eROSITA ArchiveeROSITA Archive AccessThe Cal-PV program of the SRG mission took place between mid-September and mid-December 2019. During this Cal-PV phase, over one hundred individual pointings and field scans were performed with eROSITA as prime instrument. The CAL-PV observations that were proposed by eROSITA-DE are released to the public through the eROSITA-DE Early Data Release (EDR) as of June 28 2021.
The eROSITA catalogs can be accessed through the following HEASARC multi-mission interfaces:
The eROSITA data archive can be accessed through the following:
eROSITA All-Sky Survey Data - First 6 Months (eRASS1)The eROSITA-DE DR1 comprises data from the first six months of the SRG/eROSITA all-sky survey (eRASS1) whose proprietary rights lie with the German eROSITA consortium.The primary data products of the eROSITA-DE DR1 consist of calibrated event files, which contain the information generated by the cameras used during the eRASS1 observations. The eSASS4DR1 pipeline creates these event files after the received telemetry data from eROSITA of each observation has been reformated, packaged, and archived by a pre-processor. Note that the coverage of the sky is not uniform, i.e., not all observations have been performed with all seven eROSITA TMs (see here). The eROSITA-DE team has divided the eRASS1 observations into 4700 sky tiles for practical purposes. Each sky tile has a size of 3.6x3.6 square degrees, overlapping by approximately 20 arcmin. Users can access all the data products associated with the sky tiles using the HEASARC ERASSMASTR catalog via the HEASARC Browse or Xamin services. In addition, the HEASARC provides access to two eRASS1 source catalogs: ERASS1MAIN and ERASS1HARD. The former provides X-ray sources detected in the 0.2-2.3 keV band; the latter provides Hard eRASS1 detections from the 3B (in the 2.3-5.0 keV band) eSASS source detection analysis. Additional information for eRASS1 source catalogs are available from the eROSITA-DE catalogs page. eROSITA Early Release Data (EDR)Around thirty different fields have been observed. There is a variety of covered areas and exposures. eROSITA-DE is releasing calibrated event lists for each observation so scientists around the world can use the data for their research. These data are provided here and additional information can be found from the eROSITA-DE EDR Observations page.Moreover, the eROSITA-DE team has obtained source catalogs for some of these observations. Further details can be found at the eROSITA-DE EDR Catalogues page. The HEASARC has also ingested a number of these, see column with "Available Catalogs at HEASARC". An important piece in X-ray analysis is the Filter Wheel Closed (FWC) data, which helps to assess the level of instrumental background. eROSITA-DE is also releasing FWC data and models here .
Survey Fields
[1] On September 2021 it was discovered a calibration error in the photon arrival time correction (of 1 second) on approximately half of the TM6 data of eFEDS sub-field I before a malfunction. The error causes the photons to be projected onto the sky with an offset of ~13 arcsec on either side of the true source position, resulting in an elongation of the merged all camera PSF in the scanning direction in the affected area. The affected period spans from: UTC=2019-11-03 13:03:12.25 until UTC=2019-11-03 21:04:53.03. Users are advised to take this error into account. For more details check Brunner et al. 2021. * Spectra and light curves of the sources in the eFEDS observation can be retrieved when using the eROSITA-DE cone search tool. Click here to access eFEDS images, exposure maps and background maps. Magellanic Clouds
Galactic Fields
Extragalactic Fields
eROSITA archive
eROSITA Calibration and Software |