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		<title>&gt;Jjamulla at 00:22, 13 September 2024</title>
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		<updated>2024-09-13T00:22:56Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Documentation subpage}}&lt;br /&gt;
{{High-use}}&lt;br /&gt;
&amp;lt;!-- Please place categories where indicated at the bottom of this page and interwikis at Wikidata (see [[Wikipedia:Wikidata]]) --&amp;gt;&lt;br /&gt;
{{Lua|Module:Infobox|Module:InfoboxImage|Module:Check for unknown parameters}}&lt;br /&gt;
Infobox for articles on [[galaxy|galaxies]].&lt;br /&gt;
&lt;br /&gt;
The parameters whose title has &amp;quot;(V)&amp;quot; or &amp;quot;(B)&amp;quot; refer to visible or bolometric values.&lt;br /&gt;
&lt;br /&gt;
== Usage ==&lt;br /&gt;
{| style=&amp;quot;background: transparent;&amp;quot;&lt;br /&gt;
|&amp;lt;syntaxhighlight lang=&amp;quot;wikitext&amp;quot;&amp;gt;{{Infobox galaxy&lt;br /&gt;
 | name             = {{PAGENAME}}&lt;br /&gt;
 | image            = &amp;lt;!-- image --&amp;gt;&lt;br /&gt;
 | image_scale      = &amp;lt;!-- 1.5 --&amp;gt;&lt;br /&gt;
 | caption          = &amp;lt;!-- optional caption --&amp;gt;&lt;br /&gt;
 | alt              = &amp;lt;!-- alternative description when image is not visible --&amp;gt;&lt;br /&gt;
 | epoch            = &amp;lt;!--Epoch of coordinates--&amp;gt;&lt;br /&gt;
 | pronounce        = {{IPA-en|&amp;lt;!-- IPA string --&amp;gt;|}}&lt;br /&gt;
 | constellation name = &amp;lt;!-- Link to the constellation containing the galaxy --&amp;gt;&lt;br /&gt;
 | ra               = {{RA|00|00|00}} &amp;lt;!-- Right Ascension (Alt. {{Deg2HMS|000.0000|sup=yes}}) --&amp;gt;&lt;br /&gt;
 | dec              = {{DEC|±00|00|00}} &amp;lt;!--Declination--&amp;gt;&lt;br /&gt;
 | z                = &amp;lt;!-- Redshift --&amp;gt;&lt;br /&gt;
 | h_radial_v       = &amp;lt;!-- Heliocentric radial velocity (in km/s) {{val|####|##|u=km/s|fmt=commas}} --&amp;gt;&lt;br /&gt;
 | gal_v            = &amp;lt;!--Galactocentric velocity (in km/s) --&amp;gt;&lt;br /&gt;
 | dist_pc          = {{cvt|000|±|00|Mpc|Mly|order=flip|lk=on}}{{hub|0.73}} &amp;lt;!-- comoving distance --&amp;gt;&lt;br /&gt;
 | dist_ly          = {{cvt|000|±|00|Mpc|Mly|order=flip|lk=on}}&lt;br /&gt;
 | group_cluster    = &amp;lt;!-- Identifier for the host galaxy group or cluster, if any --&amp;gt;&lt;br /&gt;
 | type             = &amp;lt;!-- Galaxy morphological classification --&amp;gt;&lt;br /&gt;
 | mass             = &amp;lt;!-- In solar masses {{Val|0|e=0}} --&amp;gt;&lt;br /&gt;
 | mass_light_ratio = &amp;lt;!-- In solar units  --&amp;gt;&lt;br /&gt;
 | size             = &amp;lt;!-- In light years  --&amp;gt;&lt;br /&gt;
 | stars            = &amp;lt;!-- Estimate of the number of stars, usually in terms of the combined stellar mass: {{Val|#.#|e=#|ul=Solar mass}} --&amp;gt;&lt;br /&gt;
 | appmag_v         = &amp;lt;!-- Apparent magnitude in V band ([[UBV photometric system|Johnson-Cousins V  system]])--&amp;gt;&lt;br /&gt;
 | appmag_b         = &amp;lt;!-- Apparent magnitude in B band --&amp;gt;&lt;br /&gt;
 | absmag_v         = &amp;lt;!-- Absolute magnitude in V Band --&amp;gt;&lt;br /&gt;
 | mag_j            = &amp;lt;!-- IR magnitude in J Band --&amp;gt;&lt;br /&gt;
