Planck intermediate results: XXXIV. The magnetic field structure in the Rosette Nebula
Abstract
Planck has mapped the polarized dust emission over the whole sky, making it possible to trace the Galactic magnetic field structure that pervades the interstellar medium (ISM). In this paper, we combine polarization data from Planck with rotation measure (RM) observations towards a massive star-forming region, the Rosette Nebula in the Monoceros molecular cloud, to study its magnetic field structure and the impact of an expanding H ii region on the morphology of the field. We derive an analytical solution for the magnetic field, assumed to evolve from an initially uniform configuration following the expansion of ionized gas and the formation of a shell of swept-up ISM. From the RM data we estimate a mean value of the line-of-sight component of the magnetic field of about 3 μG (towards the observer) in the Rosette Nebula, for a uniform electron density of about 12 cm-3. The dust shell that surrounds the Rosette H ii region is clearly observed in the Planck intensity map at 353 GHz, with a polarization signal significantly different from that of the local background when considered asa whole. The Planck observations constrain the plane-of-the-sky orientation of the magnetic field in the Rosette’s parent molecular cloud to bemore »
- 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:
- 1393020
- 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; ISM; magnetic fields; polarization; radiation mechanisms; radio continuum; submillimeter
Citation Formats
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., 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., 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., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., 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., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Guillet, V., Hansen, F. K., Hanson, D., Harrison, D. L., Henrot-Versillé, S., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jewell, J., Juvela, M., Keskitalo, R., Kisner, T. S., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Leonardi, R., Levrier, F., Liguori, M., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maffei, B., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C. B., Noviello, F., Novikov, D., Novikov, I., Oppermann, N., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Pasian, F., Patanchon, G., Perdereau, O., Pettorino, V., Piacentini, F., Piat, M., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Savini, G., Scott, D., Soler, J. D., Spencer, L. 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., Tuovinen, J., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., Wiesemeyer, H., Yvon, D., Zacchei, A., and Zonca, A. Planck intermediate results: XXXIV. The magnetic field structure in the Rosette Nebula. United States: N. p., 2016.
Web. doi:10.1051/0004-6361/201525616.
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., 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., 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., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., 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., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Guillet, V., Hansen, F. K., Hanson, D., Harrison, D. L., Henrot-Versillé, S., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jewell, J., Juvela, M., Keskitalo, R., Kisner, T. S., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Leonardi, R., Levrier, F., Liguori, M., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maffei, B., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C. B., Noviello, F., Novikov, D., Novikov, I., Oppermann, N., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Pasian, F., Patanchon, G., Perdereau, O., Pettorino, V., Piacentini, F., Piat, M., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Savini, G., Scott, D., Soler, J. D., Spencer, L. 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., Tuovinen, J., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., Wiesemeyer, H., Yvon, D., Zacchei, A., & Zonca, A. Planck intermediate results: XXXIV. The magnetic field structure in the Rosette Nebula. United States. https://doi.org/10.1051/0004-6361/201525616
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., 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., 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., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., 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., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Gruppuso, A., Guillet, V., Hansen, F. K., Hanson, D., Harrison, D. L., Henrot-Versillé, S., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hornstrup, A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jewell, J., Juvela, M., Keskitalo, R., Kisner, T. S., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Lattanzi, M., Lawrence, C. R., Leonardi, R., Levrier, F., Liguori, M., Lilje, P. B., Linden-Vørnle, M., López-Caniego, M., Lubin, P. M., Macías-Pérez, J. F., Maffei, B., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J. A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C. B., Noviello, F., Novikov, D., Novikov, I., Oppermann, N., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Pasian, F., Patanchon, G., Perdereau, O., Pettorino, V., Piacentini, F., Piat, M., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Pratt, G. W., Prézeau, G., Prunet, S., Puget, J. -L., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rubiño-Martín, J. A., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Savini, G., Scott, D., Soler, J. D., Spencer, L. 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., Tuovinen, J., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., Wiesemeyer, H., Yvon, D., Zacchei, A., and Zonca, A. Tue .
