First science with SAMI: a serendipitously discovered Galactic wind in ESO 185-G031

Lisa M. R. Fogarty; Joss Bland-Hawthorn; Scott M. Croom; Andrew W. Green; Julia J. Bryant; Jon S. Lawrence; Samuel Richards; James T. Allen; Amanda E. Bauer; Michael N. Birchall; Sarah Brough; Matthew Colless; Simon C. Ellis; Tony Farrell; Michael Goodwin; Ron Heald; Andrew M. Hopkins; Anthony Horton; D. Heath Jones; Steve Lee; Geraint Lewis; Ángel R. López-Sánchez; Stan Miziarski; Holly Trowland; Sergio G. Leon-Saval; Seong Sik Min; Christopher Trinh; Gerald Cecil; Sylvain Veilleux; Kory Kreimeyer

doi:10.1088/0004-637X/761/2/169

First science with SAMI: a serendipitously discovered Galactic wind in ESO 185-G031

Lisa M. R. Fogarty, Joss Bland-Hawthorn, Scott M. Croom, Andrew W. Green, Julia J. Bryant, Jon S. Lawrence, Samuel Richards, James T. Allen, Amanda E. Bauer, Michael N. Birchall, Sarah Brough, Matthew Colless, Simon C. Ellis, Tony Farrell, Michael Goodwin, Ron Heald, Andrew M. Hopkins, Anthony Horton, D. Heath Jones, Steve LeeGeraint Lewis, Ángel R. López-Sánchez, Stan Miziarski, Holly Trowland, Sergio G. Leon-Saval, Seong Sik Min, Christopher Trinh, Gerald Cecil, Sylvain Veilleux, Kory Kreimeyer

Research output: Contribution to journal › Article › peer-review

39 Citations (Scopus)

Abstract

We present the first scientific results from the Sydney-AAO Multi-Object IFS (SAMI) at the Anglo-Australian Telescope. This unique instrument deploys 13 fused fiber bundles (hexabundles) across a one-degree field of view allowing simultaneous spatially resolved spectroscopy of 13 galaxies. During the first SAMI commissioning run, targeting a single galaxy field, one object (ESO 185-G031) was found to have extended minor axis emission with ionization and kinematic properties consistent with a large-scale galactic wind. The importance of this result is twofold: (1) fiber bundle spectrographs are able to identify low surface brightness emission arising from extranuclear activity and (2) such activity may be more common than presently assumed because conventional multi-object spectrographs use single-aperture fibers and spectra from these are nearly always dominated by nuclear emission. These early results demonstrate the extraordinary potential of multi-object hexabundle spectroscopy in future galaxy surveys.

Original language	English
Article number	169
Pages (from-to)	1-12
Number of pages	12
Journal	Astrophysical Journal
Volume	761
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/761/2/169
Publication status	Published - 10 Dec 2012

Keywords

galaxies: evolution
galaxies: individual (ESO 185-G031)
galaxies: kinematics and dynamics
galaxies: star formation
techniques: imaging spectroscopy

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Fogarty, L. M. R., Bland-Hawthorn, J., Croom, S. M., Green, A. W., Bryant, J. J., Lawrence, J. S., Richards, S., Allen, J. T., Bauer, A. E., Birchall, M. N., Brough, S., Colless, M., Ellis, S. C., Farrell, T., Goodwin, M., Heald, R., Hopkins, A. M., Horton, A., Jones, D. H., ... Kreimeyer, K. (2012). First science with SAMI: a serendipitously discovered Galactic wind in ESO 185-G031. Astrophysical Journal, 761(2), 1-12. Article 169. https://doi.org/10.1088/0004-637X/761/2/169

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title = "First science with SAMI: a serendipitously discovered Galactic wind in ESO 185-G031",

abstract = "We present the first scientific results from the Sydney-AAO Multi-Object IFS (SAMI) at the Anglo-Australian Telescope. This unique instrument deploys 13 fused fiber bundles (hexabundles) across a one-degree field of view allowing simultaneous spatially resolved spectroscopy of 13 galaxies. During the first SAMI commissioning run, targeting a single galaxy field, one object (ESO 185-G031) was found to have extended minor axis emission with ionization and kinematic properties consistent with a large-scale galactic wind. The importance of this result is twofold: (1) fiber bundle spectrographs are able to identify low surface brightness emission arising from extranuclear activity and (2) such activity may be more common than presently assumed because conventional multi-object spectrographs use single-aperture fibers and spectra from these are nearly always dominated by nuclear emission. These early results demonstrate the extraordinary potential of multi-object hexabundle spectroscopy in future galaxy surveys.",

keywords = "galaxies: evolution, galaxies: individual (ESO 185-G031), galaxies: kinematics and dynamics, galaxies: star formation, techniques: imaging spectroscopy",

