TransferFromMARK のバックアップ(No.4)

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- 1 (2016-08-05 (金) 17:05:39)
- 2 (2017-03-18 (土) 15:51:51)
- 3 (2017-03-18 (土) 21:43:04)
- 4 (2017-03-21 (火) 12:56:41)
- 5 (2017-03-21 (火) 15:49:08)
- 6 (2017-03-21 (火) 17:42:45)

FrontPage This page contains all of the codes, scripts, and data which are used to obtain the final catalog of strong line emitters.

Step 0: Basic Data and Catalog?
Step 1: Selection of Strong Line Emitter Candidates?
Step 2: Determination of z_ph and Identification of Emission Line?
Step 3: Selection of Strong Line Emitters and Calculation of Physical Quantities?
Step 4: Classifying AGN Candidates?

Step 0: Basic Data and Catalog †

cosmos_phot_20120626bs.tbl: the latest version of i-band selected photometric catalog including the UltraVISTA DR1 data
- it has too huge file size (~11 GB) to be uploaded here
- it can be downloaded from the COSMOS internal page
- [note] the file we used in the following Step 1 are slightly modified from the original photometric catalog in the following two points by using DoPhotcat20.sh:
  - removing the header and the 1st column which shows the object name
  - sorting the IDs in ascending order
photoz_zml_vers2.0_010312-fulls.out: the latest version of photo-z catalog
- it has also too huge file size (~1.5 GB) to be uploaded here
- it can be downloaded from the COSMOS internal page
- [note] the file we used in the following Step 1 are also slightly modified from the original photo-z catalog in the following one point by using photoz_vers2.0_sort.sh:
  - sort the IDs in ascending order
NewMasking.reg: (RA,DEC) of the masked-out regions
Chandra_MatchedCatalog.dat: ID, (RA,DEC), and X-ray fluxes of the cross-matched IA-excess candidates
- cross-matching condition: angular distance is smaller than or equals to 1 arcsec
XMM_MatchedCatalog.dat: ID, (RA,DEC), and X-ray fluxes of the cross-matched IA-excess candidates
- cross-matching condition: angular distance is smaller than or equals to the positional error for the object in the XMM-Newton source catalog
VLA_MatchedCatalog.dat: ID, (RA,DEC), and X-ray fluxes of the cross-matched IA-excess candidates
- cross-matching condition: angular distance is smaller than or equals to 1 arcsec

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Step 1: Selection of Strong Line Emitter Candidates †

code (F90) and scripts to select strong line emitter candidates: Step1.f90, Step1.sh
- sub code to separate the candidates into groups (F90): Step1_makeGroup.f90
catalogs of the 6,164 Step 1 selected line emitter candidates: Step1.dat table_Step1.txt

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Step 2: Determination of z_ph and Identification of Emission Line †

catalogs of the 6,140 Step 2 selected line emitter candidates: Step2.dat table_Step2.txt
- 1,052 LAE candidates: Step2_LAE_all.dat
  - above catalog w/ Step 3 SED-fitting results: Step3_LAE_all.dat
- 4,734 low-z emitter candidates: Step2_lowz_all.dat
  - above catalog w/ Step 3 SED-fitting results: Step3_lowz_all.dat
- 354 others: Step2_others.dat
  - above catalog w/ Step 3 SED-fitting results: Step3_others.dat

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Step 3: Selection of Strong Line Emitters and Calculation of Physical Quantities †

SED fitting code (F90): Step3_SEDfit.f90
- input files: zph_list_LAE_all.txt, zph_list_lowz_all.txt, zph_list_others.txt
- scripts: Step3_SEDfit_LAE.sh Step3_SEDfit_lowz.sh Step3_SEDfit_others.sh
the SED templates:
- the SED templates have so huge file size (~ 1.5 GB at a certain redshift) that they cannot be uploaded here
- the SED templates are uploaded on newngli:
  - /net/newngli/data/kobayashi/SEDtemplates/{LAE,lowz,others}/SEDtemp_z*p***_{young,old}.dat: time evolution of fnu for 37 broadbands
  - /net/newngli/data/kobayashi/SEDtemplates/Mstar+Lnu_{young,old}.dat: time evolution of Mstar, SFR, L1350, L1500, and L2um
- their format is the following: format_SEDtemp.txt
the code making the SED templates (F90): Step3_makeSEDtemplate.f90
- [note] because making the SED templates is highly time-consuming, the SED templates were made separately by using several computers
- input files: inputfile_makeSEDtemplate.tar.gz (e.g.) makeSEDtemplate_LAE1.in
- scripts: scripts_Step3_makeSEDtemplate.tar.gz (e.g.) Step3_makeSEDtemplate_LAE1.sh
- the above input files and scripts were created by the following code, script, and input files:
  - code (F90): makescripts.f90
  - script: makescripts.sh
  - input files: makeSEDtemplate_LAE, makeSEDtemplate_nonLAE, makeSEDtemplate_others

catalogs at the end of Step 3:
- 770 LAEs: Step3_LAE_all_final.dat

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Step 4: Classifying AGN Candidates †

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