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Main Authors: Murphy, Geoff G., Bull, Philip, Santos, Mario G., Abdurashidova, Zara, Adams, Tyrone, Aguirre, James E., Alexander, Paul, Ali, Zaki S., Baartman, Rushelle, Balfour, Yanga, Beardsley, Adam P., Bernardi, Gianni, Billings, Tashalee, Bowman, Judd D., Bradley, Richard F., Burba, Jacob, Cain, Christopher, Carey, Steven, Carilli, Chris L., Cheng, Carina, DeBoer, David R., Acedo, Eloy de Lera, Dexter, Matt, Dillon, Joshua S., Eksteen, Nico, 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, Jacobs, Daniel C., Julius, Austin, Kariseb, MacCalvin, Kern, Nicholas S., Kerrigan, Joshua, Kittiwisit, Piyanat, Kohn, Saul A., Kolopanis, Matthew, Lanman, Adam, La Plante, Paul, Liu, Adrian, Loots, Anita, MacMahon, David Harold Edward, Malan, Lourence, Malgas, Cresshim, Malgas, Keith, Marero, Bradley, Martinot, Zachary E., Mesinger, Andrei, Molewa, Mathakane, Morales, Miguel F., Mosiane, Tshegofalang, Murray, Steven G., Neben, Abraham R., Nikolic, Bojan, Nuwegeld, Hans, Parsons, Aaron R., Patra, Nipanjana, Pieterse, Samantha, Razavi-Ghods, Nima, Robnett, James, Rosie, Kathryn, Sims, Peter, Sipple, Jackson, Smith, Craig, Swarts, Hilton, Thyagarajan, Nithyanandan, van Wyngaarden, Pieter, Williams, Peter K. G., Zheng, Haoxuan
Format: Preprint
Published: 2023
Subjects:
Online Access:https://arxiv.org/abs/2312.03697
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author Murphy, Geoff G.
Bull, Philip
Santos, Mario G.
Abdurashidova, Zara
Adams, Tyrone
Aguirre, James E.
Alexander, Paul
Ali, Zaki S.
Baartman, Rushelle
Balfour, Yanga
Beardsley, Adam P.
Bernardi, Gianni
Billings, Tashalee
Bowman, Judd D.
Bradley, Richard F.
Burba, Jacob
Cain, Christopher
Carey, Steven
Carilli, Chris L.
Cheng, Carina
DeBoer, David R.
Acedo, Eloy de Lera
Dexter, Matt
Dillon, Joshua S.
Eksteen, Nico
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
Jacobs, Daniel C.
Julius, Austin
Kariseb, MacCalvin
Kern, Nicholas S.
Kerrigan, Joshua
Kittiwisit, Piyanat
Kohn, Saul A.
Kolopanis, Matthew
Lanman, Adam
La Plante, Paul
Liu, Adrian
Loots, Anita
MacMahon, David Harold Edward
Malan, Lourence
Malgas, Cresshim
Malgas, Keith
Marero, Bradley
Martinot, Zachary E.
Mesinger, Andrei
Molewa, Mathakane
Morales, Miguel F.
Mosiane, Tshegofalang
Murray, Steven G.
Neben, Abraham R.
Nikolic, Bojan
Nuwegeld, Hans
Parsons, Aaron R.
Patra, Nipanjana
Pieterse, Samantha
Razavi-Ghods, Nima
Robnett, James
Rosie, Kathryn
Sims, Peter
Sipple, Jackson
Smith, Craig
Swarts, Hilton
Thyagarajan, Nithyanandan
van Wyngaarden, Pieter
Williams, Peter K. G.
Zheng, Haoxuan
author_facet Murphy, Geoff G.
Bull, Philip
Santos, Mario G.
Abdurashidova, Zara
Adams, Tyrone
Aguirre, James E.
Alexander, Paul
Ali, Zaki S.
Baartman, Rushelle
Balfour, Yanga
Beardsley, Adam P.
Bernardi, Gianni
Billings, Tashalee
Bowman, Judd D.
Bradley, Richard F.
Burba, Jacob
Cain, Christopher
Carey, Steven
Carilli, Chris L.
Cheng, Carina
DeBoer, David R.
Acedo, Eloy de Lera
Dexter, Matt
Dillon, Joshua S.
Eksteen, Nico
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
Jacobs, Daniel C.
Julius, Austin
Kariseb, MacCalvin
Kern, Nicholas S.
Kerrigan, Joshua
Kittiwisit, Piyanat
Kohn, Saul A.
Kolopanis, Matthew
Lanman, Adam
La Plante, Paul
Liu, Adrian
Loots, Anita
MacMahon, David Harold Edward
Malan, Lourence
Malgas, Cresshim
Malgas, Keith
Marero, Bradley
Martinot, Zachary E.
Mesinger, Andrei
Molewa, Mathakane
Morales, Miguel F.
