మూస:Hub
Description
మార్చుMany properties of cosmological objects are reported with the addition of the dimensionless Hubble parameter h. This template addresses only the inverse Hubble parameter h−1
0.70 (since h0.70 is more straightforward to wikicode). If no subscript is specified, then the reader may choose a value of h of their liking to modify whatever the reported measurement is. If a subscript is specified, then the property being reported has been modified by the value of that subscript. For example, 7×1013 h−1
M☉ = 1014 h−1
0.70 M☉.
Our best measurement for the Hubble parameter is currently h = 0.704+0.013
−0.014 from the Wilkinson Microwave Anisotropy Probe (WMAP) 7 year data.[1]
Usage
మార్చుInstead of writing ''h''<small>{{su|p=−1|b=0.701|a=l}}</small>, one can simply do the following.
{{hub|0.701}} gives h−1
0.701 [1]
{{hub|0.75}} gives h−1
0.75 [2]
{{hub|}} gives h−1
[3]
{{hub}} gives h−1
{{{1}}}, which is an error. Like Mario, always remember your pipes.
See also
మార్చు- {{±}} : specific form of {{su}} with hard-coded positive {{sup}} and negative {{sub}}: 1+0.2
−0.4 - {{e}} : (1.23×104)
- {{su}} : general form of {{±}} for formatting exponents, or two-values incertainty one below the other (monospaced : currently not printable to PDF)
- {{sub}} : subscript text
- {{sup}} : superscript text
- {{Val/units}} : for formatting unit names (contents of parameters u or up)
- {{Val/unitswithlink}} : for formatting unit names with links (contents of parameters ul or upl)
- Subscript and superscript
References
మార్చు- ↑ Jarosik, N.; Bennett, C. L.; Dunkley, J.; Gold, B.; Greason, M. R.; Halpern, M.; Hill, R. S.; Hinshaw, G.; Kogut, A.; Komatsu, E.; Larson, D.; Limon, M.; Meyer, S. S.; Nolta, M. R.; Odegard, N.; Page, L.; Smith, K. M.; Spergel, D. N.; Tucker, G. S.; Weiland, J. L.; Wollack, E.; Wright, E. L. (2011). "Seven-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results" (PDF). The Astrophysical Journal Supplement. 192 (2). arXiv:1001.4744. Bibcode:2011ApJS..192...14J. doi:10.1088/0067-0049/192/2/14. 14. Retrieved March 11, 2012.