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| We observed many eROSITA-selected X-ray sources which showed significant changes in their X-ray flux from one survey to another over the last years (still ongoing). This included optical photometric and optical spectroscopic data from various telescopes, as well as X-ray follow-up data (mainly XMM-Newton and Swift). The data base located in Potsdam is hosting all the accumulated data. Everyone in eROSITA_DE is welcome to access these data and use them. If you are interested, please send an email to dhoman@aip.de and mkrumpe@aip.de. We will give you a short introduction about the usage of the data base. | We observed many eROSITA-selected X-ray sources which showed significant changes in their X-ray flux from one survey to another over the last years (still ongoing). This included optical photometric and optical spectroscopic data from various telescopes, as well as X-ray follow-up data (mainly XMM-Newton and Swift). The data base, located in Potsdam, is hosting all the obtained data and additional information about the objects (X-ray and optical light curves, etc.). Everyone in eROSITA_DE is welcome to access these data and use them. If you are interested, please send an email to dhoman@aip.de and mkrumpe@aip.de. We will give you a short introduction about the usage of the data base. |
Optical photometric, optical spectroscopic, and X-ray follow-up of eROSITA sources showing X-ray changes
We observed many eROSITA-selected X-ray sources which showed significant changes in their X-ray flux from one survey to another over the last years (still ongoing). This included optical photometric and optical spectroscopic data from various telescopes, as well as X-ray follow-up data (mainly XMM-Newton and Swift). The data base, located in Potsdam, is hosting all the obtained data and additional information about the objects (X-ray and optical light curves, etc.). Everyone in eROSITA_DE is welcome to access these data and use them. If you are interested, please send an email to dhoman@aip.de and mkrumpe@aip.de. We will give you a short introduction about the usage of the data base.
The data base can be reached via: escience.aip.de/erosita-followup/
(If there are problems with the access or you recognize a problem with a source, please contact us - dhoman@aip.de and mkrumpe@aip.de)