Effects of model incompleteness on the drift-scan calibration of radio telescopes. Issue 3 (20th July 2021)
- Record Type:
- Journal Article
- Title:
- Effects of model incompleteness on the drift-scan calibration of radio telescopes. Issue 3 (20th July 2021)
- Main Title:
- Effects of model incompleteness on the drift-scan calibration of radio telescopes
- Authors:
- Gehlot, Bharat K
Jacobs, Daniel C
Bowman, Judd D
Mahesh, Nivedita
Murray, Steven G
Kolopanis, Matthew
Beardsley, Adam P
Abdurashidova, Zara
Aguirre, James E
Alexander, Paul
Ali, Zaki S
Balfour, Yanga
Bernardi, Gianni
Billings, Tashalee S
Bradley, Richard F
Bull, Phil
Burba, Jacob
Carey, Steve
Carilli, Chris L
Cheng, Carina
DeBoer, David R
Dexter, Matt
de Lera Acedo, Eloy
Dillon, Joshua S
Ely, John
Ewall-Wice, Aaron
Fagnoni, Nicolas
Fritz, Randall
Furlanetto, Steven R
Gale-Sides, Kingsley
Glendenning, Brian
Gorthi, Deepthi
Greig, Bradley
Grobbelaar, Jasper
Halday, Ziyaad
Hazelton, Bryna J
Hewitt, Jacqueline N
Hickish, Jack
Julius, Austin
Kern, Nicholas S
Kerrigan, Joshua
Kittiwisit, Piyanat
Kohn, Saul A
Lanman, Adam
La Plante, Paul
Lekalake, Telalo
Lewis, David
Liu, Adrian
Ma, Yin-Zhe
MacMahon, David
Malan, Lourence
Malgas, Cresshim
Maree, Matthys
Martinot, Zachary E
Matsetela, Eunice
Mesinger, Andrei
Molewa, Mathakane
Monsalve, Raul A
Morales, Miguel F
Mosiane, Tshegofalang
Neben, Abraham R
Nikolic, Bojan
Parsons, Aaron R
Pascua, Robert
Patra, Nipanjana
Pieterse, Samantha
Pober, Jonathan C
Razavi-Ghods, Nima
Ringuette, Jon
Robnett, James
Rosie, Kathryn
Santos, Mario G
Sims, Peter
Smith, Craig
Syce, Angelo
Tegmark, Max
Thyagarajan, Nithyanandan
Williams, Peter K G
Zheng, Haoxuan
… (more) - Abstract:
- ABSTRACT: Precision calibration poses challenges to experiments probing the redshifted 21-cm signal of neutral hydrogen from the Cosmic Dawn and Epoch of Reionization ( z ∼ 30–6). In both interferometric and global signal experiments, systematic calibration is the leading source of error. Though many aspects of calibration have been studied, the overlap between the two types of instruments has received less attention. We investigate the sky based calibration of total power measurements with a HERA dish and an EDGES-style antenna to understand the role of autocorrelations in the calibration of an interferometer and the role of sky in calibrating a total power instrument. Using simulations we study various scenarios such as time variable gain, incomplete sky calibration model, and primary beam model. We find that temporal gain drifts, sky model incompleteness, and beam inaccuracies cause biases in the receiver gain amplitude and the receiver temperature estimates. In some cases, these biases mix spectral structure between beam and sky resulting in spectrally variable gain errors. Applying the calibration method to the HERA and EDGES data, we find good agreement with calibration via the more standard methods. Although instrumental gains are consistent with beam and sky errors similar in scale to those simulated, the receiver temperatures show significant deviations from expected values. While we show that it is possible to partially mitigate biases due to model inaccuracies byABSTRACT: Precision calibration poses challenges to experiments probing the redshifted 21-cm signal of neutral hydrogen from the Cosmic Dawn and Epoch of Reionization ( z ∼ 30–6). In both interferometric and global signal experiments, systematic calibration is the leading source of error. Though many aspects of calibration have been studied, the overlap between the two types of instruments has received less attention. We investigate the sky based calibration of total power measurements with a HERA dish and an EDGES-style antenna to understand the role of autocorrelations in the calibration of an interferometer and the role of sky in calibrating a total power instrument. Using simulations we study various scenarios such as time variable gain, incomplete sky calibration model, and primary beam model. We find that temporal gain drifts, sky model incompleteness, and beam inaccuracies cause biases in the receiver gain amplitude and the receiver temperature estimates. In some cases, these biases mix spectral structure between beam and sky resulting in spectrally variable gain errors. Applying the calibration method to the HERA and EDGES data, we find good agreement with calibration via the more standard methods. Although instrumental gains are consistent with beam and sky errors similar in scale to those simulated, the receiver temperatures show significant deviations from expected values. While we show that it is possible to partially mitigate biases due to model inaccuracies by incorporating a time-dependent gain model in calibration, the resulting errors on calibration products are larger and more correlated. Completely addressing these biases will require more accurate sky and primary beam models. … (more)
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 506:Issue 3(2021)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 506:Issue 3(2021)
- Issue Display:
- Volume 506, Issue 3 (2021)
- Year:
- 2021
- Volume:
- 506
- Issue:
- 3
- Issue Sort Value:
- 2021-0506-0003-0000
- Page Start:
- 4578
- Page End:
- 4592
- Publication Date:
- 2021-07-20
- Subjects:
- instrumentation: interferometers -- instrumentation: miscellaneous -- methods: data analysis -- methods: statistical -- techniques: interferometric -- dark ages, reionization, first stars
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/stab2072 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
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