ALMA [CII] 158 [mu]m Detection of a Redshift 7 Lensed Galaxy behind RX J1347.1?1145

We present the results of ALMA spectroscopic follow-up of a z= 6.766 Ly[alpha] emitting galaxy behind the cluster RX J1347.1?1145. We report the detection of [Cii] 158 [mu] m line fully consistent with the Ly[alpha] redshift and with the peak of the optical emission. Given the magnification of [mu]=...

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Veröffentlicht in:Astrophysical journal. Letters 2017-02, Vol.836 (1), p.L2-L2
Hauptverfasser: Bradac, Marusa, Garcia-Appadoo, Diego, Huang, Kuang-Han, Vallini, Livia, Finney, Emily Quinn, Hoag, Austin, Lemaux, Brian C, Schmidt, Kasper Borello, Treu, Tommaso, Carilli, Chris
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container_issue 1
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container_title Astrophysical journal. Letters
container_volume 836
creator Bradac, Marusa
Garcia-Appadoo, Diego
Huang, Kuang-Han
Vallini, Livia
Finney, Emily Quinn
Hoag, Austin
Lemaux, Brian C
Schmidt, Kasper Borello
Treu, Tommaso
Carilli, Chris
description We present the results of ALMA spectroscopic follow-up of a z= 6.766 Ly[alpha] emitting galaxy behind the cluster RX J1347.1?1145. We report the detection of [Cii] 158 [mu] m line fully consistent with the Ly[alpha] redshift and with the peak of the optical emission. Given the magnification of [mu]= 5.0 + or - 0.3, the intrinsic (corrected for lensing) luminosity of the [CII] line is L sub([CII])= (ProQuest: Formulae and/or non-USASCII text omitted), roughlt ~5 times fainter than other detections of z~ 7 galaxies. The result indicates that low L sub([CII]) in z~ 7 galaxies compared to the local counterparts might be caused by their low metallicities and/or feedback. The small velocity offset ([Delta] sub([nu])= (ProQuest: Formulae and/or non-USASCII text omitted)) between the Ly[alpha] and [CII] line is unusual, and may be indicative of ionizing photons escaping.
doi_str_mv 10.3847/2041-8213/836/1/L2
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subjects Feedback
Galaxies
Luminosity
Metallicity
Photons
Red shift
Spectroscopy
Texts
title ALMA [CII] 158 [mu]m Detection of a Redshift 7 Lensed Galaxy behind RX J1347.1?1145
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