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Title: Shadow of colossus: A z = 2.44 galaxy protocluster detected in 3D Ly α forest tomographic mapping of the cosmos field

By using moderate-resolution optical spectra from 58 background Lyman-break galaxies and quasars at z ~ 2.3-3 within a 11'.5 × 13'.5 area of the COSMOS field (~1200 deg -2 projected area density or ~2.4 h -1 Mpc mean transverse separation), we reconstruct a 3D tomographic map of the foreground Lyα forest absorption at 2.2 < z < 2.5 with an effective smoothing scale of ϵ 3D ≈ 2.5 h -1 Mpc comoving. Comparing with 61 coeval galaxies with spectroscopic redshifts in the same volume, we find that the galaxy positions are clearly biased toward regions with enhanced intergalactic medium (IGM) absorption in the tomographic map. Here, we find an extended IGM overdensity with deep absorption troughs at z = 2.45 associated with a recently discovered galaxy protocluster at the same redshift. Based on simulations matched to our data, we estimate the enclosed dark matter mass within this IGM overdensity to be M dm (z= 2.45) = (1.1 ± 0.6) ×10 14 h -1 M ⊙ , and argue based on this mass and absorption strength that it will form at least one z ~ 0 galaxy cluster with M(z = 0) = (3 ± 1.5) ×10 14h -1 M more » , although its elongated nature suggests that it will likely collapse into two separate clusters. We also point out a compact overdensity of six MOSDEF galaxies at z = 2.30 within a r ~ 1 h -1 Mpc radius and Δz ~ 0.006, which does not appear to have a large associated IGM overdensity. Our results demonstrate the potential of Lyα forest tomography on larger volumes to study galaxy properties as a function of environment, as well as revealing the large-scale IGM overdensities associated with protoclusters or other features of large-scale structure.« less
Authors:
ORCiD logo [1] ;  [1] ; ORCiD logo [2] ; ORCiD logo [3] ;  [4] ;  [4] ;  [5] ;  [6] ; ORCiD logo [2] ; ORCiD logo [7] ;  [4] ; ORCiD logo [8] ; ORCiD logo [9]
  1. Max Planck Inst. for Astronomy, Heidelberg (Germany)
  2. Univ. of California, Berkeley, CA (United States). Dept. of Astronomy; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  3. Univ. of California, Santa Cruz, CA (United States). Dept. of Astronomy and Astrophysics; Univ. of California Observatories, Santa Cruz, CA (United States)
  4. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  5. Univ. of California, Los Angeles, CA (United States). Dept. of Physics and Astronomy
  6. Univ. of Tokyo (Japan). Kavli Inst. for the Physics and Mathematics of the Universe (IPMU)
  7. Aix-Marseille Univ., Marseille (France)
  8. Max Planck Inst. for Extraterrestrial Physics, Munich (Germany)
  9. National Inst. of Astrophysics (INAF), Bologna (Italy). Astronomical Observatory of Bologna
Publication Date:
Grant/Contract Number:
AC02-05CH11231
Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 817; Journal Issue: 2; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Research Org:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org:
USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR) (SC-21)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations; galaxies: high red-shift; intergalactic medium; quasars: absorption lines; galaxies: clusters: general; techniques: spectroscopic
OSTI Identifier:
1379068

Lee, Khee-Gan, Hennawi, Joseph F., White, Martin, Prochaska, J. Xavier, Font-Ribera, Andreu, Schlegel, David J., Rich, R. Michael, Suzuki, Nao, Stark, Casey W., Fèvre, Olivier Le, Nugent, Peter E., Salvato, Mara, and Zamorani, Gianni. Shadow of colossus: A z = 2.44 galaxy protocluster detected in 3D Lyα forest tomographic mapping of the cosmos field. United States: N. p., Web. doi:10.3847/0004-637X/817/2/160.
Lee, Khee-Gan, Hennawi, Joseph F., White, Martin, Prochaska, J. Xavier, Font-Ribera, Andreu, Schlegel, David J., Rich, R. Michael, Suzuki, Nao, Stark, Casey W., Fèvre, Olivier Le, Nugent, Peter E., Salvato, Mara, & Zamorani, Gianni. Shadow of colossus: A z = 2.44 galaxy protocluster detected in 3D Lyα forest tomographic mapping of the cosmos field. United States. doi:10.3847/0004-637X/817/2/160.
Lee, Khee-Gan, Hennawi, Joseph F., White, Martin, Prochaska, J. Xavier, Font-Ribera, Andreu, Schlegel, David J., Rich, R. Michael, Suzuki, Nao, Stark, Casey W., Fèvre, Olivier Le, Nugent, Peter E., Salvato, Mara, and Zamorani, Gianni. 2016. "Shadow of colossus: A z = 2.44 galaxy protocluster detected in 3D Lyα forest tomographic mapping of the cosmos field". United States. doi:10.3847/0004-637X/817/2/160. https://www.osti.gov/servlets/purl/1379068.
@article{osti_1379068,
title = {Shadow of colossus: A z = 2.44 galaxy protocluster detected in 3D Lyα forest tomographic mapping of the cosmos field},
author = {Lee, Khee-Gan and Hennawi, Joseph F. and White, Martin and Prochaska, J. Xavier and Font-Ribera, Andreu and Schlegel, David J. and Rich, R. Michael and Suzuki, Nao and Stark, Casey W. and Fèvre, Olivier Le and Nugent, Peter E. and Salvato, Mara and Zamorani, Gianni},
abstractNote = {By using moderate-resolution optical spectra from 58 background Lyman-break galaxies and quasars at z ~ 2.3-3 within a 11'.5 × 13'.5 area of the COSMOS field (~1200 deg -2 projected area density or ~2.4 h -1 Mpc mean transverse separation), we reconstruct a 3D tomographic map of the foreground Lyα forest absorption at 2.2 < z < 2.5 with an effective smoothing scale of ϵ3D ≈ 2.5 h -1 Mpc comoving. Comparing with 61 coeval galaxies with spectroscopic redshifts in the same volume, we find that the galaxy positions are clearly biased toward regions with enhanced intergalactic medium (IGM) absorption in the tomographic map. Here, we find an extended IGM overdensity with deep absorption troughs at z = 2.45 associated with a recently discovered galaxy protocluster at the same redshift. Based on simulations matched to our data, we estimate the enclosed dark matter mass within this IGM overdensity to be Mdm (z= 2.45) = (1.1 ± 0.6) ×10 14 h -1 M ⊙ , and argue based on this mass and absorption strength that it will form at least one z ~ 0 galaxy cluster with M(z = 0) = (3 ± 1.5) ×10 14h-1 M⊙ , although its elongated nature suggests that it will likely collapse into two separate clusters. We also point out a compact overdensity of six MOSDEF galaxies at z = 2.30 within a r ~ 1 h -1 Mpc radius and Δz ~ 0.006, which does not appear to have a large associated IGM overdensity. Our results demonstrate the potential of Lyα forest tomography on larger volumes to study galaxy properties as a function of environment, as well as revealing the large-scale IGM overdensities associated with protoclusters or other features of large-scale structure.},
doi = {10.3847/0004-637X/817/2/160},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 817,
place = {United States},
year = {2016},
month = {1}
}