Near-infrared Hydrogen and Helium QSO Emission Lines
We present 14 near-infrared (NIR) quasar spectra observed with the Flamingos-2 NIR spectrometer instrument at the Gemini South Observatory. The targets were selected with redshifts of (0.58 ≤ z ≤ 0.63) to ensure the spectral wavelength range included specifically identified hydrogen and helium broad...
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Published in | The Astronomical journal Vol. 158; no. 3; pp. 129 - 136 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
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The American Astronomical Society
01.09.2019
IOP Publishing |
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Abstract | We present 14 near-infrared (NIR) quasar spectra observed with the Flamingos-2 NIR spectrometer instrument at the Gemini South Observatory. The targets were selected with redshifts of (0.58 ≤ z ≤ 0.63) to ensure the spectral wavelength range included specifically identified hydrogen and helium broad emission lines. We present measurements of their FWHM, equivalent widths, and flux ratios relative to H . The quasars are all within the Sloan Digital Sky Survey (SDSS) Stripe 82 region which, then also provides multi-epoch rest-frame UV and optical spectroscopic observations of our targets. In future work, these data and those from Galaxy Evolution Explorer and NUV spectra will be utilized to constrain photoionization models to determine physical conditions within the broad emission line regions, such as the incident ionizing photon flux and gas density. |
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AbstractList | We present 14 near-infrared (NIR) quasar spectra observed with the Flamingos-2 NIR spectrometer instrument at the Gemini South Observatory. The targets were selected with redshifts of (0.58 ≤ z ≤ 0.63) to ensure the spectral wavelength range included specifically identified hydrogen and helium broad emission lines. We present measurements of their FWHM, equivalent widths, and flux ratios relative to H α. The quasars are all within the Sloan Digital Sky Survey (SDSS) Stripe 82 region which, then also provides multi-epoch rest-frame UV and optical spectroscopic observations of our targets. In future work, these data and those from Galaxy Evolution Explorer and NUV spectra will be utilized to constrain photoionization models to determine physical conditions within the broad emission line regions, such as the incident ionizing photon flux and gas density. Abstract We present 14 near-infrared (NIR) quasar spectra observed with the Flamingos-2 NIR spectrometer instrument at the Gemini South Observatory. The targets were selected with redshifts of (0.58 ≤ z ≤ 0.63) to ensure the spectral wavelength range included specifically identified hydrogen and helium broad emission lines. We present measurements of their FWHM, equivalent widths, and flux ratios relative to H α . The quasars are all within the Sloan Digital Sky Survey (SDSS) Stripe 82 region which, then also provides multi-epoch rest-frame UV and optical spectroscopic observations of our targets. In future work, these data and those from Galaxy Evolution Explorer and NUV spectra will be utilized to constrain photoionization models to determine physical conditions within the broad emission line regions, such as the incident ionizing photon flux and gas density. We present 14 near-infrared (NIR) quasar spectra observed with the Flamingos-2 NIR spectrometer instrument at the Gemini South Observatory. The targets were selected with redshifts of (0.58 ≤ z ≤ 0.63) to ensure the spectral wavelength range included specifically identified hydrogen and helium broad emission lines. We present measurements of their FWHM, equivalent widths, and flux ratios relative to H . The quasars are all within the Sloan Digital Sky Survey (SDSS) Stripe 82 region which, then also provides multi-epoch rest-frame UV and optical spectroscopic observations of our targets. In future work, these data and those from Galaxy Evolution Explorer and NUV spectra will be utilized to constrain photoionization models to determine physical conditions within the broad emission line regions, such as the incident ionizing photon flux and gas density. |
Author | Webster, R. L. Kenyon, C. E. G. Labrie, K. King, A. L. |
Author_xml | – sequence: 1 givenname: C. E. G. orcidid: 0000-0001-5533-6386 surname: Kenyon fullname: Kenyon, C. E. G. email: clare.kenyon@unimelb.edu.au organization: University of Melbourne School of Physics, 3010, , Australia – sequence: 2 givenname: K. orcidid: 0000-0002-6633-7891 surname: Labrie fullname: Labrie, K. email: klabrie@gemini.edu organization: Gemini Observatory, Hilo, HI 96720, USA – sequence: 3 givenname: R. L. orcidid: 0000-0002-5325-2709 surname: Webster fullname: Webster, R. L. email: r.webster@unimelb.edu.au organization: University of Melbourne School of Physics, 3010, , Australia – sequence: 4 givenname: A. L. orcidid: 0000-0001-5352-0550 surname: King fullname: King, A. L. email: anthea.king@unimelb.edu.au organization: University of Melbourne School of Physics, 3010, , Australia |
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Cites_doi | 10.5281/zenodo.804967 10.5281/zenodo.11813 10.1086/518158 10.1088/0004-637X/737/2/103 10.1086/133630 10.1093/mnras/stw1865 10.1086/522373 10.3847/0004-637X/824/1/53 10.1088/0004-637X/754/1/18 10.1086/500098 10.1086/312966 10.1117/12.968154 10.1086/316190 |
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Copyright | 2019. The American Astronomical Society. All rights reserved. Copyright IOP Publishing Sep 2019 |
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Snippet | We present 14 near-infrared (NIR) quasar spectra observed with the Flamingos-2 NIR spectrometer instrument at the Gemini South Observatory. The targets were... Abstract We present 14 near-infrared (NIR) quasar spectra observed with the Flamingos-2 NIR spectrometer instrument at the Gemini South Observatory. The... |
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StartPage | 129 |
SubjectTerms | Astronomy Emission lines Emission measurements Galactic evolution Galaxies Gas density Helium Hydrogen Infrared spectra infrared: galaxies Near infrared radiation Photoionization Quasars quasars: emission lines quasars: general Sky surveys (astronomy) |
Title | Near-infrared Hydrogen and Helium QSO Emission Lines |
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