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Main Authors: The HERA Collaboration, Abdurashidova, Zuhra, Adams, Tyrone, Aguirre, James E., Baartman, Rushelle, Barkana, Rennan, Berkhout, Lindsay M., Bernardi, Gianni, Billings, Tashalee S., Bizarria, Bruno B., Bowman, Judd D., Breitman, Daniela, Bull, Philip, Burba, Jacob, Byrne, Ruby, Carey, Steven, Chandra, Rajorshi Sushovan, Chen, Kai-Feng, Choudhuri, Samir, Cox, Tyler, DeBoer, David R., Acedo, Eloy de Lera, Dexter, Matt, Dhandha, Jiten, Dillon, Joshua S., Dynes, Scott, Eksteen, Nico, Ely, John, Ewall-Wice, Aaron, Fagnoni, Nicolas, Fialkov, Anastasia, Furlanetto, Steven R., Gale-Sides, Kingsley, Garsden, Hugh, Gorce, Adelie, Gorthi, Deepthi, Halday, Ziyaad, Hazelton, Bryna J., Hewitt, Jacqueline N., Hickish, Jack, Huang, Tian, Jacobs, Daniel C., Josaitis, Alec, Kern, Nicholas S., Kerrigan, Joshua, Kittiwisit, Piyanat, Kolopanis, Matthew, Lanman, Adam, La Plante, Paul, Liu, Adrian, Ma, Yin-Zhe, MacMahon, David H. E., Malan, Lourence, Malgas, Cresshim, Malgas, Keith, Marero, Bradley, Martinot, Zachary E., McBride, Lisa, Mesinger, Andrei, Mirocha, Jordan, Mohamed-Hinds, Nicel, Molewa, Mathakane, Morales, Miguel F., Muñoz, Julian B., Murray, Steven G., Nikolic, Bojan, Nuwegeld, Hans, Parsons, Aaron R., Pascua, Robert, Patra, Nipanjana, Pochinda, Simon, Qin, Yuxiang, Rath, Eleanor, Razavi-Ghods, Nima, Riley, Daniel, Rosie, Kathryn, Santos, Mario G., Singh, Saurabh, Storer, Dara, Swarts, Hilton, Tan, Jianrong, Thélie, Emilie, van Wyngaarden, Pieter, Wilensky, Michael J., Williams, Peter K. G., Zheng, Haoxuan
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2511.21289
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author The HERA Collaboration
Abdurashidova, Zuhra
Adams, Tyrone
Aguirre, James E.
Baartman, Rushelle
Barkana, Rennan
Berkhout, Lindsay M.
Bernardi, Gianni
Billings, Tashalee S.
Bizarria, Bruno B.
Bowman, Judd D.
Breitman, Daniela
Bull, Philip
Burba, Jacob
Byrne, Ruby
Carey, Steven
Chandra, Rajorshi Sushovan
Chen, Kai-Feng
Choudhuri, Samir
Cox, Tyler
DeBoer, David R.
Acedo, Eloy de Lera
Dexter, Matt
Dhandha, Jiten
Dillon, Joshua S.
Dynes, Scott
Eksteen, Nico
Ely, John
Ewall-Wice, Aaron
Fagnoni, Nicolas
Fialkov, Anastasia
Furlanetto, Steven R.
Gale-Sides, Kingsley
Garsden, Hugh
Gorce, Adelie
Gorthi, Deepthi
Halday, Ziyaad
Hazelton, Bryna J.
Hewitt, Jacqueline N.
Hickish, Jack
Huang, Tian
Jacobs, Daniel C.
Josaitis, Alec
Kern, Nicholas S.
Kerrigan, Joshua
Kittiwisit, Piyanat
Kolopanis, Matthew
Lanman, Adam
La Plante, Paul
Liu, Adrian
Ma, Yin-Zhe
MacMahon, David H. E.
Malan, Lourence
Malgas, Cresshim
Malgas, Keith
Marero, Bradley
Martinot, Zachary E.
McBride, Lisa
Mesinger, Andrei
Mirocha, Jordan
Mohamed-Hinds, Nicel
Molewa, Mathakane
Morales, Miguel F.
