papers

Publications (60)

astro-ph.HE2011

Fe Ka line emission from the Arches cluster region - evidence for ongoing particle bombardment?

R. Capelli, R. S. Warwick, D. Porquet +2

We present the results of eight years of XMM-Newton observations of the region surrounding the Arches cluster in the Galactic Center. We study the spatial distribution and temporal…

astro-ph2008

X-ray hiccups from SgrA* observed by XMM-Newton. The second brightest flare and three moderate flares caught in half a day

D. Porquet, N. Grosso, P. Predehl +14

[truncated] In Spring 2007, we observed SgrA* with XMM with a total exposure of ~230ks. We have performed timing and spectral analysis of the new X-ray flares detected during this…

astro-ph2003

XMM-Newton observation of the brightest X-ray flare detected so far from SgrA*

D. Porquet, P. Predehl, B. Aschenbach +5

We report the high S/N observation on October 3, 2002 with XMM-Newton of the brightest X-ray flare detected so far from SgrA* with a duration shorter than one hour (~ 2.7 ks). The…

astro-ph.CO2021

The mass function dependence on the dynamical state of dark matter haloes

R. Seppi, J. Comparat, K. Nandra +6

Galaxy clusters are luminous tracers of the most massive dark matter haloes in the Universe. To use them as a cosmological probe, a detailed description of the properties of dark m…

astro-ph2001

CHANDRA observation of the narrow-line Seyfert 1 galaxy IRAS 13224-3809

F. Pfefferkorn, Th. Boller, V. Burwitz +1

The narrow-line Seyfert 1 galaxy (NLS1) IRAS 13224-3809 has been observed with the CHANDRA High Resolution Camera (HRC-I) for 12 ksec on February, 2, 2000. The source was proposed…

astro-ph.HE2021

The SRG X-ray orbital observatory, its telescopes and first scientific results

R. Sunyaev, V. Arefiev, V. Babyshkin +39

The orbital observatory Spectrum-Roentgen-Gamma (SRG), equipped with the grazing-incidence X-ray telescopes Mikhail Pavlinsky ART-XC and eROSITA, was launched by Roscosmos to the L…

astro-ph.HE2020

A giant X-ray dust scattering ring around the black hole transient MAXI J1348-630 discovered with SRG/eROSITA

G. Lamer, A. D. Schwope, P. Predehl +3

We report the discovery of a giant dust scattering ring around the Black Hole transient MAXI J1348-630 with SRG/eROSITA during its first X-ray all-sky survey. During the discovery…

astro-ph.CO2021

Discovery of a Supercluster in the eROSITA Final Equatorial Depth Survey: X-ray Properties, Radio Halo, and Double Relics

V. Ghirardini, E. Bulbul, D. N. Hoang +27

We examine the X-ray, optical, and radio properties for the members clusters of a new supercluster discovered during the SRG/eROSITA Performance Verification phase. In the 140 deg2…

astro-ph.HE2012

eROSITA Science Book: Mapping the Structure of the Energetic Universe

A. Merloni, P. Predehl, W. Becker +22

eROSITA is the primary instrument on the Russian SRG mission. In the first four years of scientific operation after its launch, foreseen for 2014, it will perform a deep survey of…

astro-ph2002

The thermal radiation of the isolated neutron star RX J1856.5-3754 observed with Chandra and XMM-Newton

V. Burwitz, F. Haberl, R. Neuhaeuser +3

We present results of the analysis of data collected in 57-ks XMM-Newton and 505-ks Chandra observations of the nearby ~= 120 pc isolated neutron star RX J1856.5-3754. We confirm m…

astro-ph.SR2022

The high energy spectrum of Proxima Centauri simultaneously observed at X-ray and FUV wavelengths

B. Fuhrmeister, A. Zisik, P. C. Schneider +6

The M dwarf Proxima~Centauri is known to be magnetically active and it hosts a likely Earth-like planet in its habitable zone. Understanding the characteristics of stellar radiatio…

astro-ph2003

The weak-line T Tauri star V410Tau I. A multi-wavelength study of variability

B. Stelzer, M. Fernandez, V. M. Costa +10

We present the results of an intensive coordinated monitoring campaign in the optical and X-ray wavelength ranges of the low-mass, pre-main sequence star V410Tau carried out with t…

astro-ph.CO2021

The eROSITA Final Equatorial-Depth Survey (eFEDS): Characterization of Morphological Properties of Galaxy Groups and Clusters

