“Group discussions”的版本间差异

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==Time sequence==
==Time sequence==
===2015===
===2015===
====06/24====
*06/24: LAMOST spectra
'''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]]
* IDL program to obtain the spectrum file directory(e.g. Iserver:/data/data_LAMOST/DATA/DR?/spec) for the objects in LAMOST catalog
:*masking sky emission line residuals
::([[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]]
::pro: [[file:Mask_skyline.pro.txt]]
::sky emission line list file[[file:skylines_read.dat]]
::sky emission line list file[[file:skylines_read.dat]]
::usage
::useage
readcol,'skylines_read.dat',char,wave,inten,type,F='(A,D,F,I)'; ;read the sky emission line
readcol,'skylines_read.dat',char,wave,inten,type,F='(A,D,F,I)'; ;read the sky emission line
sel=where(char eq '%')
sel=where(char eq '%')

2015年6月24日 (三) 06:03的版本

subject

SDSS IV

LAMOST

Pan-STARRS1

IDL trips and utils

  • Compute the AB mag of a spectrum in a given filter.
im_filtermag.pro [1], see the impro IDL library in Hserver Service

Journal Club

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
(文件:Lspec file.pro.txt 参考LAMOST光谱的IDL可视化程序
  • masking sky emission line residuals
pro: 文件:Mask skyline.pro.txt
sky emission line list file文件:Skylines read.dat
useage
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

2013