Muñoz, Julian B.
Murray, Steven G.
Nikolic, Bojan
Nuwegeld, Hans
Parsons, Aaron R.
Pascua, Robert
Patra, Nipanjana
Pochinda, Simon
Qin, Yuxiang
Rath, Eleanor
Razavi-Ghods, Nima
Riley, Daniel
Rosie, Kathryn
Santos, Mario G.
Singh, Saurabh
Storer, Dara
Swarts, Hilton
Tan, Jianrong
Thélie, Emilie
van Wyngaarden, Pieter
Wilensky, Michael J.
Williams, Peter K. G.
Zheng, Haoxuan
author_facet The HERA Collaboration
Abdurashidova, Zuhra
Adams, Tyrone
Aguirre, James E.
Baartman, Rushelle
Barkana, Rennan
Berkhout, Lindsay M.
Bernardi, Gianni
Billings, Tashalee S.
Bizarria, Bruno B.
Bowman, Judd D.
Breitman, Daniela
Bull, Philip
Burba, Jacob
Byrne, Ruby
Carey, Steven
Chandra, Rajorshi Sushovan
Chen, Kai-Feng
Choudhuri, Samir
Cox, Tyler
DeBoer, David R.
Acedo, Eloy de Lera
Dexter, Matt
Dhandha, Jiten
Dillon, Joshua S.
Dynes, Scott
Eksteen, Nico
Ely, John
Ewall-Wice, Aaron
Fagnoni, Nicolas
Fialkov, Anastasia
Furlanetto, Steven R.
Gale-Sides, Kingsley
Garsden, Hugh
Gorce, Adelie
Gorthi, Deepthi
Halday, Ziyaad
Hazelton, Bryna J.
Hewitt, Jacqueline N.
Hickish, Jack
Huang, Tian
Jacobs, Daniel C.
Josaitis, Alec
Kern, Nicholas S.
Kerrigan, Joshua
Kittiwisit, Piyanat
Kolopanis, Matthew
Lanman, Adam
La Plante, Paul
Liu, Adrian
Ma, Yin-Zhe
MacMahon, David H. E.
Malan, Lourence
Malgas, Cresshim
Malgas, Keith
Marero, Bradley
Martinot, Zachary E.
McBride, Lisa
Mesinger, Andrei
Mirocha, Jordan
Mohamed-Hinds, Nicel
Molewa, Mathakane
Morales, Miguel F.
Muñoz, Julian B.
Murray, Steven G.
Nikolic, Bojan
Nuwegeld, Hans
Parsons, Aaron R.
Pascua, Robert
Patra, Nipanjana
Pochinda, Simon
Qin, Yuxiang
Rath, Eleanor
Razavi-Ghods, Nima
Riley, Daniel
Rosie, Kathryn
Santos, Mario G.
Singh, Saurabh
Storer, Dara
Swarts, Hilton
Tan, Jianrong
Thélie, Emilie
van Wyngaarden, Pieter
Wilensky, Michael J.
Williams, Peter K. G.
Zheng, Haoxuan
contents We report the first upper limits on the power spectrum of 21-cm fluctuations during the Epoch of Reionization and Cosmic Dawn from Phase II of the Hydrogen Epoch of Reionization Array (HERA) experiment. HERA Phase II constitutes several significant improvements in the signal chain compared to Phase I, most notably resulting in expanded frequency bandwidth, from 50-250 MHz. In these first upper limits, we investigate a small two-week subset of the available Phase II observations, with a focus on identifying new systematic characteristics of the instrument, and establishing an analysis pipeline to account for them. We report 2$σ$ upper limits in eight spectral bands, spanning $5.6 \leq z \leq 24.4$ that are consistent with thermal noise at the $2σ$ level for $k \gtrsim 0.6-0.9 h{\rm Mpc}^{-1}$ (band dependent). Our tightest limit during Cosmic Dawn ($z>12$) is $1.13\times 10^6 {\rm mK}^2$ at ($k=0.55 h{\rm Mpc}^{-1}, z=16.78$), and during the EoR ($5.5<z<12$) it is $1.78\times 10^3 {\rm mK}^2$ at ($k=0.70 h{\rm Mpc}^{-1}, z=7.05$). We find that mutual coupling has become our dominant systematic, leaking foreground power that strongly contaminates the low-$k$ modes, resulting in the loss of modes from $k=0.35-0.55$ compared to Phase I data.
format Preprint
id arxiv_https___arxiv_org_abs_2511_21289
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle First Results from HERA Phase II
The HERA Collaboration
Abdurashidova, Zuhra
Adams, Tyrone
Aguirre, James E.
