FIRST SCIENCE WITH SAMI: A SERENDIPITOUSLY DISCOVERED GALACTIC WIND IN ESO 185-G031
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 th...
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| Veröffentlicht in: | The Astrophysical journal 2012-12, Vol.761 (2), p.1-12 |
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| creator | FOGARTY, Lisa M. R BLAND-HAWTHORN, Joss BROUGH, Sarah COLLESS, Matthew ELLIS, Simon C FARRELL, Tony GOODWIN, Michael HEALD, Ron HOPKINS, Andrew M HORTON, Anthony HEATH JONES, D LEE, Steve CROOM, Scott M LEWIS, Geraint LOPEZ-SANCHEZ, Angel R MIZIARSKI, Stan TROWLAND, Holly LEON-SAVAL, Sergio G MIN, Seong-Sik TRINH, Christopher CECIL, Gerald VEILLEUX, Sylvain KREIMEYER, Kory GREEN, Andrew W BRYANT, Julia J LAWRENCE, Jon S RICHARDS, Samuel ALLEN, James T BAUER, Amanda E BIRCHALL, Michael N |
| description | 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. |
| doi_str_mv | 10.1088/0004-637X/761/2/169 |
| format | Article |
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R ; BLAND-HAWTHORN, Joss ; BROUGH, Sarah ; COLLESS, Matthew ; ELLIS, Simon C ; FARRELL, Tony ; GOODWIN, Michael ; HEALD, Ron ; HOPKINS, Andrew M ; HORTON, Anthony ; HEATH JONES, D ; LEE, Steve ; CROOM, Scott M ; LEWIS, Geraint ; LOPEZ-SANCHEZ, Angel R ; MIZIARSKI, Stan ; TROWLAND, Holly ; LEON-SAVAL, Sergio G ; MIN, Seong-Sik ; TRINH, Christopher ; CECIL, Gerald ; VEILLEUX, Sylvain ; KREIMEYER, Kory ; GREEN, Andrew W ; BRYANT, Julia J ; LAWRENCE, Jon S ; RICHARDS, Samuel ; ALLEN, James T ; BAUER, Amanda E ; BIRCHALL, Michael N</creator><creatorcontrib>FOGARTY, Lisa M. R ; BLAND-HAWTHORN, Joss ; BROUGH, Sarah ; COLLESS, Matthew ; ELLIS, Simon C ; FARRELL, Tony ; GOODWIN, Michael ; HEALD, Ron ; HOPKINS, Andrew M ; HORTON, Anthony ; HEATH JONES, D ; LEE, Steve ; CROOM, Scott M ; LEWIS, Geraint ; LOPEZ-SANCHEZ, Angel R ; MIZIARSKI, Stan ; TROWLAND, Holly ; LEON-SAVAL, Sergio G ; MIN, Seong-Sik ; TRINH, Christopher ; CECIL, Gerald ; VEILLEUX, Sylvain ; KREIMEYER, Kory ; GREEN, Andrew W ; BRYANT, Julia J ; LAWRENCE, Jon S ; RICHARDS, Samuel ; ALLEN, James T ; BAUER, Amanda E ; BIRCHALL, Michael N</creatorcontrib><description>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. 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R</creatorcontrib><creatorcontrib>BLAND-HAWTHORN, Joss</creatorcontrib><creatorcontrib>BROUGH, Sarah</creatorcontrib><creatorcontrib>COLLESS, Matthew</creatorcontrib><creatorcontrib>ELLIS, Simon C</creatorcontrib><creatorcontrib>FARRELL, Tony</creatorcontrib><creatorcontrib>GOODWIN, Michael</creatorcontrib><creatorcontrib>HEALD, Ron</creatorcontrib><creatorcontrib>HOPKINS, Andrew M</creatorcontrib><creatorcontrib>HORTON, Anthony</creatorcontrib><creatorcontrib>HEATH JONES, D</creatorcontrib><creatorcontrib>LEE, Steve</creatorcontrib><creatorcontrib>CROOM, Scott M</creatorcontrib><creatorcontrib>LEWIS, Geraint</creatorcontrib><creatorcontrib>LOPEZ-SANCHEZ, Angel R</creatorcontrib><creatorcontrib>MIZIARSKI, Stan</creatorcontrib><creatorcontrib>TROWLAND, Holly</creatorcontrib><creatorcontrib>LEON-SAVAL, Sergio G</creatorcontrib><creatorcontrib>MIN, Seong-Sik</creatorcontrib><creatorcontrib>TRINH, Christopher</creatorcontrib><creatorcontrib>CECIL, Gerald</creatorcontrib><creatorcontrib>VEILLEUX, Sylvain</creatorcontrib><creatorcontrib>KREIMEYER, Kory</creatorcontrib><creatorcontrib>GREEN, Andrew W</creatorcontrib><creatorcontrib>BRYANT, Julia J</creatorcontrib><creatorcontrib>LAWRENCE, Jon S</creatorcontrib><creatorcontrib>RICHARDS, Samuel</creatorcontrib><creatorcontrib>ALLEN, James T</creatorcontrib><creatorcontrib>BAUER, Amanda E</creatorcontrib><creatorcontrib>BIRCHALL, Michael N</creatorcontrib><title>FIRST SCIENCE WITH SAMI: A SERENDIPITOUSLY DISCOVERED GALACTIC WIND IN ESO 185-G031</title><title>The Astrophysical journal</title><description>We present the first scientific results from the Sydney-AAO Multi-Object IFS (SAMI) at the Anglo-Australian Telescope. 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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.</abstract><cop>Bristol</cop><pub>IOP</pub><doi>10.1088/0004-637X/761/2/169</doi><tpages>12</tpages><oa>free_for_read</oa></addata></record> |
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| ispartof | The Astrophysical journal, 2012-12, Vol.761 (2), p.1-12 |
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| source | IOP Publishing Free Content; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection |
| subjects | APERTURES ASTRONOMY ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BRIGHTNESS Bundles Earth, ocean, space EMISSION SPECTRA EMISSION SPECTROSCOPY Exact sciences and technology FIBERS Galactic winds GALAXIES IONIZATION Spectral emissivity Spectrographs Spectroscopy STARS STELLAR WINDS TELESCOPES |
| title | FIRST SCIENCE WITH SAMI: A SERENDIPITOUSLY DISCOVERED GALACTIC WIND IN ESO 185-G031 |
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