V. Ghirardini, E. Bahar, E. Bulbul +16

Understanding the cluster population of clusters of galaxies is of the utmost importance for using cluster samples in both astrophysical and cosmological studies. We present an in-…

astro-ph1997

Discovery of X-rays from the supernova remnant G0.9+0.1

L. Sidoli, G. L. Israel, L. Chiappetti +6

During the survey of the Galactic Center region, we have discovered X-ray emission from the central region of the supernova remnant G0.9+0.1. The high interstellar absor…

astro-ph2002

Coronal density diagnostics with Helium-like triplets: CHANDRA--LETGS observations of Algol, Capella, Procyon, Eps Eri, Alpha Cen A&B, UX Ari, AD Leo, YY Gem, and HR1099

J. -U. Ness, J. H. M. M. Schmitt, V. Burwitz +5

We present an analysis of ten cool stars (Algol, Capella, Procyon, Eps Eri, Alpha Cen A&B, UX Ari, AD Leo, YY Gem, and HR1099) observed with the Low Energy Transmission Grating Spe…

astro-ph.CO2020

The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data

T. H. Reiprich, A. Veronica, F. Pacaud +44

We used dedicated SRG/eROSITA X-ray, ASKAP/EMU radio, and DECam optical observations of a 15 sq.deg region around the interacting galaxy cluster system A3391/95 to study the warm-h…

astro-ph.HE2012

The X-ray lightcurve of Sgr A* over the past 150 years inferred from Fe-Ka line reverberation in Galactic Centre molecular clouds

R. Capelli, R. S. Warwick, D. Porquet +2

We examine the temporal and spectral properties of nine Fe-Ka bright molecular clouds within about 30 pc of Sgr A*, in order to understand and constrain the primary energising sour…

astro-ph2004

Discovery of a bright X-ray transient in the Galactic Center with XMM-Newton

D. Porquet, N. Grosso, V. Burwitz +4

We report the discovery of a bright X-ray transient object, XMMU J174554.4-285456, observed in outburst with XMM-Newton on October 3, 2002,and located at 6.3' from SgrA*, the super…

astro-ph.SR2021

Simultaneous eROSITA and TESS observations of the ultra-active star AB~Doradus

J. H. M. M. Schmitt, P. Ioannidis, J. Robradel +3

We present simultaneous multiwavelength observations of the ultra-active star AB~Doradus obtained in the X-ray range with the eROSITA instrument on board the Russian--German Spectr…

astro-ph.HE2011

Concurrent X-ray, near-infrared, sub-millimeter, and GeV gamma-ray observations of Sgr A*

G. Trap, A. Goldwurm, K. Dodds-Eden +13

The radiative counterpart of the supermassive black hole at the Galactic center (GC), Sgr A*, is subject to frequent flares visible simultaneously in X-rays and near-infrared (NIR)…

astro-ph2005

Discovery of X-ray eclipses from the transient source CXOGC J174540.0-290031 with XMM-Newton

D. Porquet, N. Grosso, G. Belanger +4

We present the XMM-Newton observations obtained during four revolutions in Spring and Summer 2004 of CXOGC J174540.0-290031, a moderately bright transient X-ray source, located at…

astro-ph.CO2024

The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts

E. Artis, E. Bulbul, S. Grandis +29

Beyond testing the current cosmological paradigm, cluster number counts can also be utilized to investigate the discrepancies currently affecting current cosmological measurements.…

astro-ph.EP2024

X-ray variability of the triplet star system LTT1445 and evaporation history of the exoplanets around its A component