"Planck intermediate results: XXXIV. The magnetic field structure in the Rosette Nebula". United States. https://doi.org/10.1051/0004-6361/201525616. https://www.osti.gov/servlets/purl/1393020.
@article{osti_1393020,
title = {Planck intermediate results: XXXIV. The magnetic field structure in the Rosette Nebula},
author = {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 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 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 Dole, H. and Donzelli, S. and Doré, O. and Douspis, M. and Ducout, A. and Dupac, X. and Efstathiou, G. 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 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 Henrot-Versillé, S. and Herranz, D. and Hildebrandt, S. R. and Hivon, E. and Hobson, M. and Holmes, W. A. and Hornstrup, A. and Hovest, W. and Huffenberger, K. M. and Hurier, G. and Jaffe, A. H. and Jaffe, T. R. and Jewell, J. 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 Lattanzi, M. 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 Maino, D. and Mandolesi, N. and Mangilli, A. and Maris, M. and Martin, P. G. and Martínez-González, E. and Masi, S. and Matarrese, S. and Melchiorri, A. and Mendes, L. and Mennella, A. and Migliaccio, M. and Miville-Deschênes, M. -A. and Moneti, A. and Montier, L. and Morgante, G. and Mortlock, D. and Moss, A. and Munshi, D. and Murphy, J. A. and Naselsky, P. and Nati, F. and Natoli, P. and Netterfield, C. B. 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 Patanchon, G. and Perdereau, O. and Pettorino, V. and Piacentini, F. and Piat, M. and Pietrobon, D. and Plaszczynski, S. and Pointecouteau, E. and Polenta, G. and Ponthieu, N. and Pratt, G. W. and Prézeau, G. and Prunet, S. and Puget, J. -L. and Rebolo, R. and Reinecke, M. and Remazeilles, M. and Renault, C. and Renzi, A. 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 Santos, D. and Savelainen, M. and Savini, G. and Scott, D. and Soler, J. D. and Spencer, L. 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 Tuovinen, J. 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 Wehus, I. K. and Wiesemeyer, H. and Yvon, D. and Zacchei, A. and Zonca, A.},
abstractNote = {Planck has mapped the polarized dust emission over the whole sky, making it possible to trace the Galactic magnetic field structure that pervades the interstellar medium (ISM). In this paper, we combine polarization data from Planck with rotation measure (RM) observations towards a massive star-forming region, the Rosette Nebula in the Monoceros molecular cloud, to study its magnetic field structure and the impact of an expanding H ii region on the morphology of the field. We derive an analytical solution for the magnetic field, assumed to evolve from an initially uniform configuration following the expansion of ionized gas and the formation of a shell of swept-up ISM. From the RM data we estimate a mean value of the line-of-sight component of the magnetic field of about 3 μG (towards the observer) in the Rosette Nebula, for a uniform electron density of about 12 cm-3. The dust shell that surrounds the Rosette H ii region is clearly observed in the Planck intensity map at 353 GHz, with a polarization signal significantly different from that of the local background when considered asa whole. The Planck observations constrain the plane-of-the-sky orientation of the magnetic field in the Rosette’s parent molecular cloud to be mostly aligned with the large-scale field along the Galactic plane. The Planck data are compared with the analytical model, which predicts the mean polarization properties of a spherical and uniform dust shell for a given orientation of the field. This comparison leads to an upper limit of about 45° on the angle between the line of sight and the magnetic field in the Rosette complex, for an assumed intrinsic dust polarization fraction of 4%. This field direction can reproduce the RM values detected in the ionized region if the magnetic field strength in the Monoceros molecular cloud is in the range 6.5–9 μG. Finally, the present analytical model is able to reproduce the RM distribution across the ionized nebula, as well as the mean dust polarization properties of the swept-up shell, and can be directly applied to other similar objects.},
doi = {10.1051/0004-6361/201525616},
journal = {Astronomy and Astrophysics},
number = ,
volume = 586,
place = {United States},
year = {2016},
month = {2}
}
Web of Science
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EXTRAGALACTIC MILLIMETER-WAVE POINT-SOURCE CATALOG, NUMBER COUNTS AND STATISTICS FROM 771 deg 2 OF THE SPT-SZ SURVEY
