A high sensitivity HI survey of the sky at δ ≤ -25° : Final data release
- Autores
- Bajaja, Esteban; Arnal, Edmundo Marcelo; Larrarte, Juan José; Morras, Ricardo; Pöppel, Wolfgang G. L.; Kalberla, P. M. W.
- Año de publicación
- 2005
- Idioma
- inglés
- Tipo de recurso
- reseña artículo
- Estado
- versión publicada
- Descripción
- We present the final data release of the high sensitivity λ 21-cm neutral hydrogen survey of the sky south of δ ≤ -25°. A total of 50 980 positions lying on a galactic coordinate grid with points spaced by (Δl, Δb) = (0°.5/cos b, 0°.5) were observed with the 30-m dish of the Instituto Argentino de Radioastronomía (IAR). The angular resolution of the survey is HPBW = 0°.5 and the velocity coverage spans the interval -450 km s-1 to +400 km s-1 (LSR). The velocity resolution is 1.27 km s-1 and the final rms noise of the entire database is 0.07 K. The data are corrected for stray radiation and converted to brightness temperatures.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto Argentino de Radioastronomía - Materia
-
Ciencias Astronómicas
Galaxy: structure
Radio lines: ISM
Surveys - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/84439
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A high sensitivity HI survey of the sky at δ ≤ -25° : Final data releaseBajaja, EstebanArnal, Edmundo MarceloLarrarte, Juan JoséMorras, RicardoPöppel, Wolfgang G. L.Kalberla, P. M. W.Ciencias AstronómicasGalaxy: structureRadio lines: ISMSurveysWe present the final data release of the high sensitivity λ 21-cm neutral hydrogen survey of the sky south of δ ≤ -25°. A total of 50 980 positions lying on a galactic coordinate grid with points spaced by (Δl, Δb) = (0°.5/cos b, 0°.5) were observed with the 30-m dish of the Instituto Argentino de Radioastronomía (IAR). The angular resolution of the survey is HPBW = 0°.5 and the velocity coverage spans the interval -450 km s<SUP>-1</SUP> to +400 km s<SUP>-1</SUP> (LSR). The velocity resolution is 1.27 km s<SUP>-1</SUP> and the final rms noise of the entire database is 0.07 K. The data are corrected for stray radiation and converted to brightness temperatures.Facultad de Ciencias Astronómicas y GeofísicasInstituto Argentino de Radioastronomía2005info:eu-repo/semantics/reviewinfo:eu-repo/semantics/publishedVersionRevisionhttp://purl.org/coar/resource_type/c_dcae04bcinfo:ar-repo/semantics/resenaArticuloapplication/pdf767-773http://sedici.unlp.edu.ar/handle/10915/84439enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20041863info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:16:14Zoai:sedici.unlp.edu.ar:10915/84439Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:15.259SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
A high sensitivity HI survey of the sky at δ ≤ -25° : Final data release |
| title |
A high sensitivity HI survey of the sky at δ ≤ -25° : Final data release |
| spellingShingle |
A high sensitivity HI survey of the sky at δ ≤ -25° : Final data release Bajaja, Esteban Ciencias Astronómicas Galaxy: structure Radio lines: ISM Surveys |
| title_short |
A high sensitivity HI survey of the sky at δ ≤ -25° : Final data release |
| title_full |
A high sensitivity HI survey of the sky at δ ≤ -25° : Final data release |
| title_fullStr |
A high sensitivity HI survey of the sky at δ ≤ -25° : Final data release |
| title_full_unstemmed |
A high sensitivity HI survey of the sky at δ ≤ -25° : Final data release |
| title_sort |
A high sensitivity HI survey of the sky at δ ≤ -25° : Final data release |
| dc.creator.none.fl_str_mv |
Bajaja, Esteban Arnal, Edmundo Marcelo Larrarte, Juan José Morras, Ricardo Pöppel, Wolfgang G. L. Kalberla, P. M. W. |
| author |
Bajaja, Esteban |
| author_facet |
Bajaja, Esteban Arnal, Edmundo Marcelo Larrarte, Juan José Morras, Ricardo Pöppel, Wolfgang G. L. Kalberla, P. M. W. |
| author_role |
author |
| author2 |
Arnal, Edmundo Marcelo Larrarte, Juan José Morras, Ricardo Pöppel, Wolfgang G. L. Kalberla, P. M. W. |
| author2_role |
author author author author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Galaxy: structure Radio lines: ISM Surveys |
| topic |
Ciencias Astronómicas Galaxy: structure Radio lines: ISM Surveys |
| dc.description.none.fl_txt_mv |
We present the final data release of the high sensitivity λ 21-cm neutral hydrogen survey of the sky south of δ ≤ -25°. A total of 50 980 positions lying on a galactic coordinate grid with points spaced by (Δl, Δb) = (0°.5/cos b, 0°.5) were observed with the 30-m dish of the Instituto Argentino de Radioastronomía (IAR). The angular resolution of the survey is HPBW = 0°.5 and the velocity coverage spans the interval -450 km s<SUP>-1</SUP> to +400 km s<SUP>-1</SUP> (LSR). The velocity resolution is 1.27 km s<SUP>-1</SUP> and the final rms noise of the entire database is 0.07 K. The data are corrected for stray radiation and converted to brightness temperatures. Facultad de Ciencias Astronómicas y Geofísicas Instituto Argentino de Radioastronomía |
| description |
We present the final data release of the high sensitivity λ 21-cm neutral hydrogen survey of the sky south of δ ≤ -25°. A total of 50 980 positions lying on a galactic coordinate grid with points spaced by (Δl, Δb) = (0°.5/cos b, 0°.5) were observed with the 30-m dish of the Instituto Argentino de Radioastronomía (IAR). The angular resolution of the survey is HPBW = 0°.5 and the velocity coverage spans the interval -450 km s<SUP>-1</SUP> to +400 km s<SUP>-1</SUP> (LSR). The velocity resolution is 1.27 km s<SUP>-1</SUP> and the final rms noise of the entire database is 0.07 K. The data are corrected for stray radiation and converted to brightness temperatures. |
| publishDate |
2005 |
| dc.date.none.fl_str_mv |
2005 |
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info:eu-repo/semantics/review info:eu-repo/semantics/publishedVersion Revision http://purl.org/coar/resource_type/c_dcae04bc info:ar-repo/semantics/resenaArticulo |
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review |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/84439 |
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http://sedici.unlp.edu.ar/handle/10915/84439 |
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eng |
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eng |
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info:eu-repo/semantics/altIdentifier/issn/0004-6361 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20041863 |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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