Holographic beam mapping of the CHIME pathfinder array

Philippe Berger; Laura B. Newburgh; Mandana Amiri; Kevin Bandura; Jean François Cliche; Liam Connor; Meiling Deng; Nolan Denman; Matt Dobbs; Mateus Fandino; Adam J. Gilbert; Deborah Good; Mark Halperne; David Hanna; Adam D. Hincks; Gary Hinshaw; Carolin Höfer; Andre M. Johnson; Tom L. Landecker; Kiyoshi W. Masui; Juan Mena Parra; Niels Oppermann; Ue Li Pen; Jeŗey B. Petersonl; Andre Recnik; Timothy Robishawj; J. Richard Shaw; Seth Siegel; Kris Sigurdson; Kendrick Smith; Emilie Storer; Ian Tretyakov; Kwinten VanGassen; Keith Vanderlinde; Donald Wiebe

doi:10.1117/12.2233782

Holographic beam mapping of the CHIME pathfinder array

Philippe Berger
, Laura B. Newburgh
, Mandana Amiri
, Kevin Bandura
, Jean François Cliche
, Liam Connor
, Meiling Deng
, Nolan Denman
, Matt Dobbs
, Mateus Fandino
, Adam J. Gilbert
, Deborah Good
, Mark Halperne
, David Hanna
, Adam D. Hincks
, Gary Hinshaw
, Carolin Höfer
, Andre M. Johnson
, Tom L. Landecker
, Kiyoshi W. Masui

Juan Mena Parra, Niels Oppermann, Ue Li Pen, Jeŗey B. Petersonl, Andre Recnik, Timothy Robishawj, J. Richard Shaw, Seth Siegel, Kris Sigurdson, Kendrick Smith, Emilie Storer, Ian Tretyakov, Kwinten VanGassen, Keith Vanderlinde, Donald Wiebe

Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

25 Scopus citations

Abstract

The Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder radio telescope is currently surveying the northern hemisphere between 400 and 800 MHz. By mapping the large scale structure of neutral hydrogen through its redshifted 21 cm line emission between z ∼0.8-2.5 CHIME will contribute to our understanding of Dark Energy. Bright astrophysical foregrounds must be separated from the neutral hydrogen signal, a task which requires precise characterization of the polarized telescope beams. Using the DRAO John A. Galt 26 m telescope, we have developed a holography instrument and technique for mapping the CHIME Pathfinder beams. We report the status of the instrument and initial results of this effort.

Original language	English
Title of host publication	Ground-Based and Airborne Telescopes VI
Editors	Heather K. Marshall, Helen J. Hall, Roberto Gilmozzi
Publisher	SPIE
ISBN (Electronic)	9781510601918
DOIs	https://doi.org/10.1117/12.2233782
State	Published - 2016
Event	Ground-Based and Airborne Telescopes VI - Edinburgh, United Kingdom Duration: Jun 26 2016 → Jul 1 2016

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9906
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Ground-Based and Airborne Telescopes VI
Country/Territory	United Kingdom
City	Edinburgh
Period	06/26/16 → 07/1/16

Keywords

BAO
Calibration
CHIME
Cosmology
Radio holography
SPIE proceedings

Access to Document

10.1117/12.2233782

Cite this

Berger, P., Newburgh, L. B., Amiri, M., Bandura, K., Cliche, J. F., Connor, L., Deng, M., Denman, N., Dobbs, M., Fandino, M., Gilbert, A. J., Good, D., Halperne, M., Hanna, D., Hincks, A. D., Hinshaw, G., Höfer, C., Johnson, A. M., Landecker, T. L., ... Wiebe, D. (2016). Holographic beam mapping of the CHIME pathfinder array. In H. K. Marshall, H. J. Hall, & R. Gilmozzi (Eds.), Ground-Based and Airborne Telescopes VI Article 99060D (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9906). SPIE. https://doi.org/10.1117/12.2233782

@inproceedings{6cc477b5e08c4d7fbd31b216a91b1bfd,

title = "Holographic beam mapping of the CHIME pathfinder array",

abstract = "The Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder radio telescope is currently surveying the northern hemisphere between 400 and 800 MHz. By mapping the large scale structure of neutral hydrogen through its redshifted 21 cm line emission between z ∼0.8-2.5 CHIME will contribute to our understanding of Dark Energy. Bright astrophysical foregrounds must be separated from the neutral hydrogen signal, a task which requires precise characterization of the polarized telescope beams. Using the DRAO John A. Galt 26 m telescope, we have developed a holography instrument and technique for mapping the CHIME Pathfinder beams. We report the status of the instrument and initial results of this effort.",

keywords = "BAO, Calibration, CHIME, Cosmology, Radio holography, SPIE proceedings",

author = "Philippe Berger and Newburgh, \{Laura B.\} and Mandana Amiri and Kevin Bandura and Cliche, \{Jean Fran{\c c}ois\} and Liam Connor and Meiling Deng and Nolan Denman and Matt Dobbs and Mateus Fandino and Gilbert, \{Adam J.\} and Deborah Good and Mark Halperne and David Hanna and Hincks, \{Adam D.\} and Gary Hinshaw and Carolin H{\"o}fer and Johnson, \{Andre M.\} and Landecker, \{Tom L.\} and Masui, \{Kiyoshi W.\} and Parra, \{Juan Mena\} and Niels Oppermann and Pen, \{Ue Li\} and Petersonl, \{Jeŗey B.\} and Andre Recnik and Timothy Robishawj and Shaw, \{J. Richard\} and Seth Siegel and Kris Sigurdson and Kendrick Smith and Emilie Storer and Ian Tretyakov and Kwinten VanGassen and Keith Vanderlinde and Donald Wiebe",

