Difference between revisions of "Template:Infobox galaxy cluster/doc"

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imported>Zackmann08
(cleaning up documentation)
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{{Documentation subpage}}
 
{{Documentation subpage}}
 
<!-- PLEASE ADD CATEGORIES AND INTERWIKIS AT THE BOTTOM OF THIS PAGE. -->
 
<!-- PLEASE ADD CATEGORIES AND INTERWIKIS AT THE BOTTOM OF THIS PAGE. -->
 +
{{Lua|Module:Infobox|Module:InfoboxImage|Module:Check for unknown parameters}}
 +
{{Parameter names example|_template=| alt | bmtype | brightest_member | caption | constellation | credit | dec | distance | epoch | flux | image | image size | image_size | imagesize | luminosity | major_axis_mpc | mass | member_no | minor_axis_mpc | name | names | notes | other_names | ra | redshift | references | richness | temperature | velocity_dispersion }}
 
Infobox for articles on [[galaxy group]]s and [[galaxy cluster]]s. Intended for the creation of new galaxy cluster pages and for updating older pages with outdated infoboxes.
 
Infobox for articles on [[galaxy group]]s and [[galaxy cluster]]s. Intended for the creation of new galaxy cluster pages and for updating older pages with outdated infoboxes.
  
{{TOC left}}
 
 
== Usage ==
 
== Usage ==
{| style="background: transparent;"
+
<pre style="overflow: auto;">
|<pre>{{Infobox galaxy cluster
+
{{Infobox galaxy cluster
| name =  
+
| name               =  
| image =  
+
| image               =
| caption =  
+
| image size          =
| credit =  
+
| image_size          =
| epoch =  
+
| imagesize          =
| constellation =  
+
| alt                =  
| ra = {{RA|00|00}} <!-- or {{Deg2HMS|000.00000|sup=yes}} -->
+
| caption             =  
| dec = {{DEC|±00|00}}
+
| credit             =  
| brightest_member =  
+
| epoch               =  
| member_no =  
+
| constellation       =  
| richness =  
+
| ra                 = {{RA|00|00}} <!-- or {{Deg2HMS|000.00000|sup=yes}} -->
| bmtype =  
+
| dec                 = {{DEC|±00|00}}
 +
| brightest_member   =  
 +
| member_no           =
 +
| major_axis_mpc      =
 +
| minor_axis_mpc      =  
 +
| richness           =  
 +
| bmtype             =  
 
| velocity_dispersion =  
 
| velocity_dispersion =  
| redshift =  
+
| redshift           =  
| distance = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0.00}}
+
| distance           = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0.00}}
| temperature =  
+
| temperature         =  
| mass = 0{{e|14}} {{hub|0.00}} <!-- In solar masses -->
+
| mass               = 0{{e|14}} {{hub|0.00}} <!-- In solar masses -->
| luminosity =  
+
| luminosity         =  
| flux =  
+
| flux               =
| other_names =  
+
| notes              =  
}}</pre><br><br><br>
+
| other_names         =
|}
+
| names              =
{{clear}}
+
| references          =
 +
| ra =  
 +
}}</pre>
  
 
== Parameters ==
 
== Parameters ==
=== name ===
+
{| class="wikitable"
Name of the object wikilinked to the parent catalog page, i.e. [[Abell catalogue|Abell]] 370, [[New General Catalogue|NGC]] 7318, etc.
+
! Parameter
 
+
! Description
=== image ===
+
|-
Associated image of the object: <tt><code><nowiki>[[Image:name.png|300px]]</nowiki></code></tt>
+
|name
 
+
|Name of the object wikilinked to the parent catalog page, i.e. [[Abell catalogue|Abell]] 370, [[New General Catalogue|NGC]] 7318, etc.
=== caption ===
+
|-
Text underneath the image.
+
|image
 
+
|Associated image of the object: <tt><code><nowiki>[[Image:name.png|300px]]</nowiki></code></tt>
=== credit ===
+
|-
To whom do we owe this great pleasure?
+
|caption
 
+
|Text underneath the image.
=== epoch ===
+
|-
Equatorial coordinates based on which epoch? If other than [[J2000]], please [http://www.google.com find] or [http://ned.ipac.caltech.edu/forms/calculator.html convert] to J2000.
+
|credit
 
+
|To whom do we owe this great pleasure?
=== constellation ===
+
|-
Wikilink to constellation.
+
|epoch
 
+
|Equatorial coordinates based on which epoch? If other than [[J2000]], please [http://www.google.com find] or [http://ned.ipac.caltech.edu/forms/calculator.html convert] to J2000.
=== ra ===
+
|-
{{tlx|RA|00|00}} or {{tlx|Deg2HMS|000.00000|sup{{=}}yes}}
+
|constellation
 
