Figure 2 from NuSTAR and XMM-Newton Observations of Luminous, Heavily Obscured, WISE-selected Quasars at z ∼ 2

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NuSTAR and XMM-Newton Observations of Luminous, Heavily Obscured, WISE-selected Quasars at z ∼ 2

Authors: D. Stern, G. B. Lansbury, R. J. Assef, W. N. Brandt, D. M. Alexander, D. R. Ballantyne, M. Baloković, F. E. Bauer, D. Benford, A. Blain, S. E. Boggs, C. Bridge, M. Brightman, F. E. Christensen, A. Comastri, W. W. Craig, A. Del Moro, P. R. M. Eisenhardt, P. Gandhi, R. L. Griffith, C. J. Hailey, F. A. Harrison, R. C. Hickox, T. H. Jarrett, M. Koss, S. Lake, S. M. LaMassa, B. Luo, C.-W. Tsai, C. M. Urry, D. J. Walton, E. L. Wright, J. Wu, L. Yan, and W. W. Zhang

Stern et al. 2014 The Astrophysical Journal 794 102.

Provider: AAS Journals

Caption: Figure 2.

Gross source counts vs. background counts (scaled to the source region) for WISE J1814+3412, WISE J2207+1939, and WISE J2357+0328 (circles, squares, and diamonds, respectively). The 1, 2, and p labels correspond to the 0.5–10 keV counts for the EPIC-MOS1, EPIC-MOS2, and EPIC-pn cameras on XMM-Newton, respectively, while the E labels correspond to merging the photons from the three EPIC cameras together. The A and B labels correspond to the 3–24 keV counts for FPMA and FPMB on NuSTAR, respectively. The dashed lines indicate Poisson no-source probabilities. Two sources are faintly detected: WISE J1814+3412 is detected with the EPIC-MOS1 and EPIC-pn cameras, and WISE J2357+0328 is detected with the EPIC-MOS2 camera.

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