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Infobox for articles on galaxy groups and galaxy clusters. Intended for the creation of new galaxy cluster pages and for updating older pages with outdated infoboxes.
{{Infobox galaxy cluster
| name =
| image =
| image_size =
| alt =
| caption =
| credit = <!-- Per MOS:CREDITS, credits are discouraged -->
| epoch =
| constellation =
| ra = {{RA|00|00}} <!-- or {{Deg2HMS|000.00000|sup=yes}} -->
| dec = {{DEC|±00|00}}
| brightest_member =
| member_no =
| parent =
| major_axis_mpc =
| minor_axis_mpc =
| richness =
| bmtype =
| velocity_dispersion =
| redshift =
| distance = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0.00}}
| temperature =
| mass = 0{{e|14}} {{hub|0.00}} <!-- In solar masses -->
| luminosity =
| flux =
| notes =
| other_names =
| names =
| references =
| ra =
}}
Parameters
Parameter
Description
name
Name of the object wikilinked to the parent catalog page, i.e. Abell 370, NGC 7318, etc.
image
Associated image of the object: [[File:name.png|300px]]
caption
Text underneath the image.
credit
To whom do we owe this great pleasure?
epoch
Equatorial coordinates based on which epoch? If other than J2000, please find or convert to J2000.
Abell (or related) richness class. Based on number of members within a magnitude range of m3 to m3+2, where m3 is the magnitude of the third brightest member of the cluster. Not to be mistaken for the total number of galaxies in the cluster. Link to the digital version of the entire Abell Catalog is here.
NED's default value for the dimensionless Hubble parameter is 0.73 using the WMAP 3-year results, but one is able to change this to match the WMAP 5-year results with h=0.705.
If measurement is left in 'units' of h: {{hub}} gives hScript error: No such module "Su".
If h=0.73 is used: {{hub|0.73}} gives hScript error: No such module "Su".
{{convert|100|Mpc|Mly|2|abbr=on|lk=on}}{{hub|0.73}} gives Script error: No such module "convert".hScript error: No such module "Su".
{{convert|100|+/-|20|Mpc|Mly|abbr=on|lk=on}}{{hub|0.73}} gives Script error: No such module "convert".hScript error: No such module "Su".
Use Gpc as appropriate and/or feel free to leave off the light-year conversion if it becomes unwieldy. Parsecs are less ambiguous and are preferred over light-years, especially at cosmological distances (and also at nearby distances were parallaxes can be measured).