Grant: Alliance Grants
McGill University
$706,317.00
CHIME Telescope Operations
FY 2024-25
Summary
CHIME, the Canadian Hydrogen Intensity-Mapping Experiment (www.chime-experiment.ca), is truly a breakthrough radio telescope. With it, Canadian researchers have transformed the field of transient astrophysics, discovering over 4,000 fast radio bursts (FRBs), including over 50 repeating sources, all arriving from across the cosmos, along with an FRB from a Milky Way magnetar. CHIME has also performed the highest redshift neutral hydrogen intensity mapping survey to date, and has become an important part of the global effort to study radio pulsars, rapidly rotating, highly magnetized neutron stars. It measures signal arrival times for all pulsars visible in North America, most of these at daily cadence. The demonstrated power of this prize-winning instrument has attracted a large and talented team to base their research on it, and multiple new experiments are planned. The team is building remote companion "outrigger" telescopes to allow precision localisation of the source of each FRB. They have also built an instrument to scan for slow spin-rate pulsars, designed a method to study the Milky Way's magnetic field, and a data analysis pipeline to search for direct evidence of cosmic acceleration. We propose here for 5 years of operating funds to allow us to continue to run CHIME to accomplish multiple forefront science goals, and to continue to engage a large fraction of the Canadian astrophysical community, as well as researchers from around the globe.
Program
Alliance Grants
Recipient
Location
Quebec, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data
As published
Application id
587197-2023
Name nom
Kaspi, Victoria VM
Department département
Physics
Organization id
61
Institution établissement
McGill University
Province en
Québec
Province fr
Québec
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2024
Competition year année de concours
2023
Award amount
706317
Program id
ALLRP
Program name en
Alliance Grants
Program name fr
Subventions Alliance
Group en
RESEARCH PARTNERSHIPS
Group fr
PARTENARIATS DE RECHERCHE
Committee code
96
Committee name en
RPP Internal Decision Cttee
Committee name fr
Cté de décision interne - PPR
Area of application code
1200
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Advancement of knowledge
Area of application fr
Avancement des connaissances
Research subject code
3200
Research subject group en
Astronomy and astrophysics
Research subject group fr
Astronomie et astrophysique
Research subject en
Astronomy and astrophysics
Research subject fr
Astronomie et astrophysique
Field of research list names en
Not available
Field of research list names fr
Non disponible
Socioeconomic objective list names en
Not available
Socioeconomic objective list names fr
Non disponible
Application title
CHIME Telescope Operations
Keywords
21-cm cosmology; fast radio transients; galactic magnetism; large scale structure; magnetars; pulsars; radio astronomy; radio polarimetry
Application summary
CHIME, the Canadian Hydrogen Intensity-Mapping Experiment (www.chime-experiment.ca), is truly a breakthrough radio telescope. With it, Canadian researchers have transformed the field of transient astrophysics, discovering over 4,000 fast radio bursts (FRBs), including over 50 repeating sources, all arriving from across the cosmos, along with an FRB from a Milky Way magnetar. CHIME has also performed the highest redshift neutral hydrogen intensity mapping survey to date, and has become an important part of the global effort to study radio pulsars, rapidly rotating, highly magnetized neutron stars. It measures signal arrival times for all pulsars visible in North America, most of these at daily cadence. The demonstrated power of this prize-winning instrument has attracted a large and talented team to base their research on it, and multiple new experiments are planned. The team is building remote companion "outrigger" telescopes to allow precision localisation of the source of each FRB. They have also built an instrument to scan for slow spin-rate pulsars, designed a method to study the Milky Way's magnetic field, and a data analysis pipeline to search for direct evidence of cosmic acceleration. We propose here for 5 years of operating funds to allow us to continue to run CHIME to accomplish multiple forefront science goals, and to continue to engage a large fraction of the Canadian astrophysical community, as well as researchers from around the globe.