Figure 3 from Post-merger Jets from Supermassive Black Hole Coalescences as Electromagnetic Counterparts of Gravitational Wave Emission

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Post-merger Jets from Supermassive Black Hole Coalescences as Electromagnetic Counterparts of Gravitational Wave Emission

Authors: Chengchao Yuan, Kohta Murase, B. Theodore Zhang, Shigeo S. Kimura, and Péter Mészáros

2021 The Astrophysical Journal Letters 911 L15.

Provider: AAS Journals

Caption: Figure 3.

Detection horizons for multiwavelength detectors, e.g., SKA, VLA, EVLA, ALMA, HST, JWST, LSST, and Chandra. The horizontal dotted line shows the 100 GHz detection window for ALMA assuming a source located at z = 3. Similar to Figure 2, the dotted vertical lines are the characteristic times of 5 GHz and 100 GHz signals.

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