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Title: Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps

Abstract

Planck observations at 353 GHz provide the first fully sampled maps of the polarized dust emission towards interstellar filaments and their backgrounds (i.e., the emission observed in the surroundings of the filaments). The data allow us to determine the intrinsic polarization properties of the filaments and therefore to provide insight into the structure of their magnetic field (B). In this paper, we present the polarization maps of three nearby (several parsecs long) star-forming filaments of moderate column density (NH about 1022 cm-2): Musca, B211, and L1506. These three filaments are detected above the background in dust total and polarized emission. We use the spatial information to separate Stokes I, Q, and U of the filaments from those of their backgrounds, an essential step in measuring the intrinsic polarization fraction (p) and angle (ψ) of each emission component. We find that the polarization angles in the three filaments (ψfil) are coherent along their lengths and not the same as in their backgrounds (ψbg). The differences between ψfil and ψbg are 12° and 54° for Musca and L1506, respectively, and only 6° in the case of B211. These differences forMusca and L1506 are larger than the dispersions of ψ, both along themore » filaments and in their backgrounds. The observed changes of ψ are direct evidence of variations of the orientation of the plane of the sky (POS) projection of the magnetic field. As in previous studies, we find a decrease of several per cent in p with NH from the backgrounds to the crest of the filaments. We show that the bulk of the drop in p within the filaments cannot be explained by random fluctuations of the orientation of the magnetic field because they are too small (σψ< 10°). We recognize the degeneracy between the dust alignment efficiency (by, e.g., radiative torques) and the structure of the B-field in causing variations in p, but we argue that the decrease in p from the backgrounds to the filaments results in part from depolarization associated with the 3D structure of the B-field: both its orientation in the POS and with respect to the POS. We do not resolve the inner structure of the filaments, but at the smallest scales accessible with Planck (~0.2 pc), the observed changes of ψ and p hold information on the magnetic field structure within filaments. Finally, they show that both the mean field and its fluctuations in the filaments are different from those of their backgrounds, which points to a coupling between the matter and the B-field in the filament formation process.« less

Authors:
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Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
Contributing Org.:
Planck Collaboration
OSTI Identifier:
1393023
Grant/Contract Number:  
AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Astronomy and Astrophysics
Additional Journal Information:
Journal Volume: 586; Journal ID: ISSN 0004-6361
Publisher:
EDP Sciences
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; dust; extinction; ISM; magnetic fields; polarization; submillimeter

