| 6613 |
2006-10-01 17:42:26 |
IGR J17497-2821 |
undef |
Gamma-ray Source |
undef |
0.0000 |
267.408430 |
-28.354840 |
19701.68 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for IGR J17497-2821 |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
0.984 |
0.441 |
0.994 |
| ACIS-I |
0.986 |
0.477 |
0.995 |
S, M, and H represent the predicted total counts in the following passbands: S: 0.3-0.9 keV M: 0.9-1.5 keV H: 1.5-8.0 keV |
| ACIS-S |
keV |
3.030 |
0.004 |
3.920 |
0.004 |
4.928 |
0.007 |
| Q-norm |
0.354 |
0.001 |
0.470 |
0.001 |
0.601 |
0.001 |
| ACIS-I |
keV |
3.117 |
0.004 |
4.022 |
0.007 |
5.059 |
0.006 |
| Q-norm |
0.366 |
0.001 |
0.483 |
0.001 |
0.618 |
0.001 |
Normalized quantiles (Q-norm) are defined as:
Qx = (Ex - Elo)/(Ehi - Elo) Where Elo = 0.3 keV and Ehi = 8.0 keV. |
Spectral Metrics
A