%0 Generic %1 guaita2016limits %A Guaita, L. %A Pentericci, L. %A Grazian, A. %A Vanzella, E. %A Nonino, M. %A Giavalisco, M. %A Zamorani, G. %A Bongiorno, A. %A Cassata, P. %A Castellano, M. %A Garilli, B. %A Gawiser, E. %A Brun, V. Le %A Fevre, O. Le %A Lemaux, B. C. %A Maccagni, D. %A Merlin, E. %A Santini, P. %A Tasca, L. A. M. %A Thomas, R. %A Zucca, E. %A De Barros, S. %A Hathi, N. P. %A Amorin, R. %A Bardelli, S. %A Fontana, A. %D 2016 %K emission galaxy high-z ionisation lyc %T Limits on the LyC signal from z~3 sources with secure redshift and HST coverage in the E-CDFS field %U http://arxiv.org/abs/1601.03057 %X Aim: We aim to measure the LyC signal from a sample of sources in the Chandra deep field south. We collect star-forming galaxies (SFGs) and active galactic nuclei (AGN) with accurate spectroscopic redshifts, for which Hubble Space Telescope (HST) coverage and multi-wavelength photometry are available. Method: We selected a sample of about 200 sources at z~3. Taking advantage of HST resolution, we applied a careful cleaning procedure and rejected sources showing nearby clumps with different colours, which could be lower-z interlopers. Our clean sample consisted of 86 SFGs (including 19 narrow-band selected Lya emitters) and 8 AGN (including 6 detected in X-rays). We measured the LyC flux from aperture photometry in four narrow-band filters covering wavelengths below a 912 A rest frame (3.11<z<3.53). We estimated the ratio between ionizing (LyC flux) and 1400 A non-ionizing emissions for AGN and galaxies. Results: By running population synthesis models, we assume an average intrinsic L(1400 A)/L(900 A) ratio of 5 as the representative value for our sample. With this value and an average treatment of the lines of sight of the inter-galactic medium, we estimate the LyC escape fraction relative to the intrinsic value (fesc_rel(LyC)). We do not directly detect ionizing radiation from any individual SFG, but we are able to set a 1(2)sigma upper limit of fesc_rel(LyC)<12(24)%. This result is consistent with other non-detections published in the literature. No meaningful limits can be calculated for the sub-sample of Lya emitters. We obtain one significant direct detection for an AGN at z=3.46, with fesc_rel(LyC) = (72+/-18)%. Conclusions: Our upper limit on fescrel(LyC) implies that the SFGs studied here do not present either the physical properties or the geometric conditions suitable for efficient LyC-photon escape.

@misc{guaita2016limits, abstract = {Aim: We aim to measure the LyC signal from a sample of sources in the Chandra deep field south. We collect star-forming galaxies (SFGs) and active galactic nuclei (AGN) with accurate spectroscopic redshifts, for which Hubble Space Telescope (HST) coverage and multi-wavelength photometry are available. Method: We selected a sample of about 200 sources at z~3. Taking advantage of HST resolution, we applied a careful cleaning procedure and rejected sources showing nearby clumps with different colours, which could be lower-z interlopers. Our clean sample consisted of 86 SFGs (including 19 narrow-band selected Lya emitters) and 8 AGN (including 6 detected in X-rays). We measured the LyC flux from aperture photometry in four narrow-band filters covering wavelengths below a 912 A rest frame (3.11<z<3.53). We estimated the ratio between ionizing (LyC flux) and 1400 A non-ionizing emissions for AGN and galaxies. Results: By running population synthesis models, we assume an average intrinsic L(1400 A)/L(900 A) ratio of 5 as the representative value for our sample. With this value and an average treatment of the lines of sight of the inter-galactic medium, we estimate the LyC escape fraction relative to the intrinsic value (fesc_rel(LyC)). We do not directly detect ionizing radiation from any individual SFG, but we are able to set a 1(2)sigma upper limit of fesc_rel(LyC)<12(24)%. This result is consistent with other non-detections published in the literature. No meaningful limits can be calculated for the sub-sample of Lya emitters. We obtain one significant direct detection for an AGN at z=3.46, with fesc_rel(LyC) = (72+/-18)%. Conclusions: Our upper limit on fescrel(LyC) implies that the SFGs studied here do not present either the physical properties or the geometric conditions suitable for efficient LyC-photon escape.}, added-at = {2016-01-14T10:25:34.000+0100}, author = {Guaita, L. and Pentericci, L. and Grazian, A. and Vanzella, E. and Nonino, M. and Giavalisco, M. and Zamorani, G. and Bongiorno, A. and Cassata, P. and Castellano, M. and Garilli, B. and Gawiser, E. and Brun, V. Le and Fevre, O. Le and Lemaux, B. C. and Maccagni, D. and Merlin, E. and Santini, P. and Tasca, L. A. M. and Thomas, R. and Zucca, E. and De Barros, S. and Hathi, N. P. and Amorin, R. and Bardelli, S. and Fontana, A.}, biburl = {https://www.bibsonomy.org/bibtex/27f47ff3959717d145897b4d4e07b3657/miki}, description = {[1601.03057] Limits on the LyC signal from z~3 sources with secure redshift and HST coverage in the E-CDFS field}, interhash = {f1108cb12b83d44585e75788f426dac4}, intrahash = {7f47ff3959717d145897b4d4e07b3657}, keywords = {emission galaxy high-z ionisation lyc}, note = {cite arxiv:1601.03057Comment: Accepted for publication in A&A on Jan 5th, 2016}, timestamp = {2016-01-14T10:26:25.000+0100}, title = {Limits on the LyC signal from z~3 sources with secure redshift and HST coverage in the E-CDFS field}, url = {http://arxiv.org/abs/1601.03057}, year = 2016 }