Документ взят из кэша поисковой машины. Адрес оригинального документа : http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/smith-cal-2012-2.pdf Дата изменения: Tue May 13 17:39:16 2014 Дата индексирования: Wed Apr 13 13:33:39 2016 Кодировка: Поисковые слова: внешние планеты

EPIC-pn Energy Resolution: Time Dependence

Michael Smith, ESAC


Calibration Source (I)

CalClosed line width monitoring: First single events, complete FOV.

Al-K: 9.4 ± 0.7 x 10-4 eV/Rev

Mn-K: 3.2 ± 0.1 x 10-3 eV/Rev

EPIC-pn Energy Resolution Time Dependence | Michael Smith | EPIC-BOC | Leicester, March 2012 | Pag.


Calibration Source (II)

CalClosed line width monitoring: First single events, RAWY > 180.

Al-K: 1.5 ± 0.2 x 10-3 eV/Rev

Mn-K: 5.9 ± 0.2 x 10-3 eV/Rev

EPIC-pn Energy Resolution Time Dependence | Michael Smith | EPIC-BOC | Leicester, March 2012 | Pag.


Astrophysical Sources
From previous results: Analysis of line width trends at Fe-K energies of SNR N132D and Eta Carinae (F. Haberl, 2010) do not confirm the time dependence of the energy resolution seen in the calibration source. E.g., even comparing over a base line of ~1000 revolutions the measured line widths were statistically consistent.

EPIC-pn Energy Resolution Time Dependence | Michael Smith | EPIC-BOC | Leicester, March 2012 | Pag.


Astrophysical Sources
From previous results: Analysis of line width trends at Fe-K energies of SNR N132D and Eta Carinae (F. Haberl, 2010) do not confirm the time dependence of the energy resolution seen in the calibration source. E.g., even comparing over a base line of ~1000 revolutions the measured line widths were statistically consistent.

Now: analysis of Fe-K emission line widths in obscured AGN. X-ray spectrum dominated by reflection components. Fe-K emission assumed to be essentially neutral in origin, and intrinsically narrow. Sample consisting of 20 observation of 12 sources. Sources are either point-like or compact extended, located at the bore sight. Spectra created w/ single + double events.
EPIC-pn Energy Resolution Time Dependence | Michael Smith | EPIC-BOC | Leicester, March 2012 | Pag.


Model
Fit in the 5.5 ­ 7.5 keV band to a generic phenomenological model: po + zgauss + zgauss + [zgauss + zgauss + zgauss]

Fe-K [Fe He-Like K [Fe H-Like K Fe-K

6.40 keV 6.63 keV]
Fe XXV K Fe XXVI K Fe-K Fe-K

6.96 keV] 7.05 keV

[Compton Shoulder 6.30 keV]

EPIC-pn Energy Resolution Time Dependence | Michael Smith | EPIC-BOC | Leicester, March 2012 | Pag.

CS


Observation Sample

Source Circinus Galaxy NGC 424 NGC 1068 ESO 138-G1 NGC 4945 Mrk 3

ObsID 0111240101 0002942301 0550950101 0111200201 0111200101 0405380201 0112310301 0204870101 0009220601 0009220901 0009220501 0009221401

Rev 0304 0367 1648 0117 0117 1317 0205 0749 0234 0322 0420 0432 1219 0560 0654 1132 0837 0568 1180 1182

Fe-K 6.400 keV

Fe-K 7.058 keV

He-like Fe-K 6.63 keV

H-like Fe-K Compton Reduced C-stat / Shoulder D.o.f. 6.96 keV 399.64 / 331 352.93 / 390 398.09 / 390 404.99 / 390 398.69 / 389 416.39 / 389 379.01 / 390 379.36 / 390 517.52 / 390 438.68 / 390 367.22 / 390 455.41 / 390 393.75 / 390 330.52 / 391 273.12 / 392

NGC 1320 NGC 1386 NGC 3393 ESO 137-G34 NGC 4968 NGC 5194

0405240201 0140950201 0140950601 0307001901 0200660201 0112840201 0303420101 0303420201



407.72 / 390 295.32 / 390 381.71 / 390 385.28 / 390 374.94 / 390

EPIC-pn Energy Resolution Time Dependence | Michael Smith | EPIC-BOC | Leicester, March 2012 | Pag.


Results

Source Circinus Galaxy NGC 424 NGC 1068 ESO 138-G1 NGC 4945 Mrk 3

ObsID 0111240101 0002942301 0550950101 0111200201 0111200101 0405380201 0112310301 0204870101 0009220601 0009220901 0009220501 0009221401

Rev 0304 0367 1648 0117 0117 1317 0205 0749 0234 0322 0420 0432 1219 0560 0654 1132 0837 0568 1180 1182

Fe-K 6.400 keV

Fe-K 7.058 keV

He-like Fe-K 6.63 keV

H-like Fe-K Compton Reduced C-stat / Shoulder D.o.f. 6.96 keV 399.64 / 331 352.93 / 390 398.09 / 390 404.99 / 390 398.69 / 389 416.39 / 389 379.01 / 390 379.36 / 390 517.52 / 390 438.68 / 390 367.22 / 390 455.41 / 390 393.75 / Linear fit: 330.52 2.6 ± 0.9 x 10-2 eV/Rev/ 273.12 / Cf. Mn-K (at RAWY > / 407.72 180): 295.32 5.9 ± 0.2 x 10-3 eV/Rev/ 381.71 / 390 391 392 390 390 390

NGC 1320 NGC 1386 NGC 3393 ESO 137-G34 NGC 4968 NGC 5194

0405240201 0140950201 0140950601 0307001901 0200660201 0112840201 0303420101 0303420201



385.28 / 390 374.94 / 390

EPIC-pn Energy Resolution Time Dependence | Michael Smith | EPIC-BOC | Leicester, March 2012 | Pag.


Results

Source Circinus Galaxy NGC 424 NGC 1068 ESO 138-G1 NGC 4945 Mrk 3

ObsID 0111240101 0002942301 0550950101 0111200201 0111200101 0405380201 0112310301 0204870101 0009220601 0009220901 0009220501 0009221401

Rev 0304 0367 1648 0117 0117 1317 0205 0749 0234 0322 0420 0432 1219 0560 0654 1132 0837 0568 1180 1182

Fe-K 6.400 keV

Fe-K 7.058 keV

He-like Fe-K 6.63 keV

H-like Fe-K Compton Reduced C-stat / Shoulder D.o.f. 6.96 keV 399.64 / 331 352.93 / 390 398.09 / 390 404.99 / 390 398.69 / 389 416.39 / 389 379.01 / 390 379.36 / 390 517.52 / 390 438.68 / 390 367.22 / 390 455.41 / 390 393.75 / Linear fit: 330.52 2.6 ± 0.9 x 10-2 eV/Rev/ 273.12 / Cf. Mn-K (at RAWY > / 407.72 180): 295.32 5.9 ± 0.2 x 10-3 eV/Rev/ 381.71 / 390 391 392 390 390 390

NGC 1320 NGC 1386 NGC 3393 ESO 137-G34 NGC 4968 NGC 5194

0405240201 0140950201 0140950601 0307001901 0200660201 0112840201 0303420101 0303420201

112 ks Circinus Galaxy


385.28 / 390 374.94 / 390

EPIC-pn Energy Resolution Time Dependence | Michael Smith | EPIC-BOC | Leicester, March 2012 | Pag.