Difference between revisions of "Template:BibCite"
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|widrow=[http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=1086334 '''A Study of Rough Amplitude Quantization by Means of Nyquist Sampling Theory'''], B Widrow, IRE Transactions on Circuit Theory, '''CT-3(4)''', 266-276, (1956). | |widrow=[http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=1086334 '''A Study of Rough Amplitude Quantization by Means of Nyquist Sampling Theory'''], B Widrow, IRE Transactions on Circuit Theory, '''CT-3(4)''', 266-276, (1956). | ||
|banta=[http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=1053732 '''On the autocorrelation function of quantized signal plus noise'''], E. Banta, Information Theory, IEEE Transactions on, '''11''', 114 - 117, (1965). | |banta=[http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=1053732 '''On the autocorrelation function of quantized signal plus noise'''], E. Banta, Information Theory, IEEE Transactions on, '''11''', 114 - 117, (1965). | ||
| − | |arnaud2010=[http://arxiv.org/pdf/0910.1234v1.pdf '''The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the | + | |arnaud2010=[http://arxiv.org/pdf/0910.1234v1.pdf '''The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ - M_500 relation'''], M. Arnaud, G. W. Pratt, R. Piffaretti, H. Böhringer, J. H. Croston, E. Pointecouteau, ApJ, 517, A92, (2010). |
|polenta_CrossSpectra=[http://arxiv.org/pdf/astro-ph/0402428v2.pdf '''Unbiased estimation of an angular power spectrum'''], G. Polenta, D. Marinucci, A. Balbi, P. de Bernardis, E. Hivon, S. Masi, P. Natoli, N. Vittorio, J. Cosmology Astropart. Phys., '''11''', 1, (2005). | |polenta_CrossSpectra=[http://arxiv.org/pdf/astro-ph/0402428v2.pdf '''Unbiased estimation of an angular power spectrum'''], G. Polenta, D. Marinucci, A. Balbi, P. de Bernardis, E. Hivon, S. Masi, P. Natoli, N. Vittorio, J. Cosmology Astropart. Phys., '''11''', 1, (2005). | ||
|master=[http://arxiv.org/pdf/astro-ph/0105302v1.pdf '''MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets'''], E. Hivon, K. M. Górski, C. B. Netterfield, B. P. Crill, S. Prunet, F. Hansen, ApJ, '''567''', 2-17, (2002). | |master=[http://arxiv.org/pdf/astro-ph/0105302v1.pdf '''MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets'''], E. Hivon, K. M. Górski, C. B. Netterfield, B. P. Crill, S. Prunet, F. Hansen, ApJ, '''567''', 2-17, (2002). | ||
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|remazeilles2015=[http://adsabs.harvard.edu/abs/2015MNRAS.451.4311R '''An improved source-subtracted and destriped 408-MHz all-sky map'''], Remazeilles, M., Dickinson, C., Banday, A. J., Bigot-Sazy, M.-A., & Ghosh, T., MNRAS, 451, 4311, (2015). | |remazeilles2015=[http://adsabs.harvard.edu/abs/2015MNRAS.451.4311R '''An improved source-subtracted and destriped 408-MHz all-sky map'''], Remazeilles, M., Dickinson, C., Banday, A. J., Bigot-Sazy, M.-A., & Ghosh, T., MNRAS, 451, 4311, (2015). | ||
|cai2013=[http://adsabs.harvard.edu/abs/2013ApJ...768...21C '''A Hybrid Model for the Evolution of Galaxies and Active Galactic Nuclei in the Infrared'''], Cai, Z.-Y., Lapi, A., Xia, J.-Q., et al., ApJ, 768, 21, (2013). | |cai2013=[http://adsabs.harvard.edu/abs/2013ApJ...768...21C '''A Hybrid Model for the Evolution of Galaxies and Active Galactic Nuclei in the Infrared'''], Cai, Z.-Y., Lapi, A., Xia, J.-Q., et al., ApJ, 768, 21, (2013). | ||
| − | |blas2011=[http://adsabs.harvard.edu/abs/2011JCAP...07..034B '''The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes''' | + | |blas2011=[http://adsabs.harvard.edu/abs/2011JCAP...07..034B '''The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes'''], Blas, D., Lesgourgues, J., & Tram, T., J. Cosmology Astropart. Phys., 7, 034, (2011). |
|didio2013=[http://adsabs.harvard.edu/abs/2013JCAP...11..044D '''The CLASSgal code for relativistic cosmological large scale structure'''], Di Dio, E., Montanari, F., Lesgourgues, J., & Durrer, R., J. Cosmology Astropart. Phys., 11, 044, (2013). | |didio2013=[http://adsabs.harvard.edu/abs/2013JCAP...11..044D '''The CLASSgal code for relativistic cosmological large scale structure'''], Di Dio, E., Montanari, F., Lesgourgues, J., & Durrer, R., J. Cosmology Astropart. Phys., 11, 044, (2013). | ||
|Delabrouille2002=[http://adsabs.harvard.edu/abs/2002ASPC..257...81D '''AMiBA 2001: High-Z Clusters, Missing Baryons, and CMB Polarization'''], Delabrouille, J., Melin, J.-B., & Bartlett, J. G., Astronomical Society of the Pacific Conference Series, Vol. 257, (2002). | |Delabrouille2002=[http://adsabs.harvard.edu/abs/2002ASPC..257...81D '''AMiBA 2001: High-Z Clusters, Missing Baryons, and CMB Polarization'''], Delabrouille, J., Melin, J.-B., & Bartlett, J. G., Astronomical Society of the Pacific Conference Series, Vol. 257, (2002). | ||
Latest revision as of 08:49, 15 May 2018
Contents
Description
The template PlanckPapers produces references for papers cited in the text. T The syntax of PlanckPapers is
{{BibCite|label}}
where the only parameter is as follows:
- label
- label used to cite the paper in LaTeX;
Examples
Citing a paper in the text
What you type
{{BibCite|huffenberger2010}}
How it appears
A very interesting result can be found in [1].
Displaying the list of references at the bottom of a page
The convention followed in the Planck Explanatory Supplement is for the references to appear in the last section of each page. In order to achieve this, we suggest using:
==References== <references />
This is how the list of references below was created.
References
- ↑ Measuring Planck beams with planets, K. M. Huffenberger, B. P. Crill, A. E. Lange, K. M. Górski, C. R. Lawrence, A&A, 510, A58+, (2010).
