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Studying and Identifying SMBH pairs
Studying and Identifying SMBH pairs
Searching for and understanding merging SMBH pairs across the electromagnetic spectrum and through time-domain techniques.
Dual SMBHs
Dual SMBHs
The beginning stages of a merger, in which the host galaxies begin to interact while the SMBHs are not yet affected by each other.
The beginning stages of a merger, in which the host galaxies begin to interact while the SMBHs are not yet affected by each other.
These stages are used to study host galaxy and SMBH co-evolution.
These stages are used to study host galaxy and SMBH co-evolution.
I am working to identify whether a dual system can be differentiated from a single active galactic nucleus using time-domain techniques.
I am working to identify whether a dual system can be differentiated from a single active galactic nucleus using time-domain techniques.
Binary SMBHs
Binary SMBHs
The last stages of a merger, in which the two SMBHs are gravitationally bound before coalescence.
The last stages of a merger, in which the two SMBHs are gravitationally bound before coalescence.
These are the direct precursors to gravitational-wave events detected by next-generation observatories such as LISA, and the likely cause of the stochastic background seen by PTAs.
These are the direct precursors to gravitational-wave events detected by next-generation observatories such as LISA, and the likely cause of the stochastic background seen by PTAs.
I use various techniques to search for binaries among strong candidates.
I use various techniques to search for binaries among strong candidates.
Articles
Articles
Cassandra Daniele, Adi Foord, Jessie Runnoe, et al.Â
Investigating the Multiwavelength Emission of Binary SMBH Candidate SDSS J095036.75+512838.1 2026
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