Citation Formats

Ade, P. A. R., Aghanim, N., Alves, M. I. R., Arnaud, M., Arzoumanian, D., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartolo, N., Battaner, E., Benabed, K., Benoit-Lévy, A., Bernard, J. -P., Berné, O., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bracco, A., Burigana, C., Calabrese, E., Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, H. C., Christensen, P. R., Clements, D. L., Colombi, S., Colombo, L. P. L., Combet, C., Couchot, F., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Ferrière, K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Ghosh, T., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Guillet, V., Hansen, F. K., Hanson, D., Harrison, D. L., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jones, W. C., Juvela, M., Keskitalo, R., Kisner, T. S., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., 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., Mandolesi, N., Mangilli, A., Maris, M., Martin, P. G., Martínez-González, E., Masi, S., 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., Nørgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., Oppermann, N., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Pasian, F., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Pratt, G. W., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ricciardi, S., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Savelainen, M., Savini, G., Scott, D., Soler, J. D., Stolyarov, V., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Yvon, D., Zacchei, A., and Zonca, A. Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps. United States: N. p., 2016. Web. doi:10.1051/0004-6361/201425305.
Ade, P. A. R., Aghanim, N., Alves, M. I. R., Arnaud, M., Arzoumanian, D., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartolo, N., Battaner, E., Benabed, K., Benoit-Lévy, A., Bernard, J. -P., Berné, O., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bracco, A., Burigana, C., Calabrese, E., Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, H. C., Christensen, P. R., Clements, D. L., Colombi, S., Colombo, L. P. L., Combet, C., Couchot, F., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Ferrière, K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Ghosh, T., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Guillet, V., Hansen, F. K., Hanson, D., Harrison, D. L., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jones, W. C., Juvela, M., Keskitalo, R., Kisner, T. S., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., 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., Mandolesi, N., Mangilli, A., Maris, M., Martin, P. G., Martínez-González, E., Masi, S., 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., Nørgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., Oppermann, N., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Pasian, F., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Pratt, G. W., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ricciardi, S., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Savelainen, M., Savini, G., Scott, D., Soler, J. D., Stolyarov, V., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Yvon, D., Zacchei, A., & Zonca, A. Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps. United States. https://doi.org/10.1051/0004-6361/201425305
Ade, P. A. R., Aghanim, N., Alves, M. I. R., Arnaud, M., Arzoumanian, D., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartolo, N., Battaner, E., Benabed, K., Benoit-Lévy, A., Bernard, J. -P., Berné, O., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., Bracco, A., Burigana, C., Calabrese, E., Cardoso, J. -F., Catalano, A., Chamballu, A., Chiang, H. C., Christensen, P. R., Clements, D. L., Colombi, S., Colombo, L. P. L., Combet, C., Couchot, F., Crill, B. P., Curto, A., Cuttaia, F., Danese, L., Davies, R. D., Davis, R. J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J. M., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Ferrière, K., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Ghosh, T., Giard, M., Giraud-Héraud, Y., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Guillet, V., Hansen, F. K., Hanson, D., Harrison, D. L., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jones, W. C., Juvela, M., Keskitalo, R., Kisner, T. S., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., 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., Mandolesi, N., Mangilli, A., Maris, M., Martin, P. G., Martínez-González, E., Masi, S., 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., Nørgaard-Nielsen, H. U., Noviello, F., Novikov, D., Novikov, I., Oppermann, N., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Pasian, F., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Pratt, G. W., Puget, J. -L., Rachen, J. P., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ricciardi, S., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Savelainen, M., Savini, G., Scott, D., Soler, J. D., Stolyarov, V., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Yvon, D., Zacchei, A., and Zonca, A. Tue . "Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps". United States. https://doi.org/10.1051/0004-6361/201425305. https://www.osti.gov/servlets/purl/1393023.
@article{osti_1393023,
title = {Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps},
