erass1sc\.fitsContent of the page.
| Name | Type | Unit | Description |
|---|---|---|---|
| name | char[20] | None | supercluster name |
| redshift | float64 | None | supercluster redshift |
| ra | float64 | deg | Right ascension J2000 |
| dec | float64 | deg | Declination J2000 |
| multiplicity | int64 | None | multiplicity, defined as the number of member clusters |
| mtot | float64 | 10**14 solMass | total mass |
| emtot | float64 | 10**14 solMass | 1sigma uncertainty in mtot |
| reliability | float64 | None | reliability |
| dmem | float64 | Mpc | average distance of supercluster members to the center |
| lproj | float64 | Mpc | supercluster length |
This work is based on data from eROSITA, the soft X-ray instrument aboard SRG, a joint Russian-German science mission supported by the Russian Space Agency (Roskosmos), in the interests of the Russian Academy of Sciences represented by its Space Research Institute (IKI), and the Deutsches Zentrum für Luft- und Raumfahrt (DLR). The SRG spacecraft was built by Lavochkin Association (NPOL) and its subcontractors and is operated by NPOL with support from the Max Planck Institute for Extraterrestrial Physics (MPE). The development and construction of the eROSITA X-ray instrument was led by MPE, with contributions from the Dr. Karl Remeis Observatory Bamberg \& ECAP (FAU Erlangen-Nuernberg), the University of Hamburg Observatory, the Leibniz Institute for Astrophysics Potsdam (AIP), and the Institute for Astronomy and Astrophysics of the University of Tübingen, with the support of DLR and the Max Planck Society. The Argelander Institute for Astronomy of the University of Bonn and the Ludwig Maximilians Universität Munich also participated in the science preparation for eROSITA. The eROSITA data shown here were processed using the eSASS/NRTA software system developed by the German eROSITA consortium.