journal, November 2013
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Kinematic Sunyaev-Zel’dovich effect with projected fields. II. Prospects, challenges, and comparison with simulations
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Filaments and striations: anisotropies in observed, supersonic, highly magnetized turbulent clouds
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Planck 2015 results : XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation
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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 Far-infrared Polarization Spectrum of ρ Ophiuchi A from HAWC+/SOFIA Observations
journal, September 2019
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Planck 2013 results. I. Overview of products and scientific results
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Planck 2013 results. XX. Cosmology from Sunyaev–Zeldovich cluster counts
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Impact of SZ cluster residuals in CMB maps and CMB–LSS cross-correlations
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Detection of thermal SZ-CMB lensing cross-correlation in Planck nominal mission data
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The environment and host haloes of the brightest z ∼ 6 Lyman-break galaxies
journal, April 2018
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- Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 3
Galactic cold cores: V. Dust opacity ⋆⋆⋆⋆⋆⋆⋆⋆⋆⋆
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- Astronomy & Astrophysics, Vol. 584
A CATALOG OF 1.5273 μ m DIFFUSE INTERSTELLAR BANDS BASED ON APOGEE HOT TELLURIC CALIBRATORS
journal, August 2016
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- The Astrophysical Journal Supplement Series, Vol. 225, Issue 2
The impact of stellar feedback on hot gas in galaxy haloes: the Sunyaev–Zel'dovich effect and soft X-ray emission
journal, September 2016
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- Monthly Notices of the Royal Astronomical Society, Vol. 463, Issue 4
ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19
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Beyond Optical Depth: Future Determination of Ionization History from the Cosmic Microwave Background
journal, January 2020
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- The Astrophysical Journal, Vol. 889, Issue 2
Predictions and sensitivity forecasts for reionization-era [C ii ] line intensity mapping
journal, March 2019
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- Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 3
Towards a realistic population of simulated galaxy groups and clusters
journal, May 2014
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- Monthly Notices of the Royal Astronomical Society, Vol. 441, Issue 2
Independent cosmological constraints from high-z H ii galaxies
journal, June 2019
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- Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
Magnetic ionization–thermal instability
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- Dudorov, A. E.; Stepanov, C. E.; Fomin, S. O.
- Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 1
The supernova-regulated ISM: IV. A comparison of simulated polarization with Planck observations
journal, June 2018
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- Astronomy & Astrophysics, Vol. 614
Evolution of oh and Co-Dark Molecular gas Fraction Across a Molecular Cloud Boundary in Taurus
journal, February 2016
- Xu, Duo; Li, Di; Yue, Nannan
- The Astrophysical Journal, Vol. 819, Issue 1
Large-Scale Features of the Radio Sky and a Model for Loop I
journal, May 2018
- Dickinson, Clive
- Galaxies, Vol. 6, Issue 2
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
Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues: II. Mg and Fe-rich amorphous silicates⋆
journal, October 2017
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- Astronomy & Astrophysics, Vol. 606
Understanding the Links among the Magnetic Fields, Filament, Bipolar Bubble, and Star Formation in RCW 57A Using NIR Polarimetry
journal, December 2017
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- The Astrophysical Journal, Vol. 850, Issue 2
Covariant polarized radiative transfer on cosmological scales for investigating large-scale magnetic field structures
journal, December 2018
- Chan, Jennifer Y. H.; Wu, Kinwah; On, Alvina Y. L.
