Ultra-low noise laser and optical frequency comb-based timing system for the Black Hole Explorer (BHEX) mission
In this effort, we demonstrate the performance of a highly stable time reference for the proposed Black Hole Explorer (BHEX) mission, a space-based extension to the Event Horizon Telescope (EHT) Very Long Baseline Interferometry (VLBI) project. This precision timing system is based on the use of a space-qualified, ultralow noise laser developed as part of the Laser Interferometer Space Antenna (LISA) mission as the timing reference, and an optical frequency comb to transfer the stability of this laser to the microwave regime for instrumentation use. We describe the implementation of this system and experimental setup to characterize the stability performance. We present the results of this experiment that demonstrate the performance of this system meets requirements for the BHEX mission.
Authors
- Peter Kurczynski (ORCID: https://orcid.org/0000-0002-8816-5146)
- Andrew Attar
- Holly Leopardi (ORCID: https://orcid.org/0000-0003-1379-3292)
- Anthony W. Yu (ORCID: https://orcid.org/0000-0002-6727-9494)
- Kenji Numata (ORCID: https://orcid.org/0000-0001-5029-3233)
- Wei Lu (ORCID: https://orcid.org/0000-0003-4804-7601)
- T. K. Sridharan (ORCID: https://orcid.org/0000-0001-5921-5784)
- Hannah Tomio
- Cheryl Gramling
- Xiaozhen Xu
- Guangning Yang
Institutions
- Goddard Space Flight Center (US)
- National Radio Astronomy Observatory (US)
- Vescent Photonics (United States) (US)
- Massachusetts Institute of Technology (US)
Publication Details
- Published
- 2024-08-26
- DOI
- https://doi.org/10.1117/12.3020732
- Citations
- 6
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 1.99