Baartman, Rushelle
Barkana, Rennan
Berkhout, Lindsay M.
Bernardi, Gianni
Billings, Tashalee S.
Bizarria, Bruno B.
Bowman, Judd D.
Breitman, Daniela
Bull, Philip
Burba, Jacob
Byrne, Ruby
Carey, Steven
Chandra, Rajorshi Sushovan
Chen, Kai-Feng
Choudhuri, Samir
Cox, Tyler
DeBoer, David R.
Acedo, Eloy de Lera
Dexter, Matt
Dhandha, Jiten
Dillon, Joshua S.
Dynes, Scott
Eksteen, Nico
Ely, John
Ewall-Wice, Aaron
Fagnoni, Nicolas
Fialkov, Anastasia
Furlanetto, Steven R.
Gale-Sides, Kingsley
Garsden, Hugh
Gorce, Adelie
Gorthi, Deepthi
Halday, Ziyaad
Hazelton, Bryna J.
Hewitt, Jacqueline N.
Hickish, Jack
Huang, Tian
Jacobs, Daniel C.
Josaitis, Alec
Kern, Nicholas S.
Kerrigan, Joshua
Kittiwisit, Piyanat
Kolopanis, Matthew
Lanman, Adam
La Plante, Paul
Liu, Adrian
Ma, Yin-Zhe
MacMahon, David H. E.
Malan, Lourence
Malgas, Cresshim
Malgas, Keith
Marero, Bradley
Martinot, Zachary E.
McBride, Lisa
Mesinger, Andrei
Mirocha, Jordan
Mohamed-Hinds, Nicel
Molewa, Mathakane
Morales, Miguel F.
Muñoz, Julian B.
Murray, Steven G.
Nikolic, Bojan
Nuwegeld, Hans
Parsons, Aaron R.
Pascua, Robert
Patra, Nipanjana
Pochinda, Simon
Qin, Yuxiang
Rath, Eleanor
Razavi-Ghods, Nima
Riley, Daniel
Rosie, Kathryn
Santos, Mario G.
Singh, Saurabh
Storer, Dara
Swarts, Hilton
Tan, Jianrong
Thélie, Emilie
van Wyngaarden, Pieter
Wilensky, Michael J.
Williams, Peter K. G.
Zheng, Haoxuan
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
We report the first upper limits on the power spectrum of 21-cm fluctuations during the Epoch of Reionization and Cosmic Dawn from Phase II of the Hydrogen Epoch of Reionization Array (HERA) experiment. HERA Phase II constitutes several significant improvements in the signal chain compared to Phase I, most notably resulting in expanded frequency bandwidth, from 50-250 MHz. In these first upper limits, we investigate a small two-week subset of the available Phase II observations, with a focus on identifying new systematic characteristics of the instrument, and establishing an analysis pipeline to account for them. We report 2$σ$ upper limits in eight spectral bands, spanning $5.6 \leq z \leq 24.4$ that are consistent with thermal noise at the $2σ$ level for $k \gtrsim 0.6-0.9 h{\rm Mpc}^{-1}$ (band dependent). Our tightest limit during Cosmic Dawn ($z>12$) is $1.13\times 10^6 {\rm mK}^2$ at ($k=0.55 h{\rm Mpc}^{-1}, z=16.78$), and during the EoR ($5.5<z<12$) it is $1.78\times 10^3 {\rm mK}^2$ at ($k=0.70 h{\rm Mpc}^{-1}, z=7.05$). We find that mutual coupling has become our dominant systematic, leaking foreground power that strongly contaminates the low-$k$ modes, resulting in the loss of modes from $k=0.35-0.55$ compared to Phase I data.
title First Results from HERA Phase II
topic Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2511.21289