Planck intermediate results: XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies

Abergel, A.; Ade, P. A.  R.; Aghanim, N.; Alves, M. I.  R.; Aniano, G.; Arnaud, M.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Bartlett, J. G.; Battaner, E.; Benabed, K.; Benoit-Lévy, A.; Bernard, J. -P.; Bersanelli, M.; Bielewicz, P.; Bobin, J.; Bonaldi, A.; Bond, J. R.; Bouchet, F. R.; Boulanger, F.; Burigana, C.; Cardoso, J. -F.; Catalano, A.; Chamballu, A.; Chiang, H. C.; Christensen, P. R.; Clements, D. L.; Colombi, S.; Colombo, L. P.  L.; Couchot, F.; Crill, B. P.; Cuttaia, F.; Danese, L.; Davis, R. J.; de Bernardis, P.; de Rosa, A.; de Zotti, G.; Delabrouille, J.; Désert, F. -X.; Dickinson, C.; Diego, J. M.; Dole, H.; Donzelli, S.; Doré, O.; Douspis, M.; Dupac, X.; Efstathiou, G.; Enßlin, T. A.; Eriksen, H. K.; Falgarone, E.; Finelli, F.; Forni, O.; Frailis, M.; Franceschi, E.; Galeotta, S.; Ganga, K.; Ghosh, T.; Giard, M.; Giraud-Héraud, Y.; González-Nuevo, J.; Górski, K. M.; Gregorio, A.; Gruppuso, A.; Guillet, V.; Hansen, F. K.; Harrison, D.; Helou, G.; Henrot-Versillé, S.; Hernández-Monteagudo, C.; Herranz, D.; Hildebrandt, S. R.; Hivon, E.; Hobson, M.; Holmes, W. A.; Hornstrup, A.; Hovest, W.; Huffenberger, K. M.; Jaffe, A. H.; Jaffe, T. R.; Joncas, G.; Jones, A.; Jones, W. C.; Juvela, M.; Kalberla, P.; Keihänen, E.; Kerp, J.; Keskitalo, R.; Kisner, T. S.; Kneissl, R.; Knoche, J.; Kunz, M.; Kurki-Suonio, H.; Lagache, G.; Lähteenmäki, A.; Lamarre, J. -M.; Lasenby, A.; Lawrence, C. R.; Leonardi, R.; Levrier, F.; Liguori, M.; Lilje, P. B.; Linden-Vørnle, M.; López-Caniego, M.; Lubin, P. M.; Macías-Pérez, J. F.; Maffei, B.; Maino, D.; Mandolesi, N.; Maris, M.; Marshall, D. J.; Martin, P. G.; Martínez-González, E.; Masi, S.; Massardi, M.; Matarrese, S.; Mazzotta, P.; Melchiorri, A.; Mendes, L.; Mennella, A.; Migliaccio, M.; Mitra, S.; Miville-Deschênes, M. -A.; Moneti, A.; Montier, L.; Morgante, G.; Mortlock, D.; Munshi, D.; Murphy, J. A.; Naselsky, P.; Nati, F.; Natoli, P.; Noviello, F.; Novikov, D.; Novikov, I.; Oxborrow, C. A.; Pagano, L.; Pajot, F.; Paoletti, D.; Pasian, F.; Perdereau, O.; Perotto, L.; Perrotta, F.; Piacentini, F.; Piat, M.; Pierpaoli, E.; Pietrobon, D.; Plaszczynski, S.; Pointecouteau, E.; Polenta, G.; Ponthieu, N.; Popa, L.; Pratt, G. W.; Prunet, S.; Puget, J. -L.; Rachen, J. P.; Reach, W. T.; Rebolo, R.; Reinecke, M.; Remazeilles, M.; Renault, C.; Ricciardi, S.; Riller, T.; Ristorcelli, I.; Rocha, G.; Rosset, C.; Roudier, G.; Rusholme, B.; Sandri, M.; Savini, G.; Spencer, L. D.; Starck, J. -L.; Sureau, F.; Sutton, D.; Suur-Uski, A. -S.; Sygnet, J. -F.; Tauber, J. A.; Terenzi, L.; Toffolatti, L.; Tomasi, M.; Tristram, M.; Tucci, M.; Umana, G.; Valenziano, L.; Valiviita, J.; Van Tent, B.; Verstraete, L.; Vielva, P.; Villa, F.; Wade, L. A.; Wandelt, B. D.; Winkel, B.; Yvon, D.; Zacchei, A.; Zonca, A.

doi:10.1051/0004-6361/201323270

Planck intermediate results: XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies

