SDSS-V: Pioneering Panoptic Spectroscopy

Juna A. Kollmeier; Gail Zasowski; Hans-Walter Rix; Matt Johns; Scott F. Anderson; Niv Drory; Jennifer A. Johnson; Richard W. Pogge; Jonathan C. Bird; Guillermo A. Blanc; Joel R. Brownstein; Jeffrey D. Crane; Nathan M. De Lee; Mark A. Klaene; Kathryn Kreckel; Nick MacDonald; Andrea Merloni; Melissa K. Ness; Thomas O'Brien; Jose R. Sanchez-Gallego; Conor C. Sayres; Yue Shen; Ani R. Thakar; Andrew Tkachenko; Conny Aerts; Michael R. Blanton; Daniel J. Eisenstein; Jon A. Holtzman; Dan Maoz; Kirpal Nandra; Constance Rockosi; David H. Weinberg; Jo Bovy; Andrew R. Casey; Julio Chaname; Nicolas Clerc; Charlie Conroy; Michael Eracleous; Boris T. Gänsicke; Saskia Hekker; Keith Horne; Jens Kauffmann; Kristen B. W. McQuinn; Eric W. Pellegrini; Eva Schinnerer; Edward F. Schlafly; Axel D. Schwope; Mark Seibert; Johanna K. Teske; Jennifer L. van Saders

doi:10.48550/arXiv.1711.03234

SDSS-V: Pioneering Panoptic Spectroscopy

Juna A. Kollmeier, Gail Zasowski, Hans-Walter Rix, Matt Johns, Scott F. Anderson, Niv Drory, Jennifer A. Johnson, Richard W. Pogge, Jonathan C. Bird, Guillermo A. Blanc, Joel R. Brownstein, Jeffrey D. Crane, Nathan M. De Lee, Mark A. Klaene, Kathryn Kreckel, Nick MacDonald, Andrea Merloni, Melissa K. Ness, Thomas O'Brien, Jose R. Sanchez-GallegoConor C. Sayres, Yue Shen, Ani R. Thakar, Andrew Tkachenko, Conny Aerts, Michael R. Blanton, Daniel J. Eisenstein, Jon A. Holtzman, Dan Maoz, Kirpal Nandra, Constance Rockosi, David H. Weinberg, Jo Bovy, Andrew R. Casey, Julio Chaname, Nicolas Clerc, Charlie Conroy, Michael Eracleous, Boris T. Gänsicke, Saskia Hekker, Keith Horne, Jens Kauffmann, Kristen B. W. McQuinn, Eric W. Pellegrini, Eva Schinnerer, Edward F. Schlafly, Axel D. Schwope, Mark Seibert, Johanna K. Teske, Jennifer L. van Saders

Research School of Astronomy & Astrophysics

Research output: Other contribution

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, 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 gas in the Galaxy and the Local Group that is 1,000x 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 extant and future spectroscopic surveys: it is all-sky, with matched survey infrastructures in both hemispheres; it provides near-IR 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, ultra-wide-field integral field spectroscopy. SDSS-V, with its programs anticipated to start in 2020, will be well-timed to multiply the scientific output from major space missions (e.g., TESS, Gaia, eROSITA) and ground-based projects. SDSS-V builds on the 25-year heritage of SDSS's advances in data analysis, collaboration infrastructure, and product deliverables. 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 as we seek to build our worldwide consortium of institutional and individual members.

Original language	English
DOIs	https://doi.org/10.48550/arXiv.1711.03234
Publication status	Published - 1 Nov 2017

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https://ui.adsabs.harvard.edu/abs/2017arXiv171103234K

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Kollmeier, J. A., Zasowski, G., Rix, H.-W., Johns, M., Anderson, S. F., Drory, N., Johnson, J. A., Pogge, R. W., Bird, J. C., Blanc, G. A., Brownstein, J. R., Crane, J. D., De Lee, N. M., Klaene, M. A., Kreckel, K., MacDonald, N., Merloni, A., Ness, M. K., O'Brien, T., ... van Saders, J. L. (2017, Nov 1). SDSS-V: Pioneering Panoptic Spectroscopy. https://doi.org/10.48550/arXiv.1711.03234

