J/A+A/374/907 The Hamburg/SAO Survey for ELGs. V. (Ugryumov+, 2001)
The Hamburg/SAO Survey for Emission-Line Galaxies.
V. The Fifth List of 161 Galaxies.
Ugryumov A.V., Engels D., Kniazev A.Y., Green R.F., Izotov Y.I., Hopp U.,
Pustilnik S.A., Pramsky A.G., Kniazeva T.F., Brosch N., Hagen H.-J.,
Lipovetsky V.A., Masegosa J., Marquez I., Martin J.-M
<Astron. Astrophys. 374, 907 (2001)>
=2001A&A...374..907U 2001A&A...374..907U
ADC_Keywords: Galaxies, spectra ; Redshifts ; Galaxies, Seyfert
Keywords: surveys - galaxies: fundamental parameters -
galaxies: distances and redshifts - galaxies: starburst -
galaxies: compact - quasars: redshifts
Description:
We present the fifth list with results of the Hamburg/SAO Survey for
Emission-Line Galaxies (HSS therein, SAO - Special Astrophysical
Observatory, Russia). The list is a result of follow-up spectroscopy
conducted with the 2.2m CAHA and 4m Kitt Peak telescopes in 1999. The
data of this snap-shot spectroscopy survey confirmed 166 emission-line
objects out of 209 observed candidates and allowed their quantitative
spectral classification and redshift determination. We could classify
98 emission-line objects as BCG/HII galaxies or probable BCGs, 5 as
QSOs, 3 as Seyfert galaxies, 2 as super-associations in subluminous
spiral galaxies. 25 low-excitation objects were classified as
starburst nuclei (SBN), 24 as dwarf amorphous nuclei starburst
galaxies (DANS) and 3 as LINERs. Due to low signal-to-noise ratio we
could not classify 6 ELGs. Furthermore, for another 4 galaxies we did
not detect any significant emission lines. For 131 emission-line
galaxies, the redshifts and/or line intensities are determined for the
first time. For the remaining 30 previously known ELGs we give either
improved data of the line intensities or some independent
measurements.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table3.dat 121 161 Names, coordinates, velocities, apparent and
absolute magnitudes and classification of
emission-line galaxies
table4.dat 71 161 Parameters of emission lines of galaxies
table5.dat 82 5 Names, coordinates, redshifts and magnitudes of QSOs
table6.dat 98 4 Galaxies without emission lines
table7.dat 84 21 Stars
tables.tex 211 831 LaTeX version of the tables
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See also:
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. (Kniiazev+, 2001)
J/A+A/442/109 : The Hamburg/SAO Survey for ELGs. VI. (Pustilnik+, 2005)
Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1- 13 A13 --- Name Name of object
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)
25 A1 --- DE- Declination sign
26- 27 I2 deg DEd Declination (B1950)
29- 30 I2 arcmin DEm Declination (B1950)
32- 33 I2 arcsec DEs Declination (B1950)
35- 39 I5 km/s HRV Heliocentric radial velocity
40 A1 --- u_HRV Uncertainty flag on HRV
41- 43 I3 km/s e_HRV Error of heliocentric radial velocity
45 A1 --- n_Bmag [+] '+': APM magnitudes
46- 49 F4.1 mag Bmag Magnitude in B filter
50 A1 --- u_Bmag Uncertainty flag on Bmag
52- 56 F5.1 mag BMAG Absolute B-magnitude (1)
57 A1 --- u_BMAG Uncertainty flag on BMAG
59- 67 A9 --- Type Spectral classification (2)
69-112 A44 --- Names Other names from NED
114-119 A6 --- r_Type References to other sources of spectral
information (3)
121 A1 --- Sam [+*] Sample set (G1)
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Note (1): Absolute magnitudes are not corrected for the Galaxy extinction.
Note (2): Only rough classification were done due to low S/N spectra.
