CONCERTO
(Carbon CII Line in Post-Reionization and Reionization Epoch)
(spectrometer aimed at mapping the [CII] line)
CONCERTO (loosely for
Carbon CII Line in Post-Reionization and Reionization Epoch)
is a spectrometer for intensity mapping of the redshifted
ionized carbon forbidden line [CII]
from the epoch of reionization and from subsequent star formation.
The spectral line is in the submillimeter range,
and the instrument will disperse wavelengths with
a Martin-Puplett interferometer
(type of adjustable Michelson interferometer)
and sense with KIDs, achieving spectral resolutions
down to 1 GHz and angular resolutions down to 20 arcseconds.
In addition to its intended intensity mapping,
the instrument was used to study galaxy clusters.
The instrument was installed in 2020-2021 on the Atacama Pathfinder Experiment (APEX), data
was collected during 2021-2022, and the instrument was removed in 2023.
As of 2/2025, I presume data analysis might be continuing.
A related effort is KISS (for KIDs Interferometer Spectrum Survey)
with an analogous instrument for a lower frequency range,
aiming to map Sunyaev-Zel'dovich effects. It is installed on one of the
two 2.25-m QUIJOTE telescopes
at Teide Observatory on the Canary Islands.
(instrument,star formation,spectrometer,intensity mapping,past)
Further reading:
https://mission.lam.fr/concerto/
https://www.apex-telescope.org/ns/observing-run/observing/the-telescope/instruments/concerto/
https://www.apex-telescope.org/ns/news/apex/it-was-a-beautiful-concerto/
https://agenda.infn.it/event/25056/contributions/137181/attachments/83182/109522/mm_conf_Rome.pdf
https://ui.adsabs.harvard.edu/abs/2020A%26A...642A..60C/abstract
https://ui.adsabs.harvard.edu/abs/2018IAUS..333..228L/abstract
https://arxiv.org/abs/2311.04704
https://ui.adsabs.harvard.edu/abs/2022EPJWC.25700017F/abstract
WaveL | Freq | Photon Energy | | |
967μm | 310GHz | 1.3meV | begin | CONCERTO |
2.4mm | 130GHz | 538μeV | end | CONCERTO |
|
Referenced by page:
intensity mapping surveys
Index