The Assembly History of Disk Galaxies: II. Probing the Emerging Tully-Fisher Relation During 1
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<24.1 in the redshift range 1<z&...
| Asıl Yazarlar: | , , , , , |
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| Materyal Türü: | Journal article |
| Dil: | English |
| Baskı/Yayın Bilgisi: |
Institute of Physics Publishing
2012
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| _version_ | 1826281345219821568 |
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| author | Miller, S Ellis, R Sullivan, M Bundy, K Newman, AB Treu, T |
| author_facet | Miller, S Ellis, R Sullivan, M Bundy, K Newman, AB Treu, T |
| author_sort | Miller, S |
| collection | OXFORD |
| 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<24.1 in the redshift range 1<z<1.7. 2.2="" 3727="" 42="" [o="" a="" acs="" and="" at="" available="" between="" body="" combining="" construct="" curves="" defined="" derived="" disk="" distribution="" dynamics="" emission="" enables="" extended="" field="" for="" formalism="" from="" galaxies.="" ground-based="" growing="" hst="" i="" ii]="" images,="" in="" integral="" interval="" introduced="" line="" mass="" masses="" measures="" near-infrared="" of="" paper="" photometry="" probed="" radius="" recover="" relation="" resolved="" rotation="" sample="" scale="" series="" spectrographs="" stellar="" successfully="" the="" these="" this="" time="" times="" to="" tully-fisher="" unit="" us="" using="" we="" well-constructed="" with="" z="" z~1="">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. Although our sample is incomplete in terms of either a fixed stellar mass or star formation rate limit, we discuss the implications that typical star-forming disk galaxies evolve to arrive on a well-defined Tully-Fisher relation within a surprisingly short period of cosmic history.</z<1.7.> |
| first_indexed | 2024-03-07T00:27:24Z |
| format | Journal article |
| id | oxford-uuid:7e9ae650-6a7c-489e-a235-a38f2a08ac2c |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-07T00:27:24Z |
| publishDate | 2012 |
| publisher | Institute of Physics Publishing |
| record_format | dspace |
| spelling | oxford-uuid:7e9ae650-6a7c-489e-a235-a38f2a08ac2c2022-03-26T21:11:11ZThe Assembly History of Disk Galaxies: II. Probing the Emerging Tully-Fisher Relation During 1Journal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:7e9ae650-6a7c-489e-a235-a38f2a08ac2cEnglishSymplectic Elements at OxfordInstitute of Physics Publishing2012Miller, SEllis, RSullivan, MBundy, KNewman, ABTreu, TThrough 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<24.1 in the redshift range 1<z<1.7. 2.2="" 3727="" 42="" [o="" a="" acs="" and="" at="" available="" between="" body="" combining="" construct="" curves="" defined="" derived="" disk="" distribution="" dynamics="" emission="" enables="" extended="" field="" for="" formalism="" from="" galaxies.="" ground-based="" growing="" hst="" i="" ii]="" images,="" in="" integral="" interval="" introduced="" line="" mass="" masses="" measures="" near-infrared="" of="" paper="" photometry="" probed="" radius="" recover="" relation="" resolved="" rotation="" sample="" scale="" series="" spectrographs="" stellar="" successfully="" the="" these="" this="" time="" times="" to="" tully-fisher="" unit="" us="" using="" we="" well-constructed="" with="" z="" z~1="">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. Although our sample is incomplete in terms of either a fixed stellar mass or star formation rate limit, we discuss the implications that typical star-forming disk galaxies evolve to arrive on a well-defined Tully-Fisher relation within a surprisingly short period of cosmic history.</z<1.7.> |
| spellingShingle | Miller, S Ellis, R Sullivan, M Bundy, K Newman, AB Treu, T The Assembly History of Disk Galaxies: II. Probing the Emerging Tully-Fisher Relation During 1 |
| title | The Assembly History of Disk Galaxies: II. Probing the Emerging
Tully-Fisher Relation During 1 |
| title_full | The Assembly History of Disk Galaxies: II. Probing the Emerging
Tully-Fisher Relation During 1 |
| title_fullStr | The Assembly History of Disk Galaxies: II. Probing the Emerging
Tully-Fisher Relation During 1 |
| title_full_unstemmed | The Assembly History of Disk Galaxies: II. Probing the Emerging
Tully-Fisher Relation During 1 |
| title_short | The Assembly History of Disk Galaxies: II. Probing the Emerging
Tully-Fisher Relation During 1 |
| title_sort | assembly history of disk galaxies ii probing the emerging tully fisher relation during 1 |
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