LAE-Catalogs のバックアップ(No.3)

バックアップ一覧
差分を表示
現在との差分を表示
ソースを表示
LAE-Catalogs へ行く。
- 1 (2015-06-28 (日) 00:57:14)
- 2 (2015-06-29 (月) 14:04:26)
- 3 (2015-06-29 (月) 17:21:08)

The format of the following catalogs is the same one as follows:

(1)ID
(2,3)RA,DEC[deg]
(4)z_phot
(5)excess IA-band
(6,7,8)EWobs[A] of best-fit, 3sigma-{upper,lower} limits
(9,10,11)Mstar[Msun] of best-fit, 3sigma-{upper,lower} limits
(12,13,14)L(Lya)[erg/s] of best-fit, 3sigma-{upper,lower} limits
(15,16,17)SFR(Lya)[Msun] of best-fit, 3sigma-{upper,lower} limits
(18,19,20)SFR(SED)[Msun] of best-fit, 3sigma-{upper,lower} limits
(21,22,23)log10[tau/Gyr] of best-fit, 3sigma-{upper,lower} limits
(24,25,26)Z of best-fit, 3sigma-{upper,lower} limits
(27,28,29)E(B-V) of best-fit, 3sigma-{upper,lower} limits
(30)chi_nu^2
(31)IA[mag]
(32)IAc,model[mag]
(33)N_IA,detect
(34--45)flag for detection in IA427,IA464,IA484,IA505,IA527,IA574,IA624,IA679,IA709,IA738,IA767,IA827[0:non-detection,1:detection]
(46,47,48)flag for the existence of {SED fitting result, (RA,DEC) information, detected IA-band information} for this galaxy[0:absent,1:exist]
(49,50,51,52,53,54,55)flag for AGNfrom IRAC color,Chandra(<1arcsec, <2arcsec),XMM,radio,MIPS,and one of them[0:non-AGN,1:AGN]

in the catalog "All", one additional information is added as
```
(56)number of excess IA bands
```

Note that catalog for IA827-excess object is not uploaded below because of the absence of the IA827-excess object in Step 2.

Step 2?
Step 3?
- matched catalog b/w LAE and new Chandra catalog by S. Toft on 2015/06/17?
Step 4?
- AGN-powered LAE?
- non-AGN-powered LAE?

Step 2 †

step2.tar.gz

individual catalog:

IA-band
IA427	IA427_wChandra.out
IA464	IA464_wChandra.out
IA484	IA484_wChandra.out
IA505	IA505_wChandra.out
IA527	IA527_wChandra.out
IA574	IA574_wChandra.out
IA624	IA624_wChandra.out
IA679	IA679_wChandra.out
IA709	IA709_wChandra.out
IA738	IA738_wChandra.out
IA767	IA767_wChandra.out
All	Step2_wChandra.out

note that 20 LAE candidates with N_ex^temp = 2 (i.e., having two excess IA bands from frequency-matched continuum) are overlappingly listed in two IA-band catalog; thier IDs, z_ph, and comibinations of excess IA-bands are as follows:
- (1) ID 862400 at z_ph = 2.896: (IA464, IA484)
- (2) ID 884165 at z_ph = 2.896: (IA464, IA484)
- (3) ID 1025225 at z_ph = 2.896: (IA464, IA484)
- (4) ID 565880 at z_ph = 3.073: (IA484, IA505)
- (5) ID 1106419 at z_ph = 3.073: (IA484, IA505)
- (6) ID 1199858 at z_ph = 3.073: (IA484, IA505)
- (7) ID 1707398 at z_ph = 3.073: (IA484, IA505)
- (8) ID 355282 at z_ph = 3.241: (IA505, IA527)
- (9) ID 373838 at z_ph = 3.241: (IA505, IA527)
- (10) ID 379762 at z_ph = 3.241: (IA505, IA527)
- (11) ID 432979 at z_ph = 3.241: (IA505, IA527)
- (12) ID 582894 at z_ph = 3.241: (IA505, IA527)
- (13) ID 1358300 at z_ph = 3.241: (IA505, IA527)
- (14) ID 1509230 at z_ph = 3.241: (IA505, IA527)
- (15) ID 1549288 at z_ph = 3.241: (IA505, IA527)
- (16) ID 1725163 at z_ph = 3.241: (IA505, IA527)
- (17) ID 1781909 at z_ph = 3.241: (IA505, IA527)
- (18) ID 1923620 at z_ph = 3.241: (IA505, IA527)
- (19) ID 786441 at z_ph = 4.699: (IA679, IA709)
- (20) ID 728837 at z_ph = 4.931: (IA709, IA738)
in the catalogs for individual IA band, their EW, L(Lya), and SFR(Lya) are evaluated separately from the IA-band excess from the best-fit stellar continuum at lambda_rest = 1300--1400 A for each excess IA band
in the all catalog, the EW, L(Lya), and SFR(Lya) of the LAE candidates with N_ex^temp = 2 are adopted as those of larger one between the two values evaluated from individual IA band excesses