Journal Article · Wed Jun 11 00:00:00 EDT 2014 · Astronomy and Astrophysics

DOI:https://doi.org/10.1051/0004-6361/201323270· OSTI ID:1523888

Abergel, A.; Ade, P. A. R.; Aghanim, N.; Alves, M. I. R.; Aniano, G.; Arnaud, M.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Bartlett, J. G.; Battaner, E.; Benabed, K.; Benoit-Lévy, A.; Bernard, J. -P.; Bersanelli, M.; Bielewicz, P.; Bobin, J.; Bonaldi, A. more »

The dust-Hi correlation is used to characterize the emission properties of dust in the diffuse interstellar medium (ISM) from far infrared wavelengths to microwave frequencies. The field of this encompasses the part of the southern sky best suited to study the cosmic infrared and microwave backgrounds. We cross-correlate sky maps from Planck, the Wilkinson Microwave Anisotropy Probe (WMAP), and the diffuse infrared background experiment (DIRBE), at 17 frequencies from 23 to 3000 GHz, with the Parkes survey of the 21 cm line emission of neutral atomic hydrogen, over a contiguous area of 7500 deg² centred on the southern Galactic pole. We present a general methodology to study the dust-Hi correlation over the sky, including simulations to quantify uncertainties. Our analysis yields four specific results. (1) We map the temperature, submillimetre emissivity, and opacity of the dust per H-atom. The dust temperature is observed to be anti-correlated with the dust emissivity and opacity. We interpret this result as evidence of dust evolution within the diffuse ISM. The mean dust opacity is measured to be (7.1 ± 0.6) × 10^-27 cm² H^-1 × (v/353 GHz)^{1.53 ± 0.03} for 100 ≤ v ≤ 353 GHz. This is a reference value to estimate hydrogen column densities from dust emission at submillimetre and millimetre wavelengths. (2) We map the spectral index β_mm of dust emission at millimetre wavelengths (defined here as v ≤ 353 GHz), and find it to be remarkably constant at β_mm = 1.51 ± 0.13. We compare it with the far infrared spectral index β_FIR derived from greybody fits at higher frequencies, and find a systematic difference, β_mm -β_FIR = -0.15, which suggests that the dust spectral energy distribution (SED) flattens at v ≤ 353 GHz. (3) We present spectral fits of the microwave emission correlated with Hi from 23 to 353 GHz, which separate dust and anomalous microwave emission (AME). We show that the flattening of the dust SED can be accounted for with an additional component with a blackbody spectrum. This additional component, which accounts for (26 ± 6)% of the dust emission at 100GHz, could represent magnetic dipole emission. Alternatively, it could account for an increasing contribution of carbon dust, or a flattening of the emissivity of amorphous silicates, at millimetre wavelengths. These interpretations make different predictions for the dust polarization SED. (4) We analyse the residuals of the dust-Hi correlation. We identify a Galactic contribution to these residuals, which we model with variations of the dust emissivity on angular scales smaller than that of our correlation analysis. This model of the residuals is used to quantify uncertainties of the CIB power spectrum in a companion Planck paper.

View Accepted Manuscript (DOE)

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

Sponsoring Organization:: USDOE

Contributing Organization:: Planck Collaboration

Grant/Contract Number:: AC02-05CH11231

OSTI ID:: 1523888

Journal Information:: Astronomy and Astrophysics, Journal Name: Astronomy and Astrophysics Vol. 566; ISSN 0004-6361