author = {Ade, P. A. R. and Aghanim, N. and Alves, M. I. R. and Arnaud, M. and Arzoumanian, D. and Aumont, J. and Baccigalupi, C. and Banday, A. J. and Barreiro, R. B. and Bartolo, N. and Battaner, E. and Benabed, K. and Benoit-Lévy, A. and Bernard, J. -P. and Berné, O. and Bersanelli, M. and Bielewicz, P. and Bonaldi, A. and Bonavera, L. and Bond, J. R. and Borrill, J. and Bouchet, F. R. and Boulanger, F. and Bracco, A. and Burigana, C. and Calabrese, E. and Cardoso, J. -F. and Catalano, A. and Chamballu, A. and Chiang, H. C. and Christensen, P. R. and Clements, D. L. and Colombi, S. and Colombo, L. P. L. and Combet, C. and Couchot, F. and Crill, B. P. and Curto, A. and Cuttaia, F. and Danese, L. and Davies, R. D. and Davis, R. J. and de Bernardis, P. and de Rosa, A. and de Zotti, G. and Delabrouille, J. and Dickinson, C. and Diego, J. M. and Donzelli, S. and Doré, O. and Douspis, M. and Ducout, A. and Dupac, X. and Elsner, F. and Enßlin, T. A. and Eriksen, H. K. and Falgarone, E. and Ferrière, K. and Finelli, F. and Forni, O. and Frailis, M. and Fraisse, A. A. and Franceschi, E. and Frejsel, A. and Galeotta, S. and Galli, S. and Ganga, K. and Ghosh, T. and Giard, M. and Giraud-Héraud, Y. and Gjerløw, E. and González-Nuevo, J. and Górski, K. M. and Gregorio, A. and Gruppuso, A. and Guillet, V. and Hansen, F. K. and Hanson, D. and Harrison, D. L. and Hernández-Monteagudo, C. and Herranz, D. and Hildebrandt, S. R. and Hivon, E. and Hobson, M. and Holmes, W. A. and Huffenberger, K. M. and Hurier, G. and Jaffe, A. H. and Jaffe, T. R. and Jones, W. C. and Juvela, M. and Keskitalo, R. and Kisner, T. S. and Knoche, J. and Kunz, M. and Kurki-Suonio, H. and Lagache, G. and Lamarre, J. -M. and Lasenby, A. and Lawrence, C. R. and Leonardi, R. and Levrier, F. and Liguori, M. and Lilje, P. B. and Linden-Vørnle, M. and López-Caniego, M. and Lubin, P. M. and Macías-Pérez, J. F. and Maffei, B. and Mandolesi, N. and Mangilli, A. and Maris, M. and Martin, P. G. and Martínez-González, E. and Masi, S. and Matarrese, S. and Mazzotta, P. and Melchiorri, A. and Mendes, L. and Mennella, A. and Migliaccio, M. and Mitra, S. and Miville-Deschênes, M. -A. and Moneti, A. and Montier, L. and Morgante, G. and Mortlock, D. and Munshi, D. and Murphy, J. A. and Naselsky, P. and Nati, F. and Natoli, P. and Nørgaard-Nielsen, H. U. and Noviello, F. and Novikov, D. and Novikov, I. and Oppermann, N. and Pagano, L. and Pajot, F. and Paladini, R. and Paoletti, D. and Pasian, F. and Perrotta, F. and Pettorino, V. and Piacentini, F. and Piat, M. and Pierpaoli, E. and Pietrobon, D. and Plaszczynski, S. and Pointecouteau, E. and Polenta, G. and Pratt, G. W. and Puget, J. -L. and Rachen, J. P. and Rebolo, R. and Reinecke, M. and Remazeilles, M. and Renault, C. and Renzi, A. and Ricciardi, S. and Ristorcelli, I. and Rocha, G. and Rosset, C. and Rossetti, M. and Roudier, G. and Rubiño-Martín, J. A. and Rusholme, B. and Sandri, M. and Savelainen, M. and Savini, G. and Scott, D. and Soler, J. D. and Stolyarov, V. and Sutton, D. and Suur-Uski, A. -S. and Sygnet, J. -F. and Tauber, J. A. and Terenzi, L. and Toffolatti, L. and Tomasi, M. and Tristram, M. and Tucci, M. and Valenziano, L. and Valiviita, J. and Van Tent, B. and Vielva, P. and Villa, F. and Wade, L. A. and Wandelt, B. D. and Yvon, D. and Zacchei, A. and Zonca, A.},
abstractNote = {Planck observations at 353 GHz provide the first fully sampled maps of the polarized dust emission towards interstellar filaments and their backgrounds (i.e., the emission observed in the surroundings of the filaments). The data allow us to determine the intrinsic polarization properties of the filaments and therefore to provide insight into the structure of their magnetic field (B). In this paper, we present the polarization maps of three nearby (several parsecs long) star-forming filaments of moderate column density (NH about 1022 cm-2): Musca, B211, and L1506. These three filaments are detected above the background in dust total and polarized emission. We use the spatial information to separate Stokes I, Q, and U of the filaments from those of their backgrounds, an essential step in measuring the intrinsic polarization fraction (p) and angle (ψ) of each emission component. We find that the polarization angles in the three filaments (ψfil) are coherent along their lengths and not the same as in their backgrounds (ψbg). The differences between ψfil and ψbg are 12° and 54° for Musca and L1506, respectively, and only 6° in the case of B211. These differences forMusca and L1506 are larger than the dispersions of ψ, both along the filaments and in their backgrounds. The observed changes of ψ are direct evidence of variations of the orientation of the plane of the sky (POS) projection of the magnetic field. As in previous studies, we find a decrease of several per cent in p with NH from the backgrounds to the crest of the filaments. We show that the bulk of the drop in p within the filaments cannot be explained by random fluctuations of the orientation of the magnetic field because they are too small (σψ< 10°). We recognize the degeneracy between the dust alignment efficiency (by, e.g., radiative torques) and the structure of the B-field in causing variations in p, but we argue that the decrease in p from the backgrounds to the filaments results in part from depolarization associated with the 3D structure of the B-field: both its orientation in the POS and with respect to the POS. We do not resolve the inner structure of the filaments, but at the smallest scales accessible with Planck (~0.2 pc), the observed changes of ψ and p hold information on the magnetic field structure within filaments. Finally, they show that both the mean field and its fluctuations in the filaments are different from those of their backgrounds, which points to a coupling between the matter and the B-field in the filament formation process.},
doi = {10.1051/0004-6361/201425305},
journal = {Astronomy and Astrophysics},
number = ,
volume = 586,
place = {United States},
year = {2016},
month = {2}
}

