The DOI matches its Crossref record; 8 of the 8 references it cites were found in a registry or an index.
The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths
Open accessAbstract
We present the Planck Sky Model (PSM), a parametric model for generating all-sky, few arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, in both intensity and polarisation. Several options are implemented to model the cosmic microwave background, Galactic diffuse emission (synchrotron, free-free, thermal and spinning dust, CO lines), Galactic H ii regions, extragalactic radio sources, dusty galaxies, and thermal and kinetic Sunyaev-Zeldovich signals from clusters of galaxies. Each component is simulated by means of educated interpolations/extrapolations of data sets available at the time of the launch of the Planck mission, complemented by state-of-the-art models of the emission. Distinctive features of the simulations are spatially varying spectral properties of synchrotron and dust; different spectral parameters for each point source; modelling of the clustering properties of extragalactic sources and of the power spectrum of fluctuations in the cosmic infrared background. The PSM enables the production of random realisations of the sky emission, constrained to match observational data within their uncertainties. It is implemented in a software package that is regularly updated with incoming information from observations. The model is expected to serve as a useful tool for optimising planned microwave and sub-millimetre surveys and testing data processing and analysis pipelines. It is, in particular, used to develop and validate data analysis pipelines within the Planck collaboration. A version of the software that can be used for simulating the observations for a variety of experiments is made available on a dedicated website.
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Cites
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The Structure of Cold Dark Matter Halos
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MethodLewis, A., Challinor, A., & Lasenby, A. (2000) · The Astrophysical Journal · doi:10.1086/309179 · Cited by 4,920
Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., Limon, M., Meyer, S. S., Page, L., Spergel, D. N., Tucker, G. S., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377253 · Cited by 4,860
Cosmological parameters from CMB and other data: A Monte Carlo approach
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“The Cosmomc tool developed by Lewis & Bridle (2002) is an approach for constraining cosmological parameters from CMB observations.”
MethodThe Cosmic Microwave Background Spectrum from the Full COBE FIRAS Data Set
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“The assumed default CMB temperature is TCMB = 2.725 K (Fixsen et al. 1996; Fixsen 2009).”
BackgroundInfluentialMicrowave Interstellar Medium Emission Observed by the Wilkinson Microwave Anisotropy Probe
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Joint Analysis of BICEP2/ Keck Array and Planck Data
Ade, P. A. R., Aghanim, N., Ahmed, Z., Aikin, R. W., Alexander, K. D., Arnaud, M., Aumont, J., Baccigalupi, C., Banday, A. J., Barkats, D., et al. (2015) · Physical Review Letters · doi:10.1103/physrevlett.114.101301 · Cited by 1,013
Self-citationPlanck 2018 results: VIII. Gravitational lensing
Planck Collaboration, Aghanim, N., Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., et al. (2020) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201833886 · Cited by 747
Self-citationPlanck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
Planck Collaboration:, Ade, P. A. R., Aghanim, N., Alina, D., Alves, M. I. R., Armitage-Caplan, C., Arnaud, M., Arzoumanian, D., Ashdown, M., Atrio-Barandela, F., et al. (2015) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201424082 · Cited by 414
Self-citationPlanck Collaboration, Aghanim, N., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., et al. (2016) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201628890 · Cited by 399
Self-citationPlanck 2013 results. XVII. Gravitational lensing by large-scale structure
Planck Collaboration, Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., et al. (2014) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201321543 · Cited by 391
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Metadata
- Authors
- Delabrouille, J., Betoule, M., Melin, J.-B., Miville-Deschênes, M.-A., Gonzalez-Nuevo, J., Le Jeune, M., Castex, G., de Zotti, G., Basak, S., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Bernard, J.-P., Bouchet, F. R., Clements, D. L., da Silva, A., Dickinson, C., Dodu, F., Dolag, K., Elsner, F., Fauvet, L., Faÿ, G., Giardino, G., Leach, S., Lesgourgues, J., Liguori, M., Macías-Pérez, J. F., Massardi, M., Matarrese, S., Mazzotta, P., Montier, L., Mottet, S., Paladini, R., Partridge, B., Piffaretti, R., Prezeau, G., Prunet, S., Ricciardi, S., Roman, M., Schaefer, B., & Toffolatti, L.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2013-05
- Volume
- 553
- Pages
- A96
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2084377030
- Cited by
- 238
- References
- 8
- FWCI
- 17.14
- Type
- journal article
- Language
- en
- Open access
- green
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- Delabrouille, J., Betoule, M., Melin, J.-B., Miville-Deschênes, M.-A., Gonzalez-Nuevo, J., Le Jeune, M., Castex, G., de Zotti, G., Basak, S., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A. J., Bernard, J.-P., Bouchet, F. R., Clements, D. L., da Silva, A., Dickinson, C., Dodu, F., . . . Toffolatti, L. (2013). The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201220019
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