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Title: Planck intermediate results: XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck $$\star$$

Abstract

The nearby Chamaeleon clouds have been observed in γ rays by the Fermi Large Area Telescope (LAT) and in thermal dust emission by Planck and IRAS. Cosmic rays and large dust grains, if smoothly mixed with gas, can jointly serve with the HI and 12CO radio data to (i) map the hydrogen column densities, NH, in the different gas phases, in particular at the dark neutral medium (DNM) transition between the HI-bright and CO-bright media; (ii) constrain the CO-to-H2 conversion factor, XCO; and (iii) probe the dust properties per gas nucleon in each phase and map their spatial variations across the clouds. We have separated clouds at local, intermediate, and Galactic velocities in HI and 12CO line emission to model in parallel the γ-ray intensity recorded between 0.4 and 100 GeV; the dust optical depth at 353 GHz, τ353; the thermal radiance of the large grains; and an estimate of the dust extinction, AVQ, empirically corrected for the starlight intensity. The dust and γ-ray models have been coupled to account for the DNM gas. The consistent γ-ray emissivity spectra recorded in the different phases confirm that the GeV-TeV cosmic rays probed by the LAT uniformly permeate all gas phases upmore » to the 12CO cores. The dust and cosmic rays both reveal large amounts of DNM gas, with comparable spatial distributions and twice as much mass as in the CO-bright clouds. We give constraints on the HI-DNM-CO transitions for five separate clouds. CO-dark H2 dominates the molecular columns up to AV ≃ 0.9 and its mass often exceeds the one-third of the molecular mass expected by theory. The corrected AVQ extinction largely provides the best fit to the total gas traced by the γ rays. Nevertheless, we find evidence for a marked rise in AVQ/NH with increasing NH and molecular fraction, and with decreasing dust temperature. The rise in τ353/NH is even steeper. We observe variations of lesser amplitude and orderliness for the specific power of the grains, except for a coherent decline by half in the CO cores. This combined information suggests grain evolution. We provide average values for the dust properties per gas nucleon in the different phases. The γ rays and dust radiance yield consistent XCO estimates near 0.7 × 1020 cm-2 K-1 km-1s. The AVQ and τ353 tracers yield biased values because of the large rise in grain opacity in the CO clouds. These results clarify a recurrent disparity in the γ-ray versus dust calibration of XCO, but they confirm the factor of 2 difference found between the XCO estimates in nearby clouds and in the neighbouring spiral arms.« less

Authors:
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; « less
Publication Date:
Research Org.:
SLAC National Accelerator Lab., Menlo Park, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
Contributing Org.:
Planck and Fermi Collaborations
OSTI Identifier:
1354894
Alternate Identifier(s):
OSTI ID: 1525111
Grant/Contract Number:  
AC02-76SF00515; AC02-05CH11231
Resource Type:
Accepted Manuscript
Journal Name:
Astronomy and Astrophysics
Additional Journal Information:
Journal Volume: 582; Journal ID: ISSN 0004-6361
Publisher:
EDP Sciences
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Gamma rays; ISM; local insterstellar matter; cosmic rays; dust; extinction; structure