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  • The Astrophysical Journal, Vol. 844, Issue 1
  • DOI: 10.3847/2041-8213/aa7e33

The First Multichroic Polarimeter Array on the Atacama Cosmology Telescope: Characterization and Performance
journal, March 2016

  • Ho, S. P.; Pappas, C. G.; Austermann, J.
  • Journal of Low Temperature Physics, Vol. 184, Issue 3-4
  • DOI: 10.1007/s10909-016-1573-1

Relieving tensions related to the lensing of the cosmic microwave background temperature power spectra
journal, January 2017


Mapping the kinetic Sunyaev-Zel’dovich effect toward MACS J0717.5+3745 with NIKA
journal, February 2017


Planck ’s dusty GEMS: III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z = 1.5⋆
journal, March 2017


Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
journal, January 2018


Dust in galaxy clusters: Modeling at millimeter wavelengths and impact on Planck cluster cosmology
journal, September 2018


PreProFit: Pressure Profile Fitter for galaxy clusters
journal, November 2019


The star Formation Histories of Local Group Dwarf Galaxies. iii. Characterizing Quenching in Low-Mass Galaxies
journal, May 2015

  • Weisz, Daniel R.; Dolphin, Andrew E.; Skillman, Evan D.
  • The Astrophysical Journal, Vol. 804, Issue 2
  • DOI: 10.1088/0004-637x/804/2/136

Background model systematics for the Fermi GeV excess
journal, March 2015

  • Calore, Francesca; Cholis, Ilias; Weniger, Christoph
  • Journal of Cosmology and Astroparticle Physics, Vol. 2015, Issue 03
  • DOI: 10.1088/1475-7516/2015/03/038

Exploring cosmic origins with CORE: B -mode component separation
journal, April 2018

  • Remazeilles, M.; Banday, A. J.; Baccigalupi, C.
  • Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 04
  • DOI: 10.1088/1475-7516/2018/04/023

Can the H 0 tension be resolved in extensions to ΛCDM cosmology?
journal, February 2019

  • Guo, Rui-Yun; Zhang, Jing-Fei; Zhang, Xin
  • Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 02
  • DOI: 10.1088/1475-7516/2019/02/054

Most Frequent Value Statistics and the Hubble Constant
journal, June 2018


Analytical model for non-thermal pressure in galaxy clusters
journal, June 2014

  • Shi, Xun; Komatsu, Eiichiro
  • Monthly Notices of the Royal Astronomical Society, Vol. 442, Issue 1
  • DOI: 10.1093/mnras/stu858

Analytical model for non-thermal pressure in galaxy clusters – III. Removing the hydrostatic mass bias
journal, November 2015

  • Shi, Xun; Komatsu, Eiichiro; Nagai, Daisuke
  • Monthly Notices of the Royal Astronomical Society, Vol. 455, Issue 3
  • DOI: 10.1093/mnras/stv2504

The magnetic field and dust filaments in the Polaris Flare
journal, August 2016

  • Panopoulou, G. V.; Psaradaki, I.; Tassis, K.
  • Monthly Notices of the Royal Astronomical Society, Vol. 462, Issue 2
  • DOI: 10.1093/mnras/stw1678

Sample variance in the local measurements of the Hubble constant
journal, August 2017

  • Wu, Hao-Yi; Huterer, Dragan
  • Monthly Notices of the Royal Astronomical Society, Vol. 471, Issue 4
  • DOI: 10.1093/mnras/stx1967

New constraints on time-dependent variations of fundamental constants using Planck data
journal, October 2017

  • Hart, Luke; Chluba, Jens
  • Monthly Notices of the Royal Astronomical Society, Vol. 474, Issue 2
  • DOI: 10.1093/mnras/stx2783

Escape of ionizing radiation from high-redshift dwarf galaxies: role of AGN feedback
journal, May 2018

  • Trebitsch, Maxime; Volonteri, Marta; Dubois, Yohan
  • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 4
  • DOI: 10.1093/mnras/sty1406

