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Title: 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 » 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.« less

Authors:
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; « less
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.
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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
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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.
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@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}
}
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    • The Astrophysical Journal, Vol. 852, Issue 2
    • DOI: 10.3847/1538-4357/aa9ff5

    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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    • DOI: 10.1093/mnras/stz1937

    On Mautner-Type Probability of Capture of Intergalactic Meteor Particles by Habitable Exoplanets
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    The Important Role of Cosmic-Ray Re-Acceleration
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    Protostellar birth with ambipolar and ohmic diffusion
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    Planck intermediate results : XXIX. All-sky dust modelling with
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    Submillimeter and Far-Infrared Polarimetric Observations of Magnetic Fields in Star-Forming Regions
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    X-Ray Morphological Analysis of the Planck ESZ Clusters
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    • DOI: 10.3847/1538-4357/aa855f

    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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    The C-Band All-Sky Survey (C-BASS): constraining diffuse Galactic radio emission in the North Celestial Pole region
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    • DOI: 10.1093/mnras/stz522

    The influence of magnetic field on the cold neutral medium mass fraction and its alignment with density structures
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    • DOI: 10.1093/mnras/sty438

    Full-sky beam convolution for cosmic microwave background applications
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    Sunyaev-Zel'dovich profile fitting with joint AMI-Planck analysis
    text, January 2019

    • Perrott, Yvette Chanel; Javid, Kamran; Carvalho, P.
    • Apollo - University of Cambridge Repository
    • DOI: 10.17863/cam.44998

    DISSECTING THE HIGH- z INTERSTELLAR MEDIUM THROUGH INTENSITY MAPPING CROSS-CORRELATIONS
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    Simulating the Galaxy Cluster “El Gordo”: Gas Motion, Kinetic Sunyaev–Zel’dovich Signal, and X-Ray Line Features
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    • DOI: 10.1093/mnras/sty3521

    A review of indirect searches for particle dark matter
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    • DOI: 10.3847/1538-4357/ab55df

    The Halo Mass of Optically Luminous Quasars at z ≈ 1–2 Measured via Gravitational Deflection of the Cosmic Microwave Background
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    DENSER SAMPLING OF THE ROSETTE NEBULA WITH FARADAY ROTATION MEASUREMENTS: IMPROVED ESTIMATES OF MAGNETIC FIELDS IN H ii REGIONS
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    • The Astrophysical Journal, Vol. 821, Issue 2
    • DOI: 10.3847/0004-637x/821/2/92

    The far-infrared polarization spectrum of Rho Ophiuchi A from HAWC+/SOFIA observations
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    Dust in galaxy clusters: Modeling at millimeter wavelengths and impact on Planck cluster cosmology
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    Statistical simulations of the dust foreground to cosmic microwave background polarization
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    Exploring cosmic origins with CORE: Extragalactic sources in cosmic microwave background maps
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    • Zotti, G. De; González-Nuevo, J.; Lopez-Caniego, M.
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    • DOI: 10.1088/1475-7516/2018/04/020

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    • Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 4
    • DOI: 10.1093/mnras/stz784

    Exploring cosmic origins with CORE: B -mode component separation
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    • Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 04
    • DOI: 10.1088/1475-7516/2018/04/023

    Very Large Interstellar Grains as Evidenced by the Mid-Infrared Extinction
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    Violent Quenching: Molecular Gas Blown to 1000 km s −1 during a Major Merger
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    • The Astrophysical Journal, Vol. 864, Issue 1
    • DOI: 10.3847/2041-8213/aad8b6

    The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization
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    • Jew, Luke; Taylor, Angela C.; Jones, Michael E.
    • Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 2
    • DOI: 10.1093/mnras/stz2697

    Fractal statistics in young star clusters: structural parameters and dynamical evolution
    journal, October 2019

    • Hetem, Annibal; Gregorio-Hetem, Jane
    • Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 2
    • DOI: 10.1093/mnras/stz2698

    The XXL Survey: XVII. X-ray and Sunyaev-Zel’dovich properties of the redshift 2.0 galaxy cluster XLSSC 122★★★
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    A dynamically young, gravitationally stable network of filaments in Orion B
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    Detection of intercluster gas in superclusters using the thermal Sunyaev–Zel’dovich effect
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    Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
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    Identifying Direct Collapse Black Hole Seeds through Their Small Host Galaxies
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    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

