TY - JOUR
T1 - Single Aperture Large Telescope for Universe Studies
T2 - Science overview
AU - Chin, Gordon
AU - Anderson, Carrie M.
AU - Bergner, Jennifer
AU - Biver, Nicolas
AU - Bjoraker, Gordon L.
AU - Cavalie, Thibault
AU - Disanti, Michael
AU - Gao, Jian Rong
AU - Hartogh, Paul
AU - Harding, Leon K.
AU - Hu, Qing
AU - Kim, Daewook
AU - Kulesa, Craig
AU - De Lange, Gert
AU - Leisawitz, David T.
AU - Levy, Rebecca C.
AU - Lichtenberger, Arthur
AU - Marrone, Daniel P.
AU - Najita, Joan
AU - Newswander, Trent
AU - Rieke, George H.
AU - Rigopoulou, Dimitra
AU - Roelfsema, Peter
AU - Roth, Nathan X.
AU - Schwarz, Kamber
AU - Shirley, Yancy
AU - Spilker, Justin
AU - Stark, Antony A.
AU - Van Der Tak, Floris
AU - Takashima, Yuzuru
AU - Tielens, Alexander
AU - Willner, David J.
AU - Wollack, Edward J.
AU - Yates, Stephen
AU - Young, Erick
AU - Walker, Christopher K.
N1 - Publisher Copyright:
© 2024 The Authors.
PY - 2024/10/1
Y1 - 2024/10/1
N2 - The Single Aperture Large Telescope for Universe Studies (SALTUS) probe mission will provide a powerful far-infrared (far-IR) pointed space observatory to explore our cosmic origins and the possibility of life elsewhere. The observatory employs an innovative deployable 14-m aperture, with a sunshield that will radiatively cool the off-axis primary to <45 K. This cooled primary reflector works in tandem with cryogenic coherent and incoherent instruments that span 34- to 660-μm far-IR range at both high and moderate spectral resolutions. The mission architecture, using proven Northrop Grumman designs, provides visibility to the entire sky every 6 months with ∼35% of the sky observable at any one time. SALTUS's spectral range is unavailable to any existing ground or current space observatory. SALTUS will have 16× the collecting area and 4× the angular resolution of Herschel and is designed for a lifetime of ≥5 years. The SALTUS science team has proposed a Guaranteed Time Observations program to demonstrate the observatory's capabilities and, at the same time, address high-priority questions from the Decadal survey that align with NASA's Astrophysics Roadmap. With a large aperture enabling high spatial resolution and sensitive instruments, SALTUS will offer >80% of its available observing time to Guest Observer programs, providing the science community with powerful capabilities to study the local and distant universe with observations of 1000s of diverse targets such as distant and nearby galaxies, star-forming regions, protoplanetary disks, and solar system objects.
AB - The Single Aperture Large Telescope for Universe Studies (SALTUS) probe mission will provide a powerful far-infrared (far-IR) pointed space observatory to explore our cosmic origins and the possibility of life elsewhere. The observatory employs an innovative deployable 14-m aperture, with a sunshield that will radiatively cool the off-axis primary to <45 K. This cooled primary reflector works in tandem with cryogenic coherent and incoherent instruments that span 34- to 660-μm far-IR range at both high and moderate spectral resolutions. The mission architecture, using proven Northrop Grumman designs, provides visibility to the entire sky every 6 months with ∼35% of the sky observable at any one time. SALTUS's spectral range is unavailable to any existing ground or current space observatory. SALTUS will have 16× the collecting area and 4× the angular resolution of Herschel and is designed for a lifetime of ≥5 years. The SALTUS science team has proposed a Guaranteed Time Observations program to demonstrate the observatory's capabilities and, at the same time, address high-priority questions from the Decadal survey that align with NASA's Astrophysics Roadmap. With a large aperture enabling high spatial resolution and sensitive instruments, SALTUS will offer >80% of its available observing time to Guest Observer programs, providing the science community with powerful capabilities to study the local and distant universe with observations of 1000s of diverse targets such as distant and nearby galaxies, star-forming regions, protoplanetary disks, and solar system objects.
KW - MKID grating spectrometer
KW - cooled deployable antenna
KW - cryogenic heterodyne instrument
KW - far-infrared observatory
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U2 - 10.1117/1.JATIS.10.4.042310
DO - 10.1117/1.JATIS.10.4.042310
M3 - Article
AN - SCOPUS:85202210556
SN - 2329-4124
VL - 10
JO - Journal of Astronomical Telescopes, Instruments, and Systems
JF - Journal of Astronomical Telescopes, Instruments, and Systems
IS - 4
M1 - 042310
ER -