Impact of SZ cluster residuals in CMB maps and CMB–LSS cross-correlations
journal, June 2018

  • Chen, T.; Remazeilles, M.; Dickinson, C.
  • Monthly Notices of the Royal Astronomical Society, Vol. 479, Issue 3
  • DOI: 10.1093/mnras/sty1730

SU(2) cmb and the cosmological model: angular power spectra
journal, November 2018

  • Hahn, Steffen; Hofmann, Ralf; Kramer, Daniel
  • Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 4
  • DOI: 10.1093/mnras/sty2981

A high-resolution, dust-selected molecular cloud catalogue of M33, the Triangulum Galaxy
journal, December 2018

  • Williams, Thomas G.; Gear, Walter K.; Smith, Matthew W. L.
  • Monthly Notices of the Royal Astronomical Society, Vol. 483, Issue 4
  • DOI: 10.1093/mnras/sty3437

LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content
journal, January 2019

  • Mulroy, Sarah L.; Farahi, Arya; Evrard, August E.
  • Monthly Notices of the Royal Astronomical Society, Vol. 484, Issue 1
  • DOI: 10.1093/mnras/sty3484

Improved CMB anisotropy constraints on primordial magnetic fields from the post-recombination ionization history
journal, January 2019

  • Paoletti, D.; Chluba, J.; Finelli, F.
  • Monthly Notices of the Royal Astronomical Society, Vol. 484, Issue 1
  • DOI: 10.1093/mnras/sty3521

The shape and size distribution of H ii regions near the percolation transition
journal, March 2018

  • Bag, Satadru; Mondal, Rajesh; Sarkar, Prakash
  • Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 2
  • DOI: 10.1093/mnras/sty714

The environment and host haloes of the brightest z ∼ 6 Lyman-break galaxies
journal, April 2018

  • Hatfield, P. W.; Bowler, R. A. A.; Jarvis, M. J.
  • Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 3
  • DOI: 10.1093/mnras/sty856

Probing galaxy cluster and intra-cluster gas with luminous red galaxies
journal, May 2019

  • Gong, Yan; Ma, Yin-Zhe; Tanimura, Hideki
  • Monthly Notices of the Royal Astronomical Society, Vol. 486, Issue 4
  • DOI: 10.1093/mnras/stz1177

Ruling out 3 keV warm dark matter using 21 cm EDGES data
journal, May 2019

  • Chatterjee, Atrideb; Dayal, Pratika; Choudhury, Tirthankar Roy
  • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 3
  • DOI: 10.1093/mnras/stz1444

Independent cosmological constraints from high-z H ii galaxies
journal, June 2019

  • González-Morán, Ana Luisa; Chávez, Ricardo; Terlevich, Roberto
  • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
  • DOI: 10.1093/mnras/stz1577

Joint estimation of the Epoch of Reionization power spectrum and foregrounds
journal, July 2019

  • Sims, Peter H.; Pober, Jonathan C.
  • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 2
  • DOI: 10.1093/mnras/stz1888

The first power spectrum limit on the 21-cm signal of neutral hydrogen during the Cosmic Dawn at z = 20–25 from LOFAR
journal, July 2019

  • Gehlot, B. K.; Mertens, F. G.; Koopmans, L. V. E.
  • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 3
  • DOI: 10.1093/mnras/stz1937

The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization
journal, October 2019

  • Jew, Luke; Taylor, Angela C.; Jones, Michael E.
  • Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 2
  • DOI: 10.1093/mnras/stz2697

The C-Band All-Sky Survey (C-BASS): constraining diffuse Galactic radio emission in the North Celestial Pole region
journal, February 2019

  • Dickinson, C.; Barr, A.; Chiang, H. C.
  • Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 2
  • DOI: 10.1093/mnras/stz522

Predictions and sensitivity forecasts for reionization-era [C  ii ] line intensity mapping
journal, March 2019

  • Dumitru, Sebastian; Kulkarni, Girish; Lagache, Guilaine
  • Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 3
  • DOI: 10.1093/mnras/stz617

Investigation of the origin of the anomalous microwave emission in Lambda Orionis
journal, October 2019