S. Rukdee, J. Buchner, V. Burwitz +3

The high-energy environment of the host stars could be deleterious for their planets. It is crucial to ascertain this contextual information to fully characterize the atmospheres o…

astro-ph2005

An X-ray Galaxy Cluster Survey for Investigations of Dark Energy

Z. Haiman, S. Allen, N. Bahcall +34

The amount and nature of dark energy (DE) can be tightly constrained by measuring the spatial correlation features and evolution of a sample of ~ 100,000 galaxy clusters over the r…

astro-ph.SR2025

The stellar corona-chromosphere connection. A comprehensive study of X-ray and Ca II IRT fluxes from eROSITA and Gaia

S. Freund, S. Czesla, B. Fuhrmeister +4

Stellar activity can be observed at different wavelengths in a variety of different activity indicators. We investigated the correlation between coronal and chromospheric emissions…

astro-ph.CO2024

The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance

E. Artis, V. Ghirardini, E. Bulbul +28

The evolution of the cluster mass function traces the growth of the linear density perturbations and can be utilized for constraining the parameters of cosmological and alternative…

astro-ph.IM2011

ORIGIN: Metal Creation and Evolution from the Cosmic Dawn

J. W. den Herder, L. Piro, T. Ohashi +156

ORIGIN is a proposal for the M3 mission call of ESA aimed at the study of metal creation from the epoch of cosmic dawn. Using high-spectral resolution in the soft X-ray band, ORIGI…

astro-ph2002

Coordinated Multiwavelength Observations of V410Tau

B. Stelzer, M. Fernandez, V. Costa +9

In November 2001 we undertook a coordinated observing campaign to study the connection between X-ray and optical variability in the weak-line T Tauri star V410Tau. The observing pl…

astro-ph2004

A Huge Drop in X-ray Luminosity of the Non-Active Galaxy RXJ1242.6-1119A, and First Post-Flare Spectrum - Testing the Tidal Disruption Scenario

S. Komossa, J. Halpern, N. Schartel +3

It has been suggested that an unavoidable consequence of the existence of supermassive black holes, and the best diagnostic of their presence in non-active galaxies, would be occas…

astro-ph2000

First Light Measurements of Capella with the Low Energy Transmission Grating Spectrometer aboard the Chandra X-ray Observatory

A. C. Brinkman, C. J. T. Gunsing, J. S. Kaastra +20

We present the first X-ray spectrum obtained by the Low Energy Transmission Grating Spectrometer (LETGS) aboard the Chandra X-ray Observatory. The spectrum is of Capella and covers…

astro-ph2004

X-ray flares reveal mass and angular momentum of the Galactic Center black hole

B. Aschenbach, N. Grosso, D. Porquet +1

We have analysed the light curve of the two brightest X-ray flares from the Galactic Center black hole, one flare observed by XMM-Newton on October 3, 2002 (Porquet et al. 2003), a…

astro-ph2000

High Resolution Spectroscopy of the X-ray Photoionized Wind in Cygnus X-3 with the Chandra High Energy Transmission Grating Spectrometer

Frits Paerels, Jean Cottam, Masao Sako +5

We present a preliminary analysis of the 1--10 keV spectrum of the massive X-ray binary Cyg X-3, obtained with the High Energy Transmission Grating Spectrometer on the Chandra X-ra…

astro-ph2001

The Chandra LETGS high resolution X-ray spectrum of the isolated neutron star RX J1856.5-3754

V. Burwitz, V. E. Zavlin, R. Neuhaeuser +3

We present the Chandra LETGS X-ray spectrum of the nearby (~60 pc) neutron star RX J1856.5-3754. Detailed spectral analysis of the combined X-ray and optical data rules out the non…

astro-ph.HE2026

The SRG/eROSITA All-Sky Survey DR2: Cumulative X-ray catalogues from the first three surveys and multi-wavelength counterparts in the western Galactic hemisphere

M. E. Ramos-Ceja, G. Lamer, M. Salvato +111

The paper presents the second data release of the SRG/eROSITA all‑sky survey, providing catalogues of nearly two million X‑ray sources (point‑like and extended) from the first thre…

#x-ray surveys#source catalogues#eROSITA#multi-wavelength identification
astro-ph2002

A New X-Ray Flare from the Galactic Nucleus Detected with the XMM-Newton Photon Imaging Cameras

