“Group discussions”的版本间差异
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==subject== |
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*[[MaNGA]] |
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==Subject== |
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*[[ALFALFA and MaNGA]] |
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===[[机器学习培训]]=== |
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===[[Galaxy_morphology_auto_classification]]=== |
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*[[APOGEE]] |
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===[[Star_cluster_group]]=== |
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: A journal club about extragalactic astronomy |
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===[[星系尺度的演化]]=== |
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*[[MaNGA science discussion]] |
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*[[MaNGA Technical Group]] |
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===LAMOST=== |
===LAMOST=== |
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*[[LAMOST |
*[[LAMOST Science]] |
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*[[LAMOST Technic]] |
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*[[Interesting object in LEGAS DR1]] |
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*[[Interesting object in LEGAS DR2]] |
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*[[EG sources in LAMOST DR1]] |
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*[[Ew(Hα) of one star forming galaxy in LAMOST survey]] |
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===Pan-STARRS1=== |
===Pan-STARRS1=== |
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*[[PS1-links]] |
*[[PS1-links]] |
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== |
=== BCD-related sciense === |
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*[[Discussion]] |
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*Compute the AB mag of a spectrum in a given filter. |
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:im_filtermag.pro [http://idl-moustakas.googlecode.com/svn/trunk/impro/pro/galaxy/im_filtermag.pro], see the impro IDL library in [[Hserver Service]] |
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== |
==Program technic== |
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*[[IDL tricks]] |
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*[[银河系结构模型的细化]] |
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*[[Simard11 Catalog]] |
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==Time sequence== |
==Time sequence== |
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===2015=== |
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*06/24: LAMOST spectra |
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:* IDL program to obtain the spectrum file directory(e.g. Iserver:/data/data_LAMOST/DATA/DR?/spec) for the objects in LAMOST catalog([[file: Lspec_file.pro.txt]] 参考[[LAMOST光谱的IDL可视化程序]] |
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:*masking sky emission line residuals |
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::pro: [[file:Mask_skyline.pro.txt]] |
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::sky emission line list file[[file:skylines_read.dat]] |
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::usage |
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readcol,'skylines_read.dat',char,wave,inten,type,F='(A,D,F,I)'; ;read the sky emission line |
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sel=where(char eq '%') |
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skywave=wave[sel] |
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mask_skyline,specname,skywave |
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===2014=== |
===2014=== |
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*[[2014/12/24]] |
*[[2014/12/24]] |
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*[[1/8]] |
*[[1/8]] |
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[[Category:Internal]] |
[[Category:Internal]] |
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2022年6月17日 (五) 09:12的最新版本
Subject
机器学习培训
Galaxy_morphology_auto_classification
Star_cluster_group
King_Kong_Club
- A journal club about extragalactic astronomy