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The Assembly History of Disk Galaxies: II. Probing the Emerging Tully-Fisher Relation During 1<z<1.7
Through extended integrations using the recently-installed deep depletion CCD on the red arm of the Keck I Low Resolution Imaging Spectrograph, we present new measurements of the resolved spectra of 70 morphologically-selected star-forming galaxies with i_AB
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| Published in: | arXiv.org 2012-04 |
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| creator | Miller, Sarah H Ellis, Richard S Sullivan, Mark Bundy, Kevin Newman, Andrew B Treu, Tommaso |
| description | Through extended integrations using the recently-installed deep depletion CCD on the red arm of the Keck I Low Resolution Imaging Spectrograph, we present new measurements of the resolved spectra of 70 morphologically-selected star-forming galaxies with i_AB |
| doi_str_mv | 10.48550/arxiv.1201.4386 |
| format | article |
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Combining these measures with stellar masses derived from HST and ground-based near-infrared photometry enables us to construct the stellar mass Tully-Fisher relation in the time interval between the well-constructed relation defined at z~1 in Paper I and the growing body of resolved dynamics probed with integral field unit spectrographs at z>2. Remarkably, we find a well-defined Tully-Fisher relation with up to 60% increase in scatter and stellar mass zero-point shift constraint of 0.02+/-0.02 dex since z~1.7, compared to the local relation. 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| identifier | EISSN: 2331-8422 |
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| issn | 2331-8422 |
| language | eng |
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| source | Publicly Available Content Database |
| subjects | Depletion Disk galaxies Galactic evolution Galaxies Image resolution Infrared photometry Photometry Red shift Spectrographs Star & galaxy formation Star formation rate Stellar evolution Stellar mass Tully-Fisher relation |
| title | The Assembly History of Disk Galaxies: II. Probing the Emerging Tully-Fisher Relation During 1<z<1.7 |
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