    The structure of galactic halos and the microwave temperature maps
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    Tomographic measurement of the intergalactic gas pressure through galaxy–tSZ cross-correlations
    journal, December 2019

    • Koukoufilippas, Nick; Alonso, David; Bilicki, Maciej
    • Monthly Notices of the Royal Astronomical Society, Vol. 491, Issue 4
    • DOI: 10.1093/mnras/stz3351

    Exploring cosmic origins with CORE: Survey requirements and mission design
    journal, April 2018

    • Delabrouille, J.; de Bernardis, P.; Bouchet, F. R.
    • Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 04
    • DOI: 10.1088/1475-7516/2018/04/014

    Probing galaxy cluster and intra-cluster gas with luminous red galaxies
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    • Gong, Yan; Ma, Yin-Zhe; Tanimura, Hideki
    • Monthly Notices of the Royal Astronomical Society, Vol. 486, Issue 4
    • DOI: 10.1093/mnras/stz1177

    Mapping the Magnetic Interstellar Medium in Three Dimensions over the Full Sky with Neutral Hydrogen
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    The link Between Turbulence, Magnetic Fields, Filaments, and star Formation in the Central Molecular zone Cloud G0.253+0.016
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    The Python Sky Model: software for simulating the Galactic microwave sky
    journal, May 2017

    • Thorne, B.; Dunkley, J.; Alonso, D.
    • Monthly Notices of the Royal Astronomical Society, Vol. 469, Issue 3
    • DOI: 10.1093/mnras/stx949

    Planck intermediate results : XLII. Large-scale Galactic magnetic fields
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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

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

    Relieving tensions related to the lensing of the cosmic microwave background temperature power spectra
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    Constraints on dark radiation from cosmological probes
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    Constraining the Neutral Fraction of Hydrogen in the IGM at Redshift 7.5
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    Planck 2013 results. XV. CMB power spectra and likelihood
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    Far-infrared photometry of OJ 287 with the Herschel Space Observatory
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    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

    Planck 2013 results. XI. All-sky model of thermal dust emission
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    Nonlinear Reconstruction of the Velocity Field
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    A new mechanical stellar wind feedback model for the Rosette Nebula
    journal, February 2018

    • Wareing, C. J.; Pittard, J. M.; Wright, N. J.
    • Monthly Notices of the Royal Astronomical Society, Vol. 475, Issue 3
    • DOI: 10.1093/mnras/sty148

    Dark energy constraints from the thermal Sunyaev–Zeldovich power spectrum
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    • Bolliet, Boris; Comis, Barbara; Komatsu, Eiichiro
    • Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 4
    • DOI: 10.1093/mnras/sty823

    Testing Sunyaev–Zel'dovich measurements of the hot gas content of dark matter haloes using synthetic skies
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    • Le Brun, Amandine M. C.; McCarthy, Ian G.; Melin, Jean-Baptiste
    • Monthly Notices of the Royal Astronomical Society, Vol. 451, Issue 4
    • DOI: 10.1093/mnras/stv1172

    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
    • DOI: 10.3847/1538-4357/ab5c1c

    Balloon-borne Cosmic Microwave Background experiments
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    Generalised uncertainty relations from superpositions of geometries
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    • Lake, Matthew J.; Miller, Marek; Ganardi, Ray F.
    • Classical and Quantum Gravity, Vol. 36, Issue 15
    • DOI: 10.1088/1361-6382/ab2160

    Link between E – B polarization modes and gas column density from interstellar dust emission
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    Hydrostatic mass profiles in X-COP galaxy clusters
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    PreProFit: Pressure Profile Fitter for galaxy clusters
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    Properties of the Inctracluster Medium Assuming an Einasto Dark Matter Profile
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    Detection of the pairwise kinematic Sunyaev-Zel'dovich effect with BOSS DR11 and the Atacama Cosmology Telescope
    journal, March 2017

    • Bernardis, F. De; Aiola, S.; Vavagiakis, E. M.
    • Journal of Cosmology and Astroparticle Physics, Vol. 2017, Issue 03
    • DOI: 10.1088/1475-7516/2017/03/008

