Galaxy Colours: Difference between revisions

From OBSCOS Wiki, Department of Physics
Jump to navigation Jump to search
 
(14 intermediate revisions by the same user not shown)
Line 1: Line 1:
==Galaxy Colours==
==Galaxy Colours==


=Filters in HyperSuprimeCame on Subaru=
[[File:Hsc2017.png]]


=Near-infrared filters on VISTA=
===Optical to nearIR Filters===
[[File:VISTA-filters.jpg]]
[[File:Hsc2017.png|300px]]
[[File:VISTA-filters.jpg|300px]]
 
When we refer to colours we usually mean a combination of these filters to highlight whether a galaxy (or star) spectrum is "red" or "blue". This is also akin to the HR diagram for stars, which uses colours an an indicator of e.g. Temperature.
 
Combining these you can see how they can be used to understands the SEDs of various objects
 
[[File:Bowler-sed.jpg|600px]]
Taken from [https://arxiv.org/pdf/1411.2976.pdf Bowler et al. (2015)].
 
===Galaxy colour-magnitude diagram===
 
The most common plot in extragalactic astrophysics, is the colour-magnitude diagram, which plots a colour (blue-red filter) against a magnitude in one of the filters. The y-axis is then the colour and the x-axis is the brightness.
 
[[File:Galaxy_color-magnitude_diagram.jpg|300px]]
[[File:Redspiral_colourmagnitude.jpg|400px]] Taken from [https://blog.galaxyzoo.org/2012/05/09/my-favourite-colour-magnitude-diagram/ GalaxyZoo].
 
===Galaxy colour-colour diagram===
But you will also see colour-colour diagrams, which are often used to select certain galaxies at certain redshifts as they can pin-point where there are "breaks" in the galaxy spectral energy distribution.
 
[[File:LBGselection.jpg |400px]]
 
Example of a colour-colour diagram to select high-redshift z>6 galaxies based on their Lyman-break. Taken from [https://arxiv.org/pdf/1411.2976.pdf Bowler et al. (2015)].

Latest revision as of 10:32, 19 November 2020

Galaxy Colours

Optical to nearIR Filters

Hsc2017.png VISTA-filters.jpg

When we refer to colours we usually mean a combination of these filters to highlight whether a galaxy (or star) spectrum is "red" or "blue". This is also akin to the HR diagram for stars, which uses colours an an indicator of e.g. Temperature.

Combining these you can see how they can be used to understands the SEDs of various objects

Bowler-sed.jpg Taken from Bowler et al. (2015).

Galaxy colour-magnitude diagram

The most common plot in extragalactic astrophysics, is the colour-magnitude diagram, which plots a colour (blue-red filter) against a magnitude in one of the filters. The y-axis is then the colour and the x-axis is the brightness.

Galaxy color-magnitude diagram.jpg Redspiral colourmagnitude.jpg Taken from GalaxyZoo.

Galaxy colour-colour diagram

But you will also see colour-colour diagrams, which are often used to select certain galaxies at certain redshifts as they can pin-point where there are "breaks" in the galaxy spectral energy distribution.

LBGselection.jpg

Example of a colour-colour diagram to select high-redshift z>6 galaxies based on their Lyman-break. Taken from Bowler et al. (2015).