Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. Absolute Calibration Strategies for the Hydrogen Epoch of Reionization Array and Their Impact on the 21 cm Power Spectrum
 

Absolute Calibration Strategies for the Hydrogen Epoch of Reionization Array and Their Impact on the 21 cm Power Spectrum

Journal
THE ASTROPHYSICAL JOURNAL  
Date Issued
2020
Author(s)
Kern, Nicholas S.
•
Dillon, Joshua S.
•
Parsons, Aaron R.
•
Carilli, Christopher L.
•
BERNARDI, GIANNI  
•
Abdurashidova, Zara
•
Aguirre, James E.
•
Alexander, Paul
•
Ali, Zaki S.
•
Balfour, Yanga
•
Beardsley, Adam P.
•
Billings, Tashalee S.
•
Bowman, Judd D.
•
Bradley, Richard F.
•
BULL, PHILIP  
•
Burba, Jacob
•
Carey, Steven
•
Cheng, Carina
•
DeBoer, David R.
•
Dexter, Matt
•
de Lera Acedo, Eloy
•
Ely, John
•
Ewall-Wice, Aaron
•
Fagnoni, Nicolas
•
Fritz, Randall
•
Furlanetto, Steve R.
•
Gale-Sides, Kingsley
•
Glendenning, Brian
•
Gorthi, Deepthi
•
Greig, Bradley
•
Grobbelaar, Jasper
•
Halday, Ziyaad
•
Hazelton, Bryna J.
•
Hewitt, Jacqueline N.
•
Hickish, Jack
•
Jacobs, Daniel C.
•
Julius, Austin
•
Kerrigan, Joshua
•
Kittiwisit, Piyanat
•
Kohn, Saul A.
•
Kolopanis, Matthew
•
Lanman, Adam
•
La Plante, Paul
•
Lekalake, Telalo
•
Liu, Adrian
•
MacMahon, David
•
Malan, Lourence
•
Malgas, Cresshim
•
Maree, Matthys
•
Martinot, Zachary E.
•
Matsetela, Eunice
•
Mesinger, Andrei  
•
Molewa, Mathakane
•
Morales, Miguel F.
•
Mosiane, Tshegofalang
•
Murray, Steven G.
•
Neben, Abraham R.
•
Nikolic, Bojan
•
Nunhokee, Chuneeta D.
•
Patra, Nipanjana
•
Pieterse, Samantha
•
Pober, Jonathan C.
•
Razavi-Ghods, Nima
•
Ringuette, Jon
•
Robnett, James
•
Rosie, Kathryn
•
Sims, Peter
•
Smith, Craig
•
Syce, Angelo
•
Thyagarajan, Nithyanandan
•
Williams, Peter K. G.
•
Zheng, Haoxuan
DOI
10.3847/1538-4357/ab67bc
Abstract
We discuss absolute calibration strategies for Phase I of the Hydrogen Epoch of Reionization Array (HERA), which aims to measure the cosmological 21 cm signal from the Epoch of Reionization. HERA is a drift-scan array with a 10° wide field of view, meaning bright, well-characterized point-source transits are scarce. This, combined with HERA's redundant sampling of the uv plane and the modest angular resolution of the Phase I instrument, make traditional sky-based and self-calibration techniques difficult to implement with high dynamic range. Nonetheless, in this work, we demonstrate calibration for HERA using point-source catalogs and electromagnetic simulations of its primary beam. We show that unmodeled diffuse flux and instrumental contaminants can corrupt the gain solutions and present a gain-smoothing approach for mitigating their impact on the 21 cm power spectrum. We also demonstrate a hybrid sky and redundant calibration scheme and compare it to pure sky-based calibration, showing only a marginal improvement to the gain solutions at intermediate delay scales. Our work suggests that the HERA Phase I system can be well calibrated for a foreground avoidance power spectrum estimator by applying direction-independent gains with a small set of degrees of freedom across the frequency and time axes.
Volume
890
Issue
2
Start page
122
Uri
http://hdl.handle.net/20.500.12386/31766
Url
https://iopscience.iop.org/article/10.3847/1538-4357/ab67bc
Issn Identifier
0004-637X
Ads BibCode
2020ApJ...890..122K
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

kern20b_archive.pdf

Description
postprint
Size

8.21 MB

Format

Adobe PDF

Checksum (MD5)

4d88e34d72cf2d8f360df01c93a8fd2b

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback