This three-year $469,307 project grant from the National Science Foundation's Mathematical and Physical Sciences program aims to advance measurements of supermassive black holes through triaxial stellar-dynamical models. The Regents of the University of California, doing business as the University of California, Berkeley, will apply recently revised triaxial orbit modeling code and highly sensitive integral-field spectrographs to uncover a new population of massive supermassive black holes and identify possible discrepancies in black hole mass measurements from different dynamical tracers and modeling assumptions. Specifically, the research team will double the number of known ultra-massive black holes over ten billion solar masses, provide critical assessment of gas and star-based dynamical measurement methods, and enable study of galaxy shapes and stellar orbital distributions. The award also supports research opportunities and career mentoring for high school and college students from diverse backgrounds.
Mod # | Description | Reason For Modification | Federal Obligation (Click to sort descending) | Date (Click to sort ascending) |
|---|---|---|---|---|
| Not listed | $469.3k | 8/22/22 |