↑

Step 3 †

step3.tar.gz

individual catalog:

IA-band	N_{undet} < 6	N_{undet} < 6 & χ_{ν}^2 <= 3	N_{undet} < 6 & χ_{ν}^2 <= 3 & EW/EW_{err,3σ} > 1
IA427	IA427_Nundet5_wChandra.out	IA427_Nundet5+chinu2lteq3_wChandra.out	IA427_step3_wChandra.out
IA464	IA464_Nundet5_wChandra.out	IA464_Nundet5+chinu2lteq3_wChandra.out	IA464_step3_wChandra.out
IA484	IA484_Nundet5_wChandra.out	IA484_Nundet5+chinu2lteq3_wChandra.out	IA484_step3_wChandra.out
IA505	IA505_Nundet5_wChandra.out	IA505_Nundet5+chinu2lteq3_wChandra.out	IA505_step3_wChandra.out
IA527	IA527_Nundet5_wChandra.out	IA527_Nundet5+chinu2lteq3_wChandra.out	IA527_step3_wChandra.out
IA574	IA574_Nundet5_wChandra.out	IA574_Nundet5+chinu2lteq3_wChandra.out	IA574_step3_wChandra.out
IA624	IA624_Nundet5_wChandra.out	IA624_Nundet5+chinu2lteq3_wChandra.out	IA624_step3_wChandra.out
IA679	IA679_Nundet5_wChandra.out	IA679_Nundet5+chinu2lteq3_wChandra.out	IA679_step3_wChandra.out
IA709	IA709_Nundet5_wChandra.out	IA709_Nundet5+chinu2lteq3_wChandra.out	IA709_step3_wChandra.out
IA738	IA738_Nundet5_wChandra.out	IA738_Nundet5+chinu2lteq3_wChandra.out	IA738_step3_wChandra.out
IA767	IA767_Nundet5_wChandra.out	IA767_Nundet5+chinu2lteq3_wChandra.out	IA767_step3_wChandra.out
All	Step3_Nundet5_wChandra.out	Step3_Nundet5+chinu2lteq3_wChandra.out	Step3_wChandra.out

in the catalogs for individual IA band, their EW, L(Lya), and SFR(Lya) are evaluated separately from the IA-band excess from the best-fit stellar continuum at lambda_rest = 1300--1400 A for each excess IA band
in the all catalog, the EW, L(Lya), and SFR(Lya) of the LAE candidates with N_ex^temp = 2 are adopted as those of larger one between the two values evaluated from individual IA band excesses