Citation Formats

Ade, P. A. R., Aghanim, N., Aniano, G., Arnaud, M., Ashdown, M., 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., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Casandjian, J. M., Catalano, A., Chamballu, A., Chiang, H. C., Christensen, P. R., 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., Désert, F. -X., Dickinson, C., Diego, J. M., Digel, S. W., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Frejsel, A., Fukui, Y., Galeotta, S., Galli, S., Ganga, K., Ghosh, T., Giard, M., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Grenier, I. A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D. L., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jones, W. C., Juvela, M., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., 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., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Mazzotta, P., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Munshi, D., Murphy, J. A., Naselsky, P., Natoli, P., Nørgaard-Nielsen, H. U., Novikov, D., Novikov, I., Oxborrow, C. A., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Pasian, F., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Plaszczynski, S., Pointecouteau, E., Polenta, G., Popa, L., Pratt, G. W., Prunet, S., Puget, J. -L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ristorcelli, I., Rocha, G., Roudier, G., Rusholme, B., Sandri, M., Santos, D., Scott, D., Spencer, L. D., Stolyarov, V., Strong, A. W., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Tibaldo, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., Yvon, D., Zacchei, A., and Zonca, A. Planck intermediate results: XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck $\star$. United States: N. p., 2015. Web. doi:10.1051/0004-6361/201424955.
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Ade, P. A. R., Aghanim, N., Aniano, G., Arnaud, M., Ashdown, M., 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., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Casandjian, J. M., Catalano, A., Chamballu, A., Chiang, H. C., Christensen, P. R., 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., Désert, F. -X., Dickinson, C., Diego, J. M., Digel, S. W., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Frejsel, A., Fukui, Y., Galeotta, S., Galli, S., Ganga, K., Ghosh, T., Giard, M., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Grenier, I. A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D. L., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jones, W. C., Juvela, M., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., 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., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Mazzotta, P., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Munshi, D., Murphy, J. A., Naselsky, P., Natoli, P., Nørgaard-Nielsen, H. U., Novikov, D., Novikov, I., Oxborrow, C. A., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Pasian, F., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Plaszczynski, S., Pointecouteau, E., Polenta, G., Popa, L., Pratt, G. W., Prunet, S., Puget, J. -L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ristorcelli, I., Rocha, G., Roudier, G., Rusholme, B., Sandri, M., Santos, D., Scott, D., Spencer, L. D., Stolyarov, V., Strong, A. W., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Tibaldo, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., Yvon, D., Zacchei, A., & Zonca, A. Planck intermediate results: XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck $\star$. United States. https://doi.org/10.1051/0004-6361/201424955
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Ade, P. A. R., Aghanim, N., Aniano, G., Arnaud, M., Ashdown, M., 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., Burigana, C., Butler, R. C., Calabrese, E., Cardoso, J. -F., Casandjian, J. M., Catalano, A., Chamballu, A., Chiang, H. C., Christensen, P. R., 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., Désert, F. -X., Dickinson, C., Diego, J. M., Digel, S. W., Dole, H., Donzelli, S., Doré, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Enßlin, T. A., Eriksen, H. K., Falgarone, E., Finelli, F., Forni, O., Frailis, M., Fraisse, A. A., Franceschi, E., Frejsel, A., Fukui, Y., Galeotta, S., Galli, S., Ganga, K., Ghosh, T., Giard, M., Gjerløw, E., González-Nuevo, J., Górski, K. M., Gregorio, A., Grenier, I. A., Gruppuso, A., Hansen, F. K., Hanson, D., Harrison, D. L., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S. R., Hivon, E., Hobson, M., Holmes, W. A., Hovest, W., Huffenberger, K. M., Hurier, G., Jaffe, A. H., Jaffe, T. R., Jones, W. C., Juvela, M., Keihänen, E., Keskitalo, R., Kisner, T. S., Kneissl, R., 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., Maris, M., Marshall, D. J., Martin, P. G., Martínez-González, E., Masi, S., Matarrese, S., Mazzotta, P., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Munshi, D., Murphy, J. A., Naselsky, P., Natoli, P., Nørgaard-Nielsen, H. U., Novikov, D., Novikov, I., Oxborrow, C. A., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Pasian, F., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Plaszczynski, S., Pointecouteau, E., Polenta, G., Popa, L., Pratt, G. W., Prunet, S., Puget, J. -L., Rachen, J. P., Reach, W. T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ristorcelli, I., Rocha, G., Roudier, G., Rusholme, B., Sandri, M., Santos, D., Scott, D., Spencer, L. D., Stolyarov, V., Strong, A. W., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J. A., Terenzi, L., Tibaldo, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L. A., Wandelt, B. D., Wehus, I. K., Yvon, D., Zacchei, A., and Zonca, A. Wed . "Planck intermediate results: XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck $\star$". United States. https://doi.org/10.1051/0004-6361/201424955. https://www.osti.gov/servlets/purl/1354894.
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@article{osti_1354894,
title = {Planck intermediate results: XXVIII. Interstellar gas and dust in the Chamaeleon clouds as seen by Fermi LAT and Planck $\star$},