  • Bell, Aaron C.; Onaka, Takashi; Galliano, Frédéric
  • Publications of the Astronomical Society of Japan
  • DOI: 10.1093/pasj/psz110

Data compression in cosmology: A compressed likelihood for Planck data
journal, October 2019


Cosmology from the thermal Sunyaev-Zel’dovich power spectrum: Primordial non-Gaussianity and massive neutrinos
journal, September 2013


Kinematic Sunyaev-Zel’dovich effect with projected fields. II. Prospects, challenges, and comparison with simulations
journal, December 2016


CMB bounds on disk-accreting massive primordial black holes
journal, October 2017


C P transformed mixed μ τ antisymmetry for neutrinos and its consequences
journal, February 2019


The Planck Mission: Recent Results, Cosmological and Fundamental Physics Perspectives
conference, March 2015

  • Mandolesi, Nazzareno; Burigana, Carlo; Gruppuso, Alessandro
  • Proceedings of the MG13 Meeting on General Relativity, The Thirteenth Marcel Grossmann Meeting
  • DOI: 10.1142/9789814623995_0018

Spatial variation of fundamental constants: Testing models with thermonuclear supernovae
journal, July 2018

  • Negrelli, C.; Kraiselburd, L.; Landau, S.
  • International Journal of Modern Physics D, Vol. 27, Issue 09
  • DOI: 10.1142/s0218271818500992

On Mautner-Type Probability of Capture of Intergalactic Meteor Particles by Habitable Exoplanets
journal, October 2019


General Relativity and Cosmology: Unsolved Questions and Future Directions
journal, September 2016


A CATALOG OF 1.5273 μ m DIFFUSE INTERSTELLAR BANDS BASED ON APOGEE HOT TELLURIC CALIBRATORS
journal, August 2016

  • Elyajouri, M.; Monreal-Ibero, A.; Remy, Q.
  • The Astrophysical Journal Supplement Series, Vol. 225, Issue 2
  • DOI: 10.3847/0067-0049/225/2/19

Spectroscopic Confirmation and Velocity Dispersions for 20 Planck Galaxy Clusters at 0.16 < z < 0.78
journal, January 2018

  • Amodeo, Stefania; Mei, Simona; Stanford, Spencer A.
  • The Astrophysical Journal, Vol. 853, Issue 1
  • DOI: 10.3847/1538-4357/aa98dd

Warm Dark Matter and Cosmic Reionization
journal, January 2018

  • Villanueva-Domingo, Pablo; Gnedin, Nickolay Y.; Mena, Olga
  • The Astrophysical Journal, Vol. 852, Issue 2
  • DOI: 10.3847/1538-4357/aa9ff5

Full-data Results of Hubble Frontier Fields: UV Luminosity Functions at z ∼ 6–10 and a Consistent Picture of Cosmic Reionization
journal, February 2018

  • Ishigaki, Masafumi; Kawamata, Ryota; Ouchi, Masami
  • The Astrophysical Journal, Vol. 854, Issue 1
  • DOI: 10.3847/1538-4357/aaa544

Forecasting the Contribution of Polarized Extragalactic Radio Sources in CMB Observations
journal, May 2018


Developing the 3-point Correlation Function for the Turbulent Interstellar Medium
journal, July 2018

  • Portillo, Stephen K. N.; Slepian, Zachary; Burkhart, Blakesley
  • The Astrophysical Journal, Vol. 862, Issue 2
  • DOI: 10.3847/1538-4357/aacb80

A Census of Galaxy Constituents in a Coma Progenitor Observed at z > 3
journal, January 2019


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

  • Miyatake, Hironao; Battaglia, Nicholas; Hilton, Matt
  • The Astrophysical Journal, Vol. 875, Issue 1
  • DOI: 10.3847/1538-4357/ab0af0

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

  • Hayashi, Katsuhiro; Mizuno, Tsunefumi; Fukui, Yasuo
  • The Astrophysical Journal, Vol. 884, Issue 2
  • DOI: 10.3847/1538-4357/ab4351

A Limit on the Warm Dark Matter Particle Mass from the Redshifted 21 cm Absorption Line
journal, May 2018

  • Safarzadeh, Mohammadtaher; Scannapieco, Evan; Babul, Arif
  • The Astrophysical Journal, Vol. 859, Issue 2
  • DOI: 10.3847/2041-8213/aac5e0