Mosiane, Tshegofalang
Murray, Steven G.
Neben, Abraham R.
Nikolic, Bojan
Nuwegeld, Hans
Parsons, Aaron R.
Patra, Nipanjana
Pieterse, Samantha
Razavi-Ghods, Nima
Robnett, James
Rosie, Kathryn
Sims, Peter
Sipple, Jackson
Smith, Craig
Swarts, Hilton
Thyagarajan, Nithyanandan
van Wyngaarden, Pieter
Williams, Peter K. G.
Zheng, Haoxuan
contents Observations with radio arrays that target the 21-cm signal originating from the early Universe suffer from a variety of systematic effects. An important class of these are reflections and spurious couplings between antennas. We apply a Hamiltonian Monte Carlo sampler to the modelling and mitigation of these systematics in simulated Hydrogen Epoch of Reionisation Array (HERA) data. This method allows us to form statistical uncertainty estimates for both our models and the recovered visibilities, which is an important ingredient in establishing robust upper limits on the Epoch of Reionisation (EoR) power spectrum. In cases where the noise is large compared to the EoR signal, this approach can constrain the systematics well enough to mitigate them down to the noise level for both systematics studied. Incoherently averaging the recovered power spectra can further reduce the noise and improve recovery. Where the noise level is lower than the EoR, our modelling can mitigate the majority of the reflections and coupling with there being only a minor level of residual systematics. Our approach performs similarly to existing filtering/fitting techniques used in the HERA pipeline, but with the added benefit of rigorously propagating uncertainties. In all cases it does not significantly attenuate the underlying signal.
format Preprint
id arxiv_https___arxiv_org_abs_2312_03697
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Bayesian estimation of cross-coupling and reflection systematics in 21cm array visibility data
Murphy, Geoff G.
Bull, Philip
Santos, Mario G.
Abdurashidova, Zara
Adams, Tyrone
Aguirre, James E.
Alexander, Paul
Ali, Zaki S.
Baartman, Rushelle
Balfour, Yanga
Beardsley, Adam P.
Bernardi, Gianni
Billings, Tashalee
Bowman, Judd D.
Bradley, Richard F.
Burba, Jacob
Cain, Christopher
Carey, Steven
Carilli, Chris L.
Cheng, Carina
DeBoer, David R.
Acedo, Eloy de Lera
Dexter, Matt
Dillon, Joshua S.
Eksteen, Nico
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
Jacobs, Daniel C.
Julius, Austin
Kariseb, MacCalvin
Kern, Nicholas S.
Kerrigan, Joshua
Kittiwisit, Piyanat
Kohn, Saul A.
Kolopanis, Matthew
Lanman, Adam
La Plante, Paul
Liu, Adrian
Loots, Anita
MacMahon, David Harold Edward
Malan, Lourence
Malgas, Cresshim
Malgas, Keith
Marero, Bradley
Martinot, Zachary E.
Mesinger, Andrei
Molewa, Mathakane
Morales, Miguel F.
Mosiane, Tshegofalang
Murray, Steven G.
Neben, Abraham R.
Nikolic, Bojan
Nuwegeld, Hans
Parsons, Aaron R.
Patra, Nipanjana
Pieterse, Samantha
Razavi-Ghods, Nima
Robnett, James
Rosie, Kathryn
Sims, Peter
Sipple, Jackson
Smith, Craig
Swarts, Hilton
Thyagarajan, Nithyanandan
van Wyngaarden, Pieter
Williams, Peter K. G.
Zheng, Haoxuan
Instrumentation and Methods for Astrophysics
Cosmology and Nongalactic Astrophysics
Observations with radio arrays that target the 21-cm signal originating from the early Universe suffer from a variety of systematic effects. An important class of these are reflections and spurious couplings between antennas. We apply a Hamiltonian Monte Carlo sampler to the modelling and mitigation of these systematics in simulated Hydrogen Epoch of Reionisation Array (HERA) data. This method allows us to form statistical uncertainty estimates for both our models and the recovered visibilities, which is an important ingredient in establishing robust upper limits on the Epoch of Reionisation (EoR) power spectrum. In cases where the noise is large compared to the EoR signal, this approach can constrain the systematics well enough to mitigate them down to the noise level for both systematics studied. Incoherently averaging the recovered power spectra can further reduce the noise and improve recovery. Where the noise level is lower than the EoR, our modelling can mitigate the majority of the reflections and coupling with there being only a minor level of residual systematics. Our approach performs similarly to existing filtering/fitting techniques used in the HERA pipeline, but with the added benefit of rigorously propagating uncertainties. In all cases it does not significantly attenuate the underlying signal.
title Bayesian estimation of cross-coupling and reflection systematics in 21cm array visibility data
topic Instrumentation and Methods for Astrophysics
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2312.03697