The Experiment for Cryogenic Large-aperture Intensity Mapping (EXCLAIM)
P. A. R. Ade, C. J. Anderson, E. M. Barrentine, N. G. Bellis, A. D., Bolatto, P. C. Breysse, B. T. Bulcha, G. Cataldo, J. A. Connors, P. W., Cursey, N. Ehsan, H. C. Grant, T. M. Essinger-Hileman, L. A. Hess, M. O., Kimball, A. J. Kogut, A. D. Lamb, L. N. Lowe, P. D. Mauskopf

TL;DR
EXCLAIM is a balloon-borne cryogenic instrument designed to map large-scale galaxy and star formation history through intensity mapping of CO and [CII] emissions across redshifts 0 to 3.5, providing insights into star formation decline.
Contribution
It introduces a novel intensity mapping approach with a cryogenic balloon-borne instrument targeting CO and [CII] lines over a broad redshift range.
Findings
Design overview of the EXCLAIM instrument
Status update on instrument development
Potential to advance understanding of star formation history
Abstract
The EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) is a cryogenic balloon-borne instrument that will survey galaxy and star formation history over cosmological time scales. Rather than identifying individual objects, EXCLAIM will be a pathfinder to demonstrate an intensity mapping approach, which measures the cumulative redshifted line emission. EXCLAIM will operate at 420-540 GHz with a spectral resolution R=512 to measure the integrated CO and [CII] in redshift windows spanning 0 < z < 3.5. CO and [CII] line emissions are key tracers of the gas phases in the interstellar medium involved in star-formation processes. EXCLAIM will shed light on questions such as why the star formation rate declines at z < 2, despite continued clustering of the dark matter. The instrument will employ an array of six superconducting integrated grating-analog spectrometers (micro-spec)…
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