The Arcus Probe Mission

Randall Smith; Jon Arenberg; Marshall Bautz; Ehud Behar; Dolon Bhattacharyya; Jay Bookbinder; Joel Bregman; Laura Brenneman; Nancy Brickhouse; G. Esra Bulbul; Vadim Burwitz; Joseph Bushman; Peter Cheimets; Elisa Costantini; Casey DeRoo; Benjamin D. Donovan; Abraham Falcone; Brian Fleming; Adam Foster; Kevin France; Peter Friedrich; Luigi Gallo; Catherine E. Grant; H. Moritz Günther; Daryl Haggard; Ralf K. Heilmann; Sarah Heine; Butler Hine; David Huenemoerder; Jelle Kaastra; Igor Kreykenbohm; Sibasish Laha; Pamela Marcum; Herman Marshall; Randall McEntaffer; Missagh Mehdipour; Eric D. Miller; Jon M. Miller; Kirpal Nandra; Nicholas Nell; Michael Nowak; Frits Paerels; Katya Poppenhaeger; Andrew Ptak; Agata Rozanska; Jenna Samra; Jeremy Sanders; Mark L. Schattenburg; Norbert S. Schulz; Leroy Mark Sparr; Pasquale Temi; Todd M. Tripp; Lynne Valencic; Joern Wilms; Stephen Walker; David Wilson; Scott Wolk

doi:https://doi.org/10.1117/12.3022452

The Arcus Probe Mission

Randall Smith, Jon Arenberg, Marshall Bautz, Ehud Behar, Dolon Bhattacharyya, Jay Bookbinder, Joel Bregman, Laura Brenneman, Nancy Brickhouse, G. Esra Bulbul, Vadim Burwitz, Joseph Bushman, Peter Cheimets, Elisa Costantini, Casey DeRoo, Benjamin D. Donovan, Abraham Falcone, Brian Fleming, Adam Foster, Kevin FrancePeter Friedrich, Luigi Gallo, Catherine E. Grant, H. Moritz Günther, Daryl Haggard, Ralf K. Heilmann, Sarah Heine, Butler Hine, David Huenemoerder, Jelle Kaastra, Igor Kreykenbohm, Sibasish Laha, Pamela Marcum, Herman Marshall, Randall McEntaffer, Missagh Mehdipour, Eric D. Miller, Jon M. Miller, Kirpal Nandra, Nicholas Nell, Michael Nowak, Frits Paerels, Katya Poppenhaeger, Andrew Ptak, Agata Rozanska, Jenna Samra, Jeremy Sanders, Mark L. Schattenburg, Norbert S. Schulz, Leroy Mark Sparr, Pasquale Temi, Todd M. Tripp, Lynne Valencic, Joern Wilms, Stephen Walker, David Wilson, Scott Wolk

Physics

Technion - Israel Institute of Technology

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

The Arcus Probe mission addresses a wide range of Astro2020 Decadal and NASA Science Mission Directorate Priority science areas, and is designed to explore astrophysical feedback across all mass scales. Arcus' three baseline science goals include: (i) Characterizing the drivers of accretion-powered feedback in supermassive black holes, (ii) Quantifying how feedback at all scales drives galaxy evolution and large-scale structure, including the tenuous cosmic web, and (iii) Analyzing stellar feedback from exoplanetary to galactic scales, including its effects on exoplanet environments targeted by current and future NASA missions. These science goals, along with a robust General Observer program, will be achieved using a mission that provides a high-sensitivity soft (10-60Å) X-ray spectrometer (XRS), working simultaneously with a co-aligned UV spectrometer (UVS; 970-1580Å). Arcus enables compelling baseline science and provides the broader astronomy community a revolutionary tool to characterize the full ionization range of warm and hot plasmas - including hydrogen, helium, and all abundant metals - in the Universe, from the halos of galaxies and clusters to the coronae of stars.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2024
Subtitle of host publication	Ultraviolet to Gamma Ray
Editors	Jan-Willem A. den Herder, Shouleh Nikzad, Kazuhiro Nakazawa
ISBN (Electronic)	9781510675094
DOIs	https://doi.org/10.1117/12.3022452
State	Published - 2024
Event	Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray - Yokohama, Japan Duration: 16 Jun 2024 → 21 Jun 2024

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	13093

Conference

Conference	Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray
Country/Territory	Japan
City	Yokohama
Period	16/06/24 → 21/06/24

Keywords

Far-UV
Probe mission
UV: Spectroscopy
X-ray gratings
X-rays: Spectroscopy

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

https://doi.org/10.1117/12.3022452

Cite this

Smith, R., Arenberg, J., Bautz, M., Behar, E., Bhattacharyya, D., Bookbinder, J., Bregman, J., Brenneman, L., Brickhouse, N., Bulbul, G. E., Burwitz, V., Bushman, J., Cheimets, P., Costantini, E., DeRoo, C., Donovan, B. D., Falcone, A., Fleming, B., Foster, A., ... Wolk, S. (2024). The Arcus Probe Mission. In J-W. A. den Herder, S. Nikzad, & K. Nakazawa (Eds.), Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray Article 1309326 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 13093). https://doi.org/10.1117/12.3022452

