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[[FrontPage]] * Catalog of 6140 IA-excess candidates selected in Step 2: &ref(Step2.dat); [#u014795e] - (2015/10/23) Note: a bug in which the old results of Step 1 was wrongly used as input of EAZY are fixed -- ID=629513, which shows an excess from the frequency-matched continuum in IA709 band, moves from Ha+[NII] emitter candidate to others --- the number of Ha+[NII] emitter candidate changes: 34 --> 33 (IA709), 295 --> 294 (Total) --- at the same time, the number of others also changes: 41 --> 42 (IA709), 552 --> 553 (Total) - (2015/10/22) Note: the treatment of the magnitude for the undetected objects is further revised -- In the previous analysis, some undetected objects have f_ν < 1.5σ because of σ is revised to the limiting flux given after f_ν is set to 1.5σ. It should be f_ν = 1.5σ with the revised σ -- In the revised analysis, these objects are revised to have f_ν = 1.5σ. -- As a result, 16 excess candidates (17 excess IA-bands) are removed from the sample of Step 1 IA-excess candidates. No candidate is newly added. - (2015/10/14) Note: the treatment of the magnitude and its error for the undetected objects is revised -- In the previous analysis, since their magnitudes are remained to be the original values, that is, 99.0, the linear fluxes are negligibly small. In the case that these fluxes are used to evaluate IAc, the resultant IAc become too faint. -- In the revised analysis, their magnitudes are revised to be 1.5σ. -- As a result, 28 excess candidates (35 excess IA-bands) are removed from the sample of Step 1 IA-excess candidates. No candidate is newly added. - (2015/10/05) Note: errors of Subaru i'- and GALEX FUV-bands magnitudes are modified -- Some objects undetected in these bands have values larger than 90 as magnitude error, although normally they should have 3σ limiting magnitudes in error slot. -- These are now modified into 26.1 ABmag and 25.7 ABmag for the Subaru i'- and GALEX FUV-bands, respectively. --- The former limiting magnitude is given in Taniguchi+07 and used originally in Step 1 as 3σ limiting magnitude of the Subaru i' band. --- The latter is taken from Salvato+09; although it is unclear whether this magnitude is total one or aperture one, we assume that this is 5σ limiting magnitude in 3.8"φ diameter aperture. Hence, it is converted to 3σ limiting magnitude in total magnitude via adding -2.5log10(3/5) + 2.5log10(0.759) and then converted to 3σ limiting magnitude in 3"φ diameter aperture using auto_offset of each object. - (2015/09/25) Note: magnitudes, errors, and limiting magnitudes of the IRAC ch1--4 are modified -- Since the magnitudes of all IRAC bands in the photometric catalog are '''total magnitudes''', they should be transformed into '''3"φ diameter aperture magnitudes''' using '''auto_offset''' provided in the photometric catalog. -- Although the definition of the limiting magnitudes of the IRAC bands given in Salvato+09 are unclear, we assume that it is the 5σ limiting magnitude in 3.8"φ diameter aperture. --- Hence, they are converted to 3σ limiting magnitudes in total magnitude via adding -2.5log10(3/5) + 2.5log10(0.759) and then converted to 3σ limiting magnitudes in 3"φ diameter aperture using auto_offset of each object. -- Related to these modifications, information of auto_offset is added in the catalog - (2015/09/07) Note: AGN