The southern stellar stream spectroscopic survey (S5): Overview, target selection, data reduction, validation, and early science
We introduce the southern stellar stream spectroscopy survey (S5), an on-going program to map the kinematics and chemistry of stellar streams in the southern hemisphere. The initial focus of S5 has been spectroscopic observations of recently identified streams within the footprint of the dark energy...
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| Published in | Monthly notices of the Royal Astronomical Society Vol. 490; no. 3; pp. 3508 - 3531 |
|---|---|
| Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
United States
Royal Astronomical Society
01.12.2019
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| Subjects | |
| Online Access | Get full text |
| ISSN | 0035-8711 1365-2966 |
| DOI | 10.1093/mnras/stz2731 |
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| Abstract | We introduce the southern stellar stream spectroscopy survey (S5), an on-going program to map the kinematics and chemistry of stellar streams in the southern hemisphere. The initial focus of S5 has been spectroscopic observations of recently identified streams within the footprint of the dark energy survey (DES), with the eventual goal of surveying streams across the entire southern sky. Stellar streams are composed of material that has been tidally striped from dwarf galaxies and globular clusters and hence are excellent dynamical probes of the gravitational potential of the Milky Way, as well as providing a detailed snapshot of its accretion history. Observing with the 3.9 m Anglo-Australian Telescope’s 2-degree-Field fibre positioner and AAOmega spectrograph, and combining the precise photometry of DES DR1 with the superb proper motions from Gaia DR2, allows us to conduct an efficient spectroscopic survey to map these stellar streams. So far S5 has mapped nine DES streams and three streams outside of DES; the former are the first spectroscopic observations of these recently discovered streams. In addition to the stream survey, we use spare fibres to undertake a Milky Way halo survey and a low-redshift galaxy survey. This paper presents an overview of the S5 program, describing the scientific motivation for the survey, target selection, observation strategy, data reduction, and survey validation. Finally, we describe early science results on stellar streams and Milky Way halo stars drawn from the survey. Updates on S5, including future public data releases, can be found at http://s5collab.github.io. |
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| AbstractList | Herein, we introduce the southern stellar stream spectroscopy survey (S5), an on-going program to map the kinematics and chemistry of stellar streams in the southern hemisphere. The initial focus of S5 has been spectroscopic observations of recently identified streams within the footprint of the dark energy survey (DES), with the eventual goal of surveying streams across the entire southern sky. Stellar streams are composed of material that has been tidally striped from dwarf galaxies and globular clusters and hence are excellent dynamical probes of the gravitational potential of the Milky Way, as well as providing a detailed snapshot of its accretion history. Observing with the 3.9 m Anglo-Australian Telescope’s 2-degree-Field fibre positioner and AAOmega spectrograph, and combining the precise photometry of DES DR1 with the superb proper motions from Gaia DR2, allows us to conduct an efficient spectroscopic survey to map these stellar streams. So far S5 has mapped nine DES streams and three streams outside of DES; the former are the first spectroscopic observations of these recently discovered streams. In addition to the stream survey, we use spare fibres to undertake a Milky Way halo survey and a low-redshift galaxy survey. This paper presents an overview of the S5 program, describing the scientific motivation for the survey, target selection, observation strategy, data reduction, and survey validation. Lastly, we describe early science results on stellar streams and Milky Way halo stars drawn from the survey. Updates on S5, including future public data releases, can be found at http://s5collab.github.io. We introduce the southern stellar stream spectroscopy survey (S5), an on-going program to map the kinematics and chemistry of stellar streams in the southern hemisphere. The initial focus of S5 has been spectroscopic observations of recently identified streams within the footprint of the dark energy survey (DES), with the eventual goal of surveying streams across the entire southern sky. Stellar streams are composed of material that has been tidally striped from dwarf galaxies and globular clusters and hence are excellent dynamical probes of the gravitational potential of the Milky Way, as well as providing a detailed snapshot of its accretion history. Observing with the 3.9 m Anglo-Australian Telescope’s 2-degree-Field fibre positioner and AAOmega spectrograph, and combining the precise photometry of DES DR1 with the superb proper motions from Gaia DR2, allows us to conduct an efficient spectroscopic survey to map these stellar streams. So far S5 has mapped nine DES streams and three streams outside of DES; the former are the first spectroscopic observations of these recently discovered streams. In addition to the stream survey, we use spare fibres to undertake a Milky Way halo survey and a low-redshift galaxy survey. This paper presents an overview of the S5 program, describing the scientific motivation for the survey, target selection, observation strategy, data reduction, and survey validation. Finally, we describe early science results on stellar streams and Milky Way halo stars drawn from the survey. Updates on S5, including future public data releases, can be found at http://s5collab.github.io. |
| Author | Balbinot, E Simpson, J D Mao, Y-Y De Silva, G M Ji, A P Bland-Hawthorn, J Pace, A B Tucker, D L Mould, J R Erkal, D Shipp, N Li, T S Geha, M Belokurov, V Mackey, A D Wan, Z Cullinane, L Vivas, A K Kuehn, K Simon, J D Yanny, B Bechtol, K Zucker, D B Casey, A R Martell, S L Lewis, G F Allam, S Wechsler, R H Koposov, S E Da Costa, G S Sharma, S Drlica-Wagner, A |
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500, Batavia, IL 60510, USA, Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA, Department of Astronomy & Astrophysics, University of Chicago, 5640 S Ellis Avenue, Chicago, IL 60637, USA – sequence: 9 givenname: Y-Y orcidid: 0000-0002-1200-0820 surname: Mao fullname: Mao, Y-Y organization: Department of Physics and Astronomy, Rutgers, The State University of New Jersey, Piscataway, NJ 08854, USA, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA, Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT PACC), University of Pittsburgh, Pittsburgh, PA 15260, USA – sequence: 10 givenname: M surname: Geha fullname: Geha, M organization: Department of Astronomy, Yale University, New Haven, CT 06520, USA – sequence: 11 givenname: A B orcidid: 0000-0002-6021-8760 surname: Pace fullname: Pace, A B organization: George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and 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givenname: J D surname: Simon fullname: Simon, J D organization: Observatories of the Carnegie Institution for Science, 813 Santa Barbara St., Pasadena, CA 91101, USA – sequence: 18 givenname: J R surname: Mould fullname: Mould, J R organization: Centre for Astrophysics and Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, VIC 3122, Australia – sequence: 19 givenname: S L orcidid: 0000-0002-3430-4163 surname: Martell fullname: Martell, S L organization: School of Physics, UNSW, Sydney, NSW 2052, Australia, Centre of Excellence for All-Sky Astrophysics in Three Dimensions (ASTRO 3D), Australia – sequence: 20 givenname: Z orcidid: 0000-0002-3105-3821 surname: Wan fullname: Wan, Z organization: Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW 2006, Australia – sequence: 21 givenname: G M surname: De Silva fullname: De Silva, G M organization: Australian Astronomical Optics, Faculty of Science and Engineering, Macquarie University, Macquarie Park, NSW 2113, Australia – sequence: 22 givenname: K surname: Bechtol fullname: Bechtol, K organization: Department of Physics, University of Wisconsin-Madison, 1150 University Avenue Madison, WI 53706, USA – sequence: 23 givenname: E orcidid: 0000-0002-1322-3153 surname: Balbinot fullname: Balbinot, E organization: Kapteyn Astronomical Institute, University of Groningen, Postbus 800, NL-9700AV Groningen, the Netherlands – sequence: 24 