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The Hamburg/SAO Survey for Emission-Line Galaxies next up previous
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V. The Fifth List of 161 Galaxies

A.Ugryumov

Abstract:

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/H II 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.

The Hamburg/SAO Survey for ELGs. V A.V. Ugryumov et al.

The Hamburg/SAO Survey for Emission-Line Galaxies

A.V. Ugryumov1,11 - D. Engels2 - A.Y. Kniazev1,11 - R.F. Green3 - Y.I. Izotov49 - U. Hopp510 - S.A. Pustilnik1,11 - A.G. Pramsky1,11 - T.F. Kniazeva1 - N. Brosch6 - H.-J. Hagen2 - V.A. Lipovetsky1[*] - J. Masegosa7 - I. Márquez7 - J.-M. Martin8


Date: Received ; Accepted

and@sao.ru


Key words and phrases: surveys - galaxies: fundamental parameters - galaxies: distances and redshifts - galaxies: starburst - galaxies: compact - quasars: redshifts


 
Table: Summary of the samples observed and breakdown of the classifications after follow-up spectroscopy

Candidate Sample
N BCG Other QSO Galaxies Stars Not
      & ELGs   without   Classified
      BCG? & SA   emission    

First priority
new 141 64 43 5 3 18 8
  already known 28 21 7 - - - -
  total 169 85 50 5 3 18 8
Random sample new 16 3 1 - 1 2 9
  already known 1 - 1 - - - -
APM selected sample new 22 10 10 - - 1 1
already known 1 - 1 - - - -
Second priority total 40 13 13 - 1 3 10

Objects presented in this paper
209 98 63 5 4 21 18

               


 
Table 2: Journal of observations
Date Telescope Instrument Grating, Wavelength Dispersion Observed

    grism range [Å] [Å/pixel] number

(1)

(2) (3) (4) (5) (6) (7)
             
09.06-18.06.1999 2.2 m CAHA CAFOS G-200 3700-9500 4.5 117
-- -- -- B-200 3500-7400 4.7 18*
17.06-20.06.1999 4 m KPNO R.C.Sp. KPC-10A 3700-8300 2.8 46
08.12-11.12.1999 2.2 m CAHA CAFOS G-200 3700-9500 9.0 46
             
* - objects reobserved



 
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Laboratory "Structure"
2001-06-08