+
|Wikilink to constellation.
=== dec ===
+
|-
{{tlx|DEC|±00|00}}
+
|ra
 
+
|{{tlx|RA|00|00}} or {{tlx|Deg2HMS|000.00000|sup{{=}}yes}}
=== brightest_member ===
+
|-
The brightest (visible) member.
+
|dec
 
+
|{{tlx|DEC|±00|00}}
=== member_no ===
+
|-
The number of galaxies belonging to the cluster, out to (at least) the [[virial theorem|virial radius]].
+
|brightest_member
 
+
|The brightest (visible) member.
=== richness ===
+
|-
[[Abell catalogue|Abell]] (or related) richness class. Based on number of members within a magnitude range of m<sub>3</sub> to m<sub>3</sub>+2, where m<sub>3</sub> 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 [http://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=VII/110A here].
+
|-
 
+
| member_no    
=== bmtype ===
+
|The number of galaxies belonging to the cluster, out to (at least) the [[virial theorem|virial radius]].
[[Bautz-Morgan classification]] type is available via [http://ned.ipac.caltech.edu/ NASA Extragalactic Database (NED)] or the [http://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=VII/110A digital version of the Abell Catalog].
+
|-
 
+
| richness    
=== velocity_dispersion ===
+
|[[Abell catalogue|Abell]] (or related) richness class. Based on number of members within a magnitude range of m<sub>3</sub> to m<sub>3</sub>+2, where m<sub>3</sub> 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 [http://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=VII/110A here].
[[Velocity dispersion]] of the cluster (as opposed to of only the core).
+
|-
 
+
| bmtype    
=== redshift ===
+
|[[Bautz-Morgan classification]] type is available via [http://ned.ipac.caltech.edu/ NASA Extragalactic Database (NED)] or the [http://vizier.u-strasbg.fr/cgi-bin/VizieR-2?-source=VII/110A digital version of the Abell Catalog].
* z, if ≳ 0.1 ''':''' <tt><code>0.8</code></tt>
+
|-
 +
| velocity_dispersion    
 +
|[[Velocity dispersion]] of the cluster (as opposed to of only the core).
 +
|-
 +
| redshift  
 +
|* z, if ≳ 0.1 ''':''' <tt><code>0.8</code></tt>
 
* z (km/s), if ≲ 0.1 ''':''' <tt><code>0.0717 (21 500 km/s)</code></tt>
 
* z (km/s), if ≲ 0.1 ''':''' <tt><code>0.0717 (21 500 km/s)</code></tt>
 
+
|-
=== distance ===
+
| distance  
NED's default value for the [[dimensionless Hubble parameter]] is 0.73 using the [[Wilkinson Microwave Anisotropy Probe|WMAP]] 3-year results, but one is able to change this to match the WMAP ''5-year'' results with h=0.705.
+
|NED's default value for the [[dimensionless Hubble parameter]] is 0.73 using the [[Wilkinson Microwave Anisotropy Probe|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: {{tlx|hub|}} gives {{hub|}}
 
* If measurement is left in 'units' of h: {{tlx|hub|}} gives {{hub|}}
 
* If h=0.73 is used: {{tlx|hub|0.73}} gives {{hub|0.73}}
 
* If h=0.73 is used: {{tlx|hub|0.73}} gives {{hub|0.73}}
Line 82: Line 96:
 
* {{tlx|convert|100|+/-|20|Mpc|Mly|abbr{{=}}on|lk{{=}}on}} {{tlx|hub|0.73}} gives {{convert|100|+/-|20|Mpc|Mly|abbr=on|lk=on}} {{hub|0.73}}
 
* {{tlx|convert|100|+/-|20|Mpc|Mly|abbr{{=}}on|lk{{=}}on}} {{tlx|hub|0.73}} gives {{convert|100|+/-|20|Mpc|Mly|abbr=on|lk=on}} {{hub|0.73}}
 
* 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).
 
* 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).
 
+
|-
=== temperature ===
+
| temperature  
[[X-ray]] temperature of the [[intracluster medium]], usually given in [[electron volt|keV]].
+
|[[X-ray]] temperature of the [[intracluster medium]], usually given in [[electron volt|keV]].
 
+
|-
=== mass ===
+
| mass    
* <tt><code><nowiki>1.4{{</nowiki>[[Template:e|e]]<nowiki>|14}} {{</nowiki>[[Template:hub|hub]]<nowiki>|0.70}}</nowiki></code></tt> gives 1.4{{e|14}} {{hub|0.70}} {{Solar mass|link=y}}
+
| <tt><code><nowiki>1.4{{</nowiki>[[Template:e|e]]<nowiki>|14}} {{</nowiki>[[Template:hub|hub]]<nowiki>|0.70}}</nowiki></code></tt> gives 1.4{{e|14}} {{hub|0.70}} {{Solar mass|link=y}}
 
+
|-
=== luminosity ===
+
| luminosity  
* [[X-ray]] luminosity, usually given in [[erg]] s<sup>−1</sup> for some [[electron volt|keV]] range.
+
|* [[X-ray]] luminosity, usually given in [[erg]] s<sup>−1</sup> for some [[electron volt|keV]] range.
 
