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IRAM 30-m-EMIR redshift search of z=3–4 lensed dusty starbursts selected from the HerBS sample

Bakx, T J L C Dannerbauer, H Frayer, D Eales, S A Pérez-Fournon, I Cai, Z-Y Clements, D L De Zotti, G González-Nuevo, J Ivison, R J Lapi, A Michałowski, M J Negrello, M Serjeant, S Smith, M W L Temi, P Urquhart, S van der Werf, P 名古屋大学

2020.08

概要

Using the Eight MIxer Receiver (EMIR) instrument on the Institut de RadioAstronomie Millimétrique (IRAM) 30-m telescope, we conducted a spectroscopic redshift search of seven zphot ∼ 4 submillimetre bright galaxies selected from the Herschel Bright Sources sample with fluxes at 500 μm greater than 80 mJy. For four sources, we obtained spectroscopic redshifts between 3.4 < z < 4.1 through the detection of multiple CO-spectral lines with J ≥ 3. Later, we detected low-J transitions for two of these sources with the Green Bank Telescope including the CO(1–0) transition. For the remaining three sources, more data are needed to determine the spectroscopic redshift unambiguously. The measured CO luminosities and line widths suggest that all these sources are gravitationally lensed. These observations demonstrate that the 2 mm window is indispensable to confirm robust spectroscopic redshifts for z < 4 sources. Finally, we present an efficient graphical method to correctly identify spectroscopic redshifts.

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Redshift searches of HerBS sources

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Figure A1. The complete spectra taken of source HerBS-52. We show the spectra at 70 km s−1 for individual polarizations (grey) and combined polarizations

(blue).

2386

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Figure A2. The complete spectra taken of source HerBS-61. We show the spectra at 70 km s−1 for individual polarizations (grey) and combined polarizations

(blue).

Redshift searches of HerBS sources

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Figure A3. The complete spectra taken of source HerBS-64. We show the spectra at 70 km s−1 for individual polarizations (grey) and combined polarizations

(blue).

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Figure A5. The complete spectra taken of source HerBS-89. We show the spectra at 70 km s−1 for individual polarizations (grey) and combined polarizations

(blue).

MNRAS 496, 2372–2390 (2020)

Downloaded from https://academic.oup.com/mnras/article-abstract/496/2/2372/5856573 by Nagoya University user on 31 July 2020

Figure A4. The complete spectra taken of source HerBS-83. We show the spectra at 70 km s−1 for individual polarizations (grey) and combined polarizations

(blue).

Redshift searches of HerBS sources

2389

MNRAS 496, 2372–2390 (2020)

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Figure A6. The complete spectra taken of source HerBS-150. We show the spectra at 70 km s−1 for individual polarizations (grey) and combined polarizations

(blue).

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This paper has been typeset from a TEX/LATEX file prepared by the author.

MNRAS 496, 2372–2390 (2020)

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Figure A7. The complete spectra taken of source HerBS-177. We show the spectra at 70 km s−1 for individual polarizations (grey) and combined polarizations

(blue).

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