Publisher:: EDP SciencesCopyright Statement

Country of Publication:: United States

Language:: English

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Optimistic estimation on probing primordial gravitational waves with CMB B-mode polarization Huang, Qing-Guo; Wang, Sai Monthly Notices of the Royal Astronomical Society, Vol. 483, Issue 2 https://doi.org/10.1093/mnras/sty3262	journal	November 2018
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Fractal statistics in young star clusters: structural parameters and dynamical evolution Hetem, Annibal; Gregorio-Hetem, Jane Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 2 https://doi.org/10.1093/mnras/stz2698	journal	October 2019
How much graphene in space? Li, Qi; Li, Aigen; Jiang, B. W. Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 3 https://doi.org/10.1093/mnras/stz2740	journal	October 2019
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CMB internal delensing with general optimal estimator for higher-order correlations Namikawa, Toshiya Physical Review D, Vol. 95, Issue 10 https://doi.org/10.1103/physrevd.95.103514	journal	May 2017
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The link Between Turbulence, Magnetic Fields, Filaments, and star Formation in the Central Molecular zone Cloud G0.253+0.016 Federrath, C.; Rathborne, J. M.; Longmore, S. N. The Astrophysical Journal, Vol. 832, Issue 2 https://doi.org/10.3847/0004-637x/832/2/143	journal	November 2016
DISSECTING THE HIGH- z INTERSTELLAR MEDIUM THROUGH INTENSITY MAPPING CROSS-CORRELATIONS Serra, Paolo; Doré, Olivier; Lagache, Guilaine The Astrophysical Journal, Vol. 833, Issue 2 https://doi.org/10.3847/1538-4357/833/2/153	journal	December 2016
SEARCHING FOR FOSSIL EVIDENCE OF AGN FEEDBACK IN WISE -SELECTED STRIPE-82 GALAXIES BY MEASURING THE THERMAL SUNYAEV–ZEL’DOVICH EFFECT WITH THE ATACAMA COSMOLOGY TELESCOPE Spacek, Alexander; Scannapieco, Evan; Cohen, Seth The Astrophysical Journal, Vol. 834, Issue 2 https://doi.org/10.3847/1538-4357/834/2/102	journal	January 2017
Planck Lensing and Cosmic Infrared Background Cross-correlation with Fermi -LAT: Tracing Dark Matter Signals in the Gamma-Ray Background Feng, Chang; Cooray, Asantha; Keating, Brian The Astrophysical Journal, Vol. 836, Issue 1 https://doi.org/10.3847/1538-4357/836/1/127	journal	February 2017
Modeling the Anomalous Microwave Emission with Spinning Nanoparticles: No PAHs Required Hensley, Brandon S.; Draine, B. T. The Astrophysical Journal, Vol. 836, Issue 2 https://doi.org/10.3847/1538-4357/aa5c37	journal	February 2017
The Fraction of Cool-core Clusters in X-Ray versus SZ Samples Using Chandra Observations Andrade-Santos, Felipe; Jones, Christine; Forman, William R. The Astrophysical Journal, Vol. 843, Issue 1 https://doi.org/10.3847/1538-4357/aa7461	journal	July 2017
X-Ray Morphological Analysis of the Planck ESZ Clusters Lovisari, Lorenzo; Forman, William R.; Jones, Christine The Astrophysical Journal, Vol. 846, Issue 1 https://doi.org/10.3847/1538-4357/aa855f	journal	August 2017
On Graphene in the Interstellar Medium Chen, X. H.; Li, Aigen; Zhang, Ke The Astrophysical Journal, Vol. 850, Issue 1 https://doi.org/10.3847/1538-4357/aa93d5	journal	November 2017
Mitigating Complex Dust Foregrounds in Future Cosmic Microwave Background Polarization Experiments Hensley, Brandon S.; Bull, Philip The Astrophysical Journal, Vol. 853, Issue 2 https://doi.org/10.3847/1538-4357/aaa489	journal	January 2018
Simulating the Galaxy Cluster “El Gordo”: Gas Motion, Kinetic Sunyaev–Zel’dovich Signal, and X-Ray Line Features Zhang, Congyao; Yu, Qingjuan; Lu, Youjun The Astrophysical Journal, Vol. 855, Issue 1 https://doi.org/10.3847/1538-4357/aaab4c	journal	March 2018
First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud Ashton, Peter C.; Ade, Peter A. R.; Angilè, Francesco E. The Astrophysical Journal, Vol. 857, Issue 1 https://doi.org/10.3847/1538-4357/aab3ca	journal	April 2018
