Abstract
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 |
|---|---|
| Media of output | pre-print server |
| Publisher | arXiv.org |
| Number of pages | 24 |
| Publication status | Published - 9 Nov 2017 |
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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; Bird, Jonathan C.; Blanc, Guillermo A.; Brownstein, Joel R.; Crane, Jeffrey D.; Klaene, Mark; Kreckel, Kathryn; MacDonald, Nick; Merloni, Andrea; O'Brien, Thomas; Sanchez-Gallego, Jose ; Sayres, Conor; Shen, Yue; Thakar, Ani; Tkachenko, Andrew; Aerts, Conny M; Blanton, Michael R.; Eisenstein, Daniel J; Holtzmann, Jon ; Moaz, Dan; Nandra, Kirpal; Rockosi, Constance; Weinberg, David; Bovy, Jo; Casey, Andrew R.; Chaname, Julio; Clerc, Nicolas; Conroy, Charlie; Eracleous, Michael; Gänsicke, Boris T.; Hekker, Saskia; Horne, Keith; Kauffman, Jens; McQuinn, Kristen; Pellegrini, Eric; Schinnerer, Eva; Schlafly, Edward; Schwope, Axel; Seibert, Mark; Teske, Johanna; van Saders, Jennifer ; Almeida, Andres; Andrews, Brett H.; Argudo-Fernández, Maria; Avila-Reese, Vladimir; Badenes, Carles; Bally, John; Ann Barger, Kathleen ; Bartosz, Curtis M; Basu, Sarbani; Bauer, Franz; Beaton, Rachael; Belfiore, Francesco; Bellm, Eric C; Bershady, Matthew A.; Bizyaev, Dmitry; Boquien, Médéric; Bouri, Mohamed; Brandt, W.; Brinkmann, Jonathan; Brooks, Alyson; Bundy, Kevin; Burgasser, Adam J.; Carlberg, Joleen; Caseiro, Stefane; Chaplin, William J; Cherinka, Brian; Chiappini, Cristina; Chuang, Chia Hsun; Collins, Chris ; Crenshaw, Michael; Cunha, Katia; Dalcanton, Julianne; MacOrra, Axel De La; Diamond-Stanic, Aleksander; Di Mille, Francesco; Donor, John; Dwelly, Tom; Eastman, Jason; Emsellem, Eric; Fan, Xiaohui; Fernandez-Trincado, J. G.; Feuillet, Diane; Filiz Ak, N; Finkbeiner, Douglas ; Finoguenov, Alexis; Frinchaboy, Peter M.; Garcia, Rafael A; Gualme, Patrick; Gerhard, Ortwin; Gillespie, Bruce A.; Chew, Yilen Gómez Maqueo; Green, Paul J; Gunn, James E; Haggard, Daryl; Hall, Patrick; Hawley, Suzanne; Hillenbrand, Lynne; Hinkel, Natalie; Hoard, D W; Hogg, David W; Hooper, Eric; Horler, Phillip; Inno, Laura; Jones, Amy; Kneib, Jean Paul; Kronig, Luzius; Kulkarni, Shrinivas R; Law, David; Leroy, Adam; Liu, Xin; MacLeod, Chelsea L.; Meza, Andres; Miglio, Andrea; Minchev, Ivan; Minniti, Dante; Mulchaey, John S.; Myers, Adam D.; Newman, Jeffrey A.; Nidever, David L.; Nitschelm, Christian; Pasetto, Stefano; Peek, J E G; Peng, Yingjie; Pepper, Joshua; Pinsonneault, Marc; Price-Whelan, Adrian M.; Raddick, M. Jordan; Rahman, Mubdi; Rapetti, David; Renaud, Florent; Román-Zúñiga, Carlos; Runnoe, Jessie; Rybizki, Jan; Schlegel, David J; Schneider, Donald P; Serenelli, Aldo; Shull, J Michael; Silva Aguirre, Victor ; Simon, Joshua D; Skrutskie, M F ; Smee, Stephen; Sobeck, Jennifer; Somers, Garrett; Stassun, Keivan; Steinmetz, Matthias; Stringfellow, Guy S.; Szabo, Robert; Tayar, Jamie; Tchernyshyov, Kirill; Ting, Yuan Sen; Troup, Nicholas; Trujillo, Juan David ; Trump, Jonathan; Walterbos, Rene; Weaver, Benjamin; Weijmans, Anne-Marie ; Wild, Vivienne; Wolf, Marsha; Xue, Yongquan; Yan, Renbin; Zwintz, Konstanze.
24 p. arXiv.org. 2017.Research output: Other contribution › Other
TY - GEN
T1 - SDSS-V: 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
AU - Bird, Jonathan C.
AU - Blanc, Guillermo A.
AU - Brownstein, Joel R.
AU - Crane, Jeffrey D.
AU - Klaene, Mark
AU - Kreckel, Kathryn
AU - MacDonald, Nick
AU - Merloni, Andrea
AU - O'Brien, Thomas
AU - Sanchez-Gallego, Jose
AU - Sayres, Conor
AU - Shen, Yue
AU - Thakar, Ani
AU - Tkachenko, Andrew
AU - Aerts, Conny M
AU - Blanton, Michael R.
AU - Eisenstein, Daniel J
AU - Holtzmann, Jon
AU - Moaz, Dan
AU - Nandra, Kirpal
AU - Rockosi, Constance
AU - Weinberg, David
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 - Kauffman, Jens
AU - McQuinn, Kristen
AU - Pellegrini, Eric
AU - Schinnerer, Eva
AU - Schlafly, Edward
AU - Schwope, Axel
AU - Seibert, Mark
AU - Teske, Johanna
AU - van Saders, Jennifer
AU - Almeida, Andres
AU - Andrews, Brett H.