givenname: V orcidid: 0000-0002-0038-9584 surname: Belokurov fullname: Belokurov, V organization: Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK – sequence: 25 givenname: J orcidid: 0000-0001-7516-4016 surname: Bland-Hawthorn fullname: Bland-Hawthorn, J organization: Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW 2006, Australia, Centre of Excellence for All-Sky Astrophysics in Three Dimensions (ASTRO 3D), Australia – sequence: 26 givenname: A R orcidid: 0000-0003-0174-0564 surname: Casey fullname: Casey, A R organization: School of Physics and Astronomy, Monash University, Wellington Rd, Clayton, VIC 3800, Australia – sequence: 27 givenname: L surname: Cullinane fullname: Cullinane, L organization: Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia – sequence: 28 givenname: A surname: Drlica-Wagner fullname: Drlica-Wagner, A organization: Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA, Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA, Department of Astronomy & Astrophysics, University of Chicago, 5640 S Ellis Avenue, Chicago, IL 60637, USA – sequence: 29 givenname: S orcidid: 0000-0002-0920-809X surname: Sharma fullname: Sharma, S organization: Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW 2006, Australia, Centre of Excellence for All-Sky Astrophysics in Three Dimensions (ASTRO 3D), Australia – sequence: 30 givenname: A K orcidid: 0000-0003-4341-6172 surname: Vivas fullname: Vivas, A K organization: Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile – sequence: 31 givenname: R H surname: Wechsler fullname: Wechsler, R H organization: Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA, Kavli Institute for Particle Astrophysics & Cosmology, PO Box 2450, Stanford University, Stanford, CA 94305, USA, SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA – sequence: 32 givenname: B surname: Yanny fullname: Yanny, B organization: Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA |
| BackLink | https://www.osti.gov/servlets/purl/1568863$$D View this record in Osti.gov |
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| Notes | arXiv:1907.09481; FERMILAB-PUB--19-290-AE USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25) AC02-07CH11359; AC02-76SF00515 |
| ORCID | 0000-0002-1200-0820 0000-0001-7019-649X 0000-0002-8165-2507 0000-0003-3081-9319 0000-0002-6021-8760 0000-0003-2644-135X 0000-0002-3105-3821 0000-0002-3430-4163 0000-0001-7516-4016 0000-0002-8448-5505 0000-0002-0920-809X 0000-0002-9110-6163 0000-0002-1322-3153 0000-0002-0038-9584 0000-0003-4341-6172 0000-0003-0174-0564 000000020920809X 0000000175164016 0000000281652507 0000000260218760 0000000212000820 0000000231053821 0000000284485505 0000000301740564 000000032644135X 0000000330819319 0000000343416172 000000017019649X 0000000213223153 0000000200389584 0000000234304163 0000000291106163 |
| OpenAccessLink | https://www.osti.gov/servlets/purl/1568863 |
| PageCount | 24 |
| ParticipantIDs | osti_scitechconnect_1568863 crossref_citationtrail_10_1093_mnras_stz2731 crossref_primary_10_1093_mnras_stz2731 |
| ProviderPackageCode | CITATION AAYXX |
| PublicationCentury | 2000 |
| PublicationDate | 2019-12-01 |
| PublicationDateYYYYMMDD | 2019-12-01 |
| PublicationDate_xml | – month: 12 year: 2019 text: 2019-12-01 day: 01 |
| PublicationDecade | 2010 |
| PublicationPlace | United States |
| PublicationPlace_xml | – name: United States |
| PublicationTitle | Monthly notices of the Royal Astronomical Society |
| PublicationYear | 2019 |
| Publisher | Royal Astronomical Society |
| Publisher_xml | – name: Royal Astronomical Society |
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| Snippet | We introduce the southern stellar stream spectroscopy survey (S5), an on-going program to map the kinematics and chemistry of stellar streams in the southern... Herein, we introduce the southern stellar stream spectroscopy survey (S5), an on-going program to map the kinematics and chemistry of stellar streams in the... |
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| SubjectTerms | galaxies: dwarf galaxy: halo galaxy: kinematics and dynamics globular clusters: general |
| Title | The southern stellar stream spectroscopic survey (S5): Overview, target selection, data reduction, validation, and early science |
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