note = "Publisher Copyright: {\textcopyright} 2016 SPIE.; Ground-Based and Airborne Telescopes VI ; Conference date: 26-06-2016 Through 01-07-2016",

year = "2016",

doi = "10.1117/12.2233782",

language = "English",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Marshall, \{Heather K.\} and Hall, \{Helen J.\} and Roberto Gilmozzi",

booktitle = "Ground-Based and Airborne Telescopes VI",

}

Berger, P, Newburgh, LB, Amiri, M, Bandura, K, Cliche, JF, Connor, L, Deng, M, Denman, N, Dobbs, M, Fandino, M, Gilbert, AJ, Good, D, Halperne, M, Hanna, D, Hincks, AD, Hinshaw, G, Höfer, C, Johnson, AM, Landecker, TL, Masui, KW, Parra, JM, Oppermann, N, Pen, UL, Petersonl, JB, Recnik, A, Robishawj, T, Shaw, JR, Siegel, S, Sigurdson, K, Smith, K, Storer, E, Tretyakov, I, VanGassen, K, Vanderlinde, K & Wiebe, D 2016, Holographic beam mapping of the CHIME pathfinder array. in HK Marshall, HJ Hall & R Gilmozzi (eds), Ground-Based and Airborne Telescopes VI., 99060D, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9906, SPIE, Ground-Based and Airborne Telescopes VI, Edinburgh, United Kingdom, 06/26/16. https://doi.org/10.1117/12.2233782

Holographic beam mapping of the CHIME pathfinder array. / Berger, Philippe; Newburgh, Laura B.; Amiri, Mandana et al.
Ground-Based and Airborne Telescopes VI. ed. / Heather K. Marshall; Helen J. Hall; Roberto Gilmozzi. SPIE, 2016. 99060D (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9906).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - Holographic beam mapping of the CHIME pathfinder array

AU - Berger, Philippe

AU - Newburgh, Laura B.

AU - Amiri, Mandana

AU - Bandura, Kevin

AU - Cliche, Jean François

AU - Connor, Liam

AU - Deng, Meiling

AU - Denman, Nolan

AU - Dobbs, Matt

AU - Fandino, Mateus

AU - Gilbert, Adam J.

AU - Good, Deborah

AU - Halperne, Mark

AU - Hanna, David

AU - Hincks, Adam D.

AU - Hinshaw, Gary

AU - Höfer, Carolin

AU - Johnson, Andre M.

AU - Landecker, Tom L.

AU - Masui, Kiyoshi W.

AU - Parra, Juan Mena

AU - Oppermann, Niels

AU - Pen, Ue Li

AU - Petersonl, Jeŗey B.

AU - Recnik, Andre

AU - Robishawj, Timothy

AU - Shaw, J. Richard

AU - Siegel, Seth

AU - Sigurdson, Kris

AU - Smith, Kendrick

AU - Storer, Emilie

AU - Tretyakov, Ian

AU - VanGassen, Kwinten

AU - Vanderlinde, Keith

AU - Wiebe, Donald

PY - 2016

Y1 - 2016

N2 - The Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder radio telescope is currently surveying the northern hemisphere between 400 and 800 MHz. By mapping the large scale structure of neutral hydrogen through its redshifted 21 cm line emission between z ∼0.8-2.5 CHIME will contribute to our understanding of Dark Energy. Bright astrophysical foregrounds must be separated from the neutral hydrogen signal, a task which requires precise characterization of the polarized telescope beams. Using the DRAO John A. Galt 26 m telescope, we have developed a holography instrument and technique for mapping the CHIME Pathfinder beams. We report the status of the instrument and initial results of this effort.

AB - The Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder radio telescope is currently surveying the northern hemisphere between 400 and 800 MHz. By mapping the large scale structure of neutral hydrogen through its redshifted 21 cm line emission between z ∼0.8-2.5 CHIME will contribute to our understanding of Dark Energy. Bright astrophysical foregrounds must be separated from the neutral hydrogen signal, a task which requires precise characterization of the polarized telescope beams. Using the DRAO John A. Galt 26 m telescope, we have developed a holography instrument and technique for mapping the CHIME Pathfinder beams. We report the status of the instrument and initial results of this effort.

KW - BAO

KW - Calibration

KW - CHIME

KW - Cosmology

KW - Radio holography

KW - SPIE proceedings

UR - https://www.scopus.com/pages/publications/85001124055

U2 - 10.1117/12.2233782

DO - 10.1117/12.2233782

M3 - Conference contribution

AN - SCOPUS:85001124055

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Ground-Based and Airborne Telescopes VI

A2 - Marshall, Heather K.

A2 - Hall, Helen J.

A2 - Gilmozzi, Roberto

PB - SPIE

T2 - Ground-Based and Airborne Telescopes VI

Y2 - 26 June 2016 through 1 July 2016

ER -

Holographic beam mapping of the CHIME pathfinder array

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Keywords

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