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Title: Planck intermediate results: XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel -SPIRE

Journal Article · · Astronomy and Astrophysics
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We have used the Planck all-sky submillimetre and millimetre maps to search for rare sources distinguished by extreme brightness, a few hundred millijanskies, and their potential for being situated at high redshift. These “cold” Planck sources, selected using the High Frequency Instrument (HFI) directly from the maps and from the Planck Catalogue of Compact Sources (PCCS), all satisfy the criterion of having their rest-frame far-infrared peak redshifted to the frequency range 353–857 GHz. This colour-selection favours galaxies in the redshift range z = 2–4, which we consider as cold peaks in the cosmic infrared background. With a 4'.5 beam at the four highest frequencies, our sample is expected to include overdensities of galaxies in groups or clusters, lensed galaxies, and chance line-of-sight projections. In this paper, we perform a dedicated Herschel-SPIRE follow-up of 234 such Planck targets, finding a significant excess of red 350 and 500μm sources, in comparison to reference SPIRE fields. About 94% of the SPIRE sources in the Planck fields are consistent with being overdensities of galaxies peaking at 350μm, with 3% peaking at 500μm, and none peaking at 250μm. About 3% are candidate lensed systems, all 12 of which have secure spectroscopic confirmations, placing them at redshifts z> 2.2. Only four targets are Galactic cirrus, yielding a success rate in our search strategy for identifying extragalactic sources within the Planck beam of better than 98%. The galaxy overdensities are detected with high significance, half of the sample showing statistical significance above 10σ. The SPIRE photometric redshifts of galaxies in overdensities suggest a peak at z ≃ 2, assuming a single common dust temperature for the sources of Td = 35 K. Under this assumption, we derive an infrared (IR) luminosity for each SPIRE source of about 4 × 1012L, yielding star formation rates of typically 700 M yr-1. If the observed overdensities are actual gravitationally-bound structures, the total IR luminosity of all their SPIRE-detected sources peaks at 4 × 1013L, leading to total star formation rates of perhaps 7 × 103M yr-1 per overdensity. Taken together, these sources show the signatures of high-z (z> 2) protoclusters of intensively star-forming galaxies. Finally, all these observations confirm the uniqueness of our sample compared to reference samples and demonstrate the ability of the all-skyPlanck-HFI cold sources to select populations of cosmological and astrophysical interest for structure formation studies.

Research Organization:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC)
Contributing Organization:
Planck Collaboration
Grant/Contract Number:
AC02-05CH11231
OSTI ID:
1392971
Journal Information:
Astronomy and Astrophysics, Vol. 582; ISSN 0004-6361
Publisher:
EDP SciencesCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 54 works
Citation information provided by
Web of Science

