Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies

Using the Planck 2015 data release (PR2) temperature maps, we separate Galactic thermal dust emission from cosmic infrared background (CIB) anisotropies. For this purpose, we implement a specifically tailored component-separation method, the so-called generalized needlet internal linear combination...

Full description

Bibliographic Details
Main Authors:	Aghanim, N., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A.J., Barreiro, R.B., Bartolo, N., Basak, S., Benabed, K., Bernard, J.-P., Bersanelli, M., Bielewicz, P., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Burigana, C., Calabrese, E., Cardoso, J.-F., Carron, J., Chiang, H.C., Colombo, L.P.L., Comis, B., Couchot, F., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., de Bernardis, P., de Zotti, G., Delabrouille, J., Di Valentino, E., Dickinson, C., Diego, J.M., Doré, O., Douspis, M., Ducout, A., Dupac, X., Dusini, S., Elsner, F., Enßlin, T.A., Eriksen, H.K., Falgarone, E., Fantaye, Y., Finelli, F., Forastieri, F., Frailis, M., Fraisse, A.A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Génova-Santos, R.T., Gerbino, M., Ghosh, T., Giraud-Héraud, Y., González-Nuevo, J., Górski, K.M., Gruppuso, A., Gudmundsson, J.E., Hansen, F.K., Helou, G., Henrot-Versillé, S., Herranz, D., Hivon, E., Huang, Z., Jaffe, A.H., Jones, W.C., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T.S., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lamarre, J.-M., Langer, M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Le Jeune, M., Levrier, F., Lilje, P.B., Lilley, M., Lindholm, V., López-Caniego, M., Ma, Y.-Z., Macías-Pérez, J.F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P.G., Martínez-González, E., Matarrese, S., Mauri, N., McEwen, J.D., Melchiorri, A., Mennella, A., Migliaccio, M., Miville-Deschênes, M.-A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Moss, A., Natoli, P., Oxborrow, C.A., Pagano, L., Paoletti, D., Patanchon, G., Perdereau, O., Perotto, L., Pettorino, V., Piacentini, F., Plaszczynski, S., Polastri, L., Polenta, G., Puget, J.-L., Rachen, J.P., Racine, B., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J.A., Ruiz-Granados, B., Salvati, L., Sandri, M., Savelainen, M., Scott, D., Sirignano, C., Sirri, G., Soler, J.D., Spencer, L.D., Suur-Uski, A.-S., Tauber, J.A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Valiviita, J., Van Tent, F., Vielva, P., Villa, F., Vittorio, N., Wandelt, B.D., Wehus, I.K., Zacchei, A., Zonca, A.
Format:	Article
Published:	EDP Sciences 2016
Subjects:	cosmology: observations; methods: data analysis; ISM: general; dust extinction; infrared: diffuse background; large-scale structure of Universe
Online Access:	https://eprints.nottingham.ac.uk/42448/

_version_	1848796489718956032
author	Aghanim, N. Ashdown, M. Aumont, J. Baccigalupi, C. Ballardini, M. Banday, A.J. Barreiro, R.B. Bartolo, N. Basak, S. Benabed, K. Bernard, J.-P. Bersanelli, M. Bielewicz, P. Bonavera, L. Bond, J.R. Borrill, J. Bouchet, F.R. Boulanger, F. Burigana, C. Calabrese, E. Cardoso, J.-F. Carron, J. Chiang, H.C. Colombo, L.P.L. Comis, B. Couchot, F. Coulais, A. Crill, B.P. Curto, A. Cuttaia, F. de Bernardis, P. de Zotti, G. Delabrouille, J. Di Valentino, E. Dickinson, C. Diego, J.M. Doré, O. Douspis, M. Ducout, A. Dupac, X. Dusini, S. Elsner, F. Enßlin, T.A. Eriksen, H.K. Falgarone, E. Fantaye, Y. Finelli, F. Forastieri, F. Frailis, M. Fraisse, A.A. Franceschi, E. Frolov, A. Galeotta, S. Galli, S. Ganga, K. Génova-Santos, R.T. Gerbino, M. Ghosh, T. Giraud-Héraud, Y. González-Nuevo, J. Górski, K.M. Gruppuso, A. Gudmundsson, J.E. Hansen, F.K. Helou, G. Henrot-Versillé, S. Herranz, D. Hivon, E. Huang, Z. Jaffe, A.H. Jones, W.C. Keihänen, E. Keskitalo, R. Kiiveri, K. Kisner, T.S. Krachmalnicoff, N. Kunz, M. Kurki-Suonio, H. Lamarre, J.