Puntos de calibración para observaciones 21-cm
Many observations of a series of calibration points on the sky were obtained. The statistical noise of the resulting average profiles is relatively low. So, they seem adequate to be used by other observers working with similar resolutions in angle and frequency. As the paper will be published elsewh...
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1973
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/98975 |
| Aporte de: |
| Sumario: | Many observations of a series of calibration points on the sky were obtained. The statistical noise of the resulting average profiles is relatively low. So, they seem adequate to be used by other observers working with similar resolutions in angle and frequency. As the paper will be published elsewhere, we give here only a synthesis. |
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