_version_ 1866910461463625728
author Lanman, Adam E.
Andrew, Shion
Lazda, Mattias
Shah, Vishwangi
Amiri, Mandana
Balasubramanian, Arvind
Bandura, Kevin
Boyle, P. J.
Brar, Charanjot
Carlson, Mark
Cliche, Jean-François
Gusinskaia, Nina
Hendricksen, Ian T.
Kaczmarek, J. F.
Landecker, Tom
Leung, Calvin
Mckinven, Ryan
Mena-Parra, Juan
Milutinovic, Nikola
Nimmo, Kenzie
Pearlman, Aaron B.
Renard, Andre
Rahman, Mubdi
Shaw, J. Richard
Siegel, Seth R.
Smegal, Rick J.
Cassanelli, Tomas
Chatterjee, Shami
Curtin, Alice P.
Dobbs, Matt
Dong, Fengqiu Adam
Halpern, Mark
Hopkins, Hans
Kaspi, Victoria M.
Khairy, Kholoud
Masui, Kiyoshi W.
Meyers, Bradley W.
Michilli, Daniele
Petroff, Emily
Pinsonneault-Marotte, Tristan
Pleunis, Ziggy
Rafiei-Ravandi, Masoud
Shin, Kaitlyn
Smith, Kendrick
Vanderlinde, Keith
Zegmott, Tarik J.
author_facet Lanman, Adam E.
Andrew, Shion
Lazda, Mattias
Shah, Vishwangi
Amiri, Mandana
Balasubramanian, Arvind
Bandura, Kevin
Boyle, P. J.
Brar, Charanjot
Carlson, Mark
Cliche, Jean-François
Gusinskaia, Nina
Hendricksen, Ian T.
Kaczmarek, J. F.
Landecker, Tom
Leung, Calvin
Mckinven, Ryan
Mena-Parra, Juan
Milutinovic, Nikola
Nimmo, Kenzie
Pearlman, Aaron B.
Renard, Andre
Rahman, Mubdi
Shaw, J. Richard
Siegel, Seth R.
Smegal, Rick J.
Cassanelli, Tomas
Chatterjee, Shami
Curtin, Alice P.
Dobbs, Matt
Dong, Fengqiu Adam
Halpern, Mark
Hopkins, Hans
Kaspi, Victoria M.
Khairy, Kholoud
Masui, Kiyoshi W.
Meyers, Bradley W.
Michilli, Daniele
Petroff, Emily
Pinsonneault-Marotte, Tristan
Pleunis, Ziggy
Rafiei-Ravandi, Masoud
Shin, Kaitlyn
Smith, Kendrick
Vanderlinde, Keith
Zegmott, Tarik J.
contents Localizing fast radio bursts (FRBs) to their host galaxies is an essential step to better understanding their origins and using them as cosmic probes. The CHIME/FRB Outrigger program aims to add VLBI-localization capabilities to CHIME, such that FRBs may be localized to tens of milliarcsecond precision at the time of their discovery, more than sufficient for host galaxy identification. The first-built outrigger telescope is KKO, located 66 kilometers west of CHIME. Cross-correlating KKO with CHIME can achieve arcsecond-scale localization in right ascension while avoiding the worst effects of the ionosphere. This paper presents measurements of KKO's performance throughout its commissioning phase, as well as a summary of its design and function. We demonstrate KKO's capabilities as a standalone instrument by producing full-sky images, mapping the angular and frequency structure of the primary beam, and measuring feed positions. To demonstrate the localization capabilities of the CHIME -- KKO baseline, we collected five separate observations each for a set of twenty bright pulsars, and aimed to measure their positions to within 5~arcseconds. All of these pulses were successfully localized to within this specification. The next two outriggers are expected to be commissioned in 2024, and will enable subarcsecond localizations for approximately hundreds of FRBs each year.
format Preprint
id arxiv_https___arxiv_org_abs_2402_07898
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle CHIME/FRB Outriggers: KKO Station System and Commissioning Results
Lanman, Adam E.
Andrew, Shion
Lazda, Mattias
Shah, Vishwangi
Amiri, Mandana
Balasubramanian, Arvind
Bandura, Kevin
Boyle, P. J.
Brar, Charanjot
Carlson, Mark
Cliche, Jean-François
Gusinskaia, Nina
Hendricksen, Ian T.
Kaczmarek, J. F.
Landecker, Tom
Leung, Calvin
Mckinven, Ryan
Mena-Parra, Juan
Milutinovic, Nikola
Nimmo, Kenzie
Pearlman, Aaron B.
Renard, Andre
Rahman, Mubdi
Shaw, J. Richard
Siegel, Seth R.
Smegal, Rick J.
Cassanelli, Tomas
Chatterjee, Shami
Curtin, Alice P.
Dobbs, Matt
Dong, Fengqiu Adam
Halpern, Mark
Hopkins, Hans
Kaspi, Victoria M.
Khairy, Kholoud
Masui, Kiyoshi W.
Meyers, Bradley W.
Michilli, Daniele
Petroff, Emily
Pinsonneault-Marotte, Tristan
Pleunis, Ziggy
Rafiei-Ravandi, Masoud
Shin, Kaitlyn
Smith, Kendrick
Vanderlinde, Keith
Zegmott, Tarik J.
Instrumentation and Methods for Astrophysics
Localizing fast radio bursts (FRBs) to their host galaxies is an essential step to better understanding their origins and using them as cosmic probes. The CHIME/FRB Outrigger program aims to add VLBI-localization capabilities to CHIME, such that FRBs may be localized to tens of milliarcsecond precision at the time of their discovery, more than sufficient for host galaxy identification. The first-built outrigger telescope is KKO, located 66 kilometers west of CHIME. Cross-correlating KKO with CHIME can achieve arcsecond-scale localization in right ascension while avoiding the worst effects of the ionosphere. This paper presents measurements of KKO's performance throughout its commissioning phase, as well as a summary of its design and function. We demonstrate KKO's capabilities as a standalone instrument by producing full-sky images, mapping the angular and frequency structure of the primary beam, and measuring feed positions. To demonstrate the localization capabilities of the CHIME -- KKO baseline, we collected five separate observations each for a set of twenty bright pulsars, and aimed to measure their positions to within 5~arcseconds. All of these pulses were successfully localized to within this specification. The next two outriggers are expected to be commissioned in 2024, and will enable subarcsecond localizations for approximately hundreds of FRBs each year.
title CHIME/FRB Outriggers: KKO Station System and Commissioning Results
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2402.07898