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An Extragalactic Spectroscopic Survey of the SSA22 Field

We present VLT VIMOS, Keck DEIMOS and Keck LRIS multi-object spectra of 367 sources in the field of the z ~ 3.09 protocluster SSA22. Sources are spectroscopically classified via template matching, allowing new identifications for 206 extragalactic sources, including 36 z > 2 Lyman-break galaxies (LBGs) and Lyman-α emitters (LAEs), 8 protocluster members, and 94 X-ray sources from the ~ 400 ks Chandra deep survey of SSA22. Additionally, in the area covered by our study, we have increased by ~ 4, 13, and 6 times the number of reliable redshifts of sources at 1.0 < z < 2.0, at z > 3.4, and with X-Ray emission, respectively. We compare our results with past spectroscopic surveys of SSA22 to investigate the completeness of the LBGs and the X-Ray properties of the new spectroscopically-classified sources in the SSA22 field.

preprint2015arXivOpen access
C. SaezB. D. LehmerF. E. BauerD. SternA. GonzalesI. RrezaD. M. AlexanderY. MatsudaJ. E. GeachF. A. HarrisonT. Havashino
astro-ph.GA
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Open access11 authors1 topic
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C. SaezB. D. LehmerF. E. BauerD. SternA. GonzalesI. RrezaD. M. AlexanderY. MatsudaJ. E. GeachF. A. HarrisonT. Havashino

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