    A high-resolution, dust-selected molecular cloud catalogue of M33, the Triangulum Galaxy
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    • 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

    Azimuthally resolved X-ray spectroscopy to the edge of the Perseus Cluster
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    • Urban, O.; Simionescu, A.; Werner, N.
    • Monthly Notices of the Royal Astronomical Society, Vol. 437, Issue 4
    • DOI: 10.1093/mnras/stt2209

    New constraints on time-dependent variations of fundamental constants using Planck data
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    • Hart, Luke; Chluba, Jens
    • Monthly Notices of the Royal Astronomical Society, Vol. 474, Issue 2
    • DOI: 10.1093/mnras/stx2783

    Linear polarization structures in LOFAR observations of the interstellar medium in the 3C 196 field
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    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

    Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope
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    The magnetic field and dust filaments in the Polaris Flare
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    • Panopoulou, G. V.; Psaradaki, I.; Tassis, K.
    • Monthly Notices of the Royal Astronomical Society, Vol. 462, Issue 2
    • DOI: 10.1093/mnras/stw1678

    Rotation of the CMB polarization by foreground lensing
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    Gas clumping in galaxy clusters
    journal, January 2015

    • Eckert, D.; Roncarelli, M.; Ettori, S.
    • Monthly Notices of the Royal Astronomical Society, Vol. 447, Issue 3
    • DOI: 10.1093/mnras/stu2590

    A plethora of diffuse steep spectrum radio sources in Abell 2034 revealed by LOFAR
    journal, March 2016

    • Shimwell, T. W.; Luckin, J.; Brüggen, M.
    • Monthly Notices of the Royal Astronomical Society, Vol. 459, Issue 1
    • DOI: 10.1093/mnras/stw661

    The C-Band All-Sky Survey (C-BASS): design and capabilities
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    • Jones, Michael E.; Taylor, Angela C.; Aich, Moumita
    • Monthly Notices of the Royal Astronomical Society, Vol. 480, Issue 3
    • DOI: 10.1093/mnras/sty1956

    AzTEC 1.1 mm observations of high-z protocluster environments: SMG overdensities and misalignment between AGN jets and SMG distribution
    journal, June 2018

    • Zeballos, M.; Aretxaga, I.; Hughes, D. H.
    • Monthly Notices of the Royal Astronomical Society, Vol. 479, Issue 4
    • DOI: 10.1093/mnras/sty1714

    Radiative Transfer with POLARIS. II. Modeling of Synthetic Galactic Synchrotron Observations
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    • Reissl, Stefan; Brauer, Robert; Klessen, Ralf S.
    • The Astrophysical Journal, Vol. 885, Issue 1
    • DOI: 10.3847/1538-4357/ab3664

    Modeling the Anomalous Microwave Emission with Spinning Nanoparticles: No PAHs Required
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    Planck 2015 results : VI. LFI mapmaking
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    CMB bounds on disk-accreting massive primordial black holes
    journal, October 2017

    Kinematic Sunyaev-Zel’dovich Effect with Projected Fields: A Novel Probe of the Baryon Distribution with Planck, WMAP, and WISE Data
    journal, July 2016

    A Limit on the Warm Dark Matter Particle Mass from the Redshifted 21 cm Absorption Line
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    • Safarzadeh, Mohammadtaher; Scannapieco, Evan; Babul, Arif
    • The Astrophysical Journal, Vol. 859, Issue 2
    • DOI: 10.3847/2041-8213/aac5e0

    Most Frequent Value Statistics and the Hubble Constant
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    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 2.3 GHz continuum survey of the GEM project
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    General Relativity and Cosmology: Unsolved Questions and Future Directions
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    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

    Gone after one orbit: How cluster environments quench galaxies
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    • Lotz, Marcel; Remus, Rhea-Silvia; Dolag, Klaus
    • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 4
    • DOI: 10.1093/mnras/stz2070

    Forecasting the Contribution of Polarized Extragalactic Radio Sources in CMB Observations
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    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