author = {Ade, P. A. R. and Aghanim, N. and Aniano, G. and Arnaud, M. and Ashdown, M. 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 Burigana, C. and Butler, R. C. and Calabrese, E. and Cardoso, J. -F. and Casandjian, J. M. and Catalano, A. and Chamballu, A. and Chiang, H. C. and Christensen, P. R. 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 Désert, F. -X. and Dickinson, C. and Diego, J. M. and Digel, S. W. 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 Finelli, F. and Forni, O. and Frailis, M. and Fraisse, A. A. and Franceschi, E. and Frejsel, A. and Fukui, Y. 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 Grenier, I. A. and Gruppuso, A. and Hansen, F. K. and Hanson, D. and Harrison, D. L. and Henrot-Versillé, S. and Hernández-Monteagudo, C. and Herranz, D. and Hildebrandt, S. R. and Hivon, E. and Hobson, M. and Holmes, W. A. and Hovest, W. and Huffenberger, K. M. and Hurier, G. and Jaffe, A. H. and Jaffe, T. R. and Jones, W. C. and Juvela, M. and Keihänen, E. and Keskitalo, R. and Kisner, T. S. and Kneissl, R. 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 Maris, M. and Marshall, D. J. 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 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 Natoli, P. and Nørgaard-Nielsen, H. U. and Novikov, D. and Novikov, I. and Oxborrow, C. A. and Pagano, L. and Pajot, F. and Paladini, R. and Paoletti, D. and Pasian, F. and Perdereau, O. and Perotto, L. and Perrotta, F. and Pettorino, V. and Piacentini, F. and Piat, M. and Plaszczynski, S. and Pointecouteau, E. and Polenta, G. and Popa, L. and Pratt, G. W. and Prunet, S. and Puget, J. -L. and Rachen, J. P. and Reach, W. T. and Rebolo, R. and Reinecke, M. and Remazeilles, M. and Renault, C. and Ristorcelli, I. and Rocha, G. and Roudier, G. and Rusholme, B. and Sandri, M. and Santos, D. and Scott, D. and Spencer, L. D. and Stolyarov, V. and Strong, A. W. and Sudiwala, R. and Sunyaev, R. and Sutton, D. and Suur-Uski, A. -S. and Sygnet, J. -F. and Tauber, J. A. and Terenzi, L. and Tibaldo, L. and Toffolatti, L. and Tomasi, M. and Tristram, M. and Tucci, M. and Umana, G. 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 Yvon, D. and Zacchei, A. and Zonca, A.},
abstractNote = {The nearby Chamaeleon clouds have been observed in γ rays by the Fermi Large Area Telescope (LAT) and in thermal dust emission by Planck and IRAS. Cosmic rays and large dust grains, if smoothly mixed with gas, can jointly serve with the HI and 12CO radio data to (i) map the hydrogen column densities, NH, in the different gas phases, in particular at the dark neutral medium (DNM) transition between the HI-bright and CO-bright media; (ii) constrain the CO-to-H2 conversion factor, XCO; and (iii) probe the dust properties per gas nucleon in each phase and map their spatial variations across the clouds. We have separated clouds at local, intermediate, and Galactic velocities in HI and 12CO line emission to model in parallel the γ-ray intensity recorded between 0.4 and 100 GeV; the dust optical depth at 353 GHz, τ353; the thermal radiance of the large grains; and an estimate of the dust extinction, AVQ, empirically corrected for the starlight intensity. The dust and γ-ray models have been coupled to account for the DNM gas. The consistent γ-ray emissivity spectra recorded in the different phases confirm that the GeV-TeV cosmic rays probed by the LAT uniformly permeate all gas phases up to the 12CO cores. The dust and cosmic rays both reveal large amounts of DNM gas, with comparable spatial distributions and twice as much mass as in the CO-bright clouds. We give constraints on the HI-DNM-CO transitions for five separate clouds. CO-dark H2 dominates the molecular columns up to AV ≃ 0.9 and its mass often exceeds the one-third of the molecular mass expected by theory. The corrected AVQ extinction largely provides the best fit to the total gas traced by the γ rays. Nevertheless, we find evidence for a marked rise in AVQ/NH with increasing NH and molecular fraction, and with decreasing dust temperature. The rise in τ353/NH is even steeper. We observe variations of lesser amplitude and orderliness for the specific power of the grains, except for a coherent decline by half in the CO cores. This combined information suggests grain evolution. We provide average values for the dust properties per gas nucleon in the different phases. The γ rays and dust radiance yield consistent XCO estimates near 0.7 × 1020 cm-2 K-1 km-1s. The AVQ and τ353 tracers yield biased values because of the large rise in grain opacity in the CO clouds. These results clarify a recurrent disparity in the γ-ray versus dust calibration of XCO, but they confirm the factor of 2 difference found between the XCO estimates in nearby clouds and in the neighbouring spiral arms.},
doi = {10.1051/0004-6361/201424955},
journal = {Astronomy and Astrophysics},
number = ,
volume = 582,
place = {United States},
year = {Wed Sep 30 00:00:00 EDT 2015},
month = {Wed Sep 30 00:00:00 EDT 2015}
}
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Fig. 1 Fig. 1: Maps toward the Chamaeleon region of the $γ$-ray counts recorded in the 0.4−100 GeV band and of the dust quantities (modified extinction $A$$VQ$ in magnitudes, optical depth $τ$353, and radiance $R$ in W m −2 sr−1). The total $γ$-ray photon counts are shown on the left and thosemore » spawned by cosmic-ray interactions with gas (after subtraction of other ancillary components) on the right. The $γ$-ray maps have been constructed on a 7.′5 pixel grid and smoothed with a Gaussian kernel of 0′.1 for display. The dust quantities are shown at 5′ resolution in the left panels, and at the Fermi LAT resolution on the right (after convolution with the energy-dependent response function of the LAT, assuming the local interstellar $γ$-ray spectrum over the 0.4−100 GeV band, tilded variables). Regions excluded from the analysis have been masked out.« less
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    • Ho, S. P.; Pappas, C. G.; Austermann, J.
    • Journal of Low Temperature Physics, Vol. 184, Issue 3-4
    • DOI: 10.1007/s10909-016-1573-1

