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Monitoring of persistent accreting pulsating neutron stars observed during the INTEGRAL Core Program

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Title: Monitoring of persistent accreting pulsating neutron stars observed during the INTEGRAL Core Program
Authors: Sidoli, L.1, Wilms, J.2, Paizis, A.1,3, Larsson, S.4, Burki, G.5, Bourban, G.5, Chernyakova, M.3, Courvoisier, T.3,5, di Cocco, G.6, Kretschmar, P.3,7, Kreykenbohm, I.2, Mereghetti, S.1, Pottschmidt, K.3,7, Santangelo, A.8, Segreto, A.8, Staubert, R.2, Westergaard, N.J.9
Source: Nuclear Physics B Proceedings Supplement. Jun2004, Vol. 132 Issue 1-3, p648-651. 4p.
Subjects: Galactic Center, Galactic nuclei, Surveys, Neutron stars
Abstract: The INTEGRAL satellite is performing regular scans of the Galactic plane (GPS) every 12 days together with a deep exposure of the Galactic Center region (GCDE). Our collaboration is processing the data from this survey on a regular basis in order to monitor the evolution of the spectral and timing properties of the pulsating persistent neutron star sources observed. We present here an overview over the whole monitoring program and the status of the project and we report on the preliminary results of the analysis of the few scans already performed. [Copyright &y& Elsevier]
Copyright of Nuclear Physics B Proceedings Supplement is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Monitoring of persistent accreting pulsating neutron stars observed during the INTEGRAL Core Program
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  Data: <searchLink fieldCode="AR" term="%22Sidoli%2C+L%2E%22">Sidoli, L.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Wilms%2C+J%2E%22">Wilms, J.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Paizis%2C+A%2E%22">Paizis, A.</searchLink><relatesTo>1,3</relatesTo><br /><searchLink fieldCode="AR" term="%22Larsson%2C+S%2E%22">Larsson, S.</searchLink><relatesTo>4</relatesTo><br /><searchLink fieldCode="AR" term="%22Burki%2C+G%2E%22">Burki, G.</searchLink><relatesTo>5</relatesTo><br /><searchLink fieldCode="AR" term="%22Bourban%2C+G%2E%22">Bourban, G.</searchLink><relatesTo>5</relatesTo><br /><searchLink fieldCode="AR" term="%22Chernyakova%2C+M%2E%22">Chernyakova, M.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Courvoisier%2C+T%2E%22">Courvoisier, T.</searchLink><relatesTo>3,5</relatesTo><br /><searchLink fieldCode="AR" term="%22di+Cocco%2C+G%2E%22">di Cocco, G.</searchLink><relatesTo>6</relatesTo><br /><searchLink fieldCode="AR" term="%22Kretschmar%2C+P%2E%22">Kretschmar, P.</searchLink><relatesTo>3,7</relatesTo><br /><searchLink fieldCode="AR" term="%22Kreykenbohm%2C+I%2E%22">Kreykenbohm, I.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Mereghetti%2C+S%2E%22">Mereghetti, S.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Pottschmidt%2C+K%2E%22">Pottschmidt, K.</searchLink><relatesTo>3,7</relatesTo><br /><searchLink fieldCode="AR" term="%22Santangelo%2C+A%2E%22">Santangelo, A.</searchLink><relatesTo>8</relatesTo><br /><searchLink fieldCode="AR" term="%22Segreto%2C+A%2E%22">Segreto, A.</searchLink><relatesTo>8</relatesTo><br /><searchLink fieldCode="AR" term="%22Staubert%2C+R%2E%22">Staubert, R.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Westergaard%2C+N%2EJ%2E%22">Westergaard, N.J.</searchLink><relatesTo>9</relatesTo>
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  Data: <searchLink fieldCode="JN" term="%22Nuclear+Physics+B++Proceedings+Supplement%22">Nuclear Physics B Proceedings Supplement</searchLink>. Jun2004, Vol. 132 Issue 1-3, p648-651. 4p.
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  Data: <searchLink fieldCode="DE" term="%22Galactic+Center%22">Galactic Center</searchLink><br /><searchLink fieldCode="DE" term="%22Galactic+nuclei%22">Galactic nuclei</searchLink><br /><searchLink fieldCode="DE" term="%22Surveys%22">Surveys</searchLink><br /><searchLink fieldCode="DE" term="%22Neutron+stars%22">Neutron stars</searchLink>
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  Data: The INTEGRAL satellite is performing regular scans of the Galactic plane (GPS) every 12 days together with a deep exposure of the Galactic Center region (GCDE). Our collaboration is processing the data from this survey on a regular basis in order to monitor the evolution of the spectral and timing properties of the pulsating persistent neutron star sources observed. We present here an overview over the whole monitoring program and the status of the project and we report on the preliminary results of the analysis of the few scans already performed. [Copyright &y& Elsevier]
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  Data: <i>Copyright of Nuclear Physics B Proceedings Supplement is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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