    Mapping stellar content to dark matter haloes – III. Environmental dependence and conformity of galaxy colours
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    • Zu, Ying; Mandelbaum, Rachel
    • Monthly Notices of the Royal Astronomical Society, Vol. 476, Issue 2
    • DOI: 10.1093/mnras/sty279

    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

    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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    LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content
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    • Mulroy, Sarah L.; Farahi, Arya; Evrard, August E.
    • Monthly Notices of the Royal Astronomical Society, Vol. 484, Issue 1
    • DOI: 10.1093/mnras/sty3484

    Developing the 3-point Correlation Function for the Turbulent Interstellar Medium
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    • Portillo, Stephen K. N.; Slepian, Zachary; Burkhart, Blakesley
    • The Astrophysical Journal, Vol. 862, Issue 2
    • DOI: 10.3847/1538-4357/aacb80

    SILCC-Zoom: Polarization and depolarization in molecular clouds
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    • Seifried, D.; Walch, S.; Reissl, S.
    • Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 2
    • DOI: 10.1093/mnras/sty2831

    Ultraviolet HST Spectroscopy of Planck Cold Clumps
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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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    Morphological estimators on Sunyaev–Zel'dovich maps of MUSIC clusters of galaxies
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    • Cialone, Giammarco; De Petris, Marco; Sembolini, Federico
    • Monthly Notices of the Royal Astronomical Society, Vol. 477, Issue 1
    • DOI: 10.1093/mnras/sty621

    Analytical model for non-thermal pressure in galaxy clusters – III. Removing the hydrostatic mass bias
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    • Shi, Xun; Komatsu, Eiichiro; Nagai, Daisuke
    • Monthly Notices of the Royal Astronomical Society, Vol. 455, Issue 3
    • DOI: 10.1093/mnras/stv2504

    EXTRAGALACTIC MILLIMETER-WAVE POINT-SOURCE CATALOG, NUMBER COUNTS AND STATISTICS FROM 771 deg 2 OF THE SPT-SZ SURVEY
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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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    • Beattie, James R.; Federrath, Christoph
    • Monthly Notices of the Royal Astronomical Society, Vol. 492, Issue 1
    • DOI: 10.1093/mnras/stz3377

    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

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

    The Far-infrared Polarization Spectrum of ρ Ophiuchi A from HAWC+/SOFIA Observations
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    • Santos, Fabio P.; Chuss, David T.; Dowell, C. Darren
    • The Astrophysical Journal, Vol. 882, Issue 2
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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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    • Chen, T.; Remazeilles, M.; Dickinson, C.
    • Monthly Notices of the Royal Astronomical Society, Vol. 479, Issue 3
    • DOI: 10.1093/mnras/sty1730

    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
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    • 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

    Galactic cold cores: V. Dust opacity ⋆⋆⋆⋆⋆⋆⋆⋆⋆⋆
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    A CATALOG OF 1.5273 μ m DIFFUSE INTERSTELLAR BANDS BASED ON APOGEE HOT TELLURIC CALIBRATORS
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    • Elyajouri, M.; Monreal-Ibero, A.; Remy, Q.
    • The Astrophysical Journal Supplement Series, Vol. 225, Issue 2
    • DOI: 10.3847/0067-0049/225/2/19

    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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    • 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

    ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19
    journal, June 2019

    Beyond Optical Depth: Future Determination of Ionization History from the Cosmic Microwave Background
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    • Watts, D. J.; Addison, G. E.; Bennett, C. L.
    • The Astrophysical Journal, Vol. 889, Issue 2
    • DOI: 10.3847/1538-4357/ab5fd5

    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

    Towards a realistic population of simulated galaxy groups and clusters
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    • Le Brun, Amandine M. C.; McCarthy, Ian G.; Schaye, Joop
    • Monthly Notices of the Royal Astronomical Society, Vol. 441, Issue 2
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    Independent cosmological constraints from high-z H ii galaxies
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    • González-Morán, Ana Luisa; Chávez, Ricardo; Terlevich, Roberto
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
    • DOI: 10.1093/mnras/stz1577

