Abstract
SDSS-V will be an all-sky, multi-epoch spectroscopic survey of over six million objects. It is designed to decode the history of the Milky Way Galaxy (MW), trace the emergence of the chemical elements, reveal the inner workings of stars, and investigate the origin of planets. It will also create an integral-field spectroscopic map of the interstellar gas in the Galaxy and the Local Group that is 1,000 times larger than the current state of the art and at high enough spatial resolution to reveal the self-regulation mechanisms of galactic ecosystems. SDSS-V will pioneer systematic, spectroscopic monitoring across the whole sky, revealing changes on timescales from 20 minutes to 20 years. The survey will thus track the flickers, flares, and radical transformations of the most luminous persistent objects in the universe: Massive black holes growing at the centers of galaxies. The scope and flexibility of SDSS-V will be unique among both extant and anticipated spectroscopic surveys: It is all-sky, with matched survey infrastructures in both hemispheres; it provides near-infrared and optical multi-object fiber spectroscopy that is rapidly reconfigurable to serve high target densities, targets of opportunity, and time-domain monitoring; and it provides optical, ultrawide-field integral field spectroscopy. SDSS-V, with its programs anticipated to start in 2020, will be perfectly timed to multiply the scientific output from major space missions (e.g., TESS, Gaia, Spektr-RG-eROSITA) and ground-based projects. SDSS-V builds on the 25-year heritage of SDSS's advances in data analysis, collaboration spirit and infrastructure, and product deliverables in astronomy. The project is now refining its science scope, optimizing the survey strategies, and developing new hardware that builds on the SDSS-IV infrastructure. We present here an overview of the current state of these developments. SDSS-V is actively seeking to build its consortium of institutional and individual members for a worldwide, partner-driven collaboration.
| Original language | English (US) |
|---|---|
| Journal | Unknown Journal |
| State | Published - Nov 8 2017 |
| Externally published | Yes |
ASJC Scopus subject areas
- General
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SDSS-V : Pioneering Panoptic Spectroscopy. / Kollmeier, Juna A.; Zasowski, Gail; Rix, Hans Walter; Johns, Matt; Anderson, Scott F.; Drory, Niv; Johnson, Jennifer A.; Pogge, Richard W.; Bird, Jonathan C.; Blanc, Guillermo A.; Brownstein, Joel R.; Crane, Jeffrey D.; Lee, Nathan M.De; Klaene, Mark A.; Kreckel, Kathryn; MacDonald, Nick; Merloni, Andrea; Ness, Melissa K.; O'Brien, Thomas; Sánchez-Gallego, José R.; Sayres, Conor C.; Shen, Yue; Thakar, Ani R.; Tkachenko, Andrew; Aerts, Conny; Blanton, Michael R.; Eisenstein, Daniel J.; Holtzman, Jon A.; Maoz, Dan; Nandra, Kirpal; Rockosi, Constance; Weinberg, David H.; Bovy, Jo; Casey, Andrew R.; Chaname, Julio; Clerc, Nicolas; Conroy, Charlie; Eracleous, Michael; Gänsicke, Boris T.; Hekker, Saskia; Horne, Keith; Kauffmann, Jens; McQuinn, Kristen B.W.; Pellegrini, Eric W.; Schinnerer, Eva; Schlafly, Edward F.; Schwope, Axel D.; Seibert, Mark; Teske, Johanna K.; Saders, Jennifer L.Van; Almeida, Andres; Andrews, Brett