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The Experiment for Cryogenic Large-aperture Intensity Mapping (EXCLAIM)

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arxiv 1912.07118 v1 pith:K3U2NPMZ submitted 2019-12-15 astro-ph.IM astro-ph.CO

P. A. R. Ade , C. J. Anderson , E. M. Barrentine , N. G. Bellis , A. D. Bolatto , P. C. Breysse , B. T. Bulcha , G. Cataldo
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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 J. McMahon M. Mirzaei S. H. Moseley J. W. Mugge-Durum O. Noroozian U. Pen A. R. Pullen S. Rodriguez P. J. Shirron R. S. Somerville T. R. Stevenson E. R. Switzer C. Tucker E. Visbal C. G. Volpert E. J. Wollack S. Yang
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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) coupled to microwave kinetic inductance detectors (MKIDs). Here we present an overview of the EXCLAIM instrument design and status.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Reading Between the Lines: Forward Modeling Dust, Continuum, and Spectral Cleaning for Multi-Line Intensity Mapping

    astro-ph.GA 2026-07 conditional novelty 5.0 of 10

    Using a SAM-based mock, multi-line intensity-mapping cross-power spectra show dust acts as a line-pair- and redshift-dependent suppression, and PCA cleaning with about 20 modes best balances line recovery against cont...

  2. On Cross-Correlating Line Intensity Maps from SPHEREx during Reionization

    astro-ph.GA 2026-06 unverdicted novelty 5.0 of 10

    Simulations of SPHEREx line intensity maps show cross-correlations (e.g., Hα × [OIII] at z=5) can reach S/N up to 99, probing galaxies with M < 4×10^10 M⊙, though most signal comes from brighter directly detectable galaxies.

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