-M. Langer, M. Lasenby, A. Lattanzi, M. Lawrence, C.R. Le Jeune, M. Levrier, F. Lilje, P.B. Lilley, M. Lindholm, V. López-Caniego, M. Ma, Y.-Z. Macías-Pérez, J.F. Maggio, G. Maino, D. Mandolesi, N. Mangilli, A. Maris, M. Martin, P.G. Martínez-González, E. Matarrese, S. Mauri, N. McEwen, J.D. Melchiorri, A. Mennella, A. Migliaccio, M. Miville-Deschênes, M.-A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Moss, A. Natoli, P. Oxborrow, C.A. Pagano, L. Paoletti, D. Patanchon, G. Perdereau, O. Perotto, L. Pettorino, V. Piacentini, F. Plaszczynski, S. Polastri, L. Polenta, G. Puget, J.-L. Rachen, J.P. Racine, B. Reinecke, M. Remazeilles, M. Renzi, A. Rocha, G. Rosset, C. Rossetti, M. Roudier, G. Rubiño-Martín, J.A. Ruiz-Granados, B. Salvati, L. Sandri, M. Savelainen, M. Scott, D. Sirignano, C. Sirri, G. Soler, J.D. Spencer, L.D. Suur-Uski, A.-S. Tauber, J.A. Tavagnacco, D. Tenti, M. Toffolatti, L. Tomasi, M. Tristram, M. Trombetti, T. Valiviita, J. Van Tent, F. Vielva, P. Villa, F. Vittorio, N. Wandelt, B.D. Wehus, I.K. Zacchei, A. Zonca, A.
author_facet	Aghanim, N. Ashdown, M. Aumont, J. Baccigalupi, C. Ballardini, M. Banday, A.J. Barreiro, R.B. Bartolo, N. Basak, S. Benabed, K. Bernard, J.-P. Bersanelli, M. Bielewicz, P. Bonavera, L. Bond, J.R. Borrill, J. Bouchet, F.R. Boulanger, F. Burigana, C. Calabrese, E. Cardoso, J.-F. Carron, J. Chiang, H.C. Colombo, L.P.L. Comis, B. Couchot, F. Coulais, A. Crill, B.P. Curto, A. Cuttaia, F. de Bernardis, P. de Zotti, G. Delabrouille, J. Di Valentino, E. Dickinson, C. Diego, J.M. Doré, O. Douspis, M. Ducout, A. Dupac, X. Dusini, S. Elsner, F. Enßlin, T.A. Eriksen, H.K. Falgarone, E. Fantaye, Y. Finelli, F. Forastieri, F. Frailis, M. Fraisse, A.A. Franceschi, E. Frolov, A. Galeotta, S. Galli, S. Ganga, K. Génova-Santos, R.T. Gerbino, M. Ghosh, T. Giraud-Héraud, Y. González-Nuevo, J. Górski, K.M. Gruppuso, A. Gudmundsson, J.E. Hansen, F.K. Helou, G. Henrot-Versillé, S. Herranz, D. Hivon, E. Huang, Z. Jaffe, A.H. Jones, W.C. Keihänen, E. Keskitalo, R. Kiiveri, K. Kisner, T.S. Krachmalnicoff, N. Kunz, M. Kurki-Suonio, H. Lamarre, J.-M. Langer, M. Lasenby, A. Lattanzi, M. Lawrence, C.R. Le Jeune, M. Levrier, F. Lilje, P.B. Lilley, M. Lindholm, V. López-Caniego, M. Ma, Y.-Z. Macías-Pérez, J.F. Maggio, G. Maino, D. Mandolesi, N. Mangilli, A. Maris, M. Martin, P.G. Martínez-González, E. Matarrese, S. Mauri, N. McEwen, J.D. Melchiorri, A. Mennella, A. Migliaccio, M. Miville-Deschênes, M.-A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Moss, A. Natoli, P. Oxborrow, C.A. Pagano, L. Paoletti, D. Patanchon, G. Perdereau, O. Perotto, L. Pettorino, V. Piacentini, F. Plaszczynski, S. Polastri, L. Polenta, G. Puget, J.-L. Rachen, J.P. Racine, B. Reinecke, M. Remazeilles, M. Renzi, A. Rocha, G. Rosset, C. Rossetti, M. Roudier, G. Rubiño-Martín, J.A. Ruiz-Granados, B. Salvati, L. Sandri, M. Savelainen, M. Scott, D. Sirignano, C. Sirri, G. Soler, J.D. Spencer, L.D. Suur-Uski, A.-S. Tauber, J.A. Tavagnacco, D. Tenti, M. Toffolatti, L. Tomasi, M. Tristram, M. Trombetti, T. Valiviita, J. Van Tent, F. Vielva, P. Villa, F. Vittorio, N. Wandelt, B.D. Wehus, I.K. Zacchei, A. Zonca, A.
