Search for CII emission on cosmological scales at redshift Z ~ 2.6

Pullen, Anthony R.; Serra, Paolo; Chang, Tzu-Ching; Doré, Olivier; Ho, Shirley

doi:10.1093/mnras/sty1243

Title: Search for C_II emission on cosmological scales at redshift Z ~ 2.6

Journal Article · Mon May 14 00:00:00 EDT 2018 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/sty1243· OSTI ID:1492322

Pullen, Anthony R. ^[1]; Serra, Paolo ^[2]; Chang, Tzu-Ching ^[3]; Doré, Olivier ^[2]; Ho, Shirley ^[4]

New York Univ. (NYU), New York, NY (United States); Carnegie Mellon Univ., Pittsburgh, PA (United States)
California Inst. of Technology (CalTech), Pasadena, CA (United States)
California Inst. of Technology (CalTech), Pasadena, CA (United States); USA Academia Sinica Institute of Astronomy and Astrophysics, Taipei (Taiwan)
California Inst. of Technology (CalTech), Pasadena, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)

We present a search for C_II emission over cosmological scales at high redshifts. The C_II line is a prime candidate to be a tracer of star formation over large-scale structure since it is one of the brightest emission lines from galaxies. Redshifted C_II emission appears in the submillimeter regime, which means it could potentially be present in the higher frequency intensity data from the Planck satellite is used to measure the cosmic infrared background (CIB). We search for C_II emission over redshifts z = 2–3.2 in the Planck 545 GHz intensity map by cross-correlating the three highest frequency Planck maps with spectroscopic quasars and CMASS galaxies from the Sloan Digital Sky Survey III, which we then use to jointly fit C_II intensity, CIB parameters, and thermal Sunyaev–Zeldovich (SZ) emission. We report a measurement of an anomalous emission I_ν = 6.6^+5.0_–4.8 × 10⁴ Jy sr^–1 at 95 percent confidence, which could be explained by C_II emission, favouring collisional excitation models of C_II emission that tend to be more optimistic than models based on C_II luminosity scaling relations from local measurements; however, a comparison of Bayesian information criteria reveals that this model and the CIB & SZ model are equally plausible. Thus, more sensitive measurements will be needed to confirm the existence of a large-scale C_II emission at high redshifts. Lastly, we forecast that intensity maps from Planck cross-correlated with quasars from the Dark Energy Spectroscopic Instrument would increase our sensitivity to C_II emission by a factor of 5, while the proposed Primordial Inflation Explorer could increase the sensitivity further.

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Research Organization:: Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: AC02-05CH11231

OSTI ID:: 1492322

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 2; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 40 works

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On Removing Interloper Contamination from Intensity Mapping Power Spectrum Measurements Lidz, Adam; Taylor, Jessie The Astrophysical Journal, Vol. 825, Issue 2 https://doi.org/10.3847/0004-637X/825/2/143	journal	July 2016
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Planck 2013 results. XVI. Cosmological parameters Collaboration, Planck; Ade, P. A. R.; Aghanim, N. arXiv https://doi.org/10.48550/arxiv.1303.5076	text	January 2013
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Foreground contamination in Ly-alpha intensity mapping during the epoch of reionization Gong, Yan; Silva, Marta; Cooray, Asantha arXiv https://doi.org/10.48550/arxiv.1312.2035	text	January 2013
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Cross-correlation of cosmic far-infrared background anisotropies with large scale structures Serra, Paolo; Lagache, Guilaine; Doré, Olivier arXiv https://doi.org/10.48550/arxiv.1404.1933	text	January 2014
Planck 2015 results. XIII. Cosmological parameters Collaboration, Planck; Ade, P. A. R.; Aghanim, N. arXiv https://doi.org/10.48550/arxiv.1502.01589	text	January 2015
Connecting CO Intensity Mapping to Molecular Gas and Star Formation in the Epoch of Galaxy Assembly Li, Tony Y.; Wechsler, Risa H.; Devaraj, Kiruthika arXiv https://doi.org/10.48550/arxiv.1503.08833	text	January 2015
SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 12: galaxy target selection and large scale structure catalogues Reid, Beth; Ho, Shirley; Padmanabhan, Nikhil arXiv https://doi.org/10.48550/arxiv.1509.06529	preprint	January 2015
Spectral Line De-confusion in an Intensity Mapping Survey Cheng, Yun-Ting; Chang, Tzu-Ching; Bock, James arXiv https://doi.org/10.48550/arxiv.1604.07833	text	January 2016
COPSS II: The Molecular Gas Content of Ten Million Cubic Megaparsecs at $z\sim3$ Keating, Garrett K.; Marrone, Daniel P.; Bower, Geoffrey C. arXiv https://doi.org/10.48550/arxiv.1605.03971	text	January 2016
Dissecting the high-z interstellar medium through intensity mapping cross-correlations Serra, Paolo; Doré, Olivier; Lagache, Guilaine arXiv https://doi.org/10.48550/arxiv.1608.00585	text	January 2016
Relativistic distortions in the large-scale clustering of SDSS-III BOSS CMASS galaxies Alam, Shadab; Zhu, Hongyu; Croft, Rupert A. C. arXiv https://doi.org/10.48550/arxiv.1709.07855	text	January 2017
Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample Eisenstein, D. J.; Annis, J.; Gunn, J. E. arXiv https://doi.org/10.48550/arxiv.astro-ph/0108153	text	January 2001
Cosmological parameters from CMB and other data: a Monte-Carlo approach Lewis, Antony; Bridle, Sarah arXiv https://doi.org/10.48550/arxiv.astro-ph/0205436	text	January 2002
Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample Strauss, Michael A.; Weinberg, David H.; Lupton, Robert H. arXiv https://doi.org/10.48550/arxiv.astro-ph/0206225	text	January 2002
What Shapes the Luminosity Function of Galaxies? Benson, A. J.; Bower, R. G.; Frenk, C. S. arXiv https://doi.org/10.48550/arxiv.astro-ph/0302450	text	January 2003
Cross-correlation of CMB with large-scale structure: weak gravitational lensing Hirata, Christopher M.; Padmanabhan, Nikhil; Seljak, Uros arXiv https://doi.org/10.48550/arxiv.astro-ph/0406004	text	January 2004
The 2.5 m Telescope of the Sloan Digital Sky Survey Gunn, James E.; Siegmund, Walter A.; al, Edward J. Mannery et arXiv https://doi.org/10.48550/arxiv.astro-ph/0602326	text	January 2006
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79 ASTRONOMY AND ASTROPHYSICS
ISM: molecules
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Title: Search for CII emission on cosmological scales at redshift Z ~ 2.6

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