Spectral cross-correlation templates
One of the redshift measurements is carried out by obtaing a cross-correlation redshift. The
ID of the best-fitting template is stored in the header keyword
BESTTEMP in the spSpec*.fits
files. Here we provide the template spectra.
- The templates have been changed slightly for DR2/DR3 (note they are
now numbered from 0-32, instead of 1-33)
- Templates are provided as fits files, in the same file format as
spSpec*.fits files.
- Get all templates:
spectemplatesDR2.tar.gz
(1.8 MB)
- We also provide ps and gif plots of the templates.
ID |
Spectral classification (SDSS pipeline classification in brackets) |
gif spectrum |
Files |
1 | O star (Star) |
![Template #1](./spDR2-000.gif) |
|
2 | O/B transition star (Star) |
![Template #2](./spDR2-001.gif) |
|
3 | B star (star) |
![Template #3](./spDR2-002.gif) |
|
4 | A star (star) |
![Template #4](./spDR2-003.gif) |
|
5 | A star (Star) |
![Template #5](./spDR2-004.gif) |
|
6 | F/A transition star (Star) |
![Template #6](./spDR2-005.gif) |
|
7 | F star (Star) |
![Template #7](./spDR2-006.gif) |
|
8 | F star (Star) |
![Template #8](./spDR2-007.gif) |
|
9 | G star (star) |
![Template #9](./spDR2-008.gif) |
|
10 | G star (Star) |
![Template #10](./spDR2-009.gif) |
|
11 | K star (Star) |
![Template #11](./spDR2-010.gif) |
|
12 | M1 star (Late-type star, M or later) |
![Template #12](./spDR2-011.gif) |
|
13 | M3 star (Late-type star, M or later) |
![Template #13](./spDR2-012.gif) |
|
14 | M5 star (Late-type star, M or later) |
![Template #14](./spDR2-013.gif) |
|
15 | M8 star (Late-type star, M or later) |
![Template #15](./spDR2-014.gif) |
|
16 | L1 star (Late-type star, M or later) |
![Template #16](./spDR2-015.gif) |
|
17 | Magnetic white dwarf (Star) |
![Template #17](./spDR2-016.gif) |
|
18 | Carbon star (Star) |
![Template #18](./spDR2-017.gif) |
|
19 | Carbon star (Star) |
![Template #19](./spDR2-018.gif) |
|
20 | Carbon star (Late-type star, M or later) |
![Template #20](./spDR2-019.gif) |
|
21 | White dwarf (Star) |
![Template #21](./spDR2-020.gif) |
|
22 | B white dwarf (Star) |
![Template #22](./spDR2-021.gif) |
|
23 | Low-metallicity K subdwarf (Star) |
![Template #23](./spDR2-022.gif) |
|
24 | "Early-type" galaxy (Galaxy) |
![Template #24](./spDR2-023.gif) |
|
25 | Galaxy |
![Template #25](./spDR2-024.gif) |
|
26 | Galaxy |
![Template #26](./spDR2-025.gif) |
|
27 | Galaxy |
![Template #27](./spDR2-026.gif) |
|
28 | "Late-type" galaxy (Galaxy) |
![Template #28](./spDR2-027.gif) |
|
29 | Luminous Red Galaxy (Galaxy) |
![Template #29](./spDR2-028.gif) |
|
30 | QSO |
![Template #30](./spDR2-029.gif) |
|
31 | QSO with some BAL activity (QSO) |
![Template #31](./spDR2-030.gif) |
|
32 | QSO with some BAL activity (QSO) |
![Template #32](./spDR2-031.gif) |
|
33 | High-luminosity QSO (QSO) |
![Template #33](./spDR2-032.gif) |
|
Last modified: Tue Jun 14 17:07:29 CDT 2005
|