The Hamburg/SAO survey for emission-line galaxies VI. the sixth list of 126 galaxies

S. A. Pustilnik; D. Engels; V. A. Lipovetsky; A. Y. Kniazev; A. G. Pramskij; A. V. Ugryumov; J. Masegosa; Y. I. Izotov; F. Chaffee; I. Márquez; A. L. Teplyakova; U. Hopp; N. Brosch; H. J. Hagen; J. M. Martin

doi:10.1051/0004-6361:20042466

The Hamburg/SAO survey for emission-line galaxies VI. the sixth list of 126 galaxies

S. A. Pustilnik^*, D. Engels, V. A. Lipovetsky, A. Y. Kniazev, A. G. Pramskij, A. V. Ugryumov, J. Masegosa, Y. I. Izotov, F. Chaffee, I. Márquez, A. L. Teplyakova, U. Hopp, N. Brosch, H. J. Hagen, J. M. Martin

^*Corresponding author for this work

School of Physics and Astronomy

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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.

Original language	English
Pages (from-to)	109-116
Number of pages	8
Journal	Astronomy and Astrophysics
Volume	442
Issue number	1
DOIs	https://doi.org/10.1051/0004-6361:20042466
State	Published - Oct 2005

Keywords

Galaxies: distances and redshifts
Galaxies: fundamental parameters
Galaxies: quasars: redshifts
Galaxies: starburst
Surveys

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10.1051/0004-6361:20042466

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Pustilnik, S. A., Engels, D., Lipovetsky, V. A., Kniazev, A. Y., Pramskij, A. G., Ugryumov, A. V., Masegosa, J., Izotov, Y. I., Chaffee, F., Márquez, I., Teplyakova, A. L., Hopp, U., Brosch, N., Hagen, H. J., & Martin, J. M. (2005). The Hamburg/SAO survey for emission-line galaxies VI. the sixth list of 126 galaxies. Astronomy and Astrophysics, 442(1), 109-116. https://doi.org/10.1051/0004-6361:20042466

@article{33e45d7c97574d58bcf925351eafba35,

title = "The Hamburg/SAO survey for emission-line galaxies VI. the sixth list of 126 galaxies",

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.",

keywords = "Galaxies: distances and redshifts, Galaxies: fundamental parameters, Galaxies: quasars: redshifts, Galaxies: starburst, Surveys",

author = "Pustilnik, {S. A.} and D. Engels and Lipovetsky, {V. A.} and Kniazev, {A. Y.} and Pramskij, {A. G.} and Ugryumov, {A. V.} and J. Masegosa and Izotov, {Y. I.} and F. Chaffee and I. M{\'a}rquez and Teplyakova, {A. L.} and U. Hopp and N. Brosch and Hagen, {H. J.} and Martin, {J. M.}",

year = "2005",

month = oct,

doi = "10.1051/0004-6361:20042466",

language = "אנגלית",

volume = "442",

pages = "109--116",

journal = "Astronomy and Astrophysics",

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Pustilnik, SA, Engels, D, Lipovetsky, VA, Kniazev, AY, Pramskij, AG, Ugryumov, AV, Masegosa, J, Izotov, YI, Chaffee, F, Márquez, I, Teplyakova, AL, Hopp, U, Brosch, N, Hagen, HJ & Martin, JM 2005, 'The Hamburg/SAO survey for emission-line galaxies VI. the sixth list of 126 galaxies', Astronomy and Astrophysics, vol. 442, no. 1, pp. 109-116. https://doi.org/10.1051/0004-6361:20042466

TY - JOUR

T1 - The Hamburg/SAO survey for emission-line galaxies VI. the sixth list of 126 galaxies

AU - Pustilnik, S. A.

AU - Engels, D.

AU - Lipovetsky, V. A.

AU - Kniazev, A. Y.

AU - Pramskij, A. G.

AU - Ugryumov, A. V.

AU - Masegosa, J.

AU - Izotov, Y. I.

AU - Chaffee, F.

AU - Márquez, I.

AU - Teplyakova, A. L.

AU - Hopp, U.

AU - Brosch, N.

AU - Hagen, H. J.

AU - Martin, J. M.

PY - 2005/10

Y1 - 2005/10

N2 - 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.

AB - 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.

KW - Galaxies: distances and redshifts

KW - Galaxies: fundamental parameters

KW - Galaxies: quasars: redshifts

KW - Galaxies: starburst

KW - Surveys

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SN - 0004-6361

VL - 442

SP - 109

EP - 116

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 1

ER -

The Hamburg/SAO survey for emission-line galaxies VI. the sixth list of 126 galaxies

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