@inproceedings{325e71b3db934bed9257c98258791d74,

title = "The Arcus Probe Mission",

abstract = "The Arcus Probe mission addresses a wide range of Astro2020 Decadal and NASA Science Mission Directorate Priority science areas, and is designed to explore astrophysical feedback across all mass scales. Arcus' three baseline science goals include: (i) Characterizing the drivers of accretion-powered feedback in supermassive black holes, (ii) Quantifying how feedback at all scales drives galaxy evolution and large-scale structure, including the tenuous cosmic web, and (iii) Analyzing stellar feedback from exoplanetary to galactic scales, including its effects on exoplanet environments targeted by current and future NASA missions. These science goals, along with a robust General Observer program, will be achieved using a mission that provides a high-sensitivity soft (10-60{\AA}) X-ray spectrometer (XRS), working simultaneously with a co-aligned UV spectrometer (UVS; 970-1580{\AA}). Arcus enables compelling baseline science and provides the broader astronomy community a revolutionary tool to characterize the full ionization range of warm and hot plasmas - including hydrogen, helium, and all abundant metals - in the Universe, from the halos of galaxies and clusters to the coronae of stars.",

keywords = "Far-UV, Probe mission, UV: Spectroscopy, X-ray gratings, X-rays: Spectroscopy",

author = "Randall Smith and Jon Arenberg and Marshall Bautz and Ehud Behar and Dolon Bhattacharyya and Jay Bookbinder and Joel Bregman and Laura Brenneman and Nancy Brickhouse and Bulbul, {G. Esra} and Vadim Burwitz and Joseph Bushman and Peter Cheimets and Elisa Costantini and Casey DeRoo and Donovan, {Benjamin D.} and Abraham Falcone and Brian Fleming and Adam Foster and Kevin France and Peter Friedrich and Luigi Gallo and Grant, {Catherine E.} and G{\"u}nther, {H. Moritz} and Daryl Haggard and Heilmann, {Ralf K.} and Sarah Heine and Butler Hine and David Huenemoerder and Jelle Kaastra and Igor Kreykenbohm and Sibasish Laha and Pamela Marcum and Herman Marshall and Randall McEntaffer and Missagh Mehdipour and Miller, {Eric D.} and Miller, {Jon M.} and Kirpal Nandra and Nicholas Nell and Michael Nowak and Frits Paerels and Katya Poppenhaeger and Andrew Ptak and Agata Rozanska and Jenna Samra and Jeremy Sanders and Schattenburg, {Mark L.} and Schulz, {Norbert S.} and Sparr, {Leroy Mark} and Pasquale Temi and Tripp, {Todd M.} and Lynne Valencic and Joern Wilms and Stephen Walker and David Wilson and Scott Wolk",

note = "Publisher Copyright: {\textcopyright} 2024 SPIE.; Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray ; Conference date: 16-06-2024 Through 21-06-2024",

year = "2024",

doi = "https://doi.org/10.1117/12.3022452",

language = "الإنجليزيّة",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

editor = "{den Herder}, {Jan-Willem A.} and Shouleh Nikzad and Kazuhiro Nakazawa",

booktitle = "Space Telescopes and Instrumentation 2024",

}

Smith, R, Arenberg, J, Bautz, M, Behar, E, Bhattacharyya, D, Bookbinder, J, Bregman, J, Brenneman, L, Brickhouse, N, Bulbul, GE, Burwitz, V, Bushman, J, Cheimets, P, Costantini, E, DeRoo, C, Donovan, BD, Falcone, A, Fleming, B, Foster, A, France, K, Friedrich, P, Gallo, L, Grant, CE, Günther, HM, Haggard, D, Heilmann, RK, Heine, S, Hine, B, Huenemoerder, D, Kaastra, J, Kreykenbohm, I, Laha, S, Marcum, P, Marshall, H, McEntaffer, R, Mehdipour, M, Miller, ED, Miller, JM, Nandra, K, Nell, N, Nowak, M, Paerels, F, Poppenhaeger, K, Ptak, A, Rozanska, A, Samra, J, Sanders, J, Schattenburg, ML, Schulz, NS, Sparr, LM, Temi, P, Tripp, TM, Valencic, L, Wilms, J, Walker, S, Wilson, D & Wolk, S 2024, The Arcus Probe Mission. in J-WA den Herder, S Nikzad & K Nakazawa (eds), Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray., 1309326, Proceedings of SPIE - The International Society for Optical Engineering, vol. 13093, Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray, Yokohama, Japan, 16/06/24. https://doi.org/10.1117/12.3022452