A. Goldwurm, E. Brion, P. Goldoni +5

Sgr A*, the compact radio source, believed to be the counterpart of the massive black hole at the galactic nucleus, was observed to undergo rapid and intense flaring activity in X-…

astro-ph.GA2020

Detection of large-scale X-ray bubbles in the Milky Way halo

P. Predehl, R. A. Sunyaev, W. Becker +25

The halo of the Milky Way provides a laboratory to study the properties of the shocked hot gas that is predicted by models of galaxy formation. There is observational evidence of e…

astro-ph.HE2024

The SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphere

A. Merloni, G. Lamer, T. Liu +142

The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite began surveying the sky in December 2019, with the aim of producing all-sky X-ray source lists and sk…

astro-ph.HE2020

The eROSITA X-ray telescope on SRG

P. Predehl, R. Andritschke, V. Arefiev +90

eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the primary instrument on the Spectrum-Roentgen-Gamma (SRG) mission, which was successfully launched on July 1…

astro-ph.SR2024

The SRG/eROSITA all-sky survey -- Identifying the coronal content with HamStar

S. Freund, S. Czesla, P. Predehl +6

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

astro-ph.CO2021

The eROSITA Final Equatorial-Depth Survey (eFEDS): Catalog of galaxy clusters and groups

A. Liu, E. Bulbul, V. Ghirardini +31

The eROSITA Final Equatorial-Depth Survey has been carried out during the PV phase of the SRG/eROSITA telescope and completed in November 2019. This survey is designed to provide t…

astro-ph2002

Chandra LETGS Observation of the Active Binary Algol

J. -U. Ness, J. H. M. M. Schmitt, V. Burwitz +2

A high-resolution spectrum obtained with the low-energy transmission grating onboard the Chandra observatory is presented and analyzed. Our analysis indicates very hot plasma with…

astro-ph.CO2024

The SRG/eROSITA All-Sky Survey: The first catalog of galaxy clusters and groups in the Western Galactic Hemisphere

E. Bulbul, A. Liu, M. Kluge +31

Clusters of galaxies can be used as powerful probes to study astrophysical processes on large scales, test theories of the growth of structure, and constrain cosmological models. T…

astro-ph2000

Helium-like triplet density diagnostics: Applications to CHANDRA--LETGS X-ray observations of Capella and Procyon

J. U. Ness, R. Mewe, J. H. M. M. Schmitt +6

Electron density diagnostics based on the triplets of Helium-like CV, NVI, and OVII are applied to the X-ray spectra of Capella and Procyon measured with the Low Energy Transmissio…

astro-ph.CO2024

The SRG/eROSITA All-Sky Survey: First catalog of superclusters in the western Galactic hemisphere

A. Liu, E. Bulbul, M. Kluge +21

Superclusters of galaxies mark the large-scale overdense regions in the Universe. Superclusters provide an ideal environment to study structure formation and to search for the emis…

astro-ph2000

Interstellar X-ray Absorption Spectroscopy of Oxygen, Neon, and Iron with the Chandra LETGS Spectrum of X0614+091

Frits Paerels, A. C. Brinkman, R. L. J. van der Meer +8

We find resolved interstellar O K, Ne K, and Fe L absorption spectra in the Chandra Low Energy Transmission Grating Spectrometer spectrum of the low mass X-ray binary X0614+091. We…

astro-ph.CO2024

The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere

V. Ghirardini, E. Bulbul, E. Artis +46

The cluster mass function traces the growth of linear density perturbations and provides valuable insights into the growth of structures, the nature of dark matter, and the cosmolo…

astro-ph2005

Absorption and scattering by interstellar dust: XMM-Newton observation of Cyg X-2

E. Costantini, M. J. Freyberg, P. Predehl

We present results of the XMM-Newton observation on the bright X-ray binary Cyg X-2. In our analysis we focus upon the absorption and scattering of the X-ray emission by interstell…

astro-ph.CO2024

The SRG/eROSITA All-Sky Survey. Optical identification and properties of galaxy clusters and groups in the western galactic hemisphere

