The Case for Probe-class NASA Astrophysics Missions
- Creators
- Elvis, Martin
- Arenberg, Jon
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Ballantyne, David
- Bautz, Mark
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Beichman, Charles
- Booth, Jeffrey
- Buckley, James
- Burns, Jack O.
- Camp, Jordan
- Conti, Alberto
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Cooray, Asantha
- Danchi, William
- Delabrouille, Jacques
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De Zotti, Gianfranco
- Flauger, Raphael
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Glenn, Jason
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Grindlay, Jonathan
- Hanany, Shaul
- Hartmann, Dieter
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Helou, George
- Herranz, Diego
- Hubmayr, Johannes
- Johnson, Bradley R.
- Jones, William
- Kasdin, N. Jeremy
- Kouvoliotou, Chryssa
- Kunze, Kerstin E.
- Lawrence, Charles
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Lazio, Joseph
- Lipscy, Sarah
- Lillie, Charles F.
- Maccarone, Tom
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Madsen, Kristin C.
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Mushotzky, Richard
- Olinto, Angela
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Plavchan, Peter
- Pogosian, Levon
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Ptak, Andrew
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Ray, Paul
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Rocha, Graca M.
- Scowen, Paul
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Seager, Sara
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Tinto, Massimo
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Tomsick, John
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Tucker, Gregory S.
- Ulmer, Mel
- Wang, Yun
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Wollack, Edward J.
Abstract
Astrophysics spans an enormous range of questions on scales from individual planets to the entire cosmos. To address the richness of 21st century astrophysics requires a corresponding richness of telescopes spanning all bands and all messengers. Much scientific benefit comes from having the multi-wavelength capability available at the same time. Most of these bands,or measurement sensitivities, require space-based missions. Historically, NASA has addressed this need for breadth with a small number of flagship-class missions and a larger number of Explorer missions. While the Explorer program continues to flourish, there is a large gap between Explorers and strategic missions. A fortunate combination of new astrophysics technologies with new, high capacity, low dollar-per-kg to orbit launchers, and new satellite buses allow for cheaper missions with capabilities approaching strategic mission levels. NASA has recognized these developments by calling for Probe-class mission ideas for mission studies, spanning most of the electromagnetic spectrum from GeV gamma-rays to the far infrared, and the new messengers of neutrinos and ultra-high energy cosmic rays. The key insight from the Probes exercise is that order-of-magnitude advances in science performance metrics are possible across the board for initial total cost estimates in the range 500M-1B dollars.
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Submitted - 2002.12739.pdf
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Additional details
- Eprint ID
- 103702
- Resolver ID
- CaltechAUTHORS:20200604-151409625
- Created
-
2020-06-08Created from EPrint's datestamp field
- Updated
-
2023-06-02Created from EPrint's last_modified field
- Series Name
- Astro2020 APC White Paper