The Arcus Probe Mission. / Smith, Randall; Arenberg, Jon; Bautz, Marshall et al.
Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray. ed. / Jan-Willem A. den Herder; Shouleh Nikzad; Kazuhiro Nakazawa. 2024. 1309326 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 13093).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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AU - Bautz, Marshall

AU - Behar, Ehud

AU - Bhattacharyya, Dolon

AU - Bookbinder, Jay

AU - Bregman, Joel

AU - Brenneman, Laura

AU - Brickhouse, Nancy

AU - Bulbul, G. Esra

AU - Burwitz, Vadim

AU - Bushman, Joseph

AU - Cheimets, Peter

AU - Costantini, Elisa

AU - DeRoo, Casey

AU - Donovan, Benjamin D.

AU - Falcone, Abraham

AU - Fleming, Brian

AU - Foster, Adam

AU - France, Kevin

AU - Friedrich, Peter

AU - Gallo, Luigi

AU - Grant, Catherine E.

AU - Günther, H. Moritz

AU - Haggard, Daryl

AU - Heilmann, Ralf K.

AU - Heine, Sarah

AU - Hine, Butler

AU - Huenemoerder, David

AU - Kaastra, Jelle

AU - Kreykenbohm, Igor

AU - Laha, Sibasish

AU - Marcum, Pamela

AU - Marshall, Herman

AU - McEntaffer, Randall

AU - Mehdipour, Missagh

AU - Miller, Eric D.

AU - Miller, Jon M.

AU - Nandra, Kirpal

AU - Nell, Nicholas

AU - Nowak, Michael

AU - Paerels, Frits

AU - Poppenhaeger, Katya

AU - Ptak, Andrew

AU - Rozanska, Agata

AU - Samra, Jenna

AU - Sanders, Jeremy

AU - Schattenburg, Mark L.

AU - Schulz, Norbert S.

AU - Sparr, Leroy Mark

AU - Temi, Pasquale

AU - Tripp, Todd M.

AU - Valencic, Lynne

AU - Wilms, Joern

AU - Walker, Stephen

AU - Wilson, David

AU - Wolk, Scott

PY - 2024

Y1 - 2024

N2 - The Arcus Probe mission addresses a wide range of Astro2020 Decadal and NASA Science Mission Directorate Priority science areas, and is designed to explore astrophysical feedback across all mass scales. Arcus' three baseline science goals include: (i) Characterizing the drivers of accretion-powered feedback in supermassive black holes, (ii) Quantifying how feedback at all scales drives galaxy evolution and large-scale structure, including the tenuous cosmic web, and (iii) Analyzing stellar feedback from exoplanetary to galactic scales, including its effects on exoplanet environments targeted by current and future NASA missions. These science goals, along with a robust General Observer program, will be achieved using a mission that provides a high-sensitivity soft (10-60Å) X-ray spectrometer (XRS), working simultaneously with a co-aligned UV spectrometer (UVS; 970-1580Å). Arcus enables compelling baseline science and provides the broader astronomy community a revolutionary tool to characterize the full ionization range of warm and hot plasmas - including hydrogen, helium, and all abundant metals - in the Universe, from the halos of galaxies and clusters to the coronae of stars.

AB - The Arcus Probe mission addresses a wide range of Astro2020 Decadal and NASA Science Mission Directorate Priority science areas, and is designed to explore astrophysical feedback across all mass scales. Arcus' three baseline science goals include: (i) Characterizing the drivers of accretion-powered feedback in supermassive black holes, (ii) Quantifying how feedback at all scales drives galaxy evolution and large-scale structure, including the tenuous cosmic web, and (iii) Analyzing stellar feedback from exoplanetary to galactic scales, including its effects on exoplanet environments targeted by current and future NASA missions. These science goals, along with a robust General Observer program, will be achieved using a mission that provides a high-sensitivity soft (10-60Å) X-ray spectrometer (XRS), working simultaneously with a co-aligned UV spectrometer (UVS; 970-1580Å). Arcus enables compelling baseline science and provides the broader astronomy community a revolutionary tool to characterize the full ionization range of warm and hot plasmas - including hydrogen, helium, and all abundant metals - in the Universe, from the halos of galaxies and clusters to the coronae of stars.

KW - Far-UV

KW - Probe mission

KW - UV: Spectroscopy

KW - X-ray gratings

KW - X-rays: Spectroscopy

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U2 - https://doi.org/10.1117/12.3022452

DO - https://doi.org/10.1117/12.3022452

M3 - منشور من مؤتمر

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Space Telescopes and Instrumentation 2024

A2 - den Herder, Jan-Willem A.

A2 - Nikzad, Shouleh

A2 - Nakazawa, Kazuhiro

T2 - Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray

Y2 - 16 June 2024 through 21 June 2024

ER -

The Arcus Probe Mission

Abstract

Publication series

Conference

Keywords

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Cite this