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- Action Items Related to Transfer to Kajisawa-san?
- Programs & Scripts?
- Catalogs?
- Fixed Action Items?
- Documents?
- 2015/08/04: executing the procedures in Step 2, 3, and 4 for the newly added 785 IA-excess candidates:
IdonBand_add_150804.dat
- these candidates are added because of the changes of (1) limiting magnitudes of 7 IA-bands (i.e., IA464, IA484, IA505, IA527, IA574, IA624, and IA827), (2) the coefficients estimating the frequency-matched continuum, and (3) the equation which judges whether each object is inside or outside of the circular-shaped masked-out regions
- the limiting magnitudes used originally were old one which were listed in the previous data paper but now were modified by M. Kajisawa on 17th Feb. 2015 --> the limiting magnitudes modified by M. Kajisawa on 17th Feb. 2015 are now adopted; the previous limiting magnitudes were wrong because they were the background fluctuations evaluated without mask to bright objects (email from M. Kajisawa on 16:24 4th Aug. 2015)
- the coefficients estimating the frequency-matched continuum were originally calculated in another program and then were substituted in the program for Step 1 by reading a data file in which the coefficients rounded up to the third decimal place are written --> the coefficients are now evaluating directly from the effective wavelengths in the program for Step 1
- the equation which judges whether an object at (RA,DEC) is inside or outside of the masked-out region with a radius of r centered on (RA0,DEC0) used originally was wrong (dr = sqrt[(RA - RA0)^2 + (DEC - DEC0)^2]) --> the correct equation is now used (dr = acos[cos(DEC)cos(DEC0)cos(RA-RA0) + sin(DEC)sin(DEC0)])
- showing the 1σ errors of the best-fit model SED for EWobs, Mstar, L(Lya), SFR(Lya), SFR(SED), log10[tau/Gyr], Z, and E(B-V)
- showing the programs, scripts, and catalogs with their manuals to select the IA-excess objects in Step 1, 2, 3, and 4
Step 1 Related †
Step 2 Related †
- the program to make the catalog for Step 2: &ref(): File not found: "Step2_zph.f" at page "Transfer-Step2-Catalogs";
- see Transfer-Step2-Catalogs? for detailed description of this program
Step 3 Related †
- the scripts and lists to make the input files for the SED fittings of low-z emitters (transferred on 2015/07/02): Step2_lowzSEDfit_scripts.tar.gz
- the parent script: DoMkSSforSF.sh
- this script (1) copies IA_zph_out/IAxxx_zph.out to MkSSforSF.in as the input file to the program, (2) executes the program, and (3) moves MkSSforSF.out as the output file from the program to SEDfit_150305_lowz_IAxxx.tcsh
- the input files for the parent script: IA427_zph.out IA464_zph.out IA484_zph.out IA505_zph.out IA527_zph.out IA574_zph.out IA624_zph.out IA679_zph.out IA709_zph.out IA738_zph.out IA767_zph.out IA827_zph.out
- in each file, all of the redshifts possible for the filter are written in the following format: [1st column] 3 digits for the IA-band name [other columns] (1)z (2)3 digits for the IA-band name (3)emission line (1:Lya, 2:CIV, 3:CIII], 4:MgII, 5:[OII], 6:[OIII]+Hb, 7:Ha+[NII], 99:others)
- the source code of the program: MkSSforSF.f
- this program generates the script file for the SED fittings of low-z emitters named "MkSSforSF.out" from the input file named "MkSSforSF.in"
- the output script files: SEDfit_150305_lowz_IA427.tcsh SEDfit_150305_lowz_IA464.tcsh SEDfit_150305_lowz_IA484.tcsh SEDfit_150305_lowz_IA505.tcsh SEDfit_150305_lowz_IA527.tcsh SEDfit_150305_lowz_IA574.tcsh SEDfit_150305_lowz_IA624.tcsh SEDfit_150305_lowz_IA679.tcsh SEDfit_150305_lowz_IA709.tcsh SEDfit_150305_lowz_IA738.tcsh SEDfit_150305_lowz_IA767.tcsh SEDfit_150305_lowz_IA827.tcsh
Step 4 Related †
Step 1 Related? †
- catalog of 5357 IA-excess candidates selected in Step 1: Step1.txt
- format: (1)ID (2,3)RA,DEC[deg] (4)flag for detection in all 4 IRAC bands[0:no, 1:yes] (5--9)flag for AGN from IRAC color, XMM, Chandra, VLA, and one of them[0:non-AGN, 1:AGN] (10--21)flag of excess IA band for 12 IA bands [0:non-excess, others:excess] (22)N_ex^temp
- (10)IA427 (11)IA464 (12)IA484 (13)IA505 (14)IA527 (15)IA574 (16)IA624 (17)IA679 (18)IA709 (19)IA738 (20)IA767 (21)IA827
Step 2 Related? †
- list of IA-band excess candidates: Step2.txt
- format: (1)ID (2,3)RA,DEC[deg] (4)flag for detection in all 4 IRAC bands[0:no, 1:yes] (5--9)flag for AGN from IRAC color, XMM, Chandra, VLA, and one of them[0:non-AGN,1:AGN] (10)Nex^temp (11)Nsol (12--27)quantities related to the primary z_ph solution (28--43)quantities related to the secondary z_ph solution (44--55)flag for 12 IA bands[0:undetected, 1:detected] (56)N_undetectedIA
- for primary solution : (12)P(z_ph) (13)chi_nu^2(z_ph) (14)z_ph (15--26)line ID for 12 IA bands (1:Lya, 2:CIV, 3:CIII], 4:MgII, 5:[OII], 6:[OIII]+Hb, 7:Ha+[NII], 99:others) (27)N_ex^cons
- for secondary solution: (28)P(z_ph2)/P(z_ph) (29)chi_nu^2(z_ph2)[-99 for the objects w/o secondary solution] (30)z_ph2[-99 for the objects w/o secondary solution] (31--42)line ID for 12 IA bands (1:Lya, 2:CIV, 3:CIII], 4:MgII, 5:[OII], 6:[OIII]+Hb, 7:Ha+[NII], 99:others) (43)N_ex^cons
- (15,31,44)IA427 (16,32,45)IA464 (17,33,46)IA484 (18,34,47)IA505 (19,35,48)IA527 (20,36,49)IA574 (21,37,50)IA624 (22,38,51)IA679 (23,39,52)IA709 (24,40,53)IA738 (25,41,54)IA767 (26,42,55)IA827
Step 3 Related †
Step 4 Related †
as of xxx †
- Determination of the Masked-out Regions from the 12 IA-band images
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