 | mag_h            = &amp;lt;!-- IR magnitude in H Band --&amp;gt;&lt;br /&gt;
 | mag_k            = &amp;lt;!-- IR magnitude in K Band --&amp;gt;&lt;br /&gt;
 | sbrightness      = &amp;lt;!-- Surface brightness per angular area, usually in mag/arcsec^2 --&amp;gt;&lt;br /&gt;
 | size_v           = &amp;lt;!-- Angular dimensions in the V band. Give units. {{Val|0.0|×|0.0|u=arcminute}} --&amp;gt;&lt;br /&gt;
 | half_light_radius_pc        = &amp;lt;!-- physical dimension, pc preferred --&amp;gt;&lt;br /&gt;
 | half_light_radius_arcminsec = &amp;lt;!-- apparent dimension --&amp;gt;&lt;br /&gt;
 | h1_scale_length_pc          = &amp;lt;!-- physical dimension, pc preferred --&amp;gt;&lt;br /&gt;
 | h1_scale_length_arcminsec   = &amp;lt;!-- apparent dimension --&amp;gt;&lt;br /&gt;
 | xray_radius_pc              = &amp;lt;!-- physical dimension, pc preferred --&amp;gt;&lt;br /&gt;
 | xray_radius_arcminsec       = &amp;lt;!-- apparent dimension --&amp;gt;&lt;br /&gt;
 | notes            = &amp;lt;!-- Unique features --&amp;gt;&lt;br /&gt;
 | names            = {{odlist | NGC= | Arp= | PGC= | UGC= }} &amp;lt;!--Other catalog designations--&amp;gt;&lt;br /&gt;
 | references       = &amp;lt;!-- Use inline references where available --&amp;gt;&lt;br /&gt;
}}&amp;lt;/syntaxhighlight&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
== Parameters ==&lt;br /&gt;
&lt;br /&gt;
=== z, h_radial_v, gal_v ===&lt;br /&gt;
These fields provide [[radial velocity]] values for the galaxy as a whole. The dimensionless quantity &amp;lt;code&amp;gt;z&amp;lt;/code&amp;gt; is the [[redshift]] parameter and is used when the value is very small, such as less than 0.1. The &amp;lt;code&amp;gt;h_radial_v&amp;lt;/code&amp;gt; gives the heliocentric radial velocity of the galaxy in units of km/s. The parameter &amp;lt;code&amp;gt;gal_v&amp;lt;/code&amp;gt; refers to the galactrocentric radial velocity (the radial velocity relative to the Milky Way), which can be found on NED under the section &amp;quot;Quantities Derived from Redshift&amp;quot; if one looks up a galaxy.&lt;br /&gt;
&lt;br /&gt;
=== dist_ly ===&lt;br /&gt;
The &amp;lt;code&amp;gt;dist_ly&amp;lt;/code&amp;gt; field lists the estimated distance to the galaxy in both [[light-year]]s and [[parsec]]s. To do so, use the {{tl|cvt}} template. For example: {{tlx|cvt|2810|+/-|90|kly|kpc|lk{{=}}on|_show_result=yes}}&lt;br /&gt;
* {{tl|hub}} identifies the [[dimensionless Hubble parameter]] used in the distance measurement. Using NED&amp;#039;s default value of 0.73, {{tlx|hub|0.73|_show_result=yes}}.&lt;br /&gt;
* {{tlx|hub|_show_result=yes}} if distance is left in &amp;#039;units&amp;#039; of h.&lt;br /&gt;
&lt;br /&gt;
=== group_cluster ===&lt;br /&gt;
The parameter {{para|group_cluster}} refers to the [[galaxy group]] or [[galaxy cluster]] that the galaxy is a member.&lt;br /&gt;
&lt;br /&gt;
=== type ===&lt;br /&gt;
The parameter {{para|type}} is the [[Galaxy morphological classification|de Vancoleurs morphological type]] of the galaxy. These can be found on NED or SIMBAD. (Note that a &amp;lt;code&amp;gt;^&amp;lt;/code&amp;gt; in NED is actually a superscript, so for example S0^0 should be written as S0&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt; .)&lt;br /&gt;
&lt;br /&gt;