flags are now complete. - (2015/08/18) Note: -- AGN flags for XMM and VLA are now complete. But those for Chandra are not complete yet [flag = -1]. -- ID=1968804 is now present -- For the 43 candidates whose Subaru i'-band magnitudes are saturated, the revised EAZY results are now used to construct the above catalog of Step2.dat - (2015/08/16) Note: -- AGN flags for Chandra, XMM, and VLA are not complete yet. -- ID=1968804 is absent because of the absence of its EAZY output. -- For the 43 candidates whose Subaru i'-band magnitudes are saturated (i.e., i' < 21 ABmag in the original photometric catalog), EAZY results should be revised because wrongly corrected CFHT i* magnitudes are assigned for them: the ID list of these 43 candidates &ref(Step1_iband_replaced_candidates.dat); - format (written as headers in the above catalog): # (1)ID (2,3)RA,DEC(J2000)[deg] # (4--19)quantities from photo-z catalog: # --- (4,5,6)median,1sigma lower,1sigma upper limits of photo-z measured using the galaxy templates[zPDF,zPDF_l68,zPDF_u68] # --- (7)best fit template at zPDF[1--8:Ell-S0, 9--15:Sa-Sc, 16--19:Sd-Sdm from Polletta et al., >=20:starburst from BC03] # --- (8)best-fit additional extinction E(B-V) at zPDF[mag] # --- (9)extinction law[1:prevot, 2:Calzetti, 3,4:Calzetti+2175bump] # --- (10)number of filters used in the fit # --- (11)best-fit BC03 model (12)best-fit model age[yr] (13)best-fit model extinction E(B-V)[mag] # --- (14,15,16)log10[Mstar/Msun] for median,1sigma lower,1sigma upper[mass_med,mass_inf,mass_sup] # --- (17,18,19)log10[SFR/(Msun/yr)] for median,1sigma lower,1sigma upper[sfr_med,sfr_inf,sfr_sup] # (20)auto-offset[mag](aperture correction from 3" diameter aperture magnitude to total magnitude, band independent) # (21+2i,22+2i)mag, 1sigma error of mag corrected for Galactic extinction and offset[i=0--36]: # --- i= 0 (21,22)CFHT u* # --- i= 1 (23,24)Subaru B # --- i= 2 (25,26)Subaru V # --- i= 3 (27,28)Subaru g' # --- i= 4 (29,30)Subaru r' # --- i= 5 (31,32)Subaru i' # --- i= 6 (33,34)CFHT i* # --- i= 7 (35,36)Subaru z' # --- i= 8 (37,38)UKIRT J # --- i= 9 (39,40)CTIO/KPNO Ks # --- i=10 (41,42)CFHT Ks # --- i=11 (43,44)Subaru IA427 # --- i=12 (45,46)Subaru IA464 # --- i=13 (47,48)Subaru IA484 # --- i=14 (49,50)Subaru IA505 # --- i=15 (51,52)Subaru IA527 # --- i=16 (53,54)Subaru IA574 # --- i=17 (55,56)Subaru IA624 # --- i=18 (57,58)Subaru IA679 # --- i=19 (59,60)Subaru IA709 # --- i=20 (61,62)Subaru IA738 # --- i=21 (63,64)Subaru IA767 # --- i=22 (65,66)Subaru IA827 # --- i=23 (67,68)Subaru NB711 # --- i=24 (69,70)Subaru NB816 # --- i=25 (71,72)Spitzer IRAC ch1 # --- i=26 (73,74)Spitzer IRAC ch2 # --- i=27 (75,76)Spitzer IRAC ch3 # --- i=28 (77,78)Spitzer IRAC ch4 # --- i=29 (79,80)GALEX FUV # --- i=30 (81,82)GALEX NUV # --- i=31 (83,84)UltraVISTA Y # --- i=32 (85,86)UltraVISTA J # --- i=33 (87,88)UltraVISTA H # --- i=34 (89,90)UltraVISTA Ks # --- i=35 (91,92)CFHT H # --- i=36 (93,94)Subaru z'' # (95--100)AGN-related flags: # --- ( 95)flag for detection in all 4 IRAC bands[0:no, 1:yes] # --- ( 96)flags for AGN from IRAC color[Donley+12 criteria][0:non-AGN, 1:AGN] # --- ( 97)flags for AGN from Chandra[0:non-AGN, 1:AGN] # --- ( 98)flags for AGN from XMM-Newton[0:non-AGN, 1:AGN] # --- ( 99)flags for AGN from VLA[0:non-AGN, 1:AGN] # --- (100)flags for AGN from one of them[0:non-AGN, 1:AGN] # (101--112)flag for 12 IA bands[0:undetected, 