A New Detection of Extragalactic Anomalous Microwave Emission in a Compact, Optically Faint Region of NGC 4725 Murphy, E. J.; Linden, S. T.; Dong, D. The Astrophysical Journal, Vol. 862, Issue 1 https://doi.org/10.3847/1538-4357/aac5f5	journal	July 2018
Dust–Gas Scaling Relations and OH Abundance in the Galactic ISM Nguyen, Hiep; Dawson, J. R.; Miville-Deschênes, M. -A. The Astrophysical Journal, Vol. 862, Issue 1 https://doi.org/10.3847/1538-4357/aac82b	journal	July 2018
Developing the 3-point Correlation Function for the Turbulent Interstellar Medium Portillo, Stephen K. N.; Slepian, Zachary; Burkhart, Blakesley The Astrophysical Journal, Vol. 862, Issue 2 https://doi.org/10.3847/1538-4357/aacb80	journal	July 2018
Optically Thick H i Does Not Dominate Dark Gas in the Local ISM Murray, Claire E.; Peek, J. E. G.; Lee, Min-Young The Astrophysical Journal, Vol. 862, Issue 2 https://doi.org/10.3847/1538-4357/aaccfe	journal	July 2018
Diffuse X-Ray Emission from the Northern Arc of Loop I Observed with Suzaku Akita, Masahiro; Kataoka, Jun; Arimoto, Makoto The Astrophysical Journal, Vol. 862, Issue 1 https://doi.org/10.3847/1538-4357/aacd08	journal	July 2018
A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment’s Sample Variance Limited E-mode Measurement Watts, Duncan J.; Wang, Bingjie; Ali, Aamir The Astrophysical Journal, Vol. 863, Issue 2 https://doi.org/10.3847/1538-4357/aad283	journal	August 2018
Planck 2015 Constraints on the Non-flat ΛCDM Inflation Model Ooba, Junpei; Ratra, Bharat; Sugiyama, Naoshi The Astrophysical Journal, Vol. 864, Issue 1 https://doi.org/10.3847/1538-4357/aad633	journal	August 2018
Properties of the Inctracluster Medium Assuming an Einasto Dark Matter Profile Mirakhor, Mohammad S. The Astrophysical Journal, Vol. 866, Issue 2 https://doi.org/10.3847/1538-4357/aadf8b	journal	October 2018
Demonstration of Magnetic Field Tomography with Starlight Polarization toward a Diffuse Sightline of the ISM Panopoulou, Georgia V.; Tassis, Konstantinos; Skalidis, Raphael The Astrophysical Journal, Vol. 872, Issue 1 https://doi.org/10.3847/1538-4357/aafdb2	journal	February 2019
Ultraviolet HST Spectroscopy of Planck Cold Clumps Dirks, Cody; Meyer, David M. The Astrophysical Journal, Vol. 872, Issue 2 https://doi.org/10.3847/1538-4357/aaff5d	journal	February 2019
Magnetic Field Tomography in Two Clouds toward Ursa Major Using H i Fibers Tritsis, Aris; Federrath, Christoph; Pavlidou, Vasiliki The Astrophysical Journal, Vol. 873, Issue 1 https://doi.org/10.3847/1538-4357/ab037d	journal	March 2019
The Halo Mass of Optically Luminous Quasars at z ≈ 1–2 Measured via Gravitational Deflection of the Cosmic Microwave Background Geach, J. E.; Peacock, J. A.; Myers, A. D. The Astrophysical Journal, Vol. 874, Issue 1 https://doi.org/10.3847/1538-4357/ab0894	journal	March 2019
Determination of the Cosmic Infrared Background from COBE /FIRAS and Planck HFI Observations Odegard, N.; Weiland, J. L.; Fixsen, D. J. The Astrophysical Journal, Vol. 877, Issue 1 https://doi.org/10.3847/1538-4357/ab14e8	journal	May 2019
On-sky Performance of the CLASS Q -band Telescope Appel, John W.; Xu, Zhilei; Padilla, Ivan L. The Astrophysical Journal, Vol. 876, Issue 2 https://doi.org/10.3847/1538-4357/ab1652	journal	May 2019
Gas and Dust Properties in the Chamaeleon Molecular Cloud Complex Based on the Optically Thick H i Hayashi, Katsuhiro; Okamoto, Ryuji; Yamamoto, Hiroaki The Astrophysical Journal, Vol. 878, Issue 2 https://doi.org/10.3847/1538-4357/ab2051	journal	June 2019
Imaging the Thermal and Kinematic Sunyaev–Zel’dovich Effect Signals in a Sample of 10 Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities Sayers, Jack; Montaña, Alfredo; Mroczkowski, Tony The Astrophysical Journal, Vol. 880, Issue 1 https://doi.org/10.3847/1538-4357/ab29ef	journal	July 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 Hayashi, Katsuhiro; Mizuno, Tsunefumi; Fukui, Yasuo The Astrophysical Journal, Vol. 884, Issue 2 https://doi.org/10.3847/1538-4357/ab4351	journal	October 2019
2 mm GISMO Observations of the Galactic Center. I. Dust Emission Arendt, Richard G.; Staguhn, Johannes; Dwek, Eli The Astrophysical Journal, Vol. 885, Issue 1 https://doi.org/10.3847/1538-4357/ab451c	journal	November 2019
Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol Kable, Joshua A.; Addison, Graeme E.; Bennett, Charles L. The Astrophysical Journal, Vol. 888, Issue 1 https://doi.org/10.3847/1538-4357/ab54cc	journal	December 2019
Nonlinear Reconstruction of the Velocity Field Yu, Yu; Zhu, Hong-Ming The Astrophysical Journal, Vol. 887, Issue 2 https://doi.org/10.3847/1538-4357/ab5580	journal	December 2019
A Self-consistent Framework for Multiline Modeling in Line Intensity Mapping Experiments Sun, Guochao; Hensley, Brandon S.; Chang, Tzu-Ching The Astrophysical Journal, Vol. 887, Issue 2 https://doi.org/10.3847/1538-4357/ab55df	journal	December 2019
Predictions of Cosmic Microwave Background Foreground Dust Polarization Using Velocity Gradients Hu, Yue; Yuen, Ka Ho; Lazarian, A. The Astrophysical Journal, Vol. 888, Issue 2 https://doi.org/10.3847/1538-4357/ab60a5	journal	January 2020
A New Probe of Line-of-sight Magnetic Field Tangling Clark, S. E. The Astrophysical Journal, Vol. 857, Issue 1 https://doi.org/10.3847/2041-8213/aabb54	journal	April 2018
Violent Quenching: Molecular Gas Blown to 1000 km s ⁻¹ during a Major Merger Geach, J. E.; Tremonti, C.; Diamond-Stanic, A. M. The Astrophysical Journal, Vol. 864, Issue 1 https://doi.org/10.3847/2041-8213/aad8b6	journal	August 2018
Planck 2013 results. I. Overview of products and scientific results Collaboration, Planck; Ade, P. A. R.; Aghanim, N. arXiv https://doi.org/10.48550/arxiv.1303.5062	text	January 2013
Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes Collaboration, Planck; Adam, R.; Ade, P. A. R. arXiv https://doi.org/10.48550/arxiv.1409.5738	text	January 2014
A Joint Analysis of BICEP2/Keck Array and Planck Data Collaborations, Planck; Ade, P. A. R.; Aghanim, N. arXiv https://doi.org/10.48550/arxiv.1502.00612	text	January 2015
Planck 2015 results. X. Diffuse component separation: Foreground maps Collaboration, Planck; Adam, R.; Ade, P. A. R. arXiv https://doi.org/10.48550/arxiv.1502.01588	text	January 2015
Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds Collaboration, Planck; Ade, P. A. R.; Aghanim, N. arXiv https://doi.org/10.48550/arxiv.1506.06660	text	January 2015
Spinning dust emission from ultrasmall silicates: emissivity and polarization spectrum Hoang, Thiem; Vinh, Nguyen Anh; Lan, Nguyen Quynh arXiv https://doi.org/10.48550/arxiv.1603.05277	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
The Herschel Virgo Cluster Survey. XX. Dust and gas in the foreground Galactic cirrus Bianchi, S.; Giovanardi, C.; Smith, M. W. L. arXiv https://doi.org/10.48550/arxiv.1609.05941	text	January 2016
Dust models compatible with Planck intensity and polarization data in translucent lines of sight Guillet, V.; Fanciullo, L.; Verstraete, L. arXiv https://doi.org/10.48550/arxiv.1710.04598	text	January 2017
Dust-Gas Scaling Relations and OH Abundance in the Galactic ISM Nguyen, Hiep; Dawson, J. R.; Miville-Deschênes, M. -A. arXiv https://doi.org/10.48550/arxiv.1805.11787	text	January 2018
Optically thick HI does not dominate dark gas in the local ISM Murray, Claire E.; Peek, J. E. G.; Lee, Min-Young arXiv https://doi.org/10.48550/arxiv.1806.01300	text	January 2018
Gas and Dust Properties in the Chamaeleon Molecular Cloud Complex based on the Optically Thick HI Hayashi, Katsuhiro; Okamoto, Ryuji; Yamamoto, Hiroaki arXiv https://doi.org/10.48550/arxiv.1905.04184	text	January 2019
A Self-consistent Framework for Multiline Modeling in Line Intensity Mapping Experiments Sun, Guochao; Hensley, Brandon S.; Chang, Tzu-Ching arXiv https://doi.org/10.48550/arxiv.1907.02999	text	January 2019
The cosmic-ray content of the Orion-Eridanus superbubble Joubaud, T.; Grenier, I. A.; Casandjian, J. -M. arXiv https://doi.org/10.48550/arxiv.2001.10139	text	January 2020
Impact of Next-to-Leading Order Contributions to Cosmic Microwave Background Lensing Marozzi, Giovanni; Fanizza, Giuseppe; Di Dio, Enea American Physical Society https://doi.org/10.5167/uzh-148007	text	January 2017