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J/A+A/442/109       Hamburg/SAO Survey for ELGs. VI.         (Pustilnik+, 2005)

The Hamburg/SAO Survey for emission-line galaxies. VI. The Sixth List of 126 Galaxies. Pustilnik S.A., Engels D., Lipovetsky V.A., Kniazev A.Y., Pramskij A.G., Ugryumov A.V., Masegosa J., Izotov Y.I., Chaffee F., Marquez I., Teplyakova A.L., Hopp U., Brosch N., Hagen H.-J., Martin J.-M. <Astron. Astrophys. 442, 109 (2005)> =2005A&A...442..109P
ADC_Keywords: Galaxies, spectra ; QSOs ; Spectroscopy ; Redshifts Keywords: surveys - galaxies: fundamental parameters - galaxies: distances and redshifts - galaxies: starburst - galaxies: quasars: redshifts Abstract: We present the sixth list with results of the Hamburg/SAO Survey for Emission-Line Galaxies. The final list resulted from follow-up spectroscopy conducted with the 4.5m MMT telescope in 1996, and with 2.2m CAHA and 6m SAO telescopes in 2000 to 2003. The data of this snap-shot spectroscopy survey confirmed 134 emission-line objects out of 182 observed candidates and allowed their quantitative spectral classification and redshift determination. We classify 73 emission-line objects as definite or probable blue compact or HII galaxies (BCG), 8 as QSOs, 4 as Seyfert 1 and 2 galaxies. 30 low-excitation objects were classified as definite or probable starburst nuclei (SBN), 3 as dwarf amorphous nuclei starburst galaxies (DANS) and 2 as LINERs. Due to the low signal-to-noise ratio we could not classify 14 ELGs (NON). For another 9 galaxies we did not detect any significant emission lines. For 98 emission-line galaxies, the redshifts and/or line intensities are determined for the first time. For the remaining 28 previously-known ELGs we give either improved data the line intensities or some independent measurements. The detection rate of ELGs is ∼70%. This paper completes the classification of strong-lined ELGs found in the zone of the Hamburg/SAO survey. Together with previously known BCG/HII galaxies in this zone, this sample of ∼500 objects is the largest to date in a well bound region. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 102 126 Parameters of the 126 observed emission line galaxies table4.dat 97 126 Results of line measurements table5.dat 85 8 Parameters of QSOs table6.dat 102 9 Galaxies without emission lines table7.dat 91 26 Stars
See also: http://www.hs.uni-hamburg.de/DE/For/Exg/Sur/hss/soucat/index.html : page of Hamburg-SAO Survey for Emission-Line Galaxies (finding charts and spectra) J/A+AS/135/511 : The Hamburg/SAO Survey for ELGs. I. (Ugryumov+ 1999) J/A+AS/137/299 : The Hamburg/SAO Survey for ELGs. II. (Pustilnik+ 1999) J/A+AS/142/417 : The Hamburg/SAO Survey for ELGs. III. (Hopp+, 2000) J/A+A/366/771 : The Hamburg/SAO Survey for ELGs. IV. (Kniazev+, 2001) J/A+A/374/907 : The Hamburg/SAO Survey for ELGs. V. (Ugryumov+, 2001) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Name of object 10 A1 --- m_Name [B] Multiplicity index on Name 12 A1 --- n_Name [*] *: galaxies from the second priority APM selected sample 15- 16 I2 h RAh Right ascension (B1950) 18- 19 I2 min RAm Right ascension (B1950) 21- 24 F4.1 s RAs Right ascension (B1950) 26 A1 --- DE- Declination sign (B1950) 27- 28 I2 deg DEd Declination (B1950) 30- 31 I2 arcmin DEm Declination (B1950) 33- 34 I2 arcsec DEs Declination (B1950) 39- 43 I5 km/s HRV Heliocentric radial velocity 46- 48 I3 km/s e_HRV Error of radial velocity 51 A1 --- n_Bmag [+] +: APM magnitudes 52- 56 F5.2 mag Bmag Magnitude in B filter 58- 63 F6.2 mag BMAG Absolute B-magnitude, not corrected for the Galaxy extinction 65- 69 A5 --- MType Spectral classification (1) 73- 95 A23 --- Names Other names from NED 99-102 A4 --- Ref References to other sources of spectral information (2)
Note (1): Only rough classification were done due to low S/N spectra. Spectral classification follows Salzer et al., 1989ApJS...70..479S, with the following abbreviations: BCG = blue compact or HII galaxy DANS = dwarf amorphous nuclei starburst galaxy LINER = LINER galaxy SBN = starburst galaxy Sy = Seyfert galaxy NON = not classified Note (2): References are numbered as follows: 1 = 2001, Cat. J/A+A/366/771, Kniazev et al., Paper IV 2 = 1999, Cat. J/A+AS/137/299, Pustilnik et al. Paper II 3 = 2001, Cat. J/A+A/374/907, Ugryumov et al., Paper V 4 = 2000, Cat. J/A+AS/142/417, Hopp et al., Paper III, 5 = 1999, Cat. J/A+AS/135/511, Ugryumov et al., Paper I 6 = 1994, Cat. J/AJ/107/1245, Schneider et al. 7 = 1996, Cat. J/A+AS/116/43, Popescu et al. 8 = 1998A&AS..133...13P, Popescu et al. 9 = 1998A&A...330...25G, Grupe et al. 10 = 1998, Cat. J/A+AS/127/145, Bade et al.
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Name Name of object 11 A1 --- pp [*] *: Objects observed under poor photometric conditions 13- 15 A3 --- Hb [Ha abs] Hβ not detected (3) 18 A1 --- Tel [BCM] Telescope used (4) 20- 24 F5.1 10-19W/m2 F4861 ? Observed flux in Hβ emission line (in 10-16erg/s/cm2) 26 A1 --- q_F4861 [abcdu] class of relative error (5) 30- 33 F4.2 --- [OII]/Hb ? Emission line fluxes ratio [OII]3727/Hβ 35 A1 --- q_[OII]/Hb [abcdu] class of relative error (5) 39- 42 F4.2 --- [OIII]/Hb ? Emission line fluxes ratio [OIII]5007/Hβ 44 A1 --- q_[OIII]/Hb [abcdu] class of relative error (5) 47 A1 --- u_[OIII]/Hb [1234] Uncertainty note (6) 49- 52 F4.2 --- Ha/Hb ? Emission line fluxes ratio Hα/Hβ 54 A1 --- q_Ha/Hb [abcdu] class of relative error (5) 58 A1 --- n_Ha/Hb Uncertainty note (6) 60- 63 F4.2 --- [NII]/Ha ? Emission line fluxes ratio [NII]6583/Hα 65 A1 --- q_[NII]/Ha [abcdu] class of relative error (5) 69- 72 F4.2 --- [SII]/Ha ? Emission line fluxes ratio [SII](6716+6730)/Hα 74 A1 --- q_[SII]/Ha [abcdu] class of relative error (5) 79- 81 I3 0.1nm W3727 ? Equivalent width of [OII]3727 emission line 83 A1 --- q_W3727 [abcdu] class of relative error (5) 86- 88 I3 0.1nm W4861 ? Equivalent width of Hβ emission line 90 A1 --- q_W4861 [abcdu] class of relative error (5) 92- 95 I4 0.1nm W5007 ? Equivalent width of [OIII]5007 emission line 97 A1 --- q_W5007 [abcdu] class of relative error (5)
