Global e-VLBI observations of the gamma-ray narrow line Seyfert 1PMN J0948+0022
Context: There is growing evidence of relativistic jets in radio-loud narrow-line Seyfert 1 (RL-NLS1) galaxies. Aims: We constrain the observational properties of the radio emission in the first RL-NLS1 galaxy ever detected in gamma-rays, PMN J0948+0022, i.e., its flux density and structure in both...
| Main Authors: | , , , , , , , , , , , , , , , , , , |
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| Format: | Journal Article |
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EDP Sciences
2011
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| Online Access: | http://hdl.handle.net/20.500.11937/21963 |
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| author | Giroletti, M. Paragi, Z. Bignall, H. Doi, A. Foschini, L. Gabányi, K. É. Reynolds, C. Blanchard, J. Campbell, R. M. Colomer, F. Hong, X. Kadler, M. Kino, M. van Langevelde, H. J. Nagai, H. Phillips, C. Sekido, M. Szomoru A. Tzioumis A. K. |
| author_facet | Giroletti, M. Paragi, Z. Bignall, H. Doi, A. Foschini, L. Gabányi, K. É. Reynolds, C. Blanchard, J. Campbell, R. M. Colomer, F. Hong, X. Kadler, M. Kino, M. van Langevelde, H. J. Nagai, H. Phillips, C. Sekido, M. Szomoru A. Tzioumis A. K. |
| author_sort | Giroletti, M. |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | Context: There is growing evidence of relativistic jets in radio-loud narrow-line Seyfert 1 (RL-NLS1) galaxies. Aims: We constrain the observational properties of the radio emission in the first RL-NLS1 galaxy ever detected in gamma-rays, PMN J0948+0022, i.e., its flux density and structure in both total intensity and polarization, its compactness, and variability. Methods: We performed three real-time e-VLBI observations of PMN J0948+0022 at 22 GHz, using a global array including telescopes in Europe, East Asia, and Australia. These are the first e-VLBI science observations ever carried out with a global array, reaching a maximum baseline length of 12 458 km. The observations were part of a large multiwavelength campaign in 2009. Results: The source is detected at all three epochs. The structure is dominated by a bright component, more compact than 55 μas, with a fainter component at a position angle θ ~ 35°. Relativistic beaming is required by the observed brightness temperature of 3.4 × 1011 K. Polarization is detected at a level of about 1%. Conclusions: The parameters derived by the VLBI observations, in addition to the broad-band properties, confirm that PMN J0948+0022 is similar to flat spectrum radio quasars. Global e-VLBI is a reliable and promising technique for future studies. |
| first_indexed | 2025-11-14T07:41:36Z |
| format | Journal Article |
| id | curtin-20.500.11937-21963 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T07:41:36Z |
| publishDate | 2011 |
| publisher | EDP Sciences |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-219632019-02-19T04:26:14Z Global e-VLBI observations of the gamma-ray narrow line Seyfert 1PMN J0948+0022 Giroletti, M. Paragi, Z. Bignall, H. Doi, A. Foschini, L. Gabányi, K. É. Reynolds, C. Blanchard, J. Campbell, R. M. Colomer, F. Hong, X. Kadler, M. Kino, M. van Langevelde, H. J. Nagai, H. Phillips, C. Sekido, M. Szomoru A. Tzioumis A. K. galaxies: active / galaxies: Seyfert / galaxies: jets / instrumentation: high angular resolution / instrumentation: interferometers Context: There is growing evidence of relativistic jets in radio-loud narrow-line Seyfert 1 (RL-NLS1) galaxies. Aims: We constrain the observational properties of the radio emission in the first RL-NLS1 galaxy ever detected in gamma-rays, PMN J0948+0022, i.e., its flux density and structure in both total intensity and polarization, its compactness, and variability. Methods: We performed three real-time e-VLBI observations of PMN J0948+0022 at 22 GHz, using a global array including telescopes in Europe, East Asia, and Australia. These are the first e-VLBI science observations ever carried out with a global array, reaching a maximum baseline length of 12 458 km. The observations were part of a large multiwavelength campaign in 2009. Results: The source is detected at all three epochs. The structure is dominated by a bright component, more compact than 55 μas, with a fainter component at a position angle θ ~ 35°. Relativistic beaming is required by the observed brightness temperature of 3.4 × 1011 K. Polarization is detected at a level of about 1%. Conclusions: The parameters derived by the VLBI observations, in addition to the broad-band properties, confirm that PMN J0948+0022 is similar to flat spectrum radio quasars. Global e-VLBI is a reliable and promising technique for future studies. 2011 Journal Article http://hdl.handle.net/20.500.11937/21963 10.1051/0004-6361/201116639 EDP Sciences fulltext |
| spellingShingle | galaxies: active / galaxies: Seyfert / galaxies: jets / instrumentation: high angular resolution / instrumentation: interferometers Giroletti, M. Paragi, Z. Bignall, H. Doi, A. Foschini, L. Gabányi, K. É. Reynolds, C. Blanchard, J. Campbell, R. M. Colomer, F. Hong, X. Kadler, M. Kino, M. van Langevelde, H. J. Nagai, H. Phillips, C. Sekido, M. Szomoru A. Tzioumis A. K. Global e-VLBI observations of the gamma-ray narrow line Seyfert 1PMN J0948+0022 |
| title | Global e-VLBI observations of the gamma-ray narrow line Seyfert 1PMN J0948+0022 |
| title_full | Global e-VLBI observations of the gamma-ray narrow line Seyfert 1PMN J0948+0022 |
| title_fullStr | Global e-VLBI observations of the gamma-ray narrow line Seyfert 1PMN J0948+0022 |
| title_full_unstemmed | Global e-VLBI observations of the gamma-ray narrow line Seyfert 1PMN J0948+0022 |
| title_short | Global e-VLBI observations of the gamma-ray narrow line Seyfert 1PMN J0948+0022 |
| title_sort | global e-vlbi observations of the gamma-ray narrow line seyfert 1pmn j0948+0022 |
| topic | galaxies: active / galaxies: Seyfert / galaxies: jets / instrumentation: high angular resolution / instrumentation: interferometers |
| url | http://hdl.handle.net/20.500.11937/21963 |