Spectral classification follows Salzer et al., 1989ApJS...70..479S 1989ApJS...70..479S
Note (3): References:
1: Klemola et al., 1987, Cat. I/199, I/200
2: Popescu et al., 1996, Cat. J/A+AS/116/43
3: Ugryumov et al., 1998, Cat. J/A+AS/131/295
4: RC3, 1991, Cat. VII/155
5: Weistrop & Downes, 1991AJ....102.1680W 1991AJ....102.1680W
6: Hopp et al., 2000, Cat. J/A+AS/142/417 (Paper III)
7: Popescu & Hopp, 2000A&AS..142..247P 2000A&AS..142..247P
8: Falco et al., 1999, Cat. J/PASP/111/438
9: Markarian et al., 1989, Cat. VII/172
10: Fisher et al., 1995, Cat. J/ApJS/100/69
11: Grupe et al., 1999, (Cat. J/A+A/350/805
12: Kirshner et al., 1987, Cat. J/ApJ/314/493
13: Tifft et al., 1986ApJ...310...75T 1986ApJ...310...75T
14: Wegner & Boley, 1993AJ....105..660W 1993AJ....105..660W
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Byte-by-byte Description of file: table4.dat
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Bytes Format Units Label Explanations
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1- 13 A13 --- Name Name of object
14 A1 --- ObsNote [*] Note about photometric conditions (1)
15 A1 --- RefLine [+] when Hα is the reference line (2)
16- 18 I3 10-19W/m2 F4861 Observed flux in Hβ emission line (3)
19 A1 --- u_F4861 Uncertainty flag (:) (4)
21- 25 F5.2 --- F3727 ? Emission line flux ratio [OII]3727Å/Hβ
or [OII]3727Å/Hα if RefLine = +
26 A1 --- u_F3727 Uncertainty flag (:) (4)
28- 32 F5.2 --- F5007 ? Emission line flux ratio [OIII]5007Å/Hβ
or [OIII]5007Å/Hα if RefLine = +
33 A1 --- u_F5007 Uncertainty flag (:) (4)
35- 39 F5.2 --- FHa/Hb ? Emission line flux ratio Hα/Hβ
40 A1 --- u_FHa/Hb Uncertainty flag (:) (4)
42- 45 F4.2 --- F6583 ? Emission line flux ratio [NII]6583Å/Hα
46 A1 --- u_F6583 Uncertainty flag (:) (4)
48- 51 F4.2 --- F6716 ? Emission line flux ratio
[SII](6716Å+6730Å)/Hα
52 A1 --- u_F6716 Uncertainty flag (:) (4)
54- 56 I3 0.1nm EW3727 ? Equivalent width of [OII]3727Å emission line
57 A1 --- u_EW3727 Uncertainty flag (:) (4)
59 A1 --- n_EW4861 [+] when Hα is the reference line (2)
60- 62 I3 0.1nm EW4861 Equivalent width of Hβ emission line
or Hα if n_EW4861 = '+
63 A1 --- u_EW4861 Uncertainty flag (:) (4)
65- 68 I4 0.1nm EW5007 ? Equivalent width [OIII]5007Å emission line
69 A1 --- u_EW5007 Uncertainty flag (:) (4)
71 A1 --- Sam [*+ ] Sample set (G1)
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Note (1): '*': Objects observed under poor photometric conditions
Note (2): '+': Parameters for Hα line and to Hα line ratio
Note (3): Absolute observed fluxes are given in 10-16erg/sec/cm2
Note (4): Parameters with less confident values
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Byte-by-byte Description of file: table5.dat
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Bytes Format Units Label Explanations
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1- 13 A13 --- Name Name of object
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)
25 A1 --- DE- Declination sign
26- 27 I2 deg DEd Declination (B1950)
29- 30 I2 arcmin DEm Declination (B1950)
32- 33 I2 arcsec DEs Declination (B1950)
35- 39 F5.3 --- z Observed redshift
40 A1 --- n_z [:] Parameters with less confident values
42 A1 --- n_Bmag [+] '+': APM magnitudes
43- 46 F4.1 mag Bmag Magnitude in B filter
48- 82 A35 --- Lines Detected emission lines
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Byte-by-byte Description of file: table6.dat
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Bytes Format Units Label Explanations
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1- 13 A13 --- Name Name of object
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)
25 A1 --- DE- Declination sign
26- 27 I2 deg DEd Declination (B1950)
29- 30 I2 arcmin DEm Declination (B1950)
32- 33 I2 arcsec DEs Declination (B1950)
35- 39 I5 km/s HRV Heliocentric radial velocity (1)
40 A1 --- u_HRV [:] Parameters with less confident values
41 A1 --- n_Bmag [+] '+': APM magnitudes
42- 46 F5.2 mag Bmag Magnitude in B filter
48- 53 F6.2 mag BMAG Absolute B-magnitude (1)
55- 96 A42 --- Lines Absorption lines
98 A1 --- Sam [*] Sample set (G1)
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Note (1): Absolute magnitudes are not corrected for the Galaxy extinction.
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Byte-by-byte Description of file: table7.dat
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Bytes Format Units Label Explanations
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1- 13 A13 --- Name Name of object
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)
25 A1 --- DE- Declination sign
26- 27 I2 deg DEd Declination (B1950)
29- 30 I2 arcmin DEm Declination (B1950)
32- 33 I2 arcsec DEs Declination (B1950)
35 A1 --- n_Bmag [+] '+': APM magnitudes
36- 40 F5.2 mag Bmag Magnitude in B filter
42- 44 A3 --- SpType Spectral type of star
46- 82 A37 --- Spectrum Spectral features
84 A1 --- Sam [*+ ] Sample set (G1)
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Global notes:
Note (G1): Objects taken from samples:
'*': objects from the second priority random sample
'+': galaxies from the APM selected sample
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History: Two corrections in table3.dat on 31-Aug-2001
Acknowledgements: Andrei Ugryumov
(End) Ugryumov Andrei [SAO RAS], Patricia Bauer [CDS] 06-Jul-2001