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; 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

doi:10.1007/s10909-019-02320-5

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, J. McMahonM. 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

Earth and Space Exploration, School of (SESE)

Research output: Contribution to journal › Article › peer-review

19 Scopus citations

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 timescales. 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 (μ-Spec) coupled to microwave kinetic inductance detectors. Here we present an overview of the EXCLAIM instrument design and status.

Original language	English (US)
Pages (from-to)	1027-1037
Number of pages	11
Journal	Journal of Low Temperature Physics
Volume	199
Issue number	3-4
DOIs	https://doi.org/10.1007/s10909-019-02320-5
State	Published - May 1 2020

Keywords

Galaxy evolution
Integrated spectrometers
Intensity mapping
MKID

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics
General Materials Science
Condensed Matter Physics

Access to Document

10.1007/s10909-019-02320-5

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Ade, P. A. R., Anderson, C. J., Barrentine, E. M., Bellis, N. G., Bolatto, A. D., Breysse, P. C., Bulcha, B. T., Cataldo, G., Connors, J. A., Cursey, P. W., Ehsan, N., Grant, H. C., Essinger-Hileman, T. M., Hess, L. A., Kimball, M. O., Kogut, A. J., Lamb, A. D., Lowe, L. N., Mauskopf, P. D., ... Yang, S. (2020). The Experiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM). Journal of Low Temperature Physics, 199(3-4), 1027-1037. https://doi.org/10.1007/s10909-019-02320-5

Ade, PAR, Anderson, CJ, Barrentine, EM, Bellis, NG, Bolatto, AD, Breysse, PC, Bulcha, BT, Cataldo, G, Connors, JA, Cursey, PW, Ehsan, N, Grant, HC, Essinger-Hileman, TM, Hess, LA, Kimball, MO, Kogut, AJ, Lamb, AD, Lowe, LN, Mauskopf, PD, McMahon, J, Mirzaei, M, Moseley, SH, Mugge-Durum, JW, Noroozian, O, Pen, U, Pullen, AR, Rodriguez, S, Shirron, PJ, Somerville, RS, Stevenson, TR, Switzer, ER, Tucker, C, Visbal, E, Volpert, CG, Wollack, EJ & Yang, S 2020, 'The Experiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM)', Journal of Low Temperature Physics, vol. 199, no. 3-4, pp. 1027-1037. https://doi.org/10.1007/s10909-019-02320-5

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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 timescales. 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 (μ-Spec) coupled to microwave kinetic inductance detectors. Here we present an overview of the EXCLAIM instrument design and status.",

keywords = "Galaxy evolution, Integrated spectrometers, Intensity mapping, MKID",

author = "Ade, {P. A.R.} and Anderson, {C. J.} and Barrentine, {E. M.} and Bellis, {N. G.} and Bolatto, {A. D.} and Breysse, {P. C.} and Bulcha, {B. T.} and G. Cataldo and Connors, {J. A.} and Cursey, {P. W.} and N. Ehsan and Grant, {H. C.} and Essinger-Hileman, {T. M.} and Hess, {L. A.} and Kimball, {M. O.} and Kogut, {A. J.} and Lamb, {A. D.} and Lowe, {L. N.} and Mauskopf, {P. D.} and J. McMahon and M. Mirzaei and Moseley, {S. H.} and Mugge-Durum, {J. W.} and O. Noroozian and U. Pen and Pullen, {A. R.} and S. Rodriguez and Shirron, {P. J.} and Somerville, {R. S.} and Stevenson, {T. R.} and Switzer, {E. R.} and C. Tucker and E. Visbal and Volpert, {C. G.} and Wollack, {E. J.} and S. Yang",

note = "Publisher Copyright: {\textcopyright} 2020, This is a U.S. Government work and not under copyright protection in the US; foreign copyright protection may apply.",

year = "2020",

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doi = "10.1007/s10909-019-02320-5",

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T1 - The Experiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM)

AU - Ade, P. A.R.

AU - Anderson, C. J.

AU - Barrentine, E. M.

AU - Bellis, N. G.

AU - Bolatto, A. D.

AU - Breysse, P. C.

AU - Bulcha, B. T.

AU - Cataldo, G.

AU - Connors, J. A.

AU - Cursey, P. W.

AU - Ehsan, N.

AU - Grant, H. C.

AU - Essinger-Hileman, T. M.

AU - Hess, L. A.

AU - Kimball, M. O.

AU - Kogut, A. J.

AU - Lamb, A. D.

AU - Lowe, L. N.

AU - Mauskopf, P. D.

AU - McMahon, J.

AU - Mirzaei, M.

AU - Moseley, S. H.

AU - Mugge-Durum, J. W.

AU - Noroozian, O.

AU - Pen, U.

AU - Pullen, A. R.

AU - Rodriguez, S.

AU - Shirron, P. J.

AU - Somerville, R. S.

AU - Stevenson, T. R.

AU - Switzer, E. R.

AU - Tucker, C.

AU - Visbal, E.

AU - Volpert, C. G.

AU - Wollack, E. J.

AU - Yang, S.

PY - 2020/5/1

Y1 - 2020/5/1

N2 - 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 timescales. 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 (μ-Spec) coupled to microwave kinetic inductance detectors. Here we present an overview of the EXCLAIM instrument design and status.

AB - 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 timescales. 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 (μ-Spec) coupled to microwave kinetic inductance detectors. Here we present an overview of the EXCLAIM instrument design and status.

KW - Galaxy evolution

KW - Integrated spectrometers

KW - Intensity mapping

KW - MKID

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UR - http://www.scopus.com/inward/citedby.url?scp=85078635981&partnerID=8YFLogxK

U2 - 10.1007/s10909-019-02320-5

DO - 10.1007/s10909-019-02320-5

M3 - Article

AN - SCOPUS:85078635981

SN - 0022-2291

VL - 199

SP - 1027

EP - 1037

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 3-4

ER -

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

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Keywords

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