H.; Argudo-Fernández, Maria; Avila-Reese, Vladimir; Badenes, Carles; Bally, John; Barger, Kathleen Ann; Bartosz, Curtis; Basu, Sarbani; Bauer, Franz E.; Beaton, Rachael L.; Belfiore, Francesco; Bellm, Eric C.; Bershady, Matthew A.; Bizyaev, Dmitry; Boquien, Médéric; Bouri, Mohamed; Brandt, W. N.; Brinkmann, Jonathan; Brooks, Alyson; Bundy, Kevin; Burgasser, Adam J.; Carlberg, Joleen K.; Caseiro, Stefane; Chaplin, W. J.; Cherinka, Brian; Chiappini, Cristina; Chuang, Chia Hsun; Collins, Chris; Crenshaw, D. Michael; Cunha, Katia; Dalcanton, Julianne J.; MacOrra, Axel De La; Diamond-Stanic, Aleksandar M.; Mille, Francesco Di; Donor, John; Dwelly, Tom; Eastman, Jason D.; Emsellem, Eric; Fan, Xiaohui; Fernandez-Trincado, J. G.; Feuillet, Diane; Ak, N. Filiz; Finkbeiner, Douglas P.; Finoguenov, Alexis; Frinchaboy, Peter M.; García, Rafael A.; Gaulme, Patrick; Gerhard, Ortwin; Gillespie, Bruce; Chew, Yilen Gómez Maqueo; Green, Paul J.; Gunn, James E.; Haggard, Daryl; Hall, Patrick B.; Hawley, Suzanne L.; Hillenbrand, Lynne; Hinkel, Natalie R.; Hoard, D. W.; Hogg, David W.; Hooper, Eric; Hörler, Philipp; Inno, Laura; Jones, Amy M.; Kneib, Jean Paul; Kronig, Luzius; Kulkarni, Shri; Law, David; Leroy, Adam K.; Liu, Xin; MacLeod, Chelsea L.; Meza, Andrés; Miglio, Andrea; Minchev, Ivan; Minniti, Dante; Mulchaey, John; Myers, Adam D.; Newman, Jeffrey A.; Nidever, David; Nitschelm, Christian; Pasetto, Stefano; Peek, J. E.G.; Peng, Yingjie; Pepper, Joshua; Pinsonneault, Marc H.; Price-Whelan, Adrian M.; Raddick, M. Jordan; Rahman, Mubdi; Rapetti, David; Renaud, Florent; Román-Zúñiga, Carlos; Runnoe, Jessie; Rybizki, Jan; Schlegel, David; Schneider, Donald P.; Serenelli, Aldo; Shull, J. Michael; Aguirre, Victor Silva; Simon, Joshua D.; Skrutskie, M. F.; Smee, Stephen A.; Sobeck, Jennifer; Somers, Garrett; Stassun, Keivan G.; Steinmetz, Matthias; Stringfellow, Guy; Szabo, Robert; Tayar, Jamie; Tchernyshyov, Kirill; Ting, Yuan Sen; Troup, Nicholas; Trujillo, Juan David; Trump, Jonathan; Walterbos, Rene; Weaver, Benjamin A.; Weijmans, Anne Marie; Wild, Vivienne; Wolf, Marsha J.; Xue, Yongquan; Yan, Renbin; Zwintz, Konstanze.
In: Unknown Journal, 08.11.2017.Research output: Contribution to journal › Article › peer-review
}
TY - JOUR
T1 - SDSS-V
T2 - Pioneering Panoptic Spectroscopy
AU - Kollmeier, Juna A.
AU - Zasowski, Gail
AU - Rix, Hans Walter
AU - Johns, Matt
AU - Anderson, Scott F.
AU - Drory, Niv
AU - Johnson, Jennifer A.
AU - Pogge, Richard W.
AU - Bird, Jonathan C.
AU - Blanc, Guillermo A.
AU - Brownstein, Joel R.
AU - Crane, Jeffrey D.
AU - Lee, Nathan M.De
AU - Klaene, Mark A.
AU - Kreckel, Kathryn
AU - MacDonald, Nick
AU - Merloni, Andrea
AU - Ness, Melissa K.
AU - O'Brien, Thomas
AU - Sánchez-Gallego, José R.
AU - Sayres, Conor C.
AU - Shen, Yue
AU - Thakar, Ani R.
AU - Tkachenko, Andrew
AU - Aerts, Conny
AU - Blanton, Michael R.
AU - Eisenstein, Daniel J.
AU - Holtzman, Jon A.
AU - Maoz, Dan
AU - Nandra, Kirpal
AU - Rockosi, Constance
AU - Weinberg, David H.
AU - Bovy, Jo
AU - Casey, Andrew R.
AU - Chaname, Julio
AU - Clerc, Nicolas
AU - Conroy, Charlie
AU - Eracleous, Michael
AU - Gänsicke, Boris T.
AU - Hekker, Saskia
AU - Horne, Keith
AU - Kauffmann, Jens
AU - McQuinn, Kristen B.W.
