Next-generation IFU instruments could detect core scouring and tangential anisotropy from MBH binaries up to z~0.14 for ~150 pc cores and higher redshifts for larger cores, expanding searchable volume by 30-40 times including lower-mass systems.
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Presents the structure, contributors, and methodology of the wavefront error budget for the MORFEO adaptive optics module on the ELT.
citing papers explorer
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Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP
Next-generation IFU instruments could detect core scouring and tangential anisotropy from MBH binaries up to z~0.14 for ~150 pc cores and higher redshifts for larger cores, expanding searchable volume by 30-40 times including lower-mass systems.
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MORFEO wavefront error budget
Presents the structure, contributors, and methodology of the wavefront error budget for the MORFEO adaptive optics module on the ELT.