The eRO-STEP research group is divided into seven different projects:
P1: Bubbles, Diffuse Emission → Q1, Q2, Q3
P2: Supernova Remnants → Q1, Q2, Q3
P3: Cataclysmic Variables → Q1, Q4
P4: Isolated Neutron Stars → Q3, Q4
P5: Accreting Neutron Stars/Black Holes → Q3, Q4, Q5
P6: Transient Objects → Q4, Q5
P7: Source populations → Q3, Q4, Q5
Multi-color composite of the first all-sky survey of eROSITA. Credit: Jeremy Sanders, Hermann Brunner and the eSASS team (MPE); Eugene Churazov, Marat Gilfanov (on behalf of IKI)
