Laura G. Spitler, Ph.D.
Affiliations: | 2013 | Cornell University, Ithaca, NY, United States |
Area:
Astronomy and Astrophysics, Astrophysics PhysicsGoogle:
"Laura Spitler"Mean distance: 3388
Parents
Sign in to add mentor| James Cordes | grad student | 2006-2013 | Cornell | |
| (Saving time: New methods and instrumentation for radio variability studies.) | ||||
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Publications
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| Nimmo K, Gajjar V, Hessels JWT, et al. (2020) No Radio Bursts Detected from FIRST J141918.9+394036 in Green Bank Telescope Observations Research Notes of the Aas. 4: 50 |
| Zhu W, Li D, Luo R, et al. (2020) A Fast Radio Burst Discovered in FAST Drift Scan Survey The Astrophysical Journal. 895: L6 |
| Hilmarsson GH, Spitler LG, Keane EF, et al. (2020) Observing superluminous supernovae and long gamma-ray bursts as potential birthplaces of repeating fast radio bursts Monthly Notices of the Royal Astronomical Society. 493: 5170-5180 |
| Caleb M, Stappers BW, Abbott TD, et al. (2020) Simultaneous multi-telescope observations of FRB 121102 Monthly Notices of the Royal Astronomical Society. 496: 4565-4573 |
| Gourdji K, Michilli D, Spitler LG, et al. (2019) A Sample of Low-energy Bursts from FRB 121102 The Astrophysical Journal. 877: L19 |
| Hessels JWT, Spitler LG, Seymour AD, et al. (2019) FRB 121102 Bursts Show Complex Time–Frequency Structure The Astrophysical Journal. 876: L23 |
| Houben LJM, Spitler LG, ter Veen S, et al. (2019) Constraints on the low frequency spectrum of FRB 121102 Astronomy & Astrophysics. 623: A42 |
| Michilli D, Seymour A, Hessels JWT, et al. (2018) An extreme magneto-ionic environment associated with the fast radio burst source FRB 121102. Nature. 553: 182-185 |
| Desvignes G, Eatough RP, Pen UL, et al. (2018) Large Magneto-ionic Variations toward the Galactic Center Magnetar, PSR J1745-2900 The Astrophysical Journal. 852: L12 |
| Spitler LG, Herrmann W, Bower GC, et al. (2018) Detection of Bursts from FRB 121102 with the Effelsberg 100 m Radio Telescope at 5 GHz and the Role of Scintillation The Astrophysical Journal. 863: 150 |