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


CO, H 2 O, H 2 O + line and dust emission in a z = 3.63 strongly lensed starburst merger at sub-kiloparsec scales
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


EXTRAGALACTIC MILLIMETER-WAVE POINT-SOURCE CATALOG, NUMBER COUNTS AND STATISTICS FROM 771 deg 2 OF THE SPT-SZ SURVEY
journal, November 2013


Generalised uncertainty relations from superpositions of geometries
journal, July 2019

  • Lake, Matthew J.; Miller, Marek; Ganardi, Ray F.
  • Classical and Quantum Gravity, Vol. 36, Issue 15
  • DOI: 10.1088/1361-6382/ab2160

The impact of stellar feedback on hot gas in galaxy haloes: the Sunyaev–Zel'dovich effect and soft X-ray emission
journal, September 2016

  • van de Voort, Freeke; Quataert, Eliot; Hopkins, Philip F.
  • Monthly Notices of the Royal Astronomical Society, Vol. 463, Issue 4
  • DOI: 10.1093/mnras/stw2322

Wide-field LOFAR-LBA power-spectra analyses: impact of calibration, polarization leakage, and ionosphere
journal, May 2018

  • Gehlot, B. K.; Koopmans, L. V. E.; de Bruyn, A. G.
  • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 2
  • DOI: 10.1093/mnras/sty1095

X-ray and SZ constraints on the properties of hot CGM
journal, May 2018

  • Singh, Priyanka; Majumdar, Subhabrata; Nath, Biman B.
  • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 3
  • DOI: 10.1093/mnras/sty1276

The FABLE simulations: a feedback model for galaxies, groups, and clusters
journal, July 2018

  • Henden, Nicholas A.; Puchwein, Ewald; Shen, Sijing
  • Monthly Notices of the Royal Astronomical Society, Vol. 479, Issue 4
  • DOI: 10.1093/mnras/sty1780

Reionization in Technicolor
journal, July 2018

  • Finlator, Kristian; Keating, Laura; Oppenheimer, Benjamin D.
  • Monthly Notices of the Royal Astronomical Society, Vol. 480, Issue 2
  • DOI: 10.1093/mnras/sty1949

The C-Band All-Sky Survey (C-BASS): design and capabilities
journal, July 2018

  • Jones, Michael E.; Taylor, Angela C.; Aich, Moumita
  • Monthly Notices of the Royal Astronomical Society, Vol. 480, Issue 3
  • DOI: 10.1093/mnras/sty1956

Mapping stellar content to dark matter haloes – III. Environmental dependence and conformity of galaxy colours
journal, February 2018

  • Zu, Ying; Mandelbaum, Rachel
  • Monthly Notices of the Royal Astronomical Society, Vol. 476, Issue 2
  • DOI: 10.1093/mnras/sty279

SILCC-Zoom: Polarization and depolarization in molecular clouds
journal, October 2018

  • Seifried, D.; Walch, S.; Reissl, S.
  • Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 2
  • DOI: 10.1093/mnras/sty2831

Polarization of seven MBM clouds at high Galactic latitude
journal, April 2018

  • Neha, S.; Maheswar, G.; Soam, A.
  • Monthly Notices of the Royal Astronomical Society, Vol. 476, Issue 4
  • DOI: 10.1093/mnras/sty485

Dark energy constraints from the thermal Sunyaev–Zeldovich power spectrum
journal, March 2018

  • Bolliet, Boris; Comis, Barbara; Komatsu, Eiichiro
  • Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 4
  • DOI: 10.1093/mnras/sty823

Magnetic ionization–thermal instability
journal, May 2019

  • Dudorov, A. E.; Stepanov, C. E.; Fomin, S. O.
  • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 1
  • DOI: 10.1093/mnras/stz1335

Measurement of the pairwise kinematic Sunyaev-Zeldovich effect with Planck and BOSS data
journal, January 2018


Observational effects of varying speed of light in quadratic gravity cosmological models
journal, April 2018

  • Izadi, Azam; Shacker, Shadi Sajedi; Olmo, Gonzalo J.
  • International Journal of Geometric Methods in Modern Physics, Vol. 15, Issue 05
  • DOI: 10.1142/s0219887818500846

