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Comparative Spectral Analysis of Astronomical X-ray Sources Using Multiple Instruments

This study presents a comprehensive analysis of X-ray spectra from various telescopes, including Chandra and XMM-Newton. Multiple exposure times, averaging around 8.5 ksec, are used for comparisons to assess the light curves and spectra across different instruments. The results include in-depth comparisons with studies by Plucinsky et al. and Sasaki et al., aiming to enhance understanding of X-ray emissions and improve model predictions in astrophysics. The findings will contribute valuable insights into the properties of astronomical sources.

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Comparative Spectral Analysis of Astronomical X-ray Sources Using Multiple Instruments

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  1. 1E0102.2-7219

  2. Spectra EXPOSURE: ~8.5ksec EXPOSURE: ~8.5ksec

  3. EXPOSURE: ~8.5ksec EXPOSURE: ~8.5ksec

  4. Light curve

  5. Comparison with Chandra (FI) Plucinsky et al. astro-ph/0111363 EXPOSURE: 10.2ksec

  6. Comparison with Chandra (BI) Plucinsky et al. astro-ph/0111363 EXPOSURE: 7.8ksec

  7. Comparison with XMM PN spectrum Sasaki et al. 2001, A&A EXPOSURE: 15.5ksec

  8. Comparison with XMM PN spectrum EXPOSURE: 15.5ksec

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