Spectra of Stars: Reliable Data & Quantitative Analysis

In summary, the Sloan Digital Sky Survey has a wealth of data on spectra of different stars. You can plot the spectra, or download FITS files with the spectra for your own analysis.
  • #1
NihalRi
134
12
I'm looking for reliable data of the spectra of different stars, anyone know any good resouces? Quantitative data would be best because I want to analyze it myself (not just find out something that was already on the site). Thanks in advance :)
 
Astronomy news on Phys.org
  • #2
NihalRi said:
I'm looking for reliable data of the spectra of different stars, anyone know any good resouces? Quantitative data would be best because I want to analyze it myself (not just find out something that was already on the site). Thanks in advance :)

did you actually try searching for data yourself ?

I typed spectra data for stars into google and got many good hits
 
  • #3
i did, and i got synthesized data and files i could not open :?
 
  • #4
The Sloan Digital Sky Survey SDSS has archived spectroscopic data on millions of stars and galaxies. You can plot the spectra, or download FITS files with the spectra for your own analysis. Here's how to use it:

Go to the site: http://mirror.sdss3.org . (don't use Internet Explorer, which has some issues with looking at this site). This site gives you access to a set of real astronomical data released in January 2011 by a team of astronomers. In the menu, go to "Spectra" and under that "Bulk Search." On the right side, enter the RA and Dec that you are interested in. One good one to start with is at coordinates 16.437201, -10.7071. Use a Tolerance of 2.0 arc seconds and click "Submit". Scroll down and under "Plot Spectrum" click "Plot". It will plot the spectrum, which is that of an A0 star with prominent H absorption lines.

There are a wealth of things you can do with this site.
 
Last edited by a moderator:
  • Like
Likes DrClaude and NihalRi
  • #6
phyzguy said:
The Sloan Digital Sky Survey SDSS has archived spectroscopic data on millions of stars and galaxies. You can plot the spectra, or download FITS files with the spectra for your own analysis. Here's how to use it:

Go to the site: http://mirror.sdss3.org . (don't use Internet Explorer, which has some issues with looking at this site). This site gives you access to a set of real astronomical data released in January 2011 by a team of astronomers. In the menu, go to "Spectra" and under that "Bulk Search." On the right side, enter the RA and Dec that you are interested in. One good one to start with is at coordinates 16.437201, -10.7071. Use a Tolerance of 2.0 arc seconds and click "Submit". Scroll down and under "Plot Spectrum" click "Plot". It will plot the spectrum, which is that of an A0 star with prominent H absorption lines.

There are a wealth of things you can do with this site.
Thank you that was really helpful, is there anywhere specific where you get the RA's and DEC's from?
 
Last edited by a moderator:
  • #7
Maybe an easier way to get started with the SDSS data is to go to this site:
http://skyserver.sdss.org/dr12/en/tools/chart/navi.aspx
This is an interactive viewer that allows you to scroll around and click on objects. If you click the box on the left that says "Objects with spectra", it will put a red box around the objects where spectra have been measured. If you click on one of those it will give you the information and show the spectrum.

On your question of how to find the coordinates for an object, there are many online tools. This site:
https://heasarc.gsfc.nasa.gov/cgi-bin/Tools/convcoord/convcoord.pl
allows you to enter the name of an object (for example "polaris"), and it will give you the coordinates.
 
  • Like
Likes NihalRi
  • #8
Here's an interesting object that I happened upon while scrolling around and writing the last post. Go to the object at:
ra 133.03722
dec 11.43490
It is a quasar at a red shift of 2.26. The Lyman Alpha line, which at zero redshift is in the far ultraviolet at 1215 Angstroms, has been redshifted all the way into the visible at about 4000 Angstroms. We are seeing the light that left this object approximately 10 billion years ago. Cool!
 
  • Like
Likes NihalRi
  • #9
Hi again, I've downloaded the fitz files from SDSS as you've recommended, and software that can open them, but all the data is in binary and I was just wondering is there an easy way of converting them? Or perhaps software that does that as well?
 
  • #10
I just use Python and the pyfits module to interrogate and plot fits files. Below is some simple code to do this, and attached is the output of that code. If you want to learn how to extract and process data, Python is a great tool, and I encourage you to learn how to use it. There are many online tutorials.

Code:
import pyfits as pf
data = pf.getdata("~/Downloads/apStar-r5-2M08505976+1139222.fits")
plot(data[0])
show()
 

Attachments

  • spectrum.png
    spectrum.png
    7.4 KB · Views: 525
  • #11
phyzguy said:
I just use Python and the pyfits module to interrogate and plot fits files. Below is some simple code to do this, and attached is the output of that code. If you want to learn how to extract and process data, Python is a great tool, and I encourage you to learn how to use it. There are many online tutorials.

Code:
import pyfits as pf
data = pf.getdata("~/Downloads/apStar-r5-2M08505976+1139222.fits")
plot(data[0])
show()

Thanks this was really helpful. I'm actually working on learning python but I'm still very new. At this frustrating part where I know what can be done but not how lol. :)
 

1. What is a spectrum of a star?

A spectrum of a star is a graph that shows the intensity of light emitted by the star at different wavelengths. It is created by passing the star's light through a prism or diffraction grating, which separates the light into its different wavelengths.

2. How is data collected for a spectrum of a star?

Data for a spectrum of a star is collected using a spectrometer, which is a device that measures the intensity of light at different wavelengths. The spectrometer records the data as a series of peaks and dips, which correspond to the different wavelengths of light.

3. Why is the data from a spectrum of a star considered reliable?

The data from a spectrum of a star is considered reliable because it is collected using advanced technology and precise instruments. The process of collecting the data is also standardized and repeatable, ensuring consistency and accuracy.

4. How can quantitative analysis be performed on a spectrum of a star?

Quantitative analysis of a spectrum of a star involves measuring the intensity of light at specific wavelengths and comparing it to known values. This can provide information about the chemical composition, temperature, and other physical properties of the star.

5. What can we learn from studying the spectra of stars?

Studying the spectra of stars can provide valuable information about the composition, temperature, and other physical properties of the star. It can also help us understand the evolution and formation of stars, as well as the larger structures of the universe, such as galaxies and clusters of galaxies.

Similar threads

Replies
8
Views
2K
  • Astronomy and Astrophysics
Replies
1
Views
1K
Replies
5
Views
939
  • Astronomy and Astrophysics
Replies
26
Views
2K
  • Astronomy and Astrophysics
Replies
21
Views
1K
  • Biology and Medical
Replies
5
Views
775
  • Astronomy and Astrophysics
Replies
11
Views
2K
  • Biology and Medical
Replies
7
Views
930
  • Astronomy and Astrophysics
Replies
6
Views
1K
  • Astronomy and Astrophysics
Replies
3
Views
956
Back
Top