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HXMT Coordinated Observation Shaolin XIONG On behalf of HXMT SGS team Institue of High Energy Physics, China 11th IACHEC, IUCAA, PUNE (Mar 1, 2016)

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Presentation on theme: "HXMT Coordinated Observation Shaolin XIONG On behalf of HXMT SGS team Institue of High Energy Physics, China 11th IACHEC, IUCAA, PUNE (Mar 1, 2016)"— Presentation transcript:

1 HXMT Coordinated Observation Shaolin XIONG On behalf of HXMT SGS team Institue of High Energy Physics, China 11th IACHEC, IUCAA, PUNE (Mar 1, 2016)

2 In-flight calibration (1): PSF
High Energy tel. NaI/CsI keV, ~5000 cm2 Medium Energy tel. Si-PIN 5-30 keV, ~950 cm2 Low Energy tel. SCD (CCD236) 1-15 keV, ~380 cm2 Collimators for HE/ME/LE Scan the constant bright 'point' source (Crab or PSR B ) Crab exposure: ~ 40 ks Crab is visible from Sep. to Mar. 2

3 In-flight calibration (2)(3):
RMF, ARF; Timing High Energy tel. NaI/CsI keV, ~5000 cm2 Medium Energy tel. Si-PIN 5-30 keV, ~950 cm2 Low Energy tel. SCD (CCD236) 1-15 keV, ~380 cm2 RMF&ARF Absolute ARFs need to be calibrated in-flight Pointing observing the Crab or other sources cross calibrated with others Adjust RMF and ARF to fit the observed data with the “known” source spectrum Timing Observe the Crab/PSR B 10ks for Crab, 1Ms for PSR B 3

4 In-flight calibration (4): Energy-Channel and FWHM
HE AGC with 241Am (1/det. unit) Temp. range : 18 ± 2 °C ME 241Am (2/det. box) Temp. range:-50 ~ 0 °C LE 55Fe (1/det. box) Temp. range:-80 ~ -30 °C Fluorescent lines (73Ta)in HE Gain & FWHM varies with Temp. Measured on ground Calibration Sources Radioactive sources on-board Fluorescent lines Sources with line features (1 – 30 keV) Tycho Spectrum Fe Kα Line, 126ks(3 σ) obs is needed 4 4

5 In-flight calibration (5): Bkg model
Cross calibrate the blank sky (~ deg)? CXB is anisotropic Especially for LE (< 7 KeV) where CXB dominates the BKG Known sources and Blank sky (blue circle for HXMT, red circle for RXTE) 5

6 In-flight calibration (6): Response of the spacecraft
GRB monitor Use CsI (200 keV - 3 MeV) detector of HE Approximately all-sky monitoring Energy response calibration will not be calibrated on ground Simultaneous GRBs by Fermi, Swift, Integral, Konus-Wind, etc. GRB GRB 6

7 List of In-flight Calibration Sources
Source Name RA DEC Usage Crab 83.63 22.01 RMF, ARF; Timing; PSF, boresight PSR B 228.48 -59.14 Cas A 58.813 Data analysis, LE temperature drift Tycho 6.334 64.150 Cyg X-1 299.59 35.20 Data analysis, quick-look Sco X-1 244.98 -15.64 Mrk421 166.11 40.09 Blank Sky #1 4.3899 Background (include: night Earth) Blank Sky #2 Blank Sky #3 8.8014 Blank Sky #4 Blank Sky #5 Blank Sky #6 Blank Sky #7 Blank Sky #8 Other (IACHEC) sources? HXMT Initial Calibration phase: – (TBC) 7 7

8 HXMT visibility to some sources
Blank sky 8 8


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