The variable radio-to-X-ray spectrum of the magnetar XTE J1810-197
We have observed the 5.54s anomalous X-ray pulsar XTE J1810-197 at radio, millimeter, and infrared (IR) wavelengths, with the aim of learning about its broad-band spectrum. At the IRAM 30m telescope, we have detected the magnetar at 88 and 144GHz, the highest radio-frequency emission ever seen from...
| প্রধান লেখক: | , , , , , , , , , , , |
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| বিন্যাস: | Journal article |
| প্রকাশিত: |
2007
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| _version_ | 1826275602630443008 |
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| author | Camilo, F Ransom, S Penalver, J Karastergiou, A Kerkwijk, M Durant, M Halpern, J Reynolds, J Thum, C Helfand, D Zimmerman, N Cognard, I |
| author_facet | Camilo, F Ransom, S Penalver, J Karastergiou, A Kerkwijk, M Durant, M Halpern, J Reynolds, J Thum, C Helfand, D Zimmerman, N Cognard, I |
| author_sort | Camilo, F |
| collection | OXFORD |
| description | We have observed the 5.54s anomalous X-ray pulsar XTE J1810-197 at radio, millimeter, and infrared (IR) wavelengths, with the aim of learning about its broad-band spectrum. At the IRAM 30m telescope, we have detected the magnetar at 88 and 144GHz, the highest radio-frequency emission ever seen from a pulsar. At 88GHz we detected numerous individual pulses, with typical widths ~2ms and peak flux densities up to 45Jy. Together with nearly contemporaneous observations with the Parkes, Nancay, and Green Bank telescopes, we find that in late 2006 July the spectral index of the pulsar was -0.5 |
| first_indexed | 2024-03-06T23:01:15Z |
| format | Journal article |
| id | oxford-uuid:6235422b-2f44-4d8d-a981-ffb2b89d8216 |
| institution | University of Oxford |
| last_indexed | 2024-03-06T23:01:15Z |
| publishDate | 2007 |
| record_format | dspace |
| spelling | oxford-uuid:6235422b-2f44-4d8d-a981-ffb2b89d82162022-03-26T18:04:47ZThe variable radio-to-X-ray spectrum of the magnetar XTE J1810-197Journal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:6235422b-2f44-4d8d-a981-ffb2b89d8216Symplectic Elements at Oxford2007Camilo, FRansom, SPenalver, JKarastergiou, AKerkwijk, MDurant, MHalpern, JReynolds, JThum, CHelfand, DZimmerman, NCognard, IWe have observed the 5.54s anomalous X-ray pulsar XTE J1810-197 at radio, millimeter, and infrared (IR) wavelengths, with the aim of learning about its broad-band spectrum. At the IRAM 30m telescope, we have detected the magnetar at 88 and 144GHz, the highest radio-frequency emission ever seen from a pulsar. At 88GHz we detected numerous individual pulses, with typical widths ~2ms and peak flux densities up to 45Jy. Together with nearly contemporaneous observations with the Parkes, Nancay, and Green Bank telescopes, we find that in late 2006 July the spectral index of the pulsar was -0.5 |
| spellingShingle | Camilo, F Ransom, S Penalver, J Karastergiou, A Kerkwijk, M Durant, M Halpern, J Reynolds, J Thum, C Helfand, D Zimmerman, N Cognard, I The variable radio-to-X-ray spectrum of the magnetar XTE J1810-197 |
| title | The variable radio-to-X-ray spectrum of the magnetar XTE J1810-197 |
| title_full | The variable radio-to-X-ray spectrum of the magnetar XTE J1810-197 |
| title_fullStr | The variable radio-to-X-ray spectrum of the magnetar XTE J1810-197 |
| title_full_unstemmed | The variable radio-to-X-ray spectrum of the magnetar XTE J1810-197 |
| title_short | The variable radio-to-X-ray spectrum of the magnetar XTE J1810-197 |
| title_sort | variable radio to x ray spectrum of the magnetar xte j1810 197 |
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