author_sort	Aghanim, N.
building	Nottingham Research Data Repository
collection	Online Access
description	Using the Planck 2015 data release (PR2) temperature maps, we separate Galactic thermal dust emission from cosmic infrared background (CIB) anisotropies. For this purpose, we implement a specifically tailored component-separation method, the so-called generalized needlet internal linear combination (GNILC) method, which uses spatial information (the angular powerspectra) to disentangle the Galactic dust emission and CIB anisotropies. We produce significantly improved all-sky maps of Planck thermal dust emission, with reduced CIB contamination, at 353, 545, and 857 GHz. By reducing the CIB contamination of the thermal dust maps, we provide more accurate estimates of the local dust temperature and dust spectral index over the sky with reduced dispersion, especially at high Galactic latitudes above b = ±20°. We find that the dust temperature is T = (19.4 ± 1.3) K and the dust spectral index is β = 1.6 ± 0.1 averaged over the whole sky, while T = (19.4 ± 1.5) K and β = 1.6 ± 0.2 on 21% of the sky at high latitudes. Moreover, subtracting the new CIB-removed thermal dust maps from the CMB-removed Planck maps gives access to the CIB anisotropies over 60% of the sky at Galactic latitudes \|b\| > 20°. Because they are a significant improvement over previous Planck products, the GNILC maps are recommended for thermal dust science. The new CIB maps can be regarded as indirect tracers of the dark matter and they are recommended for exploring cross-correlations with lensing and large-scale structure optical surveys. The reconstructed GNILC thermal dust and CIB maps are delivered as Planck products.
first_indexed	2025-11-14T19:48:48Z
format	Article
id	nottingham-42448
institution	University of Nottingham Malaysia Campus
institution_category	Local University
last_indexed	2025-11-14T19:48:48Z
publishDate	2016
publisher	EDP Sciences
recordtype	eprints
repository_type	Digital Repository
spelling	nottingham-424482020-05-04T18:26:22Z https://eprints.nottingham.ac.uk/42448/ Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies Aghanim, N. Ashdown, M. Aumont, J. Baccigalupi, C. Ballardini, M. Banday, A.J. Barreiro, R.B. Bartolo, N. Basak, S. Benabed, K. Bernard, J.-P. Bersanelli, M. Bielewicz, P. Bonavera, L. Bond, J.R. Borrill, J. Bouchet, F.R. Boulanger, F. Burigana, C. Calabrese, E. Cardoso, J.-F. Carron, J. Chiang, H.C. Colombo, L.P.L. Comis, B. Couchot, F. Coulais, A. Crill, B.P. Curto, A. Cuttaia, F. de Bernardis, P. de Zotti, G. Delabrouille, J. Di Valentino, E. Dickinson, C. Diego, J.M. Doré, O. Douspis, M. Ducout, A. Dupac, X. Dusini, S. Elsner, F. Enßlin, T.A. Eriksen, H.K. Falgarone, E. Fantaye, Y. Finelli, F. Forastieri, F. Frailis, M. Fraisse, A.A. Franceschi, E. Frolov, A. Galeotta, S. Galli, S. Ganga, K. Génova-Santos, R.T. Gerbino, M. Ghosh, T. Giraud-Héraud, Y. González-Nuevo, J. Górski, K.M. Gruppuso, A. Gudmundsson, J.E. Hansen, F.K. Helou, G. Henrot-Versillé, S. Herranz, D. Hivon, E. Huang, Z. Jaffe, A.H. Jones, W.C. Keihänen, E. Keskitalo, R. Kiiveri, K. Kisner, T.S. Krachmalnicoff, N. Kunz, M. Kurki-Suonio, H. Lamarre, J.-M. Langer, M. Lasenby, A. Lattanzi, M. Lawrence, C.R. Le Jeune, M. Levrier, F. Lilje, P.B. Lilley, M. Lindholm, V. López-Caniego, M. Ma, Y.-Z. Macías-Pérez, J.F. Maggio, G. Maino, D. Mandolesi, N. Mangilli, A. Maris, M. Martin, P.G. Martínez-González, E. Matarrese, S. Mauri, N. McEwen, J.D. Melchiorri, A. Mennella, A. Migliaccio, M. Miville-Deschênes, M.-A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Moss, A. Natoli, P. Oxborrow, C.A. Pagano, L. Paoletti, D. Patanchon, G. Perdereau, O. Perotto, L. Pettorino, V. Piacentini, F. Plaszczynski, S. Polastri, L. Polenta, G. Puget, J.