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 Y$_{SZ}$ - M$_{500}$ relation'''], M. Arnaud, G. W. Pratt, R. Piffaretti, H. Böhringer, J. H. Croston, E. Pointecouteau, ApJ, '''517''', A92, (2010).
+
|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

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

  1. 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).