In SIMBAD the morphological type is often given as a number between -6 and 11. To convert these into the de Vaucouleurs class, use this table from [[Galaxy morphological classification#Numerical Hubble stage|this article]]:&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;text-align: center; margin: 1em auto;&amp;quot;&lt;br /&gt;
|+ Converting numerical Hubble stage to de Vancoleurs classes&lt;br /&gt;
! Numerical Hubble stage&lt;br /&gt;
| −6&lt;br /&gt;
| −5&lt;br /&gt;
| −4&lt;br /&gt;
| −3&lt;br /&gt;
| −2&lt;br /&gt;
| −1&lt;br /&gt;
| 0&lt;br /&gt;
| 1&lt;br /&gt;
| 2&lt;br /&gt;
| 3&lt;br /&gt;
| 4&lt;br /&gt;
| 5&lt;br /&gt;
| 6&lt;br /&gt;
| 7&lt;br /&gt;
| 8&lt;br /&gt;
| 9&lt;br /&gt;
| 10&lt;br /&gt;
| 11&lt;br /&gt;
|-&lt;br /&gt;
!de Vaucouleurs class&lt;br /&gt;
| cE&lt;br /&gt;
| E&lt;br /&gt;
| E&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&lt;br /&gt;
| S0&amp;lt;sup&amp;gt;−&amp;lt;/sup&amp;gt;&lt;br /&gt;
| S0&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&lt;br /&gt;
| S0&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&lt;br /&gt;
| S0/a&lt;br /&gt;
| Sa&lt;br /&gt;
| Sab&lt;br /&gt;
| Sb&lt;br /&gt;
| Sbc&lt;br /&gt;
| Sc&lt;br /&gt;
| Scd&lt;br /&gt;
| Sd&lt;br /&gt;
| Sdm&lt;br /&gt;
| Sm&lt;br /&gt;
| Im&lt;br /&gt;
| Irr&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== appmag_v, appmag_b, absmag_v ===&lt;br /&gt;
The &amp;lt;code&amp;gt;appmag_v&amp;lt;/code&amp;gt; give the apparent magnitude of the galaxy in the visual band, while &amp;lt;code&amp;gt;appmag_b&amp;lt;/code&amp;gt; gives the same in the B (blue) band. The &amp;lt;code&amp;gt;absmag_v&amp;lt;/code&amp;gt; is the absolute magnitude of the galaxy. &lt;br /&gt;
&lt;br /&gt;
=== mag_j, mag_h, mag_k ===&lt;br /&gt;
The &amp;lt;code&amp;gt;mag_j&amp;lt;/code&amp;gt; give the IR magnitude of the galaxy in the infrared band at 1220 nm. The &amp;lt;code&amp;gt;mag_h&amp;lt;/code&amp;gt; give the IR magnitude of the galaxy in the infrared band at 1630 nm. The &amp;lt;code&amp;gt;mag_k&amp;lt;/code&amp;gt; give the IR magnitude of the galaxy in the infrared band at 2190 nm. &lt;br /&gt;
&lt;br /&gt;
=== size_v ===&lt;br /&gt;
The &amp;lt;code&amp;gt;size_v&amp;lt;/code&amp;gt; field lists the visual [[angular size]] of the galaxy along the major and minor axes, given in units of arc minutes or arc seconds. For example: {{nowrap|4.3′ × 0.8′}}. For non-visual dimensions, the band should be also listed, such as ([[infrared astronomy|IR]]) or ([[ultraviolet astronomy|UV]]).&lt;br /&gt;
&lt;br /&gt;
=== names ===&lt;br /&gt;
This is a list of catalog identifiers for a galaxy, preferably presented using the {{tl|odlist}} template.&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
* [[Template:Cite journal]]&lt;br /&gt;
* [[Template:Cite web]]&lt;br /&gt;
* [[Template:Infobox galaxy cluster]]&lt;br /&gt;
* [[Template:Infobox globular cluster]]&lt;br /&gt;
&lt;br /&gt;
&amp;lt;includeonly&amp;gt;{{basepage subpage|&amp;lt;!--&lt;br /&gt;
++++ PLEASE ADD CATEGORIES BELOW THIS LINE, THANK YOU. --&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:Astronomy infobox templates|Galaxy]]&lt;br /&gt;
&lt;br /&gt;
}}&amp;lt;/includeonly&amp;gt;&lt;/div&gt;</summary>
		<author><name>&gt;Jjamulla</name></author>
	</entry>
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