AU - Pellegrini, Eric W.
AU - Schinnerer, Eva
AU - Schlafly, Edward F.
AU - Schwope, Axel D.
AU - Seibert, Mark
AU - Teske, Johanna K.
AU - Saders, Jennifer L.Van
AU - Almeida, Andres
AU - Andrews, Brett H.
AU - Argudo-Fernández, Maria
AU - Avila-Reese, Vladimir
AU - Badenes, Carles
AU - Bally, John
AU - Barger, Kathleen Ann
AU - Bartosz, Curtis
AU - Basu, Sarbani
AU - Bauer, Franz E.
AU - Beaton, Rachael L.
AU - Belfiore, Francesco
AU - Bellm, Eric C.
AU - Bershady, Matthew A.
AU - Bizyaev, Dmitry
AU - Boquien, Médéric
AU - Bouri, Mohamed
AU - Brandt, W. N.
AU - Brinkmann, Jonathan
AU - Brooks, Alyson
AU - Bundy, Kevin
AU - Burgasser, Adam J.
AU - Carlberg, Joleen K.
AU - Caseiro, Stefane
AU - Chaplin, W. J.
AU - Cherinka, Brian
AU - Chiappini, Cristina
AU - Chuang, Chia Hsun
AU - Collins, Chris
AU - Crenshaw, D. Michael
AU - Cunha, Katia
AU - Dalcanton, Julianne J.
AU - MacOrra, Axel De La
AU - Diamond-Stanic, Aleksandar M.
AU - Mille, Francesco Di
AU - Donor, John
AU - Dwelly, Tom
AU - Eastman, Jason D.
AU - Emsellem, Eric
AU - Fan, Xiaohui
AU - Fernandez-Trincado, J. G.
AU - Feuillet, Diane
AU - Ak, N. Filiz
AU - Finkbeiner, Douglas P.
AU - Finoguenov, Alexis
AU - Frinchaboy, Peter M.
AU - García, Rafael A.
AU - Gaulme, Patrick
AU - Gerhard, Ortwin
AU - Gillespie, Bruce
AU - Chew, Yilen Gómez Maqueo
AU - Green, Paul J.
AU - Gunn, James E.
AU - Haggard, Daryl
AU - Hall, Patrick B.
AU - Hawley, Suzanne L.
AU - Hillenbrand, Lynne
AU - Hinkel, Natalie R.
AU - Hoard, D. W.
AU - Hogg, David W.
AU - Hooper, Eric
AU - Hörler, Philipp
AU - Inno, Laura
AU - Jones, Amy M.
AU - Kneib, Jean Paul
AU - Kronig, Luzius
AU - Kulkarni, Shri
AU - Law, David
AU - Leroy, Adam K.
AU - Liu, Xin
AU - MacLeod, Chelsea L.
AU - Meza, Andrés
AU - Miglio, Andrea
AU - Minchev, Ivan
AU - Minniti, Dante
AU - Mulchaey, John
AU - Myers, Adam D.
AU - Newman, Jeffrey A.
AU - Nidever, David
AU - Nitschelm, Christian
AU - Pasetto, Stefano
AU - Peek, J. E.G.
AU - Peng, Yingjie
AU - Pepper, Joshua
AU - Pinsonneault, Marc H.
AU - Price-Whelan, Adrian M.
AU - Raddick, M. Jordan
AU - Rahman, Mubdi
AU - Rapetti, David
AU - Renaud, Florent
AU - Román-Zúñiga, Carlos
AU - Runnoe, Jessie
AU - Rybizki, Jan
AU - Schlegel, David
AU - Schneider, Donald P.
AU - Serenelli, Aldo
AU - Shull, J. Michael
AU - Aguirre, Victor Silva
AU - Simon, Joshua D.
AU - Skrutskie, M. F.
AU - Smee, Stephen A.
AU - Sobeck, Jennifer
AU - Somers, Garrett
AU - Stassun, Keivan G.
AU - Steinmetz, Matthias
AU - Stringfellow, Guy
AU - Szabo, Robert
AU - Tayar, Jamie
AU - Tchernyshyov, Kirill
AU - Ting, Yuan Sen
AU - Troup, Nicholas
AU - Trujillo, Juan David
AU - Trump, Jonathan
AU - Walterbos, Rene
AU - Weaver, Benjamin A.
