{{{name}}}
Observation data (Epoch {{{epoch}}})
Constellation(s){{{constellation}}}
Right ascension{{{ra}}}
Declination{{{dec}}}
Brightest member{{{brightest_member}}}
Number of clusters{{{member_no}}}
Major axis{{{major_axis_mpc}}}
Minor axis{{{minor_axis_mpc}}}
Redshift{{{redshift}}}
Distance
(co-moving)
{{{distance}}}
Binding mass{{{mass}}} M
Luminosity (specify){{{luminosity}}}
Flux (specify){{{flux}}}
Other designations
{{{other_names}}}
See also: Galaxy groups, Galaxy clusters, List of superclusters

Infobox for articles on superclusters of galaxies. Intended for the creation of new supercluster pages and for updating older pages with outdated infoboxes.

{{Infobox supercluster
| name = 
| image = 
| caption = 
| credit = 
| epoch = 
| constellation = 
| ra = {{RA|00|00}} or {{Deg2HMS|000.000|sup=yes}}
| dec = {{DEC|±00|00}}
| brightest_member = 
| member_no = 
| major_axis_mpc = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0.00}}
| minor_axis_mpc = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0.00}}
| redshift = 
| distance = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0.00}}
| mass = 0{{e|14}} {{hub|0.00}} <!-- In solar masses -->
| luminosity = ({{solar luminosity|link=y}}, if applicable)
| flux = 
| other_names = 
}}




<Name of the object> Supercluster, i.e. Shapley Supercluster

Associated image of the object: [[Image:name.png|400px]]

Text underneath the image.

To whom do we owe this great pleasure?

Equatorial coordinates based on which epoch? If other than J2000, please find or convert to J2000.

Wikilink(s) to constellation(s).

{{RA|00|00}} or {{Deg2HMS|000.000|sup=yes}}

{{DEC|±00|00}}

The brightest cluster.

The number of galaxy clusters belonging to the supercluster.

The major axis of the supercluster in h−1
 
, h−1
0.70
, h−1
0.75
, etc., megaparsecs. See distance section.

The minor axis of the supercluster in h−1
 
, h−1
0.70
, h−1
0.75
, etc., megaparsecs. See distance section.

  • z, if ≳ 0.1 : 0.8
  • z (km/s), if ≲ 0.1 : 0.0717 (21 500 km/s)

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.

  • 1.4{{e|14}} {{hub|0.70}} gives 1.4×1014 h−1
    0.70
    M

Make sure to specify the passband:

  • X-ray luminosity is usually given in erg s−1 for some keV range.
    • 1.4{{e|14}} [[erg]] s<sup>−1</sup> (0.1–2.4 [[electron volt|keV]]) gives 1.4×1014 erg s−1 (0.1–2.4 keV)
  • Visible or bolometric luminosity is usually given in L.

If available, use alternatively to luminosity. Make sure to specify the passband.

  • X-ray flux, usually given in erg s−1 cm−2 for some keV range.
    • (1.4 ± 0.2){{e|-11}} [[erg]] s<sup>−1</sup> cm<sup>−2</sup> (0.1–2.4 [[electron volt|keV]]) gives (1.4 ± 0.2)×10-11 erg s−1 cm−2 (0.1–2.4 keV)

Please don't list all the cross-identifications in NED for each object.

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