    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
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    The supernova-regulated ISM: IV. A comparison of simulated polarization with Planck observations
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    Evolution of oh and Co-Dark Molecular gas Fraction Across a Molecular Cloud Boundary in Taurus
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    Large-Scale Features of the Radio Sky and a Model for Loop I
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    Unlocking Sensitivity for Visibility-based Estimators of the 21 cm Reionization Power Spectrum
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    • Zhang, Yunfan Gerry; Liu, Adrian; Parsons, Aaron R.
    • The Astrophysical Journal, Vol. 852, Issue 2
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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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    • Eswaraiah, Chakali; Lai, Shih-Ping; Chen, Wen-Ping
    • The Astrophysical Journal, Vol. 850, Issue 2
    • DOI: 10.3847/1538-4357/aa917e

    Covariant polarized radiative transfer on cosmological scales for investigating large-scale magnetic field structures
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    • Chan, Jennifer Y. H.; Wu, Kinwah; On, Alvina Y. L.
    • Monthly Notices of the Royal Astronomical Society, Vol. 484, Issue 2
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    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
    • DOI: 10.1142/9789814623995_0018

    Cosmology and astrophysics from relaxed galaxy clusters – III. Thermodynamic profiles and scaling relations
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    • Mantz, A. B.; Allen, S. W.; Morris, R. G.
    • Monthly Notices of the Royal Astronomical Society, Vol. 456, Issue 4
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    Background model systematics for the Fermi GeV excess
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    • Calore, Francesca; Cholis, Ilias; Weniger, Christoph
    • Journal of Cosmology and Astroparticle Physics, Vol. 2015, Issue 03
    • DOI: 10.1088/1475-7516/2015/03/038

    Statistical properties of polarized CMB foreground maps
    journal, June 2019

    • von Hausegger, Sebastian; Gammelgaard Ravnebjerg, Aske; Liu, Hao
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
    • DOI: 10.1093/mnras/stz1582

    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

    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

    Dust models compatible with Planck intensity and polarization data in translucent lines of sight
    journal, February 2018

    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

    2 mm GISMO Observations of the Galactic Center. I. Dust Emission
    journal, November 2019

    • Arendt, Richard G.; Staguhn, Johannes; Dwek, Eli
    • The Astrophysical Journal, Vol. 885, Issue 1
    • DOI: 10.3847/1538-4357/ab451c

    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

    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

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

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

    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

    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

    Mitigating Complex Dust Foregrounds in Future Cosmic Microwave Background Polarization Experiments
    journal, January 2018

    IMAGINE: a comprehensive view of the interstellar medium, Galactic magnetic fields and cosmic rays
    journal, August 2018

    • Boulanger, François; Enßlin, Torsten; Fletcher, Andrew
    • Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 08
    • DOI: 10.1088/1475-7516/2018/08/049

    Peak star formation efficiency and no missing baryons in massive spirals
    journal, June 2019

    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

    Constraints on Primordial Gravitational Waves Using P l a n c k , WMAP, and New BICEP2/ K e c k Observations through the 2015 Season
    journal, November 2018

    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

    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

    DEEP CHANDRA , HST -COS, AND MEGACAM OBSERVATIONS OF THE PHOENIX CLUSTER: EXTREME STAR FORMATION AND AGN FEEDBACK ON HUNDRED KILOPARSEC SCALES
    journal, September 2015

    • McDonald, Michael; McNamara, Brian R.; Weeren, Reinout J. van
    • The Astrophysical Journal, Vol. 811, Issue 2
    • DOI: 10.1088/0004-637x/811/2/111

    First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud
    journal, April 2018

    • Ashton, Peter C.; Ade, Peter A. R.; Angilè, Francesco E.
    • The Astrophysical Journal, Vol. 857, Issue 1
    • DOI: 10.3847/1538-4357/aab3ca

    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

    Planck  intermediate results. XII: Diffuse Galactic components in the Gould Belt system
    journal, August 2013

    A New Detection of Extragalactic Anomalous Microwave Emission in a Compact, Optically Faint Region of NGC 4725
    journal, July 2018

    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

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

    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

    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

    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

    Statistical analysis of the interplay between interstellar magnetic fields and filaments hosting Planck Galactic cold clumps
    journal, February 2019

    • Alina, D.; Ristorcelli, I.; Montier, L.
    • Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 2
    • DOI: 10.1093/mnras/stz508

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

    Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
    journal, April 2015

    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
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