LAE-Catalogs
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[[FrontPage]] - 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 - &color(Red){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>LAE-Catalogs#Step2]] - [[Step 3>LAE-Catalogs#Step3]] -- [[matched catalog b/w LAE and new Chandra catalog by S. Toft on 2015/06/17>LAE-Catalogs#MatchedCatalogWithChandra]] - [[Step 4>LAE-Catalogs#Step4]] -- [[AGN-powered LAE>LAE-Catalogs#AGNpowered]] -- [[non-AGN-powered LAE>LAE-Catalogs#nonAGNpowered]] * &aname(Step2){Step 2}; [#kd94e4b7] - &ref(step2.tar.gz); - individual catalog: |CENTER:BGCOLOR(cyan): IA-band |CENTER:BGCOLOR(cyan): |h |CENTER: IA427 | &ref(IA427_wChandra.out); | |CENTER: IA464 | &ref(IA464_wChandra.out); | |CENTER: IA484 | &ref(IA484_wChandra.out); | |CENTER: IA505 | &ref(IA505_wChandra.out); | |CENTER: IA527 | &ref(IA527_wChandra.out); | |CENTER: IA574 | &ref(IA574_wChandra.out); | |CENTER: IA624 | &ref(IA624_wChandra.out); | |CENTER: IA679 | &ref(IA679_wChandra.out); | |CENTER: IA709 | &ref(IA709_wChandra.out); | |CENTER: IA738 | &ref(IA738_wChandra.out); | |CENTER: IA767 | &ref(IA767_wChandra.out); | |CENTER:BGCOLOR(yellow): All |BGCOLOR(yellow): &ref(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 * &aname(Step3){Step 3}; [#s55fadc9] - &ref(step3.tar.gz); - individual catalog: |CENTER:BGCOLOR(cyan): IA-band |CENTER:BGCOLOR(cyan): N_{undet} < 6 |CENTER:BGCOLOR(cyan): N_{undet} < 6 & χ_{ν}^2 <= 3 |CENTER:BGCOLOR(cyan): N_{undet} < 6 & χ_{ν}^2 <= 3 & EW/EW_{err,3σ} > 1 |h |CENTER: IA427 | &ref(IA427_Nundet5_wChandra.out); | &ref(IA427_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA427_step3_wChandra.out); | |CENTER: IA464 | &ref(IA464_Nundet5_wChandra.out); | &ref(IA464_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA464_step3_wChandra.out); | |CENTER: IA484 | &ref(IA484_Nundet5_wChandra.out); | &ref(IA484_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA484_step3_wChandra.out); | |CENTER: IA505 | &ref(IA505_Nundet5_wChandra.out); | &ref(IA505_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA505_step3_wChandra.out); | |CENTER: IA527 | &ref(IA527_Nundet5_wChandra.out); | &ref(IA527_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA527_step3_wChandra.out); | |CENTER: IA574 | &ref(IA574_Nundet5_wChandra.out); | &ref(IA574_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA574_step3_wChandra.out); | |CENTER: IA624 | &ref(IA624_Nundet5_wChandra.out); | &ref(IA624_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA624_step3_wChandra.out); | |CENTER: IA679 | &ref(IA679_Nundet5_wChandra.out); | &ref(IA679_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA679_step3_wChandra.out); | |CENTER: IA709 | &ref(IA709_Nundet5_wChandra.out); | &ref(IA709_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA709_step3_wChandra.out); | |CENTER: IA738 | &ref(IA738_Nundet5_wChandra.out); | &ref(IA738_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA738_step3_wChandra.out); | |CENTER: IA767 | &ref(IA767_Nundet5_wChandra.out); | &ref(IA767_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA767_step3_wChandra.out); | |CENTER:BGCOLOR(yellow): All |BGCOLOR(yellow): &ref(Step3_Nundet5_wChandra.out); |BGCOLOR(yellow): &ref(Step3_Nundet5+chinu2lteq3_wChandra.out); |BGCOLOR(yellow): &ref(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 ** &aname(MatchedCatalogWithChandra){matched catalog b/w LAE and new Chandra catalog by S. Toft on 2015/06/17}; [#z9300fca] - within 1 arcsec: &ref(lya_x_1arcsec.txt); - within 2 arcsec: &ref(lya_x_2arcsec.txt); * &aname(Step4){Step 4}; [#ofd8b04a] ** &aname(AGNpowered){AGN-powered LAE}; [#b8d7f118] - &ref(step4_AGN.tar.gz); |CENTER:BGCOLOR(cyan): IA-band |CENTER:BGCOLOR(cyan): AGN (IRAC) |CENTER:BGCOLOR(cyan): AGN (Chandra) |CENTER:BGCOLOR(cyan): AGN (XMM) |CENTER:BGCOLOR(cyan): AGN (VLA) |CENTER:BGCOLOR(cyan): AGN |h |CENTER: IA427 | &ref(IA427_step4_AGN_IRAC_wChandra.out); | &ref(IA427_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA427_step4_AGN_XMM_wChandra.out); | &ref(IA427_step4_AGN_radio_wChandra.out); | &ref(IA427_step4_AGN_wChandra.out); | |CENTER: IA464 | &ref(IA464_step4_AGN_IRAC_wChandra.out); | &ref(IA464_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA464_step4_AGN_XMM_wChandra.out); | &ref(IA464_step4_AGN_radio_wChandra.out); | &ref(IA464_step4_AGN_wChandra.out); | |CENTER: IA484 | &ref(IA484_step4_AGN_IRAC_wChandra.out); | &ref(IA484_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA484_step4_AGN_XMM_wChandra.out); | &ref(IA484_step4_AGN_radio_wChandra.out); | &ref(IA484_step4_AGN_wChandra.out); | |CENTER: IA505 | &ref(IA505_step4_AGN_IRAC_wChandra.out); | &ref(IA505_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA505_step4_AGN_XMM_wChandra.out); | &ref(IA505_step4_AGN_radio_wChandra.out); | &ref(IA505_step4_AGN_wChandra.out); | |CENTER: IA527 | &ref(IA527_step4_AGN_IRAC_wChandra.out); | &ref(IA527_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA527_step4_AGN_XMM_wChandra.out); | &ref(IA527_step4_AGN_radio_wChandra.out); | &ref(IA527_step4_AGN_wChandra.out); | |CENTER: IA574 | &ref(IA574_step4_AGN_IRAC_wChandra.out); | &ref(IA574_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA574_step4_AGN_XMM_wChandra.out); | &ref(IA574_step4_AGN_radio_wChandra.out); | &ref(IA574_step4_AGN_wChandra.out); | |CENTER: IA624 | &ref(IA624_step4_AGN_IRAC_wChandra.out); | &ref(IA624_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA624_step4_AGN_XMM_wChandra.out); | &ref(IA624_step4_AGN_radio_wChandra.out); | &ref(IA624_step4_AGN_wChandra.out); | |CENTER: IA679 | &ref(IA679_step4_AGN_IRAC_wChandra.out); | &ref(IA679_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA679_step4_AGN_XMM_wChandra.out); | &ref(IA679_step4_AGN_radio_wChandra.out); | &ref(IA679_step4_AGN_wChandra.out); | |CENTER: IA709 | &ref(IA709_step4_AGN_IRAC_wChandra.out); | &ref(IA709_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA709_step4_AGN_XMM_wChandra.out); | &ref(IA709_step4_AGN_radio_wChandra.out); | &ref(IA709_step4_AGN_wChandra.out); | |CENTER: IA738 | &ref(IA738_step4_AGN_IRAC_wChandra.out); | &ref(IA738_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA738_step4_AGN_XMM_wChandra.out); | &ref(IA738_step4_AGN_radio_wChandra.out); | &ref(IA738_step4_AGN_wChandra.out); | |CENTER: IA767 | &ref(IA767_step4_AGN_IRAC_wChandra.out); | &ref(IA767_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA767_step4_AGN_XMM_wChandra.out); | &ref(IA767_step4_AGN_radio_wChandra.out); | &ref(IA767_step4_AGN_wChandra.out); | |CENTER:BGCOLOR(yellow): All |BGCOLOR(yellow): &ref(Step4_AGN_IRAC_wChandra.out); |BGCOLOR(yellow): &ref(Step4_AGN_Chandra1arcsec_wChandra.out); |BGCOLOR(yellow): &ref(Step4_AGN_XMM_wChandra.out); |BGCOLOR(yellow): &ref(Step4_AGN_radio_wChandra.out); |BGCOLOR(yellow): &ref(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 ** &aname(noAGNpowered){non-AGN-powered LAE}; [#g51b654b] - &ref(step4_nonAGN.tar.gz); |CENTER:BGCOLOR(cyan): IA-band |CENTER:BGCOLOR(cyan): SFG |CENTER:BGCOLOR(cyan): SFG w/ EW_0 >= 100 A |h |CENTER: IA427 | &ref(IA427_step4_nonAGN_wChandra.out); | &ref(IA427_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA464 | &ref(IA464_step4_nonAGN_wChandra.out); | &ref(IA464_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA484 | &ref(IA484_step4_nonAGN_wChandra.out); | &ref(IA484_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA505 | &ref(IA505_step4_nonAGN_wChandra.out); | &ref(IA505_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA527 | &ref(IA527_step4_nonAGN_wChandra.out); | &ref(IA527_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA574 | &ref(IA574_step4_nonAGN_wChandra.out); | &ref(IA574_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA624 | &ref(IA624_step4_nonAGN_wChandra.out); | &ref(IA624_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA679 | &ref(IA679_step4_nonAGN_wChandra.out); | &ref(IA679_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA709 | &ref(IA709_step4_nonAGN_wChandra.out); | &ref(IA709_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA738 | &ref(IA738_step4_nonAGN_wChandra.out); | &ref(IA738_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA767 | &ref(IA767_step4_nonAGN_wChandra.out); | &ref(IA767_step4_nonAGN_sLAE_wChandra.out); | |CENTER:BGCOLOR(yellow): All |BGCOLOR(yellow): &ref(Step4_nonAGN_wChandra.out); |BGCOLOR(yellow): &ref(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 [[FrontPage]]
タイムスタンプを変更しない
[[FrontPage]] - 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 - &color(Red){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>LAE-Catalogs#Step2]] - [[Step 3>LAE-Catalogs#Step3]] -- [[matched catalog b/w LAE and new Chandra catalog by S. Toft on 2015/06/17>LAE-Catalogs#MatchedCatalogWithChandra]] - [[Step 4>LAE-Catalogs#Step4]] -- [[AGN-powered LAE>LAE-Catalogs#AGNpowered]] -- [[non-AGN-powered LAE>LAE-Catalogs#nonAGNpowered]] * &aname(Step2){Step 2}; [#kd94e4b7] - &ref(step2.tar.gz); - individual catalog: |CENTER:BGCOLOR(cyan): IA-band |CENTER:BGCOLOR(cyan): |h |CENTER: IA427 | &ref(IA427_wChandra.out); | |CENTER: IA464 | &ref(IA464_wChandra.out); | |CENTER: IA484 | &ref(IA484_wChandra.out); | |CENTER: IA505 | &ref(IA505_wChandra.out); | |CENTER: IA527 | &ref(IA527_wChandra.out); | |CENTER: IA574 | &ref(IA574_wChandra.out); | |CENTER: IA624 | &ref(IA624_wChandra.out); | |CENTER: IA679 | &ref(IA679_wChandra.out); | |CENTER: IA709 | &ref(IA709_wChandra.out); | |CENTER: IA738 | &ref(IA738_wChandra.out); | |CENTER: IA767 | &ref(IA767_wChandra.out); | |CENTER:BGCOLOR(yellow): All |BGCOLOR(yellow): &ref(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 * &aname(Step3){Step 3}; [#s55fadc9] - &ref(step3.tar.gz); - individual catalog: |CENTER:BGCOLOR(cyan): IA-band |CENTER:BGCOLOR(cyan): N_{undet} < 6 |CENTER:BGCOLOR(cyan): N_{undet} < 6 & χ_{ν}^2 <= 3 |CENTER:BGCOLOR(cyan): N_{undet} < 6 & χ_{ν}^2 <= 3 & EW/EW_{err,3σ} > 1 |h |CENTER: IA427 | &ref(IA427_Nundet5_wChandra.out); | &ref(IA427_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA427_step3_wChandra.out); | |CENTER: IA464 | &ref(IA464_Nundet5_wChandra.out); | &ref(IA464_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA464_step3_wChandra.out); | |CENTER: IA484 | &ref(IA484_Nundet5_wChandra.out); | &ref(IA484_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA484_step3_wChandra.out); | |CENTER: IA505 | &ref(IA505_Nundet5_wChandra.out); | &ref(IA505_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA505_step3_wChandra.out); | |CENTER: IA527 | &ref(IA527_Nundet5_wChandra.out); | &ref(IA527_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA527_step3_wChandra.out); | |CENTER: IA574 | &ref(IA574_Nundet5_wChandra.out); | &ref(IA574_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA574_step3_wChandra.out); | |CENTER: IA624 | &ref(IA624_Nundet5_wChandra.out); | &ref(IA624_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA624_step3_wChandra.out); | |CENTER: IA679 | &ref(IA679_Nundet5_wChandra.out); | &ref(IA679_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA679_step3_wChandra.out); | |CENTER: IA709 | &ref(IA709_Nundet5_wChandra.out); | &ref(IA709_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA709_step3_wChandra.out); | |CENTER: IA738 | &ref(IA738_Nundet5_wChandra.out); | &ref(IA738_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA738_step3_wChandra.out); | |CENTER: IA767 | &ref(IA767_Nundet5_wChandra.out); | &ref(IA767_Nundet5+chinu2lteq3_wChandra.out); | &ref(IA767_step3_wChandra.out); | |CENTER:BGCOLOR(yellow): All |BGCOLOR(yellow): &ref(Step3_Nundet5_wChandra.out); |BGCOLOR(yellow): &ref(Step3_Nundet5+chinu2lteq3_wChandra.out); |BGCOLOR(yellow): &ref(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 ** &aname(MatchedCatalogWithChandra){matched catalog b/w LAE and new Chandra catalog by S. Toft on 2015/06/17}; [#z9300fca] - within 1 arcsec: &ref(lya_x_1arcsec.txt); - within 2 arcsec: &ref(lya_x_2arcsec.txt); * &aname(Step4){Step 4}; [#ofd8b04a] ** &aname(AGNpowered){AGN-powered LAE}; [#b8d7f118] - &ref(step4_AGN.tar.gz); |CENTER:BGCOLOR(cyan): IA-band |CENTER:BGCOLOR(cyan): AGN (IRAC) |CENTER:BGCOLOR(cyan): AGN (Chandra) |CENTER:BGCOLOR(cyan): AGN (XMM) |CENTER:BGCOLOR(cyan): AGN (VLA) |CENTER:BGCOLOR(cyan): AGN |h |CENTER: IA427 | &ref(IA427_step4_AGN_IRAC_wChandra.out); | &ref(IA427_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA427_step4_AGN_XMM_wChandra.out); | &ref(IA427_step4_AGN_radio_wChandra.out); | &ref(IA427_step4_AGN_wChandra.out); | |CENTER: IA464 | &ref(IA464_step4_AGN_IRAC_wChandra.out); | &ref(IA464_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA464_step4_AGN_XMM_wChandra.out); | &ref(IA464_step4_AGN_radio_wChandra.out); | &ref(IA464_step4_AGN_wChandra.out); | |CENTER: IA484 | &ref(IA484_step4_AGN_IRAC_wChandra.out); | &ref(IA484_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA484_step4_AGN_XMM_wChandra.out); | &ref(IA484_step4_AGN_radio_wChandra.out); | &ref(IA484_step4_AGN_wChandra.out); | |CENTER: IA505 | &ref(IA505_step4_AGN_IRAC_wChandra.out); | &ref(IA505_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA505_step4_AGN_XMM_wChandra.out); | &ref(IA505_step4_AGN_radio_wChandra.out); | &ref(IA505_step4_AGN_wChandra.out); | |CENTER: IA527 | &ref(IA527_step4_AGN_IRAC_wChandra.out); | &ref(IA527_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA527_step4_AGN_XMM_wChandra.out); | &ref(IA527_step4_AGN_radio_wChandra.out); | &ref(IA527_step4_AGN_wChandra.out); | |CENTER: IA574 | &ref(IA574_step4_AGN_IRAC_wChandra.out); | &ref(IA574_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA574_step4_AGN_XMM_wChandra.out); | &ref(IA574_step4_AGN_radio_wChandra.out); | &ref(IA574_step4_AGN_wChandra.out); | |CENTER: IA624 | &ref(IA624_step4_AGN_IRAC_wChandra.out); | &ref(IA624_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA624_step4_AGN_XMM_wChandra.out); | &ref(IA624_step4_AGN_radio_wChandra.out); | &ref(IA624_step4_AGN_wChandra.out); | |CENTER: IA679 | &ref(IA679_step4_AGN_IRAC_wChandra.out); | &ref(IA679_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA679_step4_AGN_XMM_wChandra.out); | &ref(IA679_step4_AGN_radio_wChandra.out); | &ref(IA679_step4_AGN_wChandra.out); | |CENTER: IA709 | &ref(IA709_step4_AGN_IRAC_wChandra.out); | &ref(IA709_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA709_step4_AGN_XMM_wChandra.out); | &ref(IA709_step4_AGN_radio_wChandra.out); | &ref(IA709_step4_AGN_wChandra.out); | |CENTER: IA738 | &ref(IA738_step4_AGN_IRAC_wChandra.out); | &ref(IA738_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA738_step4_AGN_XMM_wChandra.out); | &ref(IA738_step4_AGN_radio_wChandra.out); | &ref(IA738_step4_AGN_wChandra.out); | |CENTER: IA767 | &ref(IA767_step4_AGN_IRAC_wChandra.out); | &ref(IA767_step4_AGN_Chandra1arcsec_wChandra.out); | &ref(IA767_step4_AGN_XMM_wChandra.out); | &ref(IA767_step4_AGN_radio_wChandra.out); | &ref(IA767_step4_AGN_wChandra.out); | |CENTER:BGCOLOR(yellow): All |BGCOLOR(yellow): &ref(Step4_AGN_IRAC_wChandra.out); |BGCOLOR(yellow): &ref(Step4_AGN_Chandra1arcsec_wChandra.out); |BGCOLOR(yellow): &ref(Step4_AGN_XMM_wChandra.out); |BGCOLOR(yellow): &ref(Step4_AGN_radio_wChandra.out); |BGCOLOR(yellow): &ref(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 ** &aname(noAGNpowered){non-AGN-powered LAE}; [#g51b654b] - &ref(step4_nonAGN.tar.gz); |CENTER:BGCOLOR(cyan): IA-band |CENTER:BGCOLOR(cyan): SFG |CENTER:BGCOLOR(cyan): SFG w/ EW_0 >= 100 A |h |CENTER: IA427 | &ref(IA427_step4_nonAGN_wChandra.out); | &ref(IA427_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA464 | &ref(IA464_step4_nonAGN_wChandra.out); | &ref(IA464_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA484 | &ref(IA484_step4_nonAGN_wChandra.out); | &ref(IA484_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA505 | &ref(IA505_step4_nonAGN_wChandra.out); | &ref(IA505_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA527 | &ref(IA527_step4_nonAGN_wChandra.out); | &ref(IA527_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA574 | &ref(IA574_step4_nonAGN_wChandra.out); | &ref(IA574_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA624 | &ref(IA624_step4_nonAGN_wChandra.out); | &ref(IA624_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA679 | &ref(IA679_step4_nonAGN_wChandra.out); | &ref(IA679_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA709 | &ref(IA709_step4_nonAGN_wChandra.out); | &ref(IA709_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA738 | &ref(IA738_step4_nonAGN_wChandra.out); | &ref(IA738_step4_nonAGN_sLAE_wChandra.out); | |CENTER: IA767 | &ref(IA767_step4_nonAGN_wChandra.out); | &ref(IA767_step4_nonAGN_sLAE_wChandra.out); | |CENTER:BGCOLOR(yellow): All |BGCOLOR(yellow): &ref(Step4_nonAGN_wChandra.out); |BGCOLOR(yellow): &ref(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 [[FrontPage]]
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