-L. Rachen, J.P. Racine, B. Reinecke, M. Remazeilles, M. Renzi, A. Rocha, G. Rosset, C. Rossetti, M. Roudier, G. Rubiño-Martín, J.A. Ruiz-Granados, B. Salvati, L. Sandri, M. Savelainen, M. Scott, D. Sirignano, C. Sirri, G. Soler, J.D. Spencer, L.D. Suur-Uski, A.-S. Tauber, J.A. Tavagnacco, D. Tenti, M. Toffolatti, L. Tomasi, M. Tristram, M. Trombetti, T. Valiviita, J. Van Tent, F. Vielva, P. Villa, F. Vittorio, N. Wandelt, B.D. Wehus, I.K. Zacchei, A. Zonca, A. Using the Planck 2015 data release (PR2) temperature maps, we separate Galactic thermal dust emission from cosmic infrared background (CIB) anisotropies. For this purpose, we implement a specifically tailored component-separation method, the so-called generalized needlet internal linear combination (GNILC) method, which uses spatial information (the angular powerspectra) to disentangle the Galactic dust emission and CIB anisotropies. We produce significantly improved all-sky maps of Planck thermal dust emission, with reduced CIB contamination, at 353, 545, and 857 GHz. By reducing the CIB contamination of the thermal dust maps, we provide more accurate estimates of the local dust temperature and dust spectral index over the sky with reduced dispersion, especially at high Galactic latitudes above b = ±20°. We find that the dust temperature is T = (19.4 ± 1.3) K and the dust spectral index is β = 1.6 ± 0.1 averaged over the whole sky, while T = (19.4 ± 1.5) K and β = 1.6 ± 0.2 on 21% of the sky at high latitudes. Moreover, subtracting the new CIB-removed thermal dust maps from the CMB-removed Planck maps gives access to the CIB anisotropies over 60% of the sky at Galactic latitudes \|b\| > 20°. Because they are a significant improvement over previous Planck products, the GNILC maps are recommended for thermal dust science. The new CIB maps can be regarded as indirect tracers of the dark matter and they are recommended for exploring cross-correlations with lensing and large-scale structure optical surveys. The reconstructed GNILC thermal dust and CIB maps are delivered as Planck products. EDP Sciences 2016-12-12 Article PeerReviewed Aghanim, N., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A.J., Barreiro, R.B., Bartolo, N., Basak, S., Benabed, K., Bernard, J.-P., Bersanelli, M., Bielewicz, P., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Burigana, C., Calabrese, E., Cardoso, J.-F., Carron, J., Chiang, H.C., Colombo, L.P.L., Comis, B., Couchot, F., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., de Bernardis, P., de Zotti, G., Delabrouille, J., Di Valentino, E., Dickinson, C., Diego, J.M., Doré, O., Douspis, M., Ducout, A., Dupac, X., Dusini, S., Elsner, F., Enßlin, T.A., Eriksen, H.K., Falgarone, E., Fantaye, Y., Finelli, F., Forastieri, F., Frailis, M., Fraisse, A.A., Franceschi, E., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Génova-Santos, R.T., Gerbino, M., Ghosh, T., Giraud-Héraud, Y., González-Nuevo, J., Górski, K.M., Gruppuso, A., Gudmundsson, J.E., Hansen, F.K., Helou, G., Henrot-Versillé, S., Herranz, D., Hivon, E., Huang, Z., Jaffe, A.H., Jones, W.C., Keihänen, E., Keskitalo, R., Kiiveri, K., Kisner, T.S., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lamarre, J.-M., Langer, M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Le Jeune, M., Levrier, F., Lilje, P.B., Lilley, M., Lindholm, V., López-Caniego, M., Ma, Y.-Z., Macías-Pérez, J.F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P.G., Martínez-González, E., Matarrese, S., Mauri, N., McEwen, J.D., Melchiorri, A., Mennella, A., Migliaccio, M., Miville-Deschênes, M.-A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Moss, A., Natoli, P., Oxborrow, C.A., Pagano, L., Paoletti, D., Patanchon, G., Perdereau, O., Perotto, L., Pettorino, V., Piacentini, F., Plaszczynski, S., Polastri, L., Polenta, G., Puget, J.