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A. Ewall-Wice

Identifiers

  • name variant A. Ewall-Wice 0.60 · backfill

Papers (26)

  1. Comparing Redundant and Sky Model Based Interferometric Calibration: A First Look with Phase II of the MWA astro-ph.IM · 2018 · author #17
  2. Modeling the Radio Background from the First Black Holes at Cosmic Dawn: Implications for the 21 cm Absorption Amplitude astro-ph.CO · 2018 · author #1
  3. Spectral energy distribution and radio halo of NGC 253 at low radio frequencies astro-ph.GA · 2017 · author #32
  4. Delay Spectrum with Phase-Tracking Arrays: Extracting the HI power spectrum from the Epoch of Reionization astro-ph.CO · 2016 · author #14
  5. First Season MWA EoR Power Spectrum Results at Redshift 7 astro-ph.IM · 2016 · author #22
  6. Low frequency observations of linearly polarized structures in the interstellar medium near the south Galactic pole astro-ph.GA · 2016 · author #21
  7. A High Reliability Survey of Discrete Epoch of Reionization Foreground Sources in the MWA EoR0 Field astro-ph.IM · 2016 · author #19
  8. The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology astro-ph.IM · 2016 · author #18
  9. Brute-Force Mapmaking with Compact Interferometers: A MITEoR Northern Sky Map from 128 MHz to 175 MHz astro-ph.IM · 2016 · author #9
  10. First Limits on the 21 cm Power Spectrum during the Epoch of X-ray heating astro-ph.CO · 2016 · author #1
  11. Parametrising Epoch of Reionization foregrounds: A deep survey of low-frequency point-source spectra with the MWA astro-ph.IM · 2016 · author #12
  12. CHIPS: The Cosmological HI Power Spectrum Estimator astro-ph.IM · 2016 · author #17
  13. Broadband Spectral Modeling of the Extreme Gigahertz-Peaked Spectrum Radio Source PKS B0008-421 astro-ph.GA · 2015 · author #14
  14. Ionospheric modelling using GPS to calibrate the MWA. 1: Comparison of first order ionospheric effects between GPS models and MWA observations astro-ph.IM · 2015 · author #13
  15. Confirmation of Wide-Field Signatures in Redshifted 21 cm Power Spectra astro-ph.CO · 2015 · author #13
  16. Empirical Covariance Modeling for 21 cm Power Spectrum Estimation: A Method Demonstration and New Limits from Early Murchison Widefield Array 128-Tile Data astro-ph.CO · 2015 · author #11
  17. Foregrounds in Wide-Field Redshifted 21 cm Power Spectra astro-ph.IM · 2015 · author #14
  18. The low-frequency environment of the Murchison Widefield Array: radio-frequency interference analysis and mitigation astro-ph.IM · 2015 · author #17
  19. Modelling of the Spectral Energy Distribution of Fornax A: Leptonic and Hadronic Production of High Energy Emission from the Radio Lobes astro-ph.HE · 2014 · author #22
  20. First Look Murchison Widefield Array observations of Abell 3667 astro-ph.GA · 2014 · author #17
  21. The first Murchison Widefield Array low frequency radio observations of cluster scale non-thermal emission: the case of Abell 3667 astro-ph.GA · 2014 · author #17
  22. WSClean: an implementation of a fast, generic wide-field imager for radio astronomy astro-ph.IM · 2014 · author #20
  23. On the detection and tracking of space debris using the Murchison Widefield Array. I. Simulations and test observations demonstrate feasibility astro-ph.IM · 2013 · author #46
  24. Performance and on-sky optical characterization of the SPTpol instrument astro-ph.IM · 2012 · author #21
  25. South Pole Telescope Software Systems: Control, Monitoring, and Data Acquisition astro-ph.IM · 2012 · author #22
  26. Feedhorn-coupled TES polarimeter camera modules at 150 GHz for CMB polarization measurements with SPTpol astro-ph.IM · 2012 · author #19

Mentions

  • 1501.03946 #17 · backfill · confidence 0.70 A. Ewall-Wice
  • 1411.1487 #22 · backfill · confidence 0.70 A. Ewall-Wice
  • 1409.2943 #17 · backfill · confidence 0.70 A. Ewall-Wice
  • 1408.3167 #17 · backfill · confidence 0.70 A. Ewall-Wice
  • 1407.1943 #20 · backfill · confidence 0.70 A. Ewall-Wice
  • 1308.2742 #46 · backfill · confidence 0.70 A. Ewall-Wice
  • 1210.4971 #21 · backfill · confidence 0.70 A. Ewall-Wice
  • 1210.4969 #19 · backfill · confidence 0.70 A. Ewall-Wice
  • 1210.4966 #22 · backfill · confidence 0.70 A. Ewall-Wice

Frequent Coauthors