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 link Between Turbulence, Magnetic Fields, Filaments, and star Formation in the Central Molecular zone Cloud G0.253+0.016
journal, November 2016


The Fraction of Cool-core Clusters in X-Ray versus SZ Samples Using Chandra Observations
journal, July 2017

  • Andrade-Santos, Felipe; Jones, Christine; Forman, William R.
  • The Astrophysical Journal, Vol. 843, Issue 1
  • DOI: 10.3847/1538-4357/aa7461

Unlocking Sensitivity for Visibility-based Estimators of the 21 cm Reionization Power Spectrum
journal, January 2018

  • Zhang, Yunfan Gerry; Liu, Adrian; Parsons, Aaron R.
  • The Astrophysical Journal, Vol. 852, Issue 2
  • DOI: 10.3847/1538-4357/aaa029

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

  • Brandenburg, Axel; Bracco, Andrea; Kahniashvili, Tina
  • The Astrophysical Journal, Vol. 870, Issue 2
  • DOI: 10.3847/1538-4357/aaf383

Ultraviolet HST Spectroscopy of Planck Cold Clumps
journal, February 2019


Results from EDGES High-Band. III. New Constraints on Parameters of the Early Universe
journal, April 2019

  • Monsalve, Raul A.; Fialkov, Anastasia; Bowman, Judd D.
  • The Astrophysical Journal, Vol. 875, Issue 1
  • DOI: 10.3847/1538-4357/ab07be

The Far-infrared Polarization Spectrum of ρ Ophiuchi A from HAWC+/SOFIA Observations
journal, September 2019

  • Santos, Fabio P.; Chuss, David T.; Dowell, C. Darren
  • The Astrophysical Journal, Vol. 882, Issue 2
  • DOI: 10.3847/1538-4357/ab3407

Radiative Transfer with POLARIS. II. Modeling of Synthetic Galactic Synchrotron Observations
journal, October 2019

  • Reissl, Stefan; Brauer, Robert; Klessen, Ralf S.
  • The Astrophysical Journal, Vol. 885, Issue 1
  • DOI: 10.3847/1538-4357/ab3664

Large-scale Maps of the Cosmic Infrared Background from Planck
journal, September 2019

  • Lenz, Daniel; Doré, Olivier; Lagache, Guilaine
  • The Astrophysical Journal, Vol. 883, Issue 1
  • DOI: 10.3847/1538-4357/ab3c2b

An Imprint of the Galactic Magnetic Field in the Diffuse Unpolarized Dust Emission
journal, December 2019

  • Hensley, Brandon S.; Zhang, Cheng; Bock, James J.
  • The Astrophysical Journal, Vol. 887, Issue 2
  • DOI: 10.3847/1538-4357/ab5183

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

  • Wang, Jia-Wei; Lai, Shih-Ping; Clemens, Dan P.
  • The Astrophysical Journal, Vol. 888, Issue 1
  • DOI: 10.3847/1538-4357/ab5c1c

Beyond Optical Depth: Future Determination of Ionization History from the Cosmic Microwave Background
journal, January 2020

  • Watts, D. J.; Addison, G. E.; Bennett, C. L.
  • The Astrophysical Journal, Vol. 889, Issue 2
  • DOI: 10.3847/1538-4357/ab5fd5

Identifying Direct Collapse Black Hole Seeds through Their Small Host Galaxies
journal, September 2018


Planck intermediate results : XXIX. All-sky dust modelling with
journal, February 2016


Planck 2015 results : XVI. Isotropy and statistics of the CMB
journal, September 2016


Planck 2015 results : XXVI. The Second
journal, September 2016


Planck 2015 results. I. Overview of products and scientific results
text, January 2015


Modeling Dust Polarization Observations of Molecular Clouds through MHD Simulations
text, January 2017


Dust spectrum and polarisation at 850 um in the massive IRDC G035.39-00.33
text, January 2018


Magnetic Field Structure in Spheroidal Star-Forming Clouds
text, January 2018


Time Evolution of 3D Disk Formation with Misaligned Magnetic Field and Rotation Axes
text, January 2018


The role of initial magnetic field structure in the launching of protostellar jets
text, January 2019


Characterizing magnetic field morphologies in three Serpens protostellar cores with ALMA
text, January 2019