Parents

Sign in to add mentor
Paul L. Richards grad student 1985 UC Berkeley
 (Spectrum of the cosmic background radiation from 3.2 cm-1 to 11.0 cm-1.)

Collaborators

Sign in to add collaborator
Liju Philip collaborator 2016-
BETA: Related publications

Publications

You can help our author matching system! If you notice any publications incorrectly attributed to this author, please sign in and mark matches as correct or incorrect.

Amiri M, Bandura K, Berger P, et al. (2017) Limits on the Ultra-bright Fast Radio Burst Population from the CHIME Pathfinder The Astrophysical Journal. 844: 161
Berger P, Newburgh LB, Amiri M, et al. (2016) Holographic beam mapping of the CHIME pathfinder array Proceedings of Spie. 9906
Croft RAC, Miralda-Escudé J, Zheng Z, et al. (2016) Large-scale clustering of Lyman α emission intensity from SDSS/BOSS Monthly Notices of the Royal Astronomical Society. 457: 3541-3572
Masui K, Lin HH, Sievers J, et al. (2015) Dense magnetized plasma associated with a fast radio burst. Nature
Masui K, Lin HH, Sievers J, et al. (2015) Dense magnetized plasma associated with a fast radio burst. Nature
Newburgh LB, Addison GE, Amiri M, et al. (2014) Calibrating CHIME: A new radio interferometer to probe dark energy Proceedings of Spie - the International Society For Optical Engineering. 9145
Bandura K, Addison GE, Amiri M, et al. (2014) Canadian hydrogen intensity mapping experiment (CHIME) pathfinder Proceedings of Spie - the International Society For Optical Engineering. 9145
Voytek TC, Natarajan A, Jáuregui García JM, et al. (2014) Probing the dark ages at z 20:The SCI-hi 21 cm all-sky spectrum experiment Astrophysical Journal Letters. 782
La Plante P, Battaglia N, Natarajan A, et al. (2014) Reionization on large scales. IV. Predictions for the 21 cm signal incorporating the light cone effect Astrophysical Journal. 789
Natarajan A, Peterson JB, Voytek TC, et al. (2013) Bounds on dark matter properties from radio observations of Ursa Major II using the Green Bank Telescope Physical Review D - Particles, Fields, Gravitation and Cosmology. 88
See more...