AU - Argudo-Fernández, Maria
AU - Avila-Reese, Vladimir
AU - Badenes, Carles
AU - Bally, John
AU - Ann Barger, Kathleen
AU - Bartosz, Curtis M
AU - Basu, Sarbani
AU - Bauer, Franz
AU - Beaton, Rachael
AU - Belfiore, Francesco
AU - Bellm, Eric C
AU - Bershady, Matthew A.
AU - Bizyaev, Dmitry
AU - Boquien, Médéric
AU - Bouri, Mohamed
AU - Brandt, W.
AU - Brinkmann, Jonathan
AU - Brooks, Alyson
AU - Bundy, Kevin
AU - Burgasser, Adam J.
AU - Carlberg, Joleen
AU - Caseiro, Stefane
AU - Chaplin, William J
AU - Cherinka, Brian
AU - Chiappini, Cristina
AU - Chuang, Chia Hsun
AU - Collins, Chris
AU - Crenshaw, Michael
AU - Cunha, Katia
AU - Dalcanton, Julianne
AU - MacOrra, Axel De La
AU - Diamond-Stanic, Aleksander
AU - Di Mille, Francesco
AU - Donor, John
AU - Dwelly, Tom
AU - Eastman, Jason
AU - Emsellem, Eric
AU - Fan, Xiaohui
AU - Fernandez-Trincado, J. G.
AU - Feuillet, Diane
AU - Filiz Ak, N
AU - Finkbeiner, Douglas
AU - Finoguenov, Alexis
AU - Frinchaboy, Peter M.
AU - Garcia, Rafael A
AU - Gualme, Patrick
AU - Gerhard, Ortwin
AU - Gillespie, Bruce A.
AU - Chew, Yilen Gómez Maqueo
AU - Green, Paul J
AU - Gunn, James E
AU - Haggard, Daryl
AU - Hall, Patrick
AU - Hawley, Suzanne
AU - Hillenbrand, Lynne
AU - Hinkel, Natalie
AU - Hoard, D W
AU - Hogg, David W
AU - Hooper, Eric
AU - Horler, Phillip
AU - Inno, Laura
AU - Jones, Amy
AU - Kneib, Jean Paul
AU - Kronig, Luzius
AU - Kulkarni, Shrinivas R
AU - Law, David
AU - Leroy, Adam
AU - Liu, Xin
AU - MacLeod, Chelsea L.
AU - Meza, Andres
AU - Miglio, Andrea
AU - Minchev, Ivan
AU - Minniti, Dante
AU - Mulchaey, John S.
AU - Myers, Adam D.
AU - Newman, Jeffrey A.
AU - Nidever, David L.
AU - Nitschelm, Christian
AU - Pasetto, Stefano
AU - Peek, J E G
AU - Peng, Yingjie
AU - Pepper, Joshua
AU - Pinsonneault, Marc
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 J
AU - Schneider, Donald P
AU - Serenelli, Aldo
AU - Shull, J Michael
AU - Silva Aguirre, Victor
AU - Simon, Joshua D
AU - Skrutskie, M F
AU - Smee, Stephen
AU - Sobeck, Jennifer
AU - Somers, Garrett
AU - Stassun, Keivan
AU - Steinmetz, Matthias
AU - Stringfellow, Guy S.
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
AU - Weijmans, Anne-Marie
AU - Wild, Vivienne
AU - Wolf, Marsha
AU - Xue, Yongquan
AU - Yan, Renbin
AU - Zwintz, Konstanze
PY - 2017/11/9
Y1 - 2017/11/9
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 chemicalelements, 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 Groupthat is 1,000 times larger than the current state of the art and at high enough spatial resolution toreveal the self-regulation mechanisms of galactic ecosystems. SDSS-V will pioneer systematic,spectroscopic monitoring across the whole sky, revealing changes on timescales from 20 minutesto 20 years. The survey will thus track the flickers, flares, and radical transformations of the mostluminous 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 providesnear-infrared and optical multi-object fiber spectroscopy that is rapidly reconfigurable to serve hightarget 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 ofSDSS’s advances in data analysis, collaboration spirit and infrastructure, and product deliverablesin astronomy. The project is now refining its science scope, optimizing the survey strategies, anddeveloping new hardware that builds on the SDSS-IV infrastructure. We present here an overviewof the current state of these developments. SDSS-V is actively seeking to build its consortium ofinstitutional 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 chemicalelements, 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 Groupthat is 1,000 times larger than the current state of the art and at high enough spatial resolution toreveal the self-regulation mechanisms of galactic ecosystems. SDSS-V will pioneer systematic,spectroscopic monitoring across the whole sky, revealing changes on timescales from 20 minutesto 20 years. The survey will thus track the flickers, flares, and radical transformations of the mostluminous 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 providesnear-infrared and optical multi-object fiber spectroscopy that is rapidly reconfigurable to serve hightarget 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 ofSDSS’s advances in data analysis, collaboration spirit and infrastructure, and product deliverablesin astronomy. The project is now refining its science scope, optimizing the survey strategies, anddeveloping new hardware that builds on the SDSS-IV infrastructure. We present here an overviewof the current state of these developments. SDSS-V is actively seeking to build its consortium ofinstitutional and individual members for a worldwide, partner-driven collaboration.
M3 - Other contribution
PB - arXiv.org
ER -