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 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:
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FileName Lrecl Records Explanations
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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
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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
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Bytes Format Units Label Explanations
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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)
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Note (1): Only rough classification were done due to low S/N spectra.
Spectral classification follows Salzer et al., 1989ApJS...70..479S 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 1998A&AS..133...13P, Popescu et al.
9 = 1998A&A...330...25G 1998A&A...330...25G, Grupe et al.
10 = 1998, Cat. J/A+AS/127/145, Bade et al.
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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- 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)
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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
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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 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
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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- 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
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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
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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- 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
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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 1999A&AS..135..511U, Cat. J/A+AS/135/511
Pustilnik et al., Paper II 1999A&AS..135..299V 1999A&AS..135..299V, Cat. J/A+AS/137/299
Hopp et al., Paper III 2000A&AS..142..417H 2000A&AS..142..417H, Cat. J/A+AS/142/417
Kniazev et al., Paper IV 2001A&A...366..771K 2001A&A...366..771K, Cat. J/A+A/366/771
Ugryumov et al., Paper V 2001A&A...374..907U 2001A&A...374..907U, Cat. J/A+A/374/907
(End) Patricia Vannier [CDS] 03-Oct-2005