↑

matched catalog b/w LAE and new Chandra catalog by S. Toft on 2015/06/17 †

within 1 arcsec: lya_x_1arcsec.txt
within 2 arcsec: lya_x_2arcsec.txt

↑

Step 4 †

↑

AGN-powered LAE †

step4_AGN.tar.gz

IA-band	AGN (IRAC)	AGN (Chandra)	AGN (XMM)	AGN (VLA)	AGN
IA427	IA427_step4_AGN_IRAC_wChandra.out	IA427_step4_AGN_Chandra1arcsec_wChandra.out	IA427_step4_AGN_XMM_wChandra.out	IA427_step4_AGN_radio_wChandra.out	IA427_step4_AGN_wChandra.out
IA464	IA464_step4_AGN_IRAC_wChandra.out	IA464_step4_AGN_Chandra1arcsec_wChandra.out	IA464_step4_AGN_XMM_wChandra.out	IA464_step4_AGN_radio_wChandra.out	IA464_step4_AGN_wChandra.out
IA484	IA484_step4_AGN_IRAC_wChandra.out	IA484_step4_AGN_Chandra1arcsec_wChandra.out	IA484_step4_AGN_XMM_wChandra.out	IA484_step4_AGN_radio_wChandra.out	IA484_step4_AGN_wChandra.out
IA505	IA505_step4_AGN_IRAC_wChandra.out	IA505_step4_AGN_Chandra1arcsec_wChandra.out	IA505_step4_AGN_XMM_wChandra.out	IA505_step4_AGN_radio_wChandra.out	IA505_step4_AGN_wChandra.out
IA527	IA527_step4_AGN_IRAC_wChandra.out	IA527_step4_AGN_Chandra1arcsec_wChandra.out	IA527_step4_AGN_XMM_wChandra.out	IA527_step4_AGN_radio_wChandra.out	IA527_step4_AGN_wChandra.out
IA574	IA574_step4_AGN_IRAC_wChandra.out	IA574_step4_AGN_Chandra1arcsec_wChandra.out	IA574_step4_AGN_XMM_wChandra.out	IA574_step4_AGN_radio_wChandra.out	IA574_step4_AGN_wChandra.out
IA624	IA624_step4_AGN_IRAC_wChandra.out	IA624_step4_AGN_Chandra1arcsec_wChandra.out	IA624_step4_AGN_XMM_wChandra.out	IA624_step4_AGN_radio_wChandra.out	IA624_step4_AGN_wChandra.out
IA679	IA679_step4_AGN_IRAC_wChandra.out	IA679_step4_AGN_Chandra1arcsec_wChandra.out	IA679_step4_AGN_XMM_wChandra.out	IA679_step4_AGN_radio_wChandra.out	IA679_step4_AGN_wChandra.out
IA709	IA709_step4_AGN_IRAC_wChandra.out	IA709_step4_AGN_Chandra1arcsec_wChandra.out	IA709_step4_AGN_XMM_wChandra.out	IA709_step4_AGN_radio_wChandra.out	IA709_step4_AGN_wChandra.out
IA738	IA738_step4_AGN_IRAC_wChandra.out	IA738_step4_AGN_Chandra1arcsec_wChandra.out	IA738_step4_AGN_XMM_wChandra.out	IA738_step4_AGN_radio_wChandra.out	IA738_step4_AGN_wChandra.out
IA767	IA767_step4_AGN_IRAC_wChandra.out	IA767_step4_AGN_Chandra1arcsec_wChandra.out	IA767_step4_AGN_XMM_wChandra.out	IA767_step4_AGN_radio_wChandra.out	IA767_step4_AGN_wChandra.out
All	Step4_AGN_IRAC_wChandra.out	Step4_AGN_Chandra1arcsec_wChandra.out	Step4_AGN_XMM_wChandra.out	Step4_AGN_radio_wChandra.out	Step4_AGN_wChandra.out

in the catalogs for individual IA band, their EW, L(Lya), and SFR(Lya) are evaluated separately from the IA-band excess from the best-fit stellar continuum at lambda_rest = 1300--1400 A for each excess IA band
in the all catalog, the EW, L(Lya), and SFR(Lya) of the LAE candidates with N_ex = 2 are adopted as those of larger one between the two values evaluated from individual IA band excesses

↑

non-AGN-powered LAE †

step4_nonAGN.tar.gz

IA-band	SFG	SFG w/ EW_0 >= 100 A
IA427	IA427_step4_nonAGN_wChandra.out	IA427_step4_nonAGN_sLAE_wChandra.out
IA464	IA464_step4_nonAGN_wChandra.out	IA464_step4_nonAGN_sLAE_wChandra.out
IA484	IA484_step4_nonAGN_wChandra.out	IA484_step4_nonAGN_sLAE_wChandra.out
IA505	IA505_step4_nonAGN_wChandra.out	IA505_step4_nonAGN_sLAE_wChandra.out
IA527	IA527_step4_nonAGN_wChandra.out	IA527_step4_nonAGN_sLAE_wChandra.out
IA574	IA574_step4_nonAGN_wChandra.out	IA574_step4_nonAGN_sLAE_wChandra.out
IA624	IA624_step4_nonAGN_wChandra.out	IA624_step4_nonAGN_sLAE_wChandra.out
IA679	IA679_step4_nonAGN_wChandra.out	IA679_step4_nonAGN_sLAE_wChandra.out
IA709	IA709_step4_nonAGN_wChandra.out	IA709_step4_nonAGN_sLAE_wChandra.out
IA738	IA738_step4_nonAGN_wChandra.out	IA738_step4_nonAGN_sLAE_wChandra.out
IA767	IA767_step4_nonAGN_wChandra.out	IA767_step4_nonAGN_sLAE_wChandra.out
All	Step4_nonAGN_wChandra.out	Step4_nonAGN_sLAE_wChandra.out

in the catalogs for individual IA band, their EW, L(Lya), and SFR(Lya) are evaluated separately from the IA-band excess from the best-fit stellar continuum at lambda_rest = 1300--1400 A for each excess IA band
in the all catalog, the EW, L(Lya), and SFR(Lya) of the LAE candidates with N_ex = 2 are adopted as those of larger one between the two values evaluated from individual IA band excesses

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