author = "Fogarty, {Lisa M. R.} and Joss Bland-Hawthorn and Croom, {Scott M.} and Green, {Andrew W.} and Bryant, {Julia J.} and Lawrence, {Jon S.} and Samuel Richards and Allen, {James T.} and Bauer, {Amanda E.} and Birchall, {Michael N.} and Sarah Brough and Matthew Colless and Ellis, {Simon C.} and Tony Farrell and Michael Goodwin and Ron Heald and Hopkins, {Andrew M.} and Anthony Horton and Jones, {D. Heath} and Steve Lee and Geraint Lewis and L{\'o}pez-S{\'a}nchez, {{\'A}ngel R.} and Stan Miziarski and Holly Trowland and Leon-Saval, {Sergio G.} and Min, {Seong Sik} and Christopher Trinh and Gerald Cecil and Sylvain Veilleux and Kory Kreimeyer",

year = "2012",

month = dec,

day = "10",

doi = "10.1088/0004-637X/761/2/169",

language = "English",

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Fogarty, LMR, Bland-Hawthorn, J, Croom, SM, Green, AW, Bryant, JJ, Lawrence, JS, Richards, S, Allen, JT, Bauer, AE, Birchall, MN, Brough, S, Colless, M, Ellis, SC, Farrell, T, Goodwin, M, Heald, R, Hopkins, AM, Horton, A, Jones, DH, Lee, S, Lewis, G, López-Sánchez, ÁR, Miziarski, S, Trowland, H, Leon-Saval, SG, Min, SS, Trinh, C, Cecil, G, Veilleux, S & Kreimeyer, K 2012, 'First science with SAMI: a serendipitously discovered Galactic wind in ESO 185-G031', Astrophysical Journal, vol. 761, no. 2, 169, pp. 1-12. https://doi.org/10.1088/0004-637X/761/2/169

TY - JOUR

T1 - First science with SAMI

T2 - a serendipitously discovered Galactic wind in ESO 185-G031

AU - Fogarty, Lisa M. R.

AU - Bland-Hawthorn, Joss

AU - Croom, Scott M.

AU - Green, Andrew W.

AU - Bryant, Julia J.

AU - Lawrence, Jon S.

AU - Richards, Samuel

AU - Allen, James T.

AU - Bauer, Amanda E.

AU - Birchall, Michael N.

AU - Brough, Sarah

AU - Colless, Matthew

AU - Ellis, Simon C.

AU - Farrell, Tony

AU - Goodwin, Michael

AU - Heald, Ron

AU - Hopkins, Andrew M.

AU - Horton, Anthony

AU - Jones, D. Heath

AU - Lee, Steve

AU - Lewis, Geraint

AU - López-Sánchez, Ángel R.

AU - Miziarski, Stan

AU - Trowland, Holly

AU - Leon-Saval, Sergio G.

AU - Min, Seong Sik

AU - Trinh, Christopher

AU - Cecil, Gerald

AU - Veilleux, Sylvain

AU - Kreimeyer, Kory

PY - 2012/12/10

Y1 - 2012/12/10

N2 - We present the first scientific results from the Sydney-AAO Multi-Object IFS (SAMI) at the Anglo-Australian Telescope. This unique instrument deploys 13 fused fiber bundles (hexabundles) across a one-degree field of view allowing simultaneous spatially resolved spectroscopy of 13 galaxies. During the first SAMI commissioning run, targeting a single galaxy field, one object (ESO 185-G031) was found to have extended minor axis emission with ionization and kinematic properties consistent with a large-scale galactic wind. The importance of this result is twofold: (1) fiber bundle spectrographs are able to identify low surface brightness emission arising from extranuclear activity and (2) such activity may be more common than presently assumed because conventional multi-object spectrographs use single-aperture fibers and spectra from these are nearly always dominated by nuclear emission. These early results demonstrate the extraordinary potential of multi-object hexabundle spectroscopy in future galaxy surveys.

AB - We present the first scientific results from the Sydney-AAO Multi-Object IFS (SAMI) at the Anglo-Australian Telescope. This unique instrument deploys 13 fused fiber bundles (hexabundles) across a one-degree field of view allowing simultaneous spatially resolved spectroscopy of 13 galaxies. During the first SAMI commissioning run, targeting a single galaxy field, one object (ESO 185-G031) was found to have extended minor axis emission with ionization and kinematic properties consistent with a large-scale galactic wind. The importance of this result is twofold: (1) fiber bundle spectrographs are able to identify low surface brightness emission arising from extranuclear activity and (2) such activity may be more common than presently assumed because conventional multi-object spectrographs use single-aperture fibers and spectra from these are nearly always dominated by nuclear emission. These early results demonstrate the extraordinary potential of multi-object hexabundle spectroscopy in future galaxy surveys.

KW - galaxies: evolution

KW - galaxies: individual (ESO 185-G031)

KW - galaxies: kinematics and dynamics

KW - galaxies: star formation

KW - techniques: imaging spectroscopy

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U2 - 10.1088/0004-637X/761/2/169

DO - 10.1088/0004-637X/761/2/169

M3 - Article

AN - SCOPUS:84870841686

SN - 0004-637X

VL - 761

SP - 1

EP - 12

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 169

ER -

First science with SAMI: a serendipitously discovered Galactic wind in ESO 185-G031

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