Note (3): Notes are: Ha = No Hβ detected. Parameters for Hα line and to Hα line ratio abs = galaxy with the apparent underlying Balmer absorption. Hβ emission related parameters can be affected. Note (4): Telescope is abbreviated as follows: B = BTA C = Calar Alto 2.2m M = MMT Note (5): Class of relative error are defined as follows: a = <5% b = 5-10% c = 10-20% d = 20-50% u = line flux is lower than 3 σ(noise), value in the table is an upper limit. Note (6): Notes are numbered as follows: 1 = due to poor focus Hα/Hβ ratio is too high. 2 = [NII]6583/Hα is unreliable due to poor sky subtraction. 3 = Hα/Hβ is unreliable due to poor sensitivity curve. 4 = [SII]6716/6730 are outside the observed range
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1- 13 A13 --- Name Name of objects 15- 16 I2 h RAh Right ascension (B1950) 18- 19 I2 min RAm Right ascension (B1950) 21- 24 F4.1 s RAs Right ascension (B1950) 26 A1 --- DE- Declination sign (B1950) 27- 28 I2 deg DEd Declination (B1950) 30- 31 I2 arcmin DEm Declination (B1950) 33- 34 I2 arcsec DEs Declination (B1950) 37- 41 F5.3 --- z Observed redshift 43 A1 --- n_Bmag [+] +: APM magnitudes 44- 47 F4.1 mag Bmag Magnitude in B filter 51- 85 A35 --- --- Detected emission lines
Byte-by-byte Description of file: table6.dat
Bytes Format Units Label Explanations
1- 10 A10 --- Name Name of objects 11 A1 --- n_Name [1*] Note on Name (1) 15- 16 I2 h RAh Right ascension (B1950) 18- 19 I2 min RAm Right ascension (B1950) 21- 24 F4.1 s RAs Right ascension (B1950) 26 A1 --- DE- Declination sign (B1950) 27- 28 I2 deg DEd Declination (B1950) 30- 31 I2 arcmin DEm Declination (B1950) 33- 34 I2 arcsec DEs Declination (B1950) 37- 41 I5 km/s HRV Heliocentric radial velocity 43 A1 --- n_Bmag [+] +: APM magnitudes 44- 47 F4.1 mag Bmag Magnitude in B filter 49- 53 F5.1 mag BMAG Absolute B-magnitude, not corrected for the Galaxy extinction. 56-102 A47 --- Lines Absorption lines
Note (1): Notes as follows: * = galaxies from the second priority APM selected sample 1 = a galaxy near HS 1009+4906 and HS 1010+4907 in Table 4
Byte-by-byte Description of file: table7.dat
Bytes Format Units Label Explanations
1- 10 A10 --- Name Name of objects 11 A1 --- n_Name [*] *: objects from the second priority APM selected sample 15- 16 I2 h RAh Right ascension (B1950) 18- 19 I2 min RAm Right ascension (B1950) 21- 24 F4.1 s RAs Right ascension (B1950) 26 A1 --- DE- Declination sign (B1950) 27- 28 I2 deg DEd Declination (B1950) 30- 31 I2 arcmin DEm Declination (B1950) 33- 34 I2 arcsec DEs Declination (B1950) 36 A1 --- n_Bmag [+] +: APM magnitudes 37- 40 F4.1 mag Bmag Magnitude in B filter 44- 46 A3 --- SpType MK spectral type of a star 50- 91 A42 --- Lines Spectral features
Acknowledgements: Simon Pustilnik, sap(at)precise.sao.ru History: * 03-Oct-2005: Original version * 06-Oct-2014: table4.dat: the contents of the "Hb" column was fixed ("abs" and "Ha" were swapped in the original version) References: Ugryumov et al., Paper I, 1999A&AS..135..511U, Cat. J/A+AS/135/511 Pustilnik et al., Paper II 1999A&AS..135..299V, Cat. J/A+AS/137/299 Hopp et al., Paper III 2000A&AS..142..417H, Cat. J/A+AS/142/417 Kniazev et al., Paper IV 2001A&A...366..771K, Cat. J/A+A/366/771 Ugryumov et al., Paper V 2001A&A...374..907U, Cat. J/A+A/374/907
(End) Patricia Vannier [CDS] 03-Oct-2005
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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