Observational discovery of an overmassive, highly accreting black hole in the secondary galaxy of a high-redshift minor merger, providing evidence that such mergers can drive rapid BH growth.
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New observations of 4U 1323-62 detect 12 bursts, confirm 2.94-hour dips, a 0.9 Hz QPO, and suggest a ~10-year cyclic variation in burst rate.
GAMA 376183 is a rare Eddington-limited heavily obscured AGN in a merging low-mass galaxy, triggered by the merger and identified via strong [Ne V] emission.
CIAO is a mature, modular software system for X-ray astronomy data analysis that has supported the Chandra mission since 1999 with calibration, imaging, spectral, timing, modeling, and simulation capabilities.
citing papers explorer
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Minor Merger, Major Growth: An Overmassive, Highly Accreting Black Hole Powering a Secondary AGN In a Cosmic Noon Minor Merger
Observational discovery of an overmassive, highly accreting black hole in the secondary galaxy of a high-redshift minor merger, providing evidence that such mergers can drive rapid BH growth.
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A Cyclic Burst Rate Behavior of a Persistent X-ray Burster: Recent XMM-Newton and NuSTAR Observations of 4U 1323-62
New observations of 4U 1323-62 detect 12 bursts, confirm 2.94-hour dips, a 0.9 Hz QPO, and suggest a ~10-year cyclic variation in burst rate.
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A Rare Eddington-Limited, Heavily Obscured Low-Mass Active Galactic Nucleus Likely Triggered by a Galaxy Merger
GAMA 376183 is a rare Eddington-limited heavily obscured AGN in a merging low-mass galaxy, triggered by the merger and identified via strong [Ne V] emission.
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CIAO: Chandra's Data Analysis System for X-Ray Astronomy and Beyond
CIAO is a mature, modular software system for X-ray astronomy data analysis that has supported the Chandra mission since 1999 with calibration, imaging, spectral, timing, modeling, and simulation capabilities.