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  Arcus - Exploring the formation and evolution of clusters, galaxies and stars

Smith, R. K., Bautz, M., Bregman, J., Brenneman, L., Brickhouse, N., Bulbul, E., et al. (2022). Arcus - Exploring the formation and evolution of clusters, galaxies and stars. In Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray. doi:10.1117/12.2628628.

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 Creators:
Smith, Randall K., Author
Bautz, Marshall, Author
Bregman, Joel, Author
Brenneman, Laura, Author
Brickhouse, Nancy, Author
Bulbul, Esra1, Author           
Burwitz, Vadim1, Author           
Bushman, Joseph, Author
Canizares, Claude, Author
Chakrabarty, Deepto, Author
Cheimets, Peter, Author
Costantini, Elisa, Author
DeRoo, Casey, Author
Falcone, Abe, Author
Foster, Adam, Author
Gallo, Luigi, Author
Grant, Catherine, Author
Guenther, Hans Moritz, Author
Heilmann, Ralf K., Author
Heine, Sarah, Author
Hine, Butler, AuthorHuenemoerder, David, AuthorJara, Steve, AuthorKaastra, Jelle, AuthorKara, Erin, AuthorKreykenbohm, Ingo, AuthorMadsen, Kristin, AuthorMarshall, Herman, AuthorMcDonald, Michael, AuthorMcEntaffer, Randall, AuthorMiller, Jon, AuthorMiller, Eric, AuthorMushotzky, Richard, AuthorNandra, Kirpal1, Author           Nowak, Michael, AuthorPaerels, Fritis, AuthorPetre, Robert, AuthorPoppenhaeger, Katja, AuthorPtak, Andrew, AuthorReid, Paul, AuthorRonzano, Karolyn, AuthorRozanska, Agata, AuthorSamra, Jenna, AuthorSanders, Jeremy1, Author           Schattenburg, Mark, AuthorSchonfeld, Jonathan, AuthorSchulz, Norbert, AuthorSmale, Alan, AuthorTemi, Pasquale, AuthorValencic, Lynne, AuthorWalker, Stephen, AuthorWilms, Joern, AuthorWolk, Scott, Author more..
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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 Abstract: Supermassive black holes (SMBH) interact with gas in the interstellar and intergalactic media (ISM/IGM) in a process termed “feedback” that is key to the formation and evolution of galaxies and clusters. Characterizing the origins and physical mechanisms governing this feedback requires tracing the propagation of outflowing mass, energy and momentum from the vicinity of the SMBH out to megaparsec scales. Our ability to understand the interplay between feedback and structure evolution across multiple scales, as well as a wide range of other important astrophysical phenomena, depends on diagnostics only available in soft x-ray spectra (10-50 Å). Arcus combines high-resolution, efficient, lightweight x-ray gratings with silicon pore optics to provide R~2500 with an average effective area of ~200 cm2, an order of magnitude larger than the Chandra gratings. Flight-proven CCDs and instrument electronics are strong heritage components, while spacecraft and mission operations also reuse highly successful designs.

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Language(s): eng - English
 Dates: 2022-08-31
 Publication Status: Published online
 Pages: -
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 Rev. Type: -
 Identifiers: DOI: 10.1117/12.2628628
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Title: SPIE Astronomical Telescopes + Instrumentation,
Place of Event: Montréal, Québec, Canada
Start-/End Date: 2022-07-17 - 2022-07-23

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Title: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray
Source Genre: Proceedings
 Creator(s):
Nakazawa, Kazuhiro, Author
Nikzad, Shouleh , Author
A. den Herder, Jan-Willem , Author
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-
Publ. Info: -
Pages: - Volume / Issue: 12181 Sequence Number: - Start / End Page: - Identifier: -

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Title: Proceedings of SPIE
Source Genre: Series
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Publ. Info: Bellingham, WA, USA : Society of Photo-Optical Instrumentation Engineers
Pages: - Volume / Issue: - Sequence Number: 1218121 Start / End Page: - Identifier: ISSN: 0277-786X