Spatially-resolved mid-infrared spectroscopy of IC 5063
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| Format: | Artículo científico |
| Sprache: | en |
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Universidad Nacional Autónoma de México
2007
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| _version_ | 1876422403570008064 |
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| author | S. Young |
| author_facet | S. Young |
| contents | Spatially-resolved mid-infrared spectroscopy of IC 5063 S. Young C. Packham C. M. Telesco J. T. Radomski Física, Astronomía y Matemáticas N-band spectroscopy of the radio strongSeyfert 2 active galaxy IC 5063 (z=0.0110)was obtained using Gemini South in conjunc-tion with the Thermal-Region Camera Spec-trograph (T-ReCS; Telesco et al. 1998). T-ReCS uses a Raytheon 320x240 pixel SiAsIBC array, at a plate scale of 0.08900 pixel-1.The observations were conducted on thenights of UT 2005 July 7 and 9 using thestandard chop-nod technique to remove thetime-variable sky background, telescope ther-mal emission, and the so-called 1/f detectornoise. A 0.6700 wide slit was used alignedalong the position angle of the radio axis at305o(Morganti et al. 1998) and close to theextended narrow line emission region (ENLR)axis at 303_(Colina et al. 1991). The total on-source integration time was 1212 seconds. 2007 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102964 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.29 |
| format | Artículo científico |
| id | redalyc_57102964 |
| institution | Redalyc |
| language | en |
| publishDate | 2007 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Spatially-resolved mid-infrared spectroscopy of IC 5063 S. Young Física, Astronomía y Matemáticas Spatially-resolved mid-infrared spectroscopy of IC 5063 S. Young C. Packham C. M. Telesco J. T. Radomski Física, Astronomía y Matemáticas N-band spectroscopy of the radio strongSeyfert 2 active galaxy IC 5063 (z=0.0110)was obtained using Gemini South in conjunc-tion with the Thermal-Region Camera Spec-trograph (T-ReCS; Telesco et al. 1998). T-ReCS uses a Raytheon 320x240 pixel SiAsIBC array, at a plate scale of 0.08900 pixel-1.The observations were conducted on thenights of UT 2005 July 7 and 9 using thestandard chop-nod technique to remove thetime-variable sky background, telescope ther-mal emission, and the so-called 1/f detectornoise. A 0.6700 wide slit was used alignedalong the position angle of the radio axis at305o(Morganti et al. 1998) and close to theextended narrow line emission region (ENLR)axis at 303_(Colina et al. 1991). The total on-source integration time was 1212 seconds. 2007 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102964 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.29 |
| title | Spatially-resolved mid-infrared spectroscopy of IC 5063 |
| topic | Física, Astronomía y Matemáticas |
| url | https://www.redalyc.org/articulo.oa?id=57102964 |