1:detected] # (113)N_undetectedIA # (114--162)Step 1 related quantities: # --- (114+4i)flag of excess IA band for 12 IA-bands[-1:unjudged, 0:non-excess, others:excess][i=0--11] # --- (115+4i)IAc[ABmag][i=0--11] # --- (116+4i)IAc-IA[ABmag][i=0--11] # --- (117+4i)3sigma(IAc-IA)[ABmag][i=0--11] # ------ i= 0 (114,115,116,117)IA427 # ------ i= 1 (118,119,120,121)IA464 # ------ i= 2 (122,123,124,125)IA484 # ------ i= 3 (126,127,128,129)IA505 # ------ i= 4 (130,131,132,133)IA527 # ------ i= 5 (134,135,136,137)IA574 # ------ i= 6 (138,139,140,141)IA624 # ------ i= 7 (142,143,144,145)IA679 # ------ i= 8 (146,147,148,149)IA709 # ------ i= 9 (150,151,152,153)IA738 # ------ i=10 (154,155,156,157)IA767 # ------ i=11 (158,159,160,161)IA827 # --- (162)N_ex^temp # (163--195)Step 2 related quantities: # --- (163)Nsol # --- (164--179)quantities related to the primary z_ph solution: # ------ (164)P(z_ph1) # ------ (165)chi_nu^2(z_ph1) # ------ (166)z_ph1 # ------ (167--178)line ID for 12 IA bands(1:Lya, 2:CIV, 3:CIII], 4:MgII, 5:[OII], 6:[OIII]+Hb, 7:Ha+[NII], 99:others) # ------ (179)N_ex^cons # --- (180--195)quantities related to the secondary z_ph solution: # ------ (180)P(z_ph2)/P(z_ph1) # ------ (181)chi_nu^2(z_ph2) # ------ (182)z_ph2 # ------ (183--194)line ID for 12 IA bands(1:Lya, 2:CIV, 3:CIII], 4:MgII, 5:[OII], 6:[OIII]+Hb, 7:Ha+[NII], 99:others) # ------ (195)N_ex^cons //- 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 //- the above catalog is constructed by using the fortran program &ref(Step2_zph.f); and the following data sets: //-- (1) the catalog of 5357 IA-excess candidates selected in Step 1: &ref(Transfer-Step1-Catalogs/Step1.txt); //-- (2) a list of the redshift range for each combination of excess IA band and emission line (see [[below>Transfer-Step2-Catalogs#z_phDetermination]] for details): &ref(zrange4.txt); //-- (3) the likelihood and reduced χ^2 data of individual candidate calculated through EAZY: '''ID'''.pz2 //--- the sizes of these files are too large to be attached here; they are uploaded on [[here>http://cosmos.phys.sci.ehime-u.ac.jp/~kobayashi/files/PZpz2.tar.gz]] //--- format: (1)redshift z (2)xxx (3)reduced χ^2(z) (4)xxx (5)xxx (6)xxx (7)xxx (8)Pz(z) //--- an example of this formated file: &ref(1508586.pz2); (SF-MAESTLO #1) * Number Counts of Each Line Emitter Candidates for 12 IA bands [#j21e7e37] - (2015/10/23): ---------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total ---------------------------------------------------------------------------------------- Lya: 245 153 318 115 148 23 35 18 6 8 2 0 1071 CIV: 128 75 129 54 63 52 38 7 8 1 1 2 558 CIII]: 49 78 95 78 48 18 68 26 26 23 10 8 527 MgII: 27 36 49 46 43 33 59 65 54 54 30 59 555 [OII]: 64 64 101 37 34 23 57 37 24 59 50 82 632 [OIII]+Hb: 0 0 6 24 59 120 188 293 326 393 427 618 2454 Ha+[NII]: 0 0 0 0 0 0 0 18 33 69 58 116 294 others: 42 60 68 31 56 33 53 52 42 47 35 34 553 ---------------------------------------------------------------------------------------- total: 555 466 766 385 451 302 498 516 519 654 613 919 6644 ---------------------------------------------------------------------------------------- -- this modification is originated by the fix of a bug in which the old data was used as input of EAZY wrongly. see above for the details. - (2015/10/22): ---------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total ---------------------------------------------------------------------------------------- Lya: 245 153 318 115 148 23 35 18 6 8 2 0 1071 CIV: 128 75 129 54 63 52 38 7 8 1 1 2 558 CIII]: 49 78 95 78 48 18 68 26 26 23 10 8 527 MgII: 27 36 49 46 43 33 59 65 54 54 30 59 555 [OII]: 64 64 101 37 34 23 57 37 24 59 50 82 632 [OIII]+Hb: 0 0 6 24 59 120 188 293 326 393 427 618 2454 Ha+[NII]: 0 0 0 0 0 0 0 18 34 69 58 116 295 others: 42 60 68 31 56 33 53 52 41 47 35 34 552 ---------------------------------------------------------------------------------------- total: 555 466 766 385 451 302 498 516 519 654 613 919 6644 -----------------------------------------------------------------------------------------[https://seehdfilm.com Film izle] -- this modification is originated by the further revision of the treatment of the magnitude for the undetected objects. see above for the details. - (2015/10/14): ---------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total ---------------------------------------------------------------------------------------- Lya: 245 153 318 115 149 24 35 19 6 8 2 0 1074 CIV: 128 75 129 54 63 52 38 7 8 1 1 2 558 CIII]: 50 78 95 78 48 19 69 26 26 23 10 8 530 MgII: 27 36 49 46 44 34 60 66 54 55 30 59 560 [OII]: 64 64 101 37 34 25 57 37 24 59 50 82 634 [OIII]+Hb: 0 0 6 24 59 120 188 293 326 394 427 618 2455 Ha+[NII]: 0 0 0 0 0 0 0 18 34 69 58 116 295 others: 43 60 69 31 56 33 54 52 41 47 35 34 555 ---------------------------------------------------------------------------------------- total: 557 466 767 385 453 307 501 518 519 656 613 919 6661 ---------------------------------------------------------------------------------------- -- this modification is originated by the revision of the treatment of the magnitude and its error for the undetected objects. see [[Transfer-Step1-Catalogs]] for the details. - (2015/10/05): ---------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total ---------------------------------------------------------------------------------------- Lya: 247 154 323 116 150 24 35 19 6 8 2 0 1084 CIV: 128 76 130 54 63 52 38 7 8 1 1 2 560 CIII]: 51 78 95 78 48 19 69 28 27 24 10 8 535 MgII: 27 37 49 46 44 34 62 67 55 55 30 59 565 [OII]: 64 64 102 37 34 25 58 37 24 59 50 82 636 [OIII]+Hb: 0 0 6 24 59 122 188 293 326 395 427 618 2458 Ha+[NII]: 0 0 0 0 0 0 0 18 33 69 58 116 294 others: 43 60 69 31 56 34 55 55 43 48 36 34 564 ---------------------------------------------------------------------------------------- total: 560 469 774 386 454 310 505 524 522 659 614 919 6696 ---------------------------------------------------------------------------------------- -- this modification is originated by the modification of the errors of Subaru i'- and GALEX FUV-bands magnitudes. see [[Transfer-Step1-Catalogs]] for the details. - (2015/09/27): ---------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total ---------------------------------------------------------------------------------------- Lya: 247 154 322 117 149 24 35 19 6 8 2 0 1083 CIV: 128 77 130 53 63 50 38 7 8 1 1 2 558 CIII]: 51 75 95 77 47 20 69 28 27 24 10 8 531 MgII: 27 37 49 44 43 34 62 67 55 55 30 59 562 [OII]: 64 64 102 37 34 25 58 37 24 59 50 82 636 [OIII]+Hb: 0 0 6 24 59 122 188 293 326 395 427 618 2458 Ha+[NII]: 0 0 0 0 0 0 0 18 33 69 58 116 294 others: 43 62 70 34 59 35 55 55 43 48 36 34 574 ---------------------------------------------------------------------------------------- total: 