* <tt><code><nowiki>1.4{{</nowiki>[[Template:e|e]]<nowiki>|14}} [[erg]] s<sup>−1</sup> (0.1—2.4 [[electron volt|keV]])</nowiki></code></tt> gives 1.4{{e|14}} [[erg]] s<sup>−1</sup> (0.1—2.4 [[electron volt|keV]])
 
* <tt><code><nowiki>1.4{{</nowiki>[[Template:e|e]]<nowiki>|14}} [[erg]] s<sup>−1</sup> (0.1—2.4 [[electron volt|keV]])</nowiki></code></tt> gives 1.4{{e|14}} [[erg]] s<sup>−1</sup> (0.1—2.4 [[electron volt|keV]])
 
+
|-
=== flux ===
+
| flux    
* [[X-ray]] flux, usually given in [[erg]] s<sup>−1</sup> cm<sup>−2</sup> for some [[electron volt|keV]] range.
+
|* [[X-ray]] flux, usually given in [[erg]] s<sup>−1</sup> cm<sup>−2</sup> for some [[electron volt|keV]] range.
 
* <tt><code><nowiki>(1.4 ± 0.2){{</nowiki>[[Template:e|e]]<nowiki>|-11}} [[erg]] s<sup>−1</sup> cm<sup>−2</sup> (0.1—2.4 [[electron volt|keV]])</nowiki></code></tt> gives (1.4 ± 0.2){{e|-11}} [[erg]] s<sup>−1</sup> cm<sup>−2</sup> (0.1—2.4 [[electron volt|keV]])
 
* <tt><code><nowiki>(1.4 ± 0.2){{</nowiki>[[Template:e|e]]<nowiki>|-11}} [[erg]] s<sup>−1</sup> cm<sup>−2</sup> (0.1—2.4 [[electron volt|keV]])</nowiki></code></tt> gives (1.4 ± 0.2){{e|-11}} [[erg]] s<sup>−1</sup> cm<sup>−2</sup> (0.1—2.4 [[electron volt|keV]])
 
+
|-
=== other_names ===
+
| other_names    
Please don't list all the cross-identifications in NED for each object.
+
|Please don't list all the cross-identifications in NED for each object.
 
+
|-
=== references ===
+
| references  
List general references for the infobox here to prevent clutter.
+
|List general references for the infobox here to prevent clutter.
 +
|}
  
 
== See also ==
 
== See also ==

Revision as of 23:57, 10 January 2019

Template:Parameter names example 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.

Usage

{{Infobox galaxy cluster
| name                = 
| image               = 
| image size          = 
| image_size          = 
| imagesize           = 
| alt                 = 
| caption             = 
| credit              = 
| epoch               = 
| constellation       = 
| ra                  = {{RA|00|00}} <!-- or {{Deg2HMS|000.00000|sup=yes}} -->
| dec                 = {{DEC|±00|00}}
| brightest_member    = 
| member_no           = 
| 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: [[Image: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.
constellation Wikilink to constellation.
ra {{RA|00|00}} or {{Deg2HMS|000.00000|sup=yes}}
dec {{DEC|±00|00}}
brightest_member The brightest (visible) member.
member_no The number of galaxies belonging to the cluster, out to (at least) the virial radius.
richness 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.
bmtype Bautz-Morgan classification type is available via NASA Extragalactic Database (NED) or the digital version of the Abell Catalog.
velocity_dispersion Velocity dispersion of the cluster (as opposed to of only the core).
redshift * z, if ≳ 0.1 : 0.8
  • z (km/s), if ≲ 0.1 : 0.0717 (21 500 km/s)
distance 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 h−1
     
  • If h=0.73 is used: {{hub|0.73}} gives h−1
    0.73
  • {{convert|100|Mpc|Mly|2|abbr=on|lk=on}} {{hub|0.73}} gives 100 Mpc (326.16 Mly) h−1
    0.73
  • {{convert|100|+/-|20|Mpc|Mly|abbr=on|lk=on}} {{hub|0.73}} gives 100 ± 20 Mpc (326 ± 65 Mly) h−1
    0.73
  • 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).
temperature X-ray temperature of the intracluster medium, usually given in keV.
mass 1.4{{e|14}} {{hub|0.70}} gives 1.4×1014 h−1
0.70
Template:Solar mass
luminosity * X-ray luminosity, 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)
flux * 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)×1011 erg s−1 cm−2 (0.1—2.4 keV)
other_names Please don't list all the cross-identifications in NED for each object.
references List general references for the infobox here to prevent clutter.

See also

Tracking category

External links