Using Chandra-only observations from 2012 to 2018, the authors find no change in Sgr A*'s X-ray flare energy distribution around G2's pericenter passage, contrary to earlier multi-telescope claims.
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No sign of G2's encounter affecting Sgr A*'s X-ray flaring rate from $Chandra$ observations
Using Chandra-only observations from 2012 to 2018, the authors find no change in Sgr A*'s X-ray flare energy distribution around G2's pericenter passage, contrary to earlier multi-telescope claims.