560 469 774 386 454 310 505 524 522 659 614 919 6696 ---------------------------------------------------------------------------------------- -- this modification is originated by (1) the changes of the IRAC magnitudes and errors and (2) the correctly using the reduced χ^2 of the EAZY output - (2015/08/26): ---------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total ---------------------------------------------------------------------------------------- Lya: 243 120 221 99 122 20 20 20 6 8 2 0 881 CIV: 115 44 68 42 41 38 22 7 9 1 1 2 390 CIII]: 41 63 65 62 33 13 30 29 27 29 13 7 412 MgII: 24 28 24 33 33 24 31 64 55 52 30 57 455 [OII]: 59 58 69 27 30 21 27 41 25 60 48 66 531 [OIII]+Hb: 0 0 9 21 41 96 158 292 323 396 421 581 2338 Ha+[NII]: 0 0 0 0 0 0 0 18 33 59 56 105 271 others: 78 156 318 102 154 98 217 53 44 54 43 101 1418-[https://seehdfilm.com Film izle] ---------------------------------------------------------------------------------------- total: 560 469 774 386 454 310 505 524 522 659 614 919 6696 ---------------------------------------------------------------------------------------- -- this modification is caused by a change of the significant figure of the emission lines from 4 digits to 5 digits --- (e.g.) Lya: 1216 A --> 1215.7 A - (2015/08/25): ---------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total ---------------------------------------------------------------------------------------- Lya: 244 120 221 99 122 20 20 20 6 8 2 0 882 CIV: 114 44 68 42 41 38 22 7 9 1 1 2 389 CIII]: 41 63 65 62 33 13 30 29 27 29 13 7 412 MgII: 24 28 24 33 33 24 31 64 55 52 30 57 455 [OII]: 59 58 69 27 30 21 27 41 25 60 48 66 531 [OIII]+Hb: 0 0 9 21 41 96 158 291 323 396 421 581 2337 Ha+[NII]: 0 0 0 0 0 0 0 19 33 59 56 105 272 others: 78 156 318 102 154 98 217 53 44 54 43 101 1418 ---------------------------------------------------------------------------------------- total: 560 469 774 386 454 310 505 524 522 659 614 919 6696 ---------------------------------------------------------------------------------------- -- this modification is caused by a bug that there is no space between p(z) and χ_{ν}^2 of the primary solution for 8 sources in Step2.dat - (2015/08/18): ---------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total ---------------------------------------------------------------------------------------- Lya: 244 120 221 99 122 20 20 20 6 8 2 0 882 CIV: 114 44 68 42 41 38 22 7 9 1 1 2 389 CIII]: 41 63 65 62 33 13 30 29 27 29 13 7 412 MgII: 24 28 24 33 33 24 31 64 55 52 30 57 455 [OII]: 59 58 69 27 30 21 27 41 25 60 48 66 531 [OIII]+Hb: 0 0 9 21 41 96 158 291 323 396 421 581 2337 Ha+[NII]: 0 0 0 0 0 0 0 19 33 59 56 105 272 others: 78 156 317 103 154 101 213 53 44 54 43 101 1417 ---------------------------------------------------------------------------------------- total: 560 469 773 387 454 313 501 524 522 659 614 919 6695 ---------------------------------------------------------------------------------------- - (2015/08/16): -- see the above notes; the following table will be revised -------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total -------------------------------------------------------------------------------------- Lya: 244 120 221 99 122 20 20 20 6 8 2 0 882 CIV: 114 45 68 42 41 38 22 7 9 1 1 2 390 CIII]: 41 63 65 62 33 13 30 29 27 29 13 7 412 MgII: 24 