-L., Rachen, J.P., Racine, B., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J.A., Ruiz-Granados, B., Salvati, L., Sandri, M., Savelainen, M., Scott, D., Sirignano, C., Sirri, G., Soler, J.D., Spencer, L.D., Suur-Uski, A.-S., Tauber, J.A., Tavagnacco, D., Tenti, M., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Valiviita, J., Van Tent, F., Vielva, P., Villa, F., Vittorio, N., Wandelt, B.D., Wehus, I.K., Zacchei, A. and Zonca, A. (2016) Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies. Astronomy & Astrophysics, 596 . A109/1-A109/26. ISSN 1432-0746 cosmology: observations; methods: data analysis; ISM: general; dust extinction; infrared: diffuse background; large-scale structure of Universe http://www.aanda.org/articles/aa/abs/2016/12/aa29022-16/aa29022-16.html doi:10.1051/0004-6361/201629022 doi:10.1051/0004-6361/201629022
spellingShingle	cosmology: observations; methods: data analysis; ISM: general; dust extinction; infrared: diffuse background; large-scale structure of Universe Aghanim, N. Ashdown, M. Aumont, J. Baccigalupi, C. Ballardini, M. Banday, A.J. Barreiro, R.B. Bartolo, N. Basak, S. Benabed, K. Bernard, J.-P. Bersanelli, M. Bielewicz, P. Bonavera, L. Bond, J.R. Borrill, J. Bouchet, F.R. Boulanger, F. Burigana, C. Calabrese, E. Cardoso, J.-F. Carron, J. Chiang, H.C. Colombo, L.P.L. Comis, B. Couchot, F. Coulais, A. Crill, B.P. Curto, A. Cuttaia, F. de Bernardis, P. de Zotti, G. Delabrouille, J. Di Valentino, E. Dickinson, C. Diego, J.M. Doré, O. Douspis, M. Ducout, A. Dupac, X. Dusini, S. Elsner, F. Enßlin, T.A. Eriksen, H.K. Falgarone, E. Fantaye, Y. Finelli, F. Forastieri, F. Frailis, M. Fraisse, A.A. Franceschi, E. Frolov, A. Galeotta, S. Galli, S. Ganga, K. Génova-Santos, R.T. Gerbino, M. Ghosh, T. Giraud-Héraud, Y. González-Nuevo, J. Górski, K.M. Gruppuso, A. Gudmundsson, J.E. Hansen, F.K. Helou, G. Henrot-Versillé, S. Herranz, D. Hivon, E. Huang, Z. Jaffe, A.H. Jones, W.C. Keihänen, E. Keskitalo, R. Kiiveri, K. Kisner, T.S. Krachmalnicoff, N. Kunz, M. Kurki-Suonio, H. Lamarre, J.-M. Langer, M. Lasenby, A. Lattanzi, M. Lawrence, C.R. Le Jeune, M. Levrier, F. Lilje, P.B. Lilley, M. Lindholm, V. López-Caniego, M. Ma, Y.-Z. Macías-Pérez, J.F. Maggio, G. Maino, D. Mandolesi, N. Mangilli, A. Maris, M. Martin, P.G. Martínez-González, E. Matarrese, S. Mauri, N. McEwen, J.D. Melchiorri, A. Mennella, A. Migliaccio, M. Miville-Deschênes, M.-A. Molinari, D. Moneti, A. Montier, L. Morgante, G. Moss, A. Natoli, P. Oxborrow, C.A. Pagano, L. Paoletti, D. Patanchon, G. Perdereau, O. Perotto, L. Pettorino, V. Piacentini, F. Plaszczynski, S. Polastri, L. Polenta, G. Puget, J.-L. Rachen, J.P. Racine, B. Reinecke, M. Remazeilles, M. Renzi, A. Rocha, G. Rosset, C. Rossetti, M. Roudier, G. Rubiño-Martín, J.A. Ruiz-Granados, B. Salvati, L. Sandri, M. Savelainen, M. Scott, D. Sirignano, C. Sirri, G. Soler, J.D. Spencer, L.D. Suur-Uski, A.-S. Tauber, J.A. Tavagnacco, D. Tenti, M. Toffolatti, L. Tomasi, M. Tristram, M. Trombetti, T. Valiviita, J. Van Tent, F. Vielva, P. Villa, F. Vittorio, N. Wandelt, B.D. Wehus, I.K. Zacchei, A. Zonca, A. Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
title	Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
title_full	Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
title_fullStr	Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
title_full_unstemmed	Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
title_short	Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies
title_sort	planck intermediate results. xlviii. disentangling galactic dust emission and cosmic infrared background anisotropies
topic	cosmology: observations; methods: data analysis; ISM: general; dust extinction; infrared: diffuse background; large-scale structure of Universe
url	https://eprints.nottingham.ac.uk/42448/ https://eprints.nottingham.ac.uk/42448/ https://eprints.nottingham.ac.uk/42448/

Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies

Similar Items