    Relieving tensions related to the lensing of the cosmic microwave background temperature power spectra
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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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    Star-forming content of the giant molecular filaments in the Milky Way
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    Link between E – B polarization modes and gas column density from interstellar dust emission
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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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    • DOI: 10.1088/1475-7516/2015/03/038

    Exploring cosmic origins with CORE: B -mode component separation
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    • Remazeilles, M.; Banday, A. J.; Baccigalupi, C.
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    • DOI: 10.1088/1475-7516/2018/04/023

    Can the H 0 tension be resolved in extensions to ΛCDM cosmology?
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    • Guo, Rui-Yun; Zhang, Jing-Fei; Zhang, Xin
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    Analytical model for non-thermal pressure in galaxy clusters
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    • Shi, Xun; Komatsu, Eiichiro
    • Monthly Notices of the Royal Astronomical Society, Vol. 442, Issue 1
    • DOI: 10.1093/mnras/stu858

    Analytical model for non-thermal pressure in galaxy clusters – III. Removing the hydrostatic mass bias
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    • Shi, Xun; Komatsu, Eiichiro; Nagai, Daisuke
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    • DOI: 10.1093/mnras/stv2504

    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

    Sample variance in the local measurements of the Hubble constant
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    • Wu, Hao-Yi; Huterer, Dragan
    • Monthly Notices of the Royal Astronomical Society, Vol. 471, Issue 4
    • DOI: 10.1093/mnras/stx1967

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

    Escape of ionizing radiation from high-redshift dwarf galaxies: role of AGN feedback
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    • Trebitsch, Maxime; Volonteri, Marta; Dubois, Yohan
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    • DOI: 10.1093/mnras/sty1406

    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

    SU(2) cmb and the cosmological model: angular power spectra
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    • Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 4
    • DOI: 10.1093/mnras/sty2981

    A high-resolution, dust-selected molecular cloud catalogue of M33, the Triangulum Galaxy
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    • Monthly Notices of the Royal Astronomical Society, Vol. 483, Issue 4
    • DOI: 10.1093/mnras/sty3437

    LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content
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    • DOI: 10.1093/mnras/sty3484

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    • DOI: 10.1093/mnras/sty3521

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    journal, March 2018

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    • DOI: 10.1093/mnras/sty714

    The environment and host haloes of the brightest z ∼ 6 Lyman-break galaxies
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    • DOI: 10.1093/mnras/sty856

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

    • Gong, Yan; Ma, Yin-Zhe; Tanimura, Hideki
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    • DOI: 10.1093/mnras/stz1177

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

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

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

    • González-Morán, Ana Luisa; Chávez, Ricardo; Terlevich, Roberto
    • Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
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    Joint estimation of the Epoch of Reionization power spectrum and foregrounds
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    • Sims, Peter H.; Pober, Jonathan C.
    • Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 2
    • DOI: 10.1093/mnras/stz1888

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

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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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    • Jew, Luke; Taylor, Angela C.; Jones, Michael E.
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    • DOI: 10.1093/mnras/stz2697

    Statistical analysis of the interplay between interstellar magnetic fields and filaments hosting Planck Galactic cold clumps
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    • Alina, D.; Ristorcelli, I.; Montier, L.
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    • DOI: 10.1093/mnras/stz508

    The C-Band All-Sky Survey (C-BASS): constraining diffuse Galactic radio emission in the North Celestial Pole region
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    • Dickinson, C.; Barr, A.; Chiang, H. C.
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    • DOI: 10.1093/mnras/stz522

    Predictions and sensitivity forecasts for reionization-era [C  ii ] line intensity mapping
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    • DOI: 10.1093/mnras/stz617

