Name Size Creator Creation Date Labels Comment  
PDF File n132d_xis_allobs_v2p10_spectra.pdf 10.98 MB Eric D Miller Mar 24, 2017 09:14
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Suzaku XIS spectra fit with v2.10 of the model, free line norms, all observations
PDF File N132D_E0310_v2.9_20150402_1.5_3.5_0.3_10.0.pdf 712 kB Unknown User (plucinsky_1@touchstonenetwork.net) Apr 02, 2015 16:08
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Version 2.9 overplotted on the pn and MOS spectra, first page shows 0.3-10.0 keV and second page shows 1.5-3.5 keV.
PDF File N132D.pdf 300 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) Mar 26, 2015 19:26
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How the N132D model was originally derived. Presentation given at the 2012 WG meeting
GIF File EPICpnN132D_HardEnergyModel.gif 212 kB Unknown User (plucinsky_1@touchstonenetwork.net) May 09, 2011 13:38
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Data (upper panel) and residuals in units of data/model ratio (lower panel) when N132D_E212_v1.0_20110439.xcm is applied to the EPIC-pn spectrum  
File all3_N132D_E0310_v2.7_20150324.ps 175 kB Unknown User (plucinsky_1@touchstonenetwork.net) Apr 01, 2015 11:18
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Version 2.7 overplotted on the merged pn, and MOS1, MOS2 spectra  
GIF File EPICpnN132D_vs_EPICpnFWCLW.gif 158 kB Unknown User (plucinsky_1@touchstonenetwork.net) May 09, 2011 13:38
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EPIC-pn: N132D versus instrumental background spectrum  
File N132D_E0212_v2.4_20120530_RGS.ps 150 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) Jun 01, 2012 09:10
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Application of v.2.4 to the RGS spectrum (minimum S/N ratio equal to 10)  
File N132D_E0212_v2.4_20120530_PN.ps 133 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) Jun 01, 2012 09:11
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Application of v2.4 to the PN spectrum (SW/Thin); minimum S/N ratio equal to 10  
File f_N132D_E0310_v2.6_20140511.ps 117 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) May 13, 2014 07:21
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Spectra (upper panel) and residuals in units of data/model ratio (lower panel) when v2.6 is applied to the EPIC-pn and RGS spectra used to generate it  
GIF File N132D_E0212_v2.3_20120324_RGS.gif 99 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) Mar 28, 2012 09:31
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Data (upper panel) and residuals in units of data/model ratio (lower panel) when N132D_E0212_v2.3_20120324_RGS.mdl is applied to the RGS spectra  
File N132D_E0310_v2.9_20150402_all.mdl 46 kB Unknown User (plucinsky_1@touchstonenetwork.net) Apr 02, 2015 16:07
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Version 2.9 from Paul, this fits much better in the 0.3-1.5 keV range and the fit is only slightly worse in the 1.5-3.5 keV range compared to v2.8. I suggest this model is good enough to determine line normalizations in the 1.5-3.5 keV bandpass.  
File N132D_E0310_v2.8_20150401_dev.mdl 43 kB Unknown User (plucinsky_1@touchstonenetwork.net) Apr 02, 2015 16:05
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Version 2.8 from Paul, optimized for the energy range 1.5-3.5 keV but fits poorly in the 0.3-1.5 keV range  
File N132D_E0310_v2.14_20210511.mdl 27 kB Unknown User (plucinsky_1@touchstonenetwork.net) Jun 11, 2021 15:17
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Martin reformatted the v2.13 model to be more logical and added lines. This is an intermediate model. The high energy component (kT=5.47 keV) should be identical to the v2.13 model. All the changes should be at low energies.  
GIF File N132D_E0212_v2.3.1_20120324_PN_RGSLinesFrozen.gif 27 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) Mar 28, 2012 09:33
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Data (upper panel) and residuals in units of data/model ratio (lower panel) when N132D_E0212_v2.3.1_20120324_PN_RGSLinesFrozen.mdl is applied to the EPIC-pn spectrum  
GIF File N132D_E0212_v2.3_20120324_PN.gif 27 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) Mar 28, 2012 09:32
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Data (upper panel) and residuals in units of data/model ratio (lower panel) when N132D_E0212_v2.3_20120324_PN.mdl is applied to the EPIC-pn spectrum  
Text File N132D_E0212_v2.3.3_20120324.txt 26 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) Mar 28, 2012 15:44
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Version 2.3.3, Text file with the complete line idnetification according to the ATOMDB nomenclature  
File N132D_E0212_v2.4_20120530_PN_zoomSXVI.ps 26 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) Jun 01, 2012 09:12
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Application of v2.4 to the PN spectrum (SW/Thin) in the 2.3-2.9 keV energy range (SXVI); minimum S/N ratio equal to 10  
File N132D_E0212_v2.5_20140425_zoomSXVI.ps 26 kB Unknown User (matteo.guainazzi_1@touchstonenetwork.net) Apr 25, 2014 05:48
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Application of v2.5 to the PN spectrum (SW/Thin) in the 2.3-2.9 keV energy range (SXVI); minimum S/N ratio equal to 10. To be compared to: https://wikis.mit.edu/confluence/download/attachments/75637213/N132D_E0212_v2.4_20120530_PN_zoomSXVI.ps?api=v2  
File N132D_E0310_v2.12_20200324.mdl 21 kB Unknown User (bwgref_1@touchstonenetwork.net) Apr 15, 2020 14:38
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Added neutral 6.4 keV, Fe XXV K-beta: 7.88 keV and Ni XXVII: 7.78 keV. Cross-norm is set for NuSTAR 0.75.  
File N132D_E0310_v2.13_20210421.mdl 21 kB Eric D Miller Apr 22, 2021 14:46
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Fixed corrupted 1.5 keV line flux, reset global norm to 1, zeroed neutral Fe K line, fit Ca XIX 3.9 keV flux, froze all components, cleaned things up.  
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