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 »
- Authors:
- more »
- 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 = {Tue Feb 09 00:00:00 EST 2016},
month = {Tue Feb 09 00:00:00 EST 2016}
}
Web of Science
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Magnetic seismology of interstellar gas clouds: Unveiling a hidden dimension
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Submillimeter and Far-Infrared Polarimetric Observations of Magnetic Fields in Star-Forming Regions
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Understanding the Links among the Magnetic Fields, Filament, Bipolar Bubble, and Star Formation in RCW 57A Using NIR Polarimetry
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Magnetic Field Structure in Spheroidal Star-forming Clouds
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Time Evolution of 3D Disk Formation with Misaligned Magnetic Field and Rotation Axes
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Characterizing Magnetic Field Morphologies in Three Serpens Protostellar Cores with ALMA
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The Evidence of Radio Polarization Induced by the Radiative Grain Alignment and Self-scattering of Dust Grains in a Protoplanetary Disk
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The First Multichroic Polarimeter Array on the Atacama Cosmology Telescope: Characterization and Performance
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Relieving tensions related to the lensing of the cosmic microwave background temperature power spectra
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Mapping the kinetic Sunyaev-Zel’dovich effect toward MACS J0717.5+3745 with NIKA
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Planck ’s dusty GEMS: III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z = 1.5⋆
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Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
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Dust in galaxy clusters: Modeling at millimeter wavelengths and impact on Planck cluster cosmology
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PreProFit: Pressure Profile Fitter for galaxy clusters
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Background model systematics for the Fermi GeV excess
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Exploring cosmic origins with CORE: B -mode component separation
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Can the H 0 tension be resolved in extensions to ΛCDM cosmology?
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Most Frequent Value Statistics and the Hubble Constant
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Analytical model for non-thermal pressure in galaxy clusters
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Analytical model for non-thermal pressure in galaxy clusters – III. Removing the hydrostatic mass bias
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The magnetic field and dust filaments in the Polaris Flare
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Sample variance in the local measurements of the Hubble constant
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New constraints on time-dependent variations of fundamental constants using Planck data
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Escape of ionizing radiation from high-redshift dwarf galaxies: role of AGN feedback
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Impact of SZ cluster residuals in CMB maps and CMB–LSS cross-correlations
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SU(2) cmb and the cosmological model: angular power spectra
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A high-resolution, dust-selected molecular cloud catalogue of M33, the Triangulum Galaxy
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LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content
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Improved CMB anisotropy constraints on primordial magnetic fields from the post-recombination ionization history
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The shape and size distribution of H ii regions near the percolation transition
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The environment and host haloes of the brightest z ∼ 6 Lyman-break galaxies
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Probing galaxy cluster and intra-cluster gas with luminous red galaxies
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Ruling out 3 keV warm dark matter using 21 cm EDGES data
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Independent cosmological constraints from high-z H ii galaxies
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Joint estimation of the Epoch of Reionization power spectrum and foregrounds
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The first power spectrum limit on the 21-cm signal of neutral hydrogen during the Cosmic Dawn at z = 20–25 from LOFAR
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The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization
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The C-Band All-Sky Survey (C-BASS): constraining diffuse Galactic radio emission in the North Celestial Pole region
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Predictions and sensitivity forecasts for reionization-era [C ii ] line intensity mapping
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Investigation of the origin of the anomalous microwave emission in Lambda Orionis
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- Publications of the Astronomical Society of Japan
The Planck Mission: Recent Results, Cosmological and Fundamental Physics Perspectives
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- Proceedings of the MG13 Meeting on General Relativity, The Thirteenth Marcel Grossmann Meeting
Spatial variation of fundamental constants: Testing models with thermonuclear supernovae
journal, July 2018
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- International Journal of Modern Physics D, Vol. 27, Issue 09
On Mautner-Type Probability of Capture of Intergalactic Meteor Particles by Habitable Exoplanets
journal, October 2019
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General Relativity and Cosmology: Unsolved Questions and Future Directions
journal, September 2016
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- Universe, Vol. 2, Issue 4
A CATALOG OF 1.5273 μ m DIFFUSE INTERSTELLAR BANDS BASED ON APOGEE HOT TELLURIC CALIBRATORS
journal, August 2016
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A Search for FRB 121102-like Persistent Radio-luminous Sources—Candidates and Implications for the FRB Rate and Searches
journal, August 2017
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Spectroscopic Confirmation and Velocity Dispersions for 20 Planck Galaxy Clusters at 0.16 < z < 0.78
journal, January 2018
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- The Astrophysical Journal, Vol. 853, Issue 1
Warm Dark Matter and Cosmic Reionization
journal, January 2018
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Full-data Results of Hubble Frontier Fields: UV Luminosity Functions at z ∼ 6–10 and a Consistent Picture of Cosmic Reionization
journal, February 2018
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Forecasting the Contribution of Polarized Extragalactic Radio Sources in CMB Observations
journal, May 2018
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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
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Developing the 3-point Correlation Function for the Turbulent Interstellar Medium
journal, July 2018
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A Census of Galaxy Constituents in a Coma Progenitor Observed at z > 3
journal, January 2019
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The Halo Mass of Optically Luminous Quasars at z ≈ 1–2 Measured via Gravitational Deflection of the Cosmic Microwave Background
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Weak-lensing Mass Calibration of ACTPol Sunyaev–Zel’dovich Clusters with the Hyper Suprime-Cam Survey
journal, April 2019
