• Does the Fe L-shell blend bias abundance measurements in intermediate-temperature clusters?
• X-ray study of the double source plane gravitational lens system Eye of Horus observed with XMM-Newton
• EWOCS-IV: 1Ms ACIS Chandra observation of the supergiant B[e] star Wd1-9
• Estimating Ejecta Mass Ratios in Kepler's SNR: Global X-Ray Spectral Analysis Including Suzaku Systematics and Emitting Volume Uncertainties
• X-ray and Hα superflare on an RS CVn-type star, UX Arietis: Constraint on the flare location from radial velocity change during the flare
• The average X-ray spectrum of the volume-complete M-, F-, G-, and K-type star sample within 10 pc of the Sun
• Do blue galaxy-clusters have hot intracluster gas?
• Constraining black hole spin in PG 1535+547 amidst complex multi-layered absorption
• Constraints on the Velocity and Spatial Distribution of Helium-like Ions in the Wind of SMC X-1 from Observations with XMM-Newton/RGS
• Galaxy cluster count cosmology with simulation-based inference
• Estimating Global Ejecta Mass Ratios in Tycho's SNR
• XMM-Newton and Canadian Galactic Plane Survey Observations of the Supernova Remnant G107.5-1.5
• XMM-Newton observation of V1504 Cyg as a probe for the existence of an evaporated corona
• Deprojection of X-ray data in galaxy clusters: confronting simulations with observations
• Estimating the Mass Escaping Rates of Radius-valley-spanning Planets in the TOI-431 System via X-Ray and Ultraviolet Evaporation
• Distant clusters of galaxies in the 2XMM/SDSS footprint: follow-up observations with the LBT
• Signatures of large-scale cold fronts in the optically-selected merging cluster HSC J085024+001536
• Beginning of the Super-Soft Phase of the Classical Nova V2491 Cygni
• Constraining cosmic ray transport models using circumgalactic medium properties and observables
• Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
• New X-ray Supernova Remnants in NGC 7793
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• Studying the multi-phase interstellar medium in the Large Magellanic Cloud with SRG/eROSITA -- I. Analysis of diffuse X-ray emission
• The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray stacking analysis of Subaru's optically selected clusters spanning low richness regime
• Time-resolved X-ray spectra of Proxima Centauri as seen by XMM-Newton
• Einstein Probe Discovery of an X-ray Flare from K-type Star PM J23221-0301
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• New Active Galactic Nuclei Detected by the ART-XC and eROSITA Telescopes during the First Five SRG All-Sky X-ray Surveys. Part 2
• Spherical bias on the 3D reconstruction of the ICM density profile in galaxy clusters
• RXCJ1111.6+4050 galaxy cluster: the observational evidence of a transitional fossil group
• Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters
• HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
• Non-thermal processes in coronae and beyond
• X-ray spectral diagnostics of activity in massive stars
• X-ray analysis of the Planck-detected triplet-cluster system PLCK G334.8-38
• Chandra X-ray Observatory High-resolution X-ray Spectroscopy of Stars: Modeling and Interpretation
• On the thermal line emission from the outflows in ultraluminous X-ray sources
• Charge-exchange emission in the starburst galaxies M82 and NGC3256
• Searching for X-ray sources in nearby late-type galaxies with low star formation rates
• Discovery of an Overlapping Cluster in Abell 1674 Field with Suzaku
• On the diffuse soft X-ray emission from the nuclear region of M51
• Cool-core, X-ray cavities and cold front revealed in RXCJ0352.9+1941 cluster by Chandra and GMRT observations
• Merger of massive galaxy cluster CL0238.3+2005 at z~0.4: just after pericenter passage?
• Testing the Limits of AGN Feedback and the Onset of Thermal Instability in the Most Rapidly Star Forming Brightest Cluster Galaxies
• Simulated X-ray Emission in Galaxy Clusters with Feedback from Active Galactic Nuclei
• Predictions for the X-ray circumgalactic medium of edge-on discs and spheroids
• A census of Dark Energy Survey Year 3 redMaPPer galaxy clusters in a high exposure eROSITA All Sky Survey region
• Long Term X-Ray Spectral Variation of the Wolf-Rayet Binary WR 102-1 in the Galactic bulge: evidence for wind distortion in the binary
• Modelling the thermal X-ray emission around the Galactic centre from colliding Wolf-Rayet winds
• Selection of Compton-thick AGN from a hard photometric sample using XMM-Newton observations
• The Sun as an X-ray star V.: A new method to retrieve coronal filling factors
• eROSITA (eRASS1) study of the Canis Major overdensity: Developing a multi-wavelength algorithm for classifying faint X-ray sources
• XMM-Newton follow-up of two eROSITA X-ray binary candidates
• High-resolution X-ray spectroscopy of clusters of galaxies
• Multiwavelength view of massive binaries
• IGR J12580+0134: The Nearest Tidal Disruption Event and its Faint Resurrection
• Chemical Enrichment of Isolated Relic Galaxy Mrk1216
• Astrophysical Fluids of Novae: High Resolution Pre-decay X-ray spectrum of V4743 Sagittarii
• Global Hot Gas Excess in (U)LIRGs: Replicating Galactic Nuclei Scaling Relations between Diffuse X-ray Emission and Star Formation on Galaxy-Wide Scales
• A Chandra view of SPT-CL J0217-5014: a massive galaxy cluster at a cosmic intersection at z=0.53
• Superflare on a rapidly-rotating solar-type star captured in X-rays
• X-ray and radio data obtained by XMM-Newton and VLA constrain the stellar wind of the magnetic quasi-Wolf-Rayet star in HD45166
• In medio stat virtus: enrichment history in poor galaxy clusters
• Galactic X-ray Transients in the First eROSITA All Sky Survey
• Multi-wavelength insights into the pulsar wind nebula candidate near 1LHAASO J0343+5254u: an obscured merging galaxy cluster?
• Extracting latent representations from X-ray spectra. Classification, regression, and accretion signatures of Chandra sources
• Chandra and XMM-Newton X-ray Study on the Core-collapse Supernova Remnant N63A in an H II Region
• Bound or blown: the fate of hot gas in galaxy groups
• Multiwavelength Characterization of a Dynamically Relaxed Cool Core Galaxy Cluster at $z=1.5$
• Evidence of sloshing-driven mini-halo formation in the cool-core cluster RXCJ1558.3-1410
• Unveiling the Nature of an X-ray flare from 3XMM J014528.9+610729: A candidate spiral galaxy
• The MALATANG survey: star formation, dense gas, and AGN feedback in NGC 1068
• Metals in the Intracluster Medium of MS 1512.4+3647 Observed with Suzaku: Implications for the Metal Enrichment History
• Cross Calibration of Galaxy Cluster Temperatures Measured with NuSTAR, XMM-Newton, and Chandra
• ExoplANETS-A: A VO database for host stars and planetary systems: The effect of XUV on planet atmospheres
• Chandra X-ray Observations of V830 Tau: A T Tauri Star Hosting an Evanescent Planet
• The Unusual Weak-Line Quasar PG1407+265 and its Foreground z~0.7 X-ray Cluster
• The structure of cluster merger shocks: turbulent width and the electron heating timescale
• Suzaku Observations of Fe K-shell Lines in the Supernova Remnant W51C and Hard X-ray Sources in the Proximity
• Simulating Jellyfish Galaxies: A Case Study for a Gas-Rich Dwarf Galaxy
• The NuSTAR, XMM-Newton, and Suzaku view of A3395 at the intercluster filament interface
• Are Active Galactic Nuclei in Post-Starburst Galaxies Driving the Change or Along for the Ride?