Essinger-Hileman, Thomas M., Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Anderson, Christopher J., Barlis, Alyssa, Barrentine, Emily M., Beeman, Jeffrey W., Bellis, Nicholas G., Bolatto, Alberto D., Breysse, Patrick, Bulcha, Berhanu, Cataldo, Giuseppe, Chevres Fernandez, Lee Roger, Cho, Chullhee, Connors, Jake A., Cursey, Paul W., Ehsan, Negar, Glenn, Jason, Golec, Joseph E., Hays-Wehle, James, Hess, Larry A., Jahromi, Amir E., Jenkins, Trevian, Kimball, Mark, Kogut, Alan J., Lowe, Luke N., Mauskopf, Philip D., McMahon, Jeffrey J., Mirzaei, Mona, Moseley, Samuel H., Mugge-Durum, Jonas W., Noroozian, Omid, Oxholm, Trevor M., Parekh, Tatsat, Pen, Ue-Li, Pullen, Anthony R., Rahmani, Maryam, Rodriguez, Samelys, Shire, Konrad, Siebert, Gage L., Sinclair, Adrian K., Somerville, Rachel, Stephenson, Ryan C., Stevenson, Thomas R., Switzer, Eric R., Timbie, Peter T., Termini, Jared, Trenkamp, Justin, Tucker, Carole E. ORCID: https://orcid.org/0000-0002-1851-3918, Visbal, Elijah, Volpert, Carolyn, Watson, Joseph, Wollack, Edward, Yang, Shengqi, Yung, L. Y. Aaron, Zmuidzinas, Jonas and Gao, Jian-Rong 2022. EXCLAIM: the EXperiment for cryogenic large-aperture intensity mapping. Presented at: SPIE Astronomical Telescopes + Instrumentation, 2022, Montréal, Québec, Canada, 17-22 July 2022. Proceedings Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI; 1219009 (2022). , vol.12190 SPIE, 10.1117/12.2630054 |
Official URL: http://dx.doi.org/10.1117/12.2630054
Abstract
The EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) will constrain star formation over cosmic time by carrying out a blind and complete census of redshifted carbon monoxide (CO) and ionized carbon ([CII]) emission in cross-correlation with galaxy survey data in redshift windows from the present to z=3.5 with a fully cryogenic, balloon-borne telescope. EXCLAIM will carry out extragalactic and Galactic surveys in a conventional balloon flight planned for 2023. EXCLAIM will be the first instrument to deploy µ-Spec silicon integrated spectrometers with a spectral resolving power R=512 covering 420-540 GHz. We summarize the design, science goals, and status of EXCLAIM.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Published Online |
Status: | Published |
Schools: | Physics and Astronomy |
Publisher: | SPIE |
Last Modified: | 27 Feb 2023 13:00 |
URI: | https://orca.cardiff.ac.uk/id/eprint/157306 |
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