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Constraining the Neutral Fraction of Hydrogen in the IGM at Redshift 7.5
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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
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A Limit on the Warm Dark Matter Particle Mass from the Redshifted 21 cm Absorption Line
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Planck 2013 results. XV. CMB power spectra and likelihood
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Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
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Planck 2015 results : VI. LFI mapmaking
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Statistical simulations of the dust foreground to cosmic microwave background polarization
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The XXL Survey: XVII. X-ray and Sunyaev-Zel’dovich properties of the redshift 2.0 galaxy cluster XLSSC 122★★★
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Dust models compatible with Planck intensity and polarization data in translucent lines of sight
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The supernova-regulated ISM: IV. A comparison of simulated polarization with Planck observations
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Protostellar birth with ambipolar and ohmic diffusion
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Far-infrared photometry of OJ 287 with the Herschel Space Observatory
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A dynamically young, gravitationally stable network of filaments in Orion B
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CO, H 2 O, H 2 O + line and dust emission in a z = 3.63 strongly lensed starburst merger at sub-kiloparsec scales
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Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters
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ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19
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Peak star formation efficiency and no missing baryons in massive spirals
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Generalised uncertainty relations from superpositions of geometries
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The impact of stellar feedback on hot gas in galaxy haloes: the Sunyaev–Zel'dovich effect and soft X-ray emission
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Wide-field LOFAR-LBA power-spectra analyses: impact of calibration, polarization leakage, and ionosphere
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X-ray and SZ constraints on the properties of hot CGM
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The FABLE simulations: a feedback model for galaxies, groups, and clusters
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Reionization in Technicolor
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The C-Band All-Sky Survey (C-BASS): design and capabilities
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Mapping stellar content to dark matter haloes – III. Environmental dependence and conformity of galaxy colours
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SILCC-Zoom: Polarization and depolarization in molecular clouds
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Polarization of seven MBM clouds at high Galactic latitude
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Dark energy constraints from the thermal Sunyaev–Zeldovich power spectrum
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Magnetic ionization–thermal instability
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Observational effects of varying speed of light in quadratic gravity cosmological models
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The Important Role of Cosmic-Ray Re-Acceleration
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Practical Modeling of Large-Scale Galactic Magnetic Fields: Status and Prospects
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Evolution of oh and Co-Dark Molecular gas Fraction Across a Molecular Cloud Boundary in Taurus
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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
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The Fraction of Cool-core Clusters in X-Ray versus SZ Samples Using Chandra Observations
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Unlocking Sensitivity for Visibility-based Estimators of the 21 cm Reionization Power Spectrum
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On the Faint End of the Galaxy Luminosity Function in the Epoch of Reionization: Updated Constraints from the HST Frontier Fields
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E and B Polarizations from Inhomogeneous and Solar Surface Turbulence
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- The Astrophysical Journal, Vol. 870, Issue 2
Ultraviolet HST Spectroscopy of Planck Cold Clumps
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Results from EDGES High-Band. III. New Constraints on Parameters of the Early Universe
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The Far-infrared Polarization Spectrum of ρ Ophiuchi A from HAWC+/SOFIA Observations
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- The Astrophysical Journal, Vol. 882, Issue 2
Radiative Transfer with POLARIS. II. Modeling of Synthetic Galactic Synchrotron Observations
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Large-scale Maps of the Cosmic Infrared Background from Planck
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An Imprint of the Galactic Magnetic Field in the Diffuse Unpolarized Dust Emission
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Mapping the Magnetic Interstellar Medium in Three Dimensions over the Full Sky with Neutral Hydrogen
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Multiwavelength Polarimetry of the Filamentary Cloud IC 5146. II. Magnetic Field Structures
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- Wang, Jia-Wei; Lai, Shih-Ping; Clemens, Dan P.
- The Astrophysical Journal, Vol. 888, Issue 1
Beyond Optical Depth: Future Determination of Ionization History from the Cosmic Microwave Background
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Identifying Direct Collapse Black Hole Seeds through Their Small Host Galaxies
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- Visbal, Eli; Haiman, Zoltán
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Planck intermediate results : XXIX. All-sky dust modelling with
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Planck 2015 results : XVI. Isotropy and statistics of the CMB
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Planck 2015 results : XXVI. The Second
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Planck 2015 results. I. Overview of products and scientific results
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Two-fluid dusty shocks: simple benchmarking problems and applications to protoplanetary discs
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The evidence of radio polarization induced by the radiative grain alignment and self-scattering of dust grains in a protoplanetary disk
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Modeling Dust Polarization Observations of Molecular Clouds through MHD Simulations
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Understanding the links among magnetic fields, filament, the bipolar bubble, and star formation in RCW57A using NIR polarimetry
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Dust spectrum and polarisation at 850 um in the massive IRDC G035.39-00.33
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Magnetic Field Structure in Spheroidal Star-Forming Clouds
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Time Evolution of 3D Disk Formation with Misaligned Magnetic Field and Rotation Axes
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The role of initial magnetic field structure in the launching of protostellar jets
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Characterizing magnetic field morphologies in three Serpens protostellar cores with ALMA
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