Abstract
For the last half-century, relativistic outflows accompanying the final collapse of massive stars have predominantly been detected via high-energy emission (i.e., gamma-ray bursts, or GRBs). From wide-field optical and radio time-domain surveys, there have been hints of related phenomena at lower energies (e.g., X-ray flashes). For my thesis, I used the Zwicky Transient Facility to conduct the first large-scale optical survey dedicated to finding relativistic stellar explosions. I successfully detected a suite of GRB-related phenomena without relying on a GRB trigger, and followed them up with facilities across the electromagnetic spectrum including ALMA: relativistic afterglows at cosmological distances, broad-lined Ic (Ic-BL) supernovae with X-ray and radio emission, and fast-luminous transients powered by circumstellar interaction. Based on the rate of fast (intra-night) optical transients, I showed that a "clean" jet seems central to the phenomenon of collimated energetic outflows, i.e., there is no evidence for afterglow-like optical transients whose area (sky) rate greatly exceed the classical GRB rate. With a radio and millimeter-wave investigation of AT2018cow, and the discovery of a similar event in ZTF, I established a new class of engine-driven stellar explosions that arise from different progenitors to GRBs and explode embedded in dense circumstellar material. I showed that fast-luminous thermal emission can arise from late-stage eruptive mass-loss and is not necessarily linked to the presence of relativistic ejecta, complicating searches for choked jets in Ic-BL SNe. My work sets the stage for discovering and characterizing relativistic stellar explosions in large numbers during the era of ZTF Phase II, the Large Synoptic Survey Telescope (LSST), and millimeter-band facilities like ALMA and NOEMA.
Item Type: | Thesis (Dissertation (Ph.D.)) |
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Subject Keywords: | Catalogs; gamma-ray burst: general; stars: activity; stars: flare; stars: jets; surveys; methods: observational; shock waves; stars: mass-loss; supernovae: individual; radio continuum: general; submillimeter: general; supernovae: general; X-rays: general; Radio transient sources; High energy astrophysics; Supernovae; Core-collapse supernovae; Jets; Sky surveys |
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Degree Grantor: | California Institute of Technology |
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Division: | Physics, Mathematics and Astronomy |
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Major Option: | Astrophysics |
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Awards: | Rodger Doxsey Travel Prize of the American Astronomical Society, 2020.
France A. Córdova Graduate Student Fund (Garmire Scholar), 2017. |
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Thesis Availability: | Public (worldwide access) |
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Research Advisor(s): | |
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Thesis Committee: | - Steidel, Charles C. (chair)
- Hallinan, Gregg W.
- Kasliwal, Mansi M.
- Perley, Daniel
- Phinney, E. Sterl
- Kulkarni, Shrinivas R.
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Defense Date: | 2 July 2020 |
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Non-Caltech Author Email: | annayqho (AT) gmail.com |
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Funders: | Funding Agency | Grant Number |
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NSF Graduate Research Fellowship Program | DGE-1144469 | NSF | Pire Grant 1545949 |
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Record Number: | CaltechTHESIS:07132020-190219502 |
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Persistent URL: | https://resolver.caltech.edu/CaltechTHESIS:07132020-190219502 |
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DOI: | 10.7907/99s8-vj17 |
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Related URLs: | |
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ORCID: | |
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Default Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
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ID Code: | 13841 |
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Collection: | CaltechTHESIS |
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Deposited By: |
Anna Ho
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Deposited On: | 24 Jul 2020 15:50 |
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Last Modified: | 28 Oct 2021 16:33 |
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