- Monthly Notices of the Royal Astronomical Society, Vol. 484, Issue 2
The Planck Mission: Recent Results, Cosmological and Fundamental Physics Perspectives
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- Mandolesi, Nazzareno; Burigana, Carlo; Gruppuso, Alessandro
- Proceedings of the MG13 Meeting on General Relativity, The Thirteenth Marcel Grossmann Meeting
Cosmology and astrophysics from relaxed galaxy clusters – III. Thermodynamic profiles and scaling relations
journal, January 2016
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- Monthly Notices of the Royal Astronomical Society, Vol. 456, Issue 4
Background model systematics for the Fermi GeV excess
journal, March 2015
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- Journal of Cosmology and Astroparticle Physics, Vol. 2015, Issue 03
Statistical properties of polarized CMB foreground maps
journal, June 2019
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Large-scale Maps of the Cosmic Infrared Background from Planck
journal, September 2019
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Results from EDGES High-Band. III. New Constraints on Parameters of the Early Universe
journal, April 2019
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- The Astrophysical Journal, Vol. 875, Issue 1
Dust models compatible with Planck intensity and polarization data in translucent lines of sight
journal, February 2018
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- Astronomy & Astrophysics, Vol. 610
The star Formation Histories of Local Group Dwarf Galaxies. iii. Characterizing Quenching in Low-Mass Galaxies
journal, May 2015
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2 mm GISMO Observations of the Galactic Center. I. Dust Emission
journal, November 2019
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- The Astrophysical Journal, Vol. 885, Issue 1
The FABLE simulations: a feedback model for galaxies, groups, and clusters
journal, July 2018
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An Imprint of the Galactic Magnetic Field in the Diffuse Unpolarized Dust Emission
journal, December 2019
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- The Astrophysical Journal, Vol. 887, Issue 2
Data compression in cosmology: A compressed likelihood for Planck data
journal, October 2019
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- Physical Review D, Vol. 100, Issue 8
Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-variable Horizontal-branch Stars. III. M55 and NGC 6362
journal, July 2018
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Measurement of the pairwise kinematic Sunyaev-Zeldovich effect with Planck and BOSS data
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Exposing the plural nature of molecular clouds: Extracting filaments and the cosmic infrared background against the true scale-free interstellar medium
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The First Multichroic Polarimeter Array on the Atacama Cosmology Telescope: Characterization and Performance
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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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Analytical model for non-thermal pressure in galaxy clusters
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Mitigating Complex Dust Foregrounds in Future Cosmic Microwave Background Polarization Experiments
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A Search for FRB 121102-like Persistent Radio-luminous Sources—Candidates and Implications for the FRB Rate and Searches
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IMAGINE: a comprehensive view of the interstellar medium, Galactic magnetic fields and cosmic rays
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Peak star formation efficiency and no missing baryons in massive spirals
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Wide-field LOFAR-LBA power-spectra analyses: impact of calibration, polarization leakage, and ionosphere
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Constraints on Primordial Gravitational Waves Using , WMAP, and New BICEP2/ Observations through the 2015 Season
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- Physical Review Letters, Vol. 121, Issue 22
Sample variance in the local measurements of the Hubble constant
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SU(2) cmb and the cosmological model: angular power spectra
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DEEP CHANDRA , HST -COS, AND MEGACAM OBSERVATIONS OF THE PHOENIX CLUSTER: EXTREME STAR FORMATION AND AGN FEEDBACK ON HUNDRED KILOPARSEC SCALES
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First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud
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Escape of ionizing radiation from high-redshift dwarf galaxies: role of AGN feedback
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Planck intermediate results. XII: Diffuse Galactic components in the Gould Belt system
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A New Detection of Extragalactic Anomalous Microwave Emission in a Compact, Optically Faint Region of NGC 4725
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Investigation of the origin of the anomalous microwave emission in Lambda Orionis
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Planck 2015 results : XXVI. The Second
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E and B Polarizations from Inhomogeneous and Solar Surface Turbulence
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Spatial variation of fundamental constants: Testing models with thermonuclear supernovae
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The Fraction of Cool-core Clusters in X-Ray versus SZ Samples Using Chandra Observations
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Statistical analysis of the interplay between interstellar magnetic fields and filaments hosting Planck Galactic cold clumps
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Cosmology from the thermal Sunyaev-Zel’dovich power spectrum: Primordial non-Gaussianity and massive neutrinos
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Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
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Ruling out 3 keV warm dark matter using 21 cm EDGES data
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