28 25 33 33 24 31 64 55 52 30 58 457 [OII]: 60 58 69 27 30 21 27 41 25 60 48 66 532 [OIII]+Hb: 0 0 9 22 44 100 160 292 324 396 424 582 2353 Ha+[NII]: 0 0 0 0 0 0 0 20 36 67 60 114 297 others: 78 154 317 101 151 95 211 51 40 46 36 90 1370 -------------------------------------------------------------------------------------- total: 561 468 774 386 454 311 501 524 522 659 614 919 6693 -------------------------------------------------------------------------------------- - table: &ref(p46_COSMOS20_LAE.jpg,,75%); -- the above table is found to be wrong on 9th July, 2015 -- correct counts are the following based on &ref(lineID_150305.txt);: -------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total -------------------------------------------------------------------------------------- Lya: 243 119 220 97 122 20 20 20 6 8 2 0 877 CIV: 114 46 68 43 41 37 21 7 9 1 1 2 390 CIII]: 41 61 65 61 31 12 29 29 27 30 13 7 406 MgII: 25 28 26 33 33 24 31 65 55 53 30 58 461 [OII]: 61 56 68 26 28 21 28 41 25 60 48 66 528 [OIII]+Hb: 0 0 9 22 42 101 160 292 325 395 424 581 2351 Ha+[NII]: 0 0 0 0 0 0 0 20 36 66 60 112 294 others: 35 55 56 27 39 30 41 51 39 46 36 28 483 -------------------------------------------------------------------------------------- total: 519 365 512 309 336 245 330 525 522 659 614 854 5790 -------------------------------------------------------------------------------------- -- the above counts are found to still include several errors on 10--13th July, 2015. correct counts are the following based on &ref(lineID_150710.txt); (19:08 13th July, 2015 from MARK): -------------------------------------------------------------------------------------- IA427 IA464 IA484 IA505 IA527 IA574 IA624 IA679 IA709 IA738 IA767 IA827 Total -------------------------------------------------------------------------------------- Lya: 244 119 220 97 122 20 20 20 6 8 2 0 878 CIV: 114 46 68 43 41 37 21 7 9 1 1 2 390 CIII]: 41 61 65 61 31 12 29 29 27 30 13 7 406 MgII: 24 28 26 33 33 24 31 65 55 53 30 58 460 [OII]: 61 56 68 26 28 21 28 41 25 60 48 66 528 [OIII]+Hb: 0 0 9 22 42 101 160 292 325 395 424 581 2351 Ha+[NII]: 0 0 0 0 0 0 0 20 36 66 60 112 294 others: 35 55 56 27 39 30 41 51 39 46 36 28 483 -------------------------------------------------------------------------------------- total: 519 365 512 309 336 245 330 525 522 659 614 854 5790 -------------------------------------------------------------------------------------- --- this table is reproduced if we use the above &ref(Step2.txt); and the awk script to count the number of individual line emitter candidates of &ref(count_Step2.awk); * &aname(z_phDetermination){determination of the redshift range for each combination of excess IA band and emission line}; [#y21ca552] - Table: -- (2015/08/26): Ha+[NII] [OIII]+Hb [OII] MgII CIII] CIV Lya 1 -0.3692 -0.3342 -0.1705 -0.1032 0.1142 0.1696 0.4843 0.5581 1.1759 1.2840 1.6803 1.8135 2.4162 2.5860 ! IA427 2 -0.3128 -0.2758 -0.0964 -0.0245 0.2138 0.2723 0.6170 0.6949 1.3704 1.4846 1.9198 2.0605 2.7216 2.9009 ! IA464 3 -0.2813 -0.2425 -0.0550 0.0203 0.2694 0.3307 0.6911 0.7727 1.4790 1.5987 2.0537 2.2011 2.8921 3.0801 ! IA484 4 -0.2488 -0.2095 -0.0123 0.0647 0.3268 0.3886 0.7675 0.8499 1.5910 1.7118 2.1916 2.3404 3.0680 3.2576 ! IA505 5 -0.2196 -0.1784 0.0262 0.1067 0.3784 0.4433 0.8363 0.9228 1.6918 1.8186 2.3158 2.4720 3.2263 3.4254 ! IA527 6 -0.1454 -0.0993 0.1237 0.2132 0.5095 0.5823 1.0108 1.1079 1.9477 2.0900 2.6311 2.8063 3.6281 3.8514 ! IA574 7 -0.0765 -0.0256 0.2143 0.3125 0.6311 0.7117 1.1729 1.2803 2.1853 2.3427 2.9237 3.1176 4.0010 4.2482 ! IA624 8 0.0041 0.0609 0.3204 0.4290 0.7736 0.8637 1.3627 1.4828 2.4635 2.6395 3.2664 3.4833 4.4379 4.7142 ! IA679 9 0.0500 0.1039 0.3807 0.4869 0.8546 0.9393 1.4707 1.5834 2.6218 2.7871 3.4614 3.6650 4.6864 4.9459 ! IA709 10 0.0932 0.1485 0.4374 0.5470 0.9308 1.0176 1.5722 1.6878 2.7706 2.9401 3.6447 3.8535 4.9200 5.1861 ! IA738 11 0.1391 0.2008 0.4978 0.6175 1.0119 1.1096 1.6802 1.8103 2.9290 3.1197 3.8398 4.0747 5.1686 5.4680 ! IA767 12 0.2257 0.2847 0.6116 0.7305 1.1648 1.2570 1.8839 2.0067 3.2276 3.4075 4.2076 4.4293 5.6375 5.9200 ! IA827 --- this modification is caused by a change of the significant figure of the emission lines from 4 digits to 5 digits (e.g.) Lya: 1216 A --> 1215.7 A --- corresponding z_ph for each line emitter in each IA band 1:Lya 2:CIV 3:CIII] 4:MgII 5:[OII] 6:[OIII]+Hb 7:Ha+[NII] IA427: 2.501 1.747 1.230 0.521 0.142 0.000 0.000 IA464: 2.811 1.990 1.427 0.656 0.243 0.000 0.000 IA484: 2.986 2.127 1.539 0.732 0.300 0.010 0.000 IA505: 3.163 2.266 1.651 0.809 0.358 0.032 0.000 IA527: 3.326 2.394 1.755 0.880 0.411 0.066 0.000 IA574: 3.740 2.719 2.019 1.059 0.546 0.168 0.000 IA624: 4.125 3.021 2.264 1.227 0.671 0.263 0.000 IA679: 4.576 3.375 2.552 1.423 0.819 0.375 0.033 IA709: 4.816 3.563 2.704 1.527 0.897 0.434 0.077 IA738: 5.053 3.749 2.855 1.630 0.974 0.492 0.121 IA767: 5.318 3.957 3.024 1.745 1.061 0.558 0.170 IA827: 5.779 4.318 3.318 1.945 1.211 0.671 0.255 //-- &ref(zrange4.txt); &ref(p45_COSMOS20_LAE.jpg,,50%); - Figures: &ref(AGNset_COSMOS18_multi_IA_AGNset.jpg,,75%); &ref(AGNset_each_COSMOS18_multi_IA_AGNset.jpg,,50%); - these redshift ranges of z_min--z_max are calculated using λ_eff +/- FWHM/2 of each IA band and λ_rest of each line -- if z_max < 0, physically there is no chance detecting the emission line with the IA band: in this case, a straight line is inserted in the above table -- if z_max > 0 and z_min < 0, z_min = 0 is adopted in the above table - for single line emitters, z_ph is adopted to be the center of the possible redshift range: that is, z_ph = (z_max + z_min) / 2 -- for the lines with z_min > 0, z_ph corresponds to the redshift corresponding to λ_eff -- for [OIII]+Hβ and Hα+[NII] lines, z_max and z_min are evaluated as the redshift at which either one of the lines is out and in the wavelengths of λ +/- FWHM/2 (22:43 9th July, 2015 from Y. Shioya) - for dual and multiple line emitters, z_ph is also adopted to be the center of the possible redshift range in which the combination of the IA-band excesses can be explained as a combination of the redshifted several emission lines - the list of the redshifts assigned to the IA-excess candidates in Step 2 (replaced into the correct list on 14th July, 2015 by MARK and then modified on 20th July, 2015 by MARK) made by using the above &ref(Step2.txt); and an awk script of &ref(make_zph_list.awk);: &ref(zph_list.txt); -- old list is found to (1) suffer from the computational noise caused by coding without an explicit expression for the variables of double precision and (2) fail to assign correct redshift range in which each emission line is included according to the coding to judge the edges of the range (see email from MARK on 19:08 13th July, 2015).