    The role of initial magnetic field structure in the launching of protostellar jets
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    • Gerrard, Isabella A.; Federrath, Christoph; Kuruwita, Rajika
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    • DOI: 10.1093/mnras/stz784

    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

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

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

    Spatial variation of fundamental constants: Testing models with thermonuclear supernovae
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    Spectroscopic Confirmation and Velocity Dispersions for 20 Planck Galaxy Clusters at 0.16 < z < 0.78
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    Warm Dark Matter and Cosmic Reionization
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    • DOI: 10.3847/1538-4357/aa9ff5

    Full-data Results of Hubble Frontier Fields: UV Luminosity Functions at z ∼ 6–10 and a Consistent Picture of Cosmic Reionization
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    • Portillo, Stephen K. N.; Slepian, Zachary; Burkhart, Blakesley
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    • DOI: 10.3847/1538-4357/aacb80

    A Census of Galaxy Constituents in a Coma Progenitor Observed at z > 3
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    Weak-lensing Mass Calibration of ACTPol Sunyaev–Zel’dovich Clusters with the Hyper Suprime-Cam Survey
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    • Miyatake, Hironao; Battaglia, Nicholas; Hilton, Matt
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    • DOI: 10.3847/1538-4357/ab0af0

    Constraining the Neutral Fraction of Hydrogen in the IGM at Redshift 7.5
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    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
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    • DOI: 10.3847/2041-8213/aac5e0

    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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    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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    Generalised uncertainty relations from superpositions of geometries
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    • Classical and Quantum Gravity, Vol. 36, Issue 15
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    • van de Voort, Freeke; Quataert, Eliot; Hopkins, Philip F.
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    • DOI: 10.1093/mnras/stw2322

    Wide-field LOFAR-LBA power-spectra analyses: impact of calibration, polarization leakage, and ionosphere
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    • Gehlot, B. K.; Koopmans, L. V. E.; de Bruyn, A. G.
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    • DOI: 10.1093/mnras/sty1095

    X-ray and SZ constraints on the properties of hot CGM
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    • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 3
    • DOI: 10.1093/mnras/sty1276

    The FABLE simulations: a feedback model for galaxies, groups, and clusters
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    • Henden, Nicholas A.; Puchwein, Ewald; Shen, Sijing
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    Reionization in Technicolor
    journal, July 2018

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    • Monthly Notices of the Royal Astronomical Society, Vol. 480, Issue 2
    • DOI: 10.1093/mnras/sty1949

    The C-Band All-Sky Survey (C-BASS): design and capabilities
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    • DOI: 10.1093/mnras/sty1956

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

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

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

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

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

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

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

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

    Magnetic ionization–thermal instability
    journal, May 2019

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

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

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

    The Important Role of Cosmic-Ray Re-Acceleration
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    • The Astrophysical Journal, Vol. 843, Issue 1
    • DOI: 10.3847/1538-4357/aa7461

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

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

    On the Faint End of the Galaxy Luminosity Function in the Epoch of Reionization: Updated Constraints from the HST Frontier Fields
    journal, November 2018

    E and B Polarizations from Inhomogeneous and Solar Surface Turbulence
    journal, January 2019

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

    Ultraviolet HST Spectroscopy of Planck Cold Clumps
    journal, February 2019

    Time Evolution of 3D Disk Formation with Misaligned Magnetic Field and Rotation Axes
    journal, March 2019

    • Väisälä, Miikka S.; Shang, Hsien; Krasnopolsky, Ruben
    • The Astrophysical Journal, Vol. 873, Issue 2
    • DOI: 10.3847/1538-4357/ab0307

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

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

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

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

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

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

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

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

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

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

    Mapping the Magnetic Interstellar Medium in Three Dimensions over the Full Sky with Neutral Hydrogen
    journal, December 2019

    Multiwavelength Polarimetry of the Filamentary Cloud IC 5146. II. Magnetic Field Structures
    journal, December 2019

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

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

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

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

    Planck intermediate results : XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
    journal, February 2016

    A catalog of 1.5273 micron diffuse interstellar bands based on APOGEE hot telluric calibrators
    text, January 2016

    The comoving mass density of MgII from $z\sim2$ to $5.5$
    text, January 2017

    Dust-Gas Scaling Relations and OH Abundance in the Galactic ISM
    text, January 2018

    Optically thick HI does not dominate dark gas in the local ISM
    text, January 2018

    Gas and Dust Properties in the Chamaeleon Molecular Cloud Complex based on the Optically Thick HI
    text, January 2019

    The cosmic-ray content of the Orion-Eridanus superbubble
    text, January 2020

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