AU - Weijmans, Anne Marie
AU - Wild, Vivienne
AU - Wolf, Marsha J.
AU - Xue, Yongquan
AU - Yan, Renbin
AU - Zwintz, Konstanze
N1 - Publisher Copyright: Copyright © 2017, The Authors. All rights reserved. Copyright: Copyright 2020 Elsevier B.V., All rights reserved.
PY - 2017/11/8
Y1 - 2017/11/8
N2 - SDSS-V will be an all-sky, multi-epoch spectroscopic survey of over six million objects. It is designed to decode the history of the Milky Way Galaxy (MW), trace the emergence of the chemical elements, reveal the inner workings of stars, and investigate the origin of planets. It will also create an integral-field spectroscopic map of the interstellar gas in the Galaxy and the Local Group that is 1,000 times larger than the current state of the art and at high enough spatial resolution to reveal the self-regulation mechanisms of galactic ecosystems. SDSS-V will pioneer systematic, spectroscopic monitoring across the whole sky, revealing changes on timescales from 20 minutes to 20 years. The survey will thus track the flickers, flares, and radical transformations of the most luminous persistent objects in the universe: Massive black holes growing at the centers of galaxies. The scope and flexibility of SDSS-V will be unique among both extant and anticipated spectroscopic surveys: It is all-sky, with matched survey infrastructures in both hemispheres; it provides near-infrared and optical multi-object fiber spectroscopy that is rapidly reconfigurable to serve high target densities, targets of opportunity, and time-domain monitoring; and it provides optical, ultrawide-field integral field spectroscopy. SDSS-V, with its programs anticipated to start in 2020, will be perfectly timed to multiply the scientific output from major space missions (e.g., TESS, Gaia, Spektr-RG-eROSITA) and ground-based projects. SDSS-V builds on the 25-year heritage of SDSS's advances in data analysis, collaboration spirit and infrastructure, and product deliverables in astronomy. The project is now refining its science scope, optimizing the survey strategies, and developing new hardware that builds on the SDSS-IV infrastructure. We present here an overview of the current state of these developments. SDSS-V is actively seeking to build its consortium of institutional and individual members for a worldwide, partner-driven collaboration.
AB - SDSS-V will be an all-sky, multi-epoch spectroscopic survey of over six million objects. It is designed to decode the history of the Milky Way Galaxy (MW), trace the emergence of the chemical elements, reveal the inner workings of stars, and investigate the origin of planets. It will also create an integral-field spectroscopic map of the interstellar gas in the Galaxy and the Local Group that is 1,000 times larger than the current state of the art and at high enough spatial resolution to reveal the self-regulation mechanisms of galactic ecosystems. SDSS-V will pioneer systematic, spectroscopic monitoring across the whole sky, revealing changes on timescales from 20 minutes to 20 years. The survey will thus track the flickers, flares, and radical transformations of the most luminous persistent objects in the universe: Massive black holes growing at the centers of galaxies. The scope and flexibility of SDSS-V will be unique among both extant and anticipated spectroscopic surveys: It is all-sky, with matched survey infrastructures in both hemispheres; it provides near-infrared and optical multi-object fiber spectroscopy that is rapidly reconfigurable to serve high target densities, targets of opportunity, and time-domain monitoring; and it provides optical, ultrawide-field integral field spectroscopy. SDSS-V, with its programs anticipated to start in 2020, will be perfectly timed to multiply the scientific output from major space missions (e.g., TESS, Gaia, Spektr-RG-eROSITA) and ground-based projects. SDSS-V builds on the 25-year heritage of SDSS's advances in data analysis, collaboration spirit and infrastructure, and product deliverables in astronomy. The project is now refining its science scope, optimizing the survey strategies, and developing new hardware that builds on the SDSS-IV infrastructure. We present here an overview of the current state of these developments. SDSS-V is actively seeking to build its consortium of institutional and individual members for a worldwide, partner-driven collaboration.
UR - http://www.scopus.com/inward/record.url?scp=85095293445&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85095293445&partnerID=8YFLogxK
M3 - Article
AN - SCOPUS:85095293445
JO - Nuclear Physics A
JF - Nuclear Physics A
SN - 0375-9474
ER -