M. Kluge, J. Comparat, A. Liu +29

The first SRG/eROSITA All-Sky Survey (eRASS1) provides the largest intracluster medium-selected galaxy cluster and group catalog covering the western galactic hemisphere. Compared…

astro-ph.HE2022

The Curious Case of the "Heartworm" Nebula

W. D. Cotton, F. Camilo, W. Becker +9

The curious Galactic features near G357.20.2 were observed with the MeerKAT radio interferometer array in the UHF and L bands (0.56--1.68 GHz). There are two possibly related fe…

astro-ph2002

1ES 1927+654: Persistent and rapid X-ray variability in an AGN with low intrinsic neutral X-ray absorption and narrow optical emission lines

Th. Boller, W. Voges, M. Dennefeld +7

We present X-ray and optical observations of the X-ray bright AGN 1ES 1927+654. The X-ray observations obtained with ROSAT and Chandra reveal persistent, rapid and large scale vari…

astro-ph.CO2024

The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy Clusters

S. Grandis, V. Ghirardini, S. Bocquet +119

Number counts of galaxy clusters across redshift are a powerful cosmological probe, if a precise and accurate reconstruction of the underlying mass distribution is performed -- a c…

astro-ph.IM2010

eROSITA on SRG: a X-ray all-sky survey mission

N. Cappelluti, P. Predehl, H. Boehringer +23

eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the core instrument on the Russian Spektrum-Roentgen-Gamma (SRG) mission which is scheduled for launch in late…

astro-ph2004

Chandra Observations of the NLS1 RX J2217.9-5941

D. Grupe, K. M. Leighly, V. Burwitz +2

We report the results of two Chandra ACIS-S observations from February and August 2003 of the highly X-ray variable Narrow-Line Seyfert 1 galaxy RX J2217.9--5941. Observations span…

astro-ph2003

A New X-Ray Flare from the Galactic Nucleus Detected with the XMM-Newton

A. Goldwurm, E. Brion, P. Goldoni +5

The compact radio source Sgr A*, believed to be the counterpart of the massive black hole at the Galactic nucleus, was observed to undergo rapid and intense flaring activity in X-r…

astro-ph1996

ROSAT observation of GRS 1739-278

J. Greiner, K. Dennerl, P. Predehl

We have observed GRS 1739-278 with the ROSAT HRI on March 31, 1996. The improved X-ray position proves the identification with an earlier discovered variable radio source. We deriv…

astro-ph.HE2022

The eROSITA Final Equatorial Depth Survey (eFEDS): The X-ray catalog

H. Brunner, T. Liu, G. Lamer +35

Context. The eROSITA X-ray telescope on board the Spectrum-Roentgen-Gamma (SRG) observatory combines a large field of view and collecting area in the energy range 0.2 to $\si…

astro-ph.HE2024

The SRG/eROSITA all-sky survey. X-ray emission from the warm-hot phase gas in long cosmic filaments

X. Zhang, E. Bulbul, N. Malavasi +24

The properties of the warm-hot intergalactic medium (WHIM) in cosmic filaments are among the least quantified units in modern astrophysics. The Spectrum Roentgen Gamma/eROSITA All…

astro-ph2002

Simultaneous X-ray spectroscopy of YY Gem with Chandra and XMM-Newton

B. Stelzer, V. Burwitz, M. Audard +7

We report on a detailed study of the X-ray spectrum of the nearby eclipsing spectroscopic binary YY Gem. Observations were obtained simultaneously with both large X-ray observatori…

astro-ph.SR2020

Proxima Centauri -- the nearest planet host observed simultaneously with AstroSat, Chandra and HST

S. Lalitha, J. H. M. M. Schmitt, K. P. Singh +6

Our nearest stellar neighbour, Proxima Centauri, is a low mass star with spectral typedM5.5 and hosting an Earth-like planet orbiting within its habitable zone. However, the habita…

astro-ph.HE2015

The XMM-Newton view of the central degrees of the Milky Way

G. Ponti, M. R. Morris, R. Terrier +10

The deepest XMM-Newton mosaic map of the central 1.5 deg of the Galaxy is presented, including a total of about 1.5 Ms of EPIC-pn cleaned exposures in the central 15" and about 200…