“Stellar library”的版本间差异
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(创建页面,内容为“MANGA里面用了11个库,下面的主要是对DAP里面的用的库的注释 ==M11-STELIB== * stellar library STELIB by Le Borgne et al. (2003). *Usable wav...”) |
无编辑摘要 |
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第12行: | 第12行: | ||
:'.kr' ==> Kroupa IMF |
:'.kr' ==> Kroupa IMF |
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:'.cha' ==> Chabrier IMF |
:'.cha' ==> Chabrier IMF |
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*DAP 只用了3个金属丰度,一共85个SSP, |
*DAP 只用了3个金属丰度,一共85个SSP, |
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''':ssp_M11_MILES.ss.z002 (solar metallicity)''' |
''':ssp_M11_MILES.ss.z002 (solar metallicity)''' |
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: 39 ages, 30 Myr to 15 Gyr |
: 39 ages, 30 Myr to 15 Gyr |
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'''ssp_M11_MILES.ss.z004 (z=0.04)''' |
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:22 ages, 400 Myr to 15 Gyr |
:22 ages, 400 Myr to 15 Gyr |
2016年5月17日 (二) 03:00的版本
MANGA里面用了11个库,下面的主要是对DAP里面的用的库的注释
M11-STELIB
- stellar library STELIB by Le Borgne et al. (2003).
- Usable wavelength range for all ages is 3201.0 - 7900.0 AA!
- 原始分辨率:0.5 A/pixel, and a FWHM of the resolution element of 3.1 angstroms. Resampled this to 1 A/pixel to reduce the oversampling of the spectra. The resampled spectra are named *_s.fits; the original spectra do not have the _s suffix. When constructing the library to fit the spectra, only the *_s.fits spectra are read.
- IMF
- '.ss' ==> Salpeter IMF
- '.kr' ==> Kroupa IMF
- '.cha' ==> Chabrier IMF
- DAP 只用了3个金属丰度,一共85个SSP,
ssp_M11_MILES.ss.z001 (z=0.01)
- 24 ages, 200 Myr to 15 Gyr,3201.0 - 9296.5 AA 12192 flux point
:ssp_M11_MILES.ss.z002 (solar metallicity)
- 39 ages, 30 Myr to 15 Gyr
ssp_M11_MILES.ss.z004 (z=0.04)
- 22 ages, 400 Myr to 15 Gyr