Difference between revisions of "Group discussions"

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==subject==
===SDSS IV===
*[[MaNGA]]


*[[ALFALFA and MaNGA]]
==Subject==
===[[机器学习培训]]===


*[[APOGEE]]
===[[Galaxy_morphology_auto_classification]]===
 
===[[Star_cluster_group]]===
 
===[[King_Kong_Club]]===
: A journal club about extragalactic astronomy
 
===[[星系尺度的演化]]===
 
 
 
===MaNGA===
*[[MaNGA science discussion]]
*[[MaNGA Technical Group]]


===LAMOST===
===LAMOST===
*[[LAMOST光谱的IDL可视化程序]]
*[[LAMOST Science]]
*[[Interesting object in LEGAS DR1]]
*[[LAMOST Technic]]
*[[Interesting object in LEGAS DR2]]
*[[EG sources in LAMOST DR1]]
*[[Ew(Hα) of one star forming galaxy in LAMOST survey]]


===Pan-STARRS1===
===Pan-STARRS1===
*[[PS1-links]]
*[[PS1-links]]


==IDL trips and utils==
=== BCD-related sciense ===
*Compute the AB mag of a spectrum in a given filter.
*[[Discussion]]
:im_filtermag.pro  [http://idl-moustakas.googlecode.com/svn/trunk/impro/pro/galaxy/im_filtermag.pro], see the impro IDL  library in [[Hserver Service]]


===Journal Club===
==Program technic==
*[[银河系结构模型的细化]]
*[[IDL tricks]]
*[[Simard11 Catalog]]


==Time sequence==
==Time sequence==
===2015===
*06/24: LAMOST spectra
:* 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]]
:*masking sky emission line residuals (pro: [[file:Mask_skyline.pro.txt]], sky emission line file[[file:skylines_read.dat.txt]]
::usage
readcol,'skylines_read.dat',char,wave,inten,type,F='(A,D,F,I)'; ;read the sky emission line
sel=where(char eq '%')
skywave=wave[sel]
mask_skyline,specname,skywave
===2014===
===2014===
*[[2014/12/24]]
*[[2014/12/24]]
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*[[1/8]]
*[[1/8]]


===[[2013]]===


[[Category:Internal]]
[[Category:Internal]]

Latest revision as of 09:12, 17 June 2022