@misc{e0f4260327c541f2a0645789c9cad0dc,

title = "SDSS-V: Pioneering Panoptic Spectroscopy",

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, 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 gas in the Galaxy and the Local Group that is 1,000x 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 extant and future spectroscopic surveys: it is all-sky, with matched survey infrastructures in both hemispheres; it provides near-IR 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, ultra-wide-field integral field spectroscopy. SDSS-V, with its programs anticipated to start in 2020, will be well-timed to multiply the scientific output from major space missions (e.g., TESS, Gaia, eROSITA) and ground-based projects. SDSS-V builds on the 25-year heritage of SDSS's advances in data analysis, collaboration infrastructure, and product deliverables. 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 as we seek to build our worldwide consortium of institutional and individual members.",

keywords = "Astrophysics - Astrophysics of Galaxies",

author = "Kollmeier, {Juna A.} and Gail Zasowski and Hans-Walter Rix and Matt Johns and Anderson, {Scott F.} and Niv Drory and Johnson, {Jennifer A.} and Pogge, {Richard W.} and Bird, {Jonathan C.} and Blanc, {Guillermo A.} and Brownstein, {Joel R.} and Crane, {Jeffrey D.} and {De Lee}, {Nathan M.} and Klaene, {Mark A.} and Kathryn Kreckel and Nick MacDonald and Andrea Merloni and Ness, {Melissa K.} and Thomas O'Brien and Sanchez-Gallego, {Jose R.} and Sayres, {Conor C.} and Yue Shen and Thakar, {Ani R.} and Andrew Tkachenko and Conny Aerts and Blanton, {Michael R.} and Eisenstein, {Daniel J.} and Holtzman, {Jon A.} and Dan Maoz and Kirpal Nandra and Constance Rockosi and Weinberg, {David H.} and Jo Bovy and Casey, {Andrew R.} and Julio Chaname and Nicolas Clerc and Charlie Conroy and Michael Eracleous and G{\"a}nsicke, {Boris T.} and Saskia Hekker and Keith Horne and Jens Kauffmann and McQuinn, {Kristen B. W.} and Pellegrini, {Eric W.} and Eva Schinnerer and Schlafly, {Edward F.} and Schwope, {Axel D.} and Mark Seibert and Teske, {Johanna K.} and {van Saders}, {Jennifer L.}",

year = "2017",

month = nov,

day = "1",

doi = "10.48550/arXiv.1711.03234",

language = "English",

type = "Other",

}

Kollmeier, JA, Zasowski, G, Rix, H-W, Johns, M, Anderson, SF, Drory, N, Johnson, JA, Pogge, RW, Bird, JC, Blanc, GA, Brownstein, JR, Crane, JD, De Lee, NM, Klaene, MA, Kreckel, K, MacDonald, N, Merloni, A, Ness, MK, O'Brien, T, Sanchez-Gallego, JR, Sayres, CC, Shen, Y, Thakar, AR, Tkachenko, A, Aerts, C, Blanton, MR, Eisenstein, DJ, Holtzman, JA, Maoz, D, Nandra, K, Rockosi, C, Weinberg, DH, Bovy, J, Casey, AR, Chaname, J, Clerc, N, Conroy, C, Eracleous, M, Gänsicke, BT, Hekker, S, Horne, K, Kauffmann, J, McQuinn, KBW, Pellegrini, EW, Schinnerer, E, Schlafly, EF, Schwope, AD, Seibert, M, Teske, JK & van Saders, JL 2017, SDSS-V: Pioneering Panoptic Spectroscopy.. https://doi.org/10.48550/arXiv.1711.03234

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 W.

AU - Bird, Jonathan C.

AU - Blanc, Guillermo A.

AU - Brownstein, Joel R.

AU - Crane, Jeffrey D.

AU - De Lee, Nathan M.

AU - Klaene, Mark A.

AU - Kreckel, Kathryn

AU - MacDonald, Nick

AU - Merloni, Andrea

AU - Ness, Melissa K.

AU - O'Brien, Thomas

AU - Sanchez-Gallego, Jose 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 - van Saders, Jennifer L.

PY - 2017/11/1

Y1 - 2017/11/1

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, 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 gas in the Galaxy and the Local Group that is 1,000x 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 extant and future spectroscopic surveys: it is all-sky, with matched survey infrastructures in both hemispheres; it provides near-IR 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, ultra-wide-field integral field spectroscopy. SDSS-V, with its programs anticipated to start in 2020, will be well-timed to multiply the scientific output from major space missions (e.g., TESS, Gaia, eROSITA) and ground-based projects. SDSS-V builds on the 25-year heritage of SDSS's advances in data analysis, collaboration infrastructure, and product deliverables. 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 as we seek to build our worldwide consortium of institutional and individual members.

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, 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 gas in the Galaxy and the Local Group that is 1,000x 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 extant and future spectroscopic surveys: it is all-sky, with matched survey infrastructures in both hemispheres; it provides near-IR 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, ultra-wide-field integral field spectroscopy. SDSS-V, with its programs anticipated to start in 2020, will be well-timed to multiply the scientific output from major space missions (e.g., TESS, Gaia, eROSITA) and ground-based projects. SDSS-V builds on the 25-year heritage of SDSS's advances in data analysis, collaboration infrastructure, and product deliverables. 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 as we seek to build our worldwide consortium of institutional and individual members.

KW - Astrophysics - Astrophysics of Galaxies

U2 - 10.48550/arXiv.1711.03234

DO - 10.48550/arXiv.1711.03234

M3 - Other contribution

ER -

SDSS-V: Pioneering Panoptic Spectroscopy

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