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Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-variable Horizontal-branch Stars. III. M55 and NGC 6362 journal July 2018
Developing the 3-point Correlation Function for the Turbulent Interstellar Medium journal July 2018
The Halo Mass of Optically Luminous Quasars at z ≈ 1–2 Measured via Gravitational Deflection of the Cosmic Microwave Background journal March 2019
Weak-lensing Mass Calibration of ACTPol Sunyaev–Zel’dovich Clusters with the Hyper Suprime-Cam Survey journal April 2019
Constraining the Neutral Fraction of Hydrogen in the IGM at Redshift 7.5 journal June 2019
Fermi -LAT γ -Ray Study of the Interstellar Medium and Cosmic Rays in the Chamaeleon Molecular Cloud Complex: A Look at the Dark Gas as Optically Thick H i journal October 2019
A Limit on the Warm Dark Matter Particle Mass from the Redshifted 21 cm Absorption Line journal May 2018
Planck 2013 results. XV. CMB power spectra and likelihood journal October 2014
Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust journal April 2015
Planck 2015 results : VI. LFI mapmaking journal September 2016
Statistical simulations of the dust foreground to cosmic microwave background polarization journal July 2017
The XXL Survey: XVII. X-ray and Sunyaev-Zel’dovich properties of the redshift 2.0 galaxy cluster XLSSC 122★★★ journal November 2018
Dust models compatible with Planck intensity and polarization data in translucent lines of sight journal February 2018
The supernova-regulated ISM: IV. A comparison of simulated polarization with Planck observations journal June 2018
Protostellar birth with ambipolar and ohmic diffusion journal July 2018
Far-infrared photometry of OJ 287 with the Herschel Space Observatory journal February 2018
A dynamically young, gravitationally stable network of filaments in Orion B journal April 2019
Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters journal January 2019
ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19 journal June 2019
Peak star formation efficiency and no missing baryons in massive spirals journal June 2019
Generalised uncertainty relations from superpositions of geometries journal July 2019
The impact of stellar feedback on hot gas in galaxy haloes: the Sunyaev–Zel'dovich effect and soft X-ray emission journal September 2016
Wide-field LOFAR-LBA power-spectra analyses: impact of calibration, polarization leakage, and ionosphere journal May 2018
X-ray and SZ constraints on the properties of hot CGM journal May 2018
The FABLE simulations: a feedback model for galaxies, groups, and clusters journal July 2018
Reionization in Technicolor journal July 2018
The C-Band All-Sky Survey (C-BASS): design and capabilities journal July 2018
Mapping stellar content to dark matter haloes – III. Environmental dependence and conformity of galaxy colours journal February 2018
SILCC-Zoom: Polarization and depolarization in molecular clouds journal October 2018
Polarization of seven MBM clouds at high Galactic latitude journal April 2018
Dark energy constraints from the thermal Sunyaev–Zeldovich power spectrum journal March 2018
Magnetic ionization–thermal instability journal May 2019
Observational effects of varying speed of light in quadratic gravity cosmological models journal April 2018
The Important Role of Cosmic-Ray Re-Acceleration journal April 2019
Practical Modeling of Large-Scale Galactic Magnetic Fields: Status and Prospects journal April 2019
Evolution of oh and Co-Dark Molecular gas Fraction Across a Molecular Cloud Boundary in Taurus journal February 2016
The Grism Lens-Amplified Survey from Space (Glass). vi. Comparing the mass and Light in macs J0416.1-2403 Using Frontier Field Imaging and Glass Spectroscopy journal November 2016
The Fraction of Cool-core Clusters in X-Ray versus SZ Samples Using Chandra Observations journal July 2017
Unlocking Sensitivity for Visibility-based Estimators of the 21 cm Reionization Power Spectrum journal January 2018
On the Faint End of the Galaxy Luminosity Function in the Epoch of Reionization: Updated Constraints from the HST Frontier Fields journal November 2018
E and B Polarizations from Inhomogeneous and Solar Surface Turbulence journal January 2019
Ultraviolet HST Spectroscopy of Planck Cold Clumps journal February 2019
Time Evolution of 3D Disk Formation with Misaligned Magnetic Field and Rotation Axes journal March 2019
Results from EDGES High-Band. III. New Constraints on Parameters of the Early Universe journal April 2019
The Far-infrared Polarization Spectrum of ρ Ophiuchi A from HAWC+/SOFIA Observations journal September 2019
Radiative Transfer with POLARIS. II. Modeling of Synthetic Galactic Synchrotron Observations journal October 2019
Large-scale Maps of the Cosmic Infrared Background from Planck journal September 2019
An Imprint of the Galactic Magnetic Field in the Diffuse Unpolarized Dust Emission journal December 2019
Mapping the Magnetic Interstellar Medium in Three Dimensions over the Full Sky with Neutral Hydrogen journal December 2019
Multiwavelength Polarimetry of the Filamentary Cloud IC 5146. II. Magnetic Field Structures journal December 2019
Beyond Optical Depth: Future Determination of Ionization History from the Cosmic Microwave Background journal January 2020
Identifying Direct Collapse Black Hole Seeds through Their Small Host Galaxies journal September 2018
Planck intermediate results : XXXIX. The journal December 2016
Planck ’s dusty GEMS: VI. Multi- J CO excitation and interstellar medium conditions in dusty starburst galaxies at z = 2–4 journal November 2018
Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates text January 2015
Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE text January 2017
PLCK G165.7+67.0: Analysis of a Massive Lensing Cluster in a Hubble Space Telescope Census of Submillimeter Giant Arcs Selected Using Planck/Herschel text January 2018
Planck's Dusty GEMS. VII. Atomic carbon and molecular gas in dusty starburst galaxies at z=2 to 4 text January 2018
CO, H2O, H2O+ line and dust emission in a z = 3.63 strongly lensed starburst merger at sub-kiloparsec scales text January 2019
The "Red Radio Ring": Ionised and Molecular Gas in a Starburst/Active Galactic Nucleus at $z \sim 2.55$ text January 2019