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A Deep Narrow Band Imaging Search for CIVλ1548Å and HeIIλ1640Å Emission from Lyman Alpha Blobs

Published online by Cambridge University Press:  25 July 2014

Fabrizio Arrigoni Battaia ,
Y. Yang ,
J. F. Hennawi ,
Y. Matsuda ,
T. Yamada  and
T. Hayashino
Fabrizio Arrigoni Battaia
Affiliation:
Max-Planck-Institut für Astronomie Königstuhl 17, D-69117 Heidelberg, Germany email: arrigoni@mpia.de
Y. Yang
Affiliation:
Max-Planck-Institut für Astronomie Königstuhl 17, D-69117 Heidelberg, Germany email: arrigoni@mpia.de
J. F. Hennawi
Affiliation:
Max-Planck-Institut für Astronomie Königstuhl 17, D-69117 Heidelberg, Germany email: arrigoni@mpia.de
Y. Matsuda
Affiliation:
Max-Planck-Institut für Astronomie Königstuhl 17, D-69117 Heidelberg, Germany email: arrigoni@mpia.de
T. Yamada
Affiliation:
Max-Planck-Institut für Astronomie Königstuhl 17, D-69117 Heidelberg, Germany email: arrigoni@mpia.de
T. Hayashino
Affiliation:
Max-Planck-Institut für Astronomie Königstuhl 17, D-69117 Heidelberg, Germany email: arrigoni@mpia.de
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Abstract

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To study the nature of Lyα blobs (aka LABs), we conduct a deep C IV and He II narrowband imaging survey of 13 Lyα blobs located in SSA22 proto-cluster at z ~ 3.1. We reach the unprecedented sensitivity, 5σ surface brightness limit of 2.1 − 3.4 × 10−18 erg s−1 cm−2 arcsec−2 per 1 arcsec2 aperture for two emission lines. We do not detect any extended C IV and He II emission, placing strong upper limits on the He II/Lyα and C IV/Lyα line ratios. We compare our limits with data in the literature related to the nebulae associated with high-redshift radio galaxies (HzRGs) and quasars, and we recover the data by modeling the LABs as nebulosities powered by a central QSO. For further information see Arrigoni Battaia et al. (2014).

Keywords

LABQSOCGMphotoionization
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S304: Multiwavelength AGN Surveys and Studies , October 2013 , pp. 32 - 33
Copyright
Copyright © International Astronomical Union 2014 

References

Arrigoni Battaia, F., Yang, Y., Hennawi, J. F., et al. 2014, in prep.Google Scholar
Hayashino, T., Matsuda, Y., Tamura, H., et al. 2004, AJ, 128, 2073Google Scholar
Hennawi, J. F. & Prochaska, J. X. 2013, ApJ, 766, 58Google Scholar
Matsuda, Y., Yamada, T., Hayashino, T., et al. 2004, AJ, 128, 569Google Scholar
Prescott, M. K. M., Dey, A., & Jannuzi, B. T. 2013, ApJ, 762, 38Google Scholar
Steidel, C. C., Adelberger, K. L., Shapley, A. E., et al. 2000, ApJ, 532, 170Google Scholar
Yang, Y., Zabludoff, A., Tremonti, C., Eisenstein, D., & Davé, R. 2009, ApJ, 693, 1579Google Scholar