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J/A+A/396/503       Spectra of blue compact galaxies         (Kong+, 2002)

Spectroscopic study of blue compact galaxies. II. Spectral analysis and correlations. Kong X., Cheng F.Z., Weiss A., Charlot S. <Astron. Astrophys. 396, 503 (2002)> =2002A&A...396..503K
ADC_Keywords: Galaxies, spectra Keywords: galaxies: active - galaxies: Seyfert - galaxies: general - galaxies: stellar content Abstract: This is the second paper in a series studying the star formation rates, stellar components, metallicities, and star formation histories and evolution of a sample of blue compact galaxies. We analyzed spectral properties of 97 blue compact galaxies, obtained with the Beijing Astronomical Observatory (China) 2.16m telescope, with spectral range 3580Å-7400Å. We classify the spectra according to their emission lines: 13 of the total 97 BCG sample are non-emission line galaxies (non-ELGs); 10 have AGN-like emission (AGNs), and 74 of them are star-forming galaxies (SFGs). Emission line fluxes and equivalent widths, continuum fluxes, the 4000A Balmer break index and equivalent widths of absorption lines are measured from the spectra. Please find more detail information in File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 158 82 *Equivalent widths of emission lines, 72 SFGs + 10 AGNs table2.dat 175 82 *Observed flux of emission lines, 72 SFGs + 10 AGNs table3.dat 104 81 *Intrinsic flux of emission lines, 72 SFGs + 9 AGNs table4.dat 185 85 Average fluxes of continuum, 72 SFG + 13 non-SFG table6.dat 118 85 Equivalent widths of absorption features, 72 SFG + 13 non-SFG
Note on table1.dat and table2.dat: There are 74 star-forming BCG (SFG) in our sample, but the spectrum of I Zw207 has not 3600-4100Å, and the spectrum of IIZw67 has no Hβ emission line. Note on table3.dat: V II Zw 631 has not Hβ lines, and is not included in table3.
See also: J/A+A/389/845 : Spectra of blue compact galaxies (Kong+, 2002) J/A+A/425/417 : Star formation rates of blue compact galaxies (Kong+, 2004) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Galaxy names 11- 16 F6.2 0.1nm EWOII ?=0. Equivalent width of [OII]3727 (G1) 18- 23 F6.2 0.1nm EWHb ?=0. Equivalent width of Hβ4861 (G1) 25- 30 F6.2 0.1nm EWO3a ?=0. Equivalent width of [OIII]4959 (G1) 32- 38 F7.2 0.1nm EWO3b ?=0. Equivalent width of [OIII]5007 (G1) 40- 46 F7.2 0.1nm EWHa ?=0. Equivalent width of Hα6563 (G1) 48- 53 F6.2 0.1nm EWNII ?=0. Equivalent width of [NII]6583 (G1) 55- 59 F5.2 0.1nm EWSIIa ?=0. Equivalent width of [SII]6717 (G1) 61- 65 F5.2 0.1nm EWSIIb ?=0. Equivalent width of [SII]6731 (G1) 67- 71 F5.2 0.1nm EWHg ?=0. Equivalent width of Hγ4340 (G1) 73- 77 F5.2 0.1nm EWO3c ?=0. Equivalent width of [OIII]4363 (G1) 79- 83 F5.2 0.1nm EWHeI ?=0. Equivalent width of HeI5876 (G1) 85- 89 F5.2 0.1nm EWOI ?=0. Equivalent width of [OI]6300 (G1) 91- 93 A3 0.1nm Type AGN or SFG 95- 99 F5.2 0.1nm e_EWOII rms uncertainty of EWOII 101-104 F4.2 0.1nm e_EWHb rms uncertainty of EWHb 106-110 F5.2 0.1nm e_EWO3a rms uncertainty of EWO3a 112-116 F5.2 0.1nm e_EWO3b rms uncertainty of EWO3b 118-122 F5.2 0.1nm e_EWHa rms uncertainty of EWHa 124-127 F4.2 0.1nm e_EWNII rms uncertainty of EWNII 129-132 F4.2 0.1nm e_EWSIIa rms uncertainty of EWSIIa 134-137 F4.2 0.1nm e_EWSIIb rms uncertainty of EWSIIb 139-142 F4.2 0.1nm e_EWHg rms uncertainty of EWHg 144-147 F4.2 0.1nm e_EWO3c rms uncertainty of EWO3c 149-152 F4.2 0.1nm e_EWHeI rms uncertainty of EWHeI 154-157 F4.2 0.1nm e_EWOI rms uncertainty of EWOI
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Galaxy names 11- 17 F7.2 10-18W/m2 FOII ?=0. Flux of [OII]3727 (1) 19- 25 F7.2 10-18W/m2 FHb ?=0. Flux of Hbeta4861 (1) 27- 33 F7.2 10-18W/m2 FO3a ?=0. Flux of [OIII]4959 (1) 35- 42 F8.2 10-18W/m2 FO3b ?=0. Flux of [OIII]5007 (1) 44- 50 F7.2 10-18W/m2 FHa ?=0. Flux of Halpha6563 (1) 52- 57 F6.2 10-18W/m2 FNII ?=0. Flux of [NII]6583 (1) 59- 64 F6.2 10-18W/m2 FSIIa ?=0. Flux of [SII]6717 (1) 66- 70 F5.2 10-18W/m2 FSIIb ?=0. Flux of [SII]6731 (1) 72- 77 F6.2 10-18W/m2 FHg ?=0. Flux of Hgamma4340 (1) 79- 85 F7.2 10-18W/m2 FO3c ?=0. Flux of [OIII]4363 (1) 87- 92 F6.2 10-18W/m2 FHeI ?=0. Flux of HeI5876 (1) 94- 99 F6.2 10-18W/m2 FOI ?=0. Flux of [OI]6300 (1) 101-103 A3 --- Type AGN or SFG 105-110 F6.2 10-18W/m2 e_FOII rms uncertainty of FOII 112-116 F5.2 10-18W/m2 e_FHb rms uncertainty of FHb 118-122 F5.2 10-18W/m2 e_FO3a rms uncertainty of FO3a 124-128 F5.2 10-18W/m2 e_FO3b rms uncertainty of FO3b 130-134 F5.2 10-18W/m2 e_FHa rms uncertainty of FHa 136-140 F5.2 10-18W/m2 e_FNII rms uncertainty of FNII 142-146 F5.2 10-18W/m2 e_FSIIa rms uncertainty of FSIIa 148-151 F4.2 10-18W/m2 e_FSIIb rms uncertainty of FSIIb 153-157 F5.2 10-18W/m2 e_FHg rms uncertainty of FHg 159-163 F5.2 10-18W/m2 e_FO3c rms uncertainty of FO3c 165-170 F6.2 10-18W/m2 e_FHeI rms uncertainty of FHeI 171-175 F5.2 10-18W/m2 e_FOI rms uncertainty of FOI
Note (1): Fluxes in units of 10-15erg/cm2/s A 0.00 in the table indicates either that the corresponding segment of the spectrum is lacking or that the spectrum was too noisy in the region to give a reliable value of fluxes.
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Galaxy name 11- 17 F7.2 --- IOII ?=0. Intrinsic [OII]3727 flux relative to Hβ4861 (G1) 19- 24 F6.2 --- IO3a ?=0. Intrinsic [OIII]4959 flux relative to Hβ4861 (G1) 26- 32 F7.2 --- IO3b ?=0. Intrinsic [OIII]5007 flux relative to Hβ4861 (G1) 34- 39 F6.2 --- IHa ?=0. Intrinsic Halpha6563 flux relative to Hβ4861 (G1) 41- 46 F6.2 --- INII ?=0. Intrinsic [NII]6583 flux relative to Hβ4861 (G1) 48- 53 F6.2 --- ISIIa ?=0. Intrinsic [SII]6717 flux relative to Hβ4861 (G1) 55- 60 F6.2 --- ISIIb ?=0. Intrinsic [SII]6731 flux relative to Hβ4861 (G1) 62- 67 F6.2 --- IHg ?=0. Intrinsic Hgamma434 flux relative to Hβ4861 (G1) 69- 74 F6.2 --- IO3c ?=0. Intrinsic [OIII]4363 flux relative to Hβ4861 (G1) 76- 80 F5.2 --- IHeI ?=0. Intrinsic HeI5876 flux relative to Hβ4861 (G1) 82- 86 F5.2 --- IOI ?=0. Intrinsic [OI]6300 flux relative to Hβ4861 (G1) 88- 95 F8.2 10-18W/m2 IHb Intrinsic line flux of Hβ4861 97-100 F4.2 mag FHb Color excess 102-104 A3 --- Type AGN or SFG
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Galaxy name 11- 16 F6.3 10-18W/m2 F3660 ?=0. Average continuum flux at 3660Å (G1) 18- 24 F7.3 10-18W/m2 F3784 ?=0. Average continuum flux at 3784Å (G1) 26- 32 F7.3 10-18W/m2 F3814 ?=0. Average continuum flux at 3814Å (G1) 34- 40 F7.3 10-18W/m2 F3908 ?=0. Average continuum flux at 3908Å (G1) 42- 48 F7.3 10-18W/m2 F4020 ?=0. Average continuum flux at 4020Å (G1) 50- 56 F7.3 10-18W/m2 F4510 ?=0. Average continuum flux at 4510Å (G1) 58- 64 F7.3 10-18W/m2 F4630 ?=0. Average continuum flux at 4630Å (G1) 66- 72 F7.3 10-18W/m2 F5313 ?=0. Average continuum flux at 5313Å (G1) 74- 80 F7.3 10-18W/m2 F5500 ?=0. Average continuum flux at 5500Å (G1) 82- 88 F7.3 10-18W/m2 F6080 ?=0. Average continuum flux at 6080Å (G1) 90- 96 F7.3 10-18W/m2 F6630 ?=0. Average continuum flux at 6630Å (G1) 98-104 F7.3 10-18W/m2 F7040 ?=0. Average continuum flux at 7040Å (G1) 106-112 A7 --- Type non-SFG or SFG 114-118 F5.3 10-18W/m2 e_F3660 rms uncertainty on F3660 120-124 F5.3 10-18W/m2 e_F3784 rms uncertainty on F3784 126-130 F5.3 10-18W/m2 e_F3814 rms uncertainty on F3814 132-136 F5.3 10-18W/m2 e_F3908 rms uncertainty on F3908 138-143 F6.3 10-18W/m2 e_F4020 rms uncertainty on F4020 145-149 F5.3 10-18W/m2 e_F4510 rms uncertainty on F4510 151-155 F5.3 10-18W/m2 e_F4630 rms uncertainty on F4630 157-161 F5.3 10-18W/m2 e_F5313 rms uncertainty on F5313 163-167 F5.3 10-18W/m2 e_F5500 rms uncertainty on F5500 169-173 F5.3 10-18W/m2 e_F6080 rms uncertainty on F6080 175-179 F5.3 10-18W/m2 e_F6630 rms uncertainty on F6630 181-185 F5.3 10-18W/m2 e_F7040 rms uncertainty on F7040
Byte-by-byte Description of file: table6.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Galaxy names 11- 17 F7.3 0.1nm EWK ?=0. Equivalent width of CaIIK (G1) 19- 24 F6.3 0.1nm EWH ?=0. Equivalent width of CaIIH (G1) 26- 30 F5.3 0.1nm EWHd ?=0. Equivalent width of Hdelta (G1) 32- 37 F6.3 0.1nm EWCN ?=0. Equivalent width of CN (G1) 39- 44 F6.3 0.1nm EWGb ?=0. Equivalent width of Gband (G1) 46- 50 F5.3 0.1nm EWMg ?=0. Equivalent width of MgI+H (G1) 52- 56 F5.3 0.1nm EWNaI ?=0. Equivalent width of NaIIK (G1) 58- 62 F5.3 0.1nm EWD4n ?=0. 4000Å Break (G1) 64- 70 A7 --- Type non-SFG or SFG 72- 76 F5.3 0.1nm e_EWK rms uncertainty on EWK 78- 82 F5.3 0.1nm e_EWH rms uncertainty on EWH 84- 88 F5.3 0.1nm e_EWHd rms uncertainty on EWHd 90- 94 F5.3 0.1nm e_EWCN rms uncertainty on EWCN 96-100 F5.3 0.1nm e_EWGb rms uncertainty on EWGb 102-106 F5.3 0.1nm e_EWMg rms uncertainty on EWMg 108-112 F5.3 0.1nm e_EWNaI rms uncertainty on EWNaI 114-118 F5.3 0.1nm e_EWD4n rms uncertainty on EWD4n
Global notes: Note (G1): A 0.00 in the table indicates either that the corresponding segment of the spectrum is lacking or that the spectrum was too noisy in the region to give a reliable value of equivalent widths.
Acknowledgements: Xu Kong, xkong(at) References: Kong et al., Paper I 2002A&A...389..845K, Cat. J/A+A/389/845 Kong et al., Paper III 2003A&A...403..877K Kong, Paper IV 2004A&A...425..417K, Cat. J/A+A/425/417
(End) Patricia Bauer [CDS] 01-Aug-2003
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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