Name | Size | Creator | Creation Date | Labels | Comment | ||
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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. | ||
Version 1 (current) | 27 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Jun 11, 2021 15:17 | 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. | |||
File n132d_afoster_suzuki_vrnei_20210420.mdl | 15 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | May 06, 2021 10:33 |
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"Physical" model for N132D that uses the Suzuki et al. 2020 model based on the RGS data for the low energy part of the spectrum and a vrnei component for the high energy part of the spectrum based on Adam Foster's fits to the pn and MOS data | ||
Version 1 (current) | 15 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | May 06, 2021 10:33 | "Physical" model for N132D that uses the Suzuki et al. 2020 model based on the RGS data for the low energy part of the spectrum and a vrnei component for the high energy part of the spectrum based on Adam Foster's fits to the pn and MOS data | |||
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. | ||
Version 1 (current) | 21 kB | Eric D Miller | Apr 22, 2021 14:46 | 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. | |||
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. | ||
Version 1 (current) | 21 kB | Unknown User (bwgref_1@touchstonenetwork.net) | Apr 15, 2020 14:38 | 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_v2.11b_20190806.mdl | 21 kB | Eric D Miller | Aug 13, 2019 14:15 |
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Updated with third Gaussian for FeXXV triplet, 5.7 keV nlapec, with parameter fits from Suzaku FI CCDs. | ||
Version 1 (current) | 21 kB | Eric D Miller | Aug 13, 2019 14:15 | Updated with third Gaussian for FeXXV triplet, 5.7 keV nlapec, with parameter fits from Suzaku FI CCDs. | |||
File N132D_E0310_v2.11_20180406.mdl | 20 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 06, 2018 13:58 |
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Version 2.11 of the model, I updated the APEC version to v3.0.9 in the model file. You need to make sure you have these files, they are included in the XSPEC 12.10.0 release. | ||
Version 1 (current) | 20 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 06, 2018 13:58 | Version 2.11 of the model, I updated the APEC version to v3.0.9 in the model file. You need to make sure you have these files, they are included in the XSPEC 12.10.0 release. | |||
Text File n132d_xis_obs20100727_v2p10_linenorms.txt | 0.4 kB | Eric D Miller | Mar 24, 2017 09:15 |
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Suzaku XIS line norms using v2.10 of the model, data file, obs 2010-07-27 | ||
Version 1 (current) | 0.4 kB | Eric D Miller | Mar 24, 2017 09:15 | Suzaku XIS line norms using v2.10 of the model, data file, obs 2010-07-27 | |||
PDF File n132d_xis_allobs_v2p10_linenorms.pdf | 13 kB | Eric D Miller | Mar 24, 2017 09:15 |
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Suzaku XIS line norms history using v2.10 of the model, all observations | ||
Version 1 (current) | 13 kB | Eric D Miller | Mar 24, 2017 09:15 | Suzaku XIS line norms history using v2.10 of the model, all observations | |||
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 | ||
Version 1 (current) | 10.98 MB | Eric D Miller | Mar 24, 2017 09:14 | Suzaku XIS spectra fit with v2.10 of the model, free line norms, all observations | |||
File N132D_E0310_v2.10_20170319.mdl | 20 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Mar 20, 2017 16:24 |
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Version 2.10 of the model, I replaced the APEC no-line model with the "nlapec", I switched to APEC v3.0.8, and I removed the power-law component that was there as a crude background model | ||
Version 1 (current) | 20 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Mar 20, 2017 16:24 | Version 2.10 of the model, I replaced the APEC no-line model with the "nlapec", I switched to APEC v3.0.8, and I removed the power-law component that was there as a crude background model | |||
File N132D_E0310_v2.8_20150401_simple.mdl | 18 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Mar 09, 2017 11:43 |
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Version 2.8 of the model with parameters for one spectrum instead of for multiple data sets | ||
Version 1 (current) | 18 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Mar 09, 2017 11:43 | Version 2.8 of the model with parameters for one spectrum instead of for multiple data sets | |||
File N132D_E0310_v2.9_20150402_simple.mdl | 18 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 17, 2015 11:43 |
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v2.9 model, just the model | ||
Version 1 (current) | 18 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 17, 2015 11:43 | v2.9 model, just the model | |||
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. | ||
Version 1 (current) | 712 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 02, 2015 16:08 | 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. | |||
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. | ||
Version 1 (current) | 46 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 02, 2015 16:07 | 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 | ||
Version 1 (current) | 43 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 02, 2015 16:05 | 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 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 | ||
Version 1 (current) | 175 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 01, 2015 11:18 | Version 2.7 overplotted on the merged pn, and MOS1, MOS2 spectra | |||
File N132D_E0310_v2.7_20150324.mdl | 18 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 01, 2015 11:16 |
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Paul changed the Si XIII and S XV triplets to have four lines with the ratios of f,i,r expected for CIE with kT=1.2 keV, added a Si line at 2.294 keV, and reduced the widths of the Si and S lines. | ||
Version 1 (current) | 18 kB | Unknown User (plucinsky_1@touchstonenetwork.net) | Apr 01, 2015 11:16 | Paul changed the Si XIII and S XV triplets to have four lines with the ratios of f,i,r expected for CIE with kT=1.2 keV, added a Si line at 2.294 keV, and reduced the widths of the Si and S lines. | |||
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 | ||
Version 1 (current) | 300 kB | Unknown User (matteo.guainazzi_1@touchstonenetwork.net) | Mar 26, 2015 19:26 | How the N132D model was originally derived. Presentation given at the 2012 WG meeting | |||
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 | ||
Version 1 (current) | 117 kB | Unknown User (matteo.guainazzi_1@touchstonenetwork.net) | May 13, 2014 07:21 | 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 | |||
File N132D_E0310_v2.6_20140511_frozen.mdl | 20 kB | Unknown User (matteo.guainazzi_1@touchstonenetwork.net) | May 13, 2014 07:21 |
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Version 2.6 with all the parameters frozen. Main changes from 2.5: a) an overall normalization constant was added; b) abund wilm | ||
Version 1 (current) | 20 kB | Unknown User (matteo.guainazzi_1@touchstonenetwork.net) | May 13, 2014 07:21 | Version 2.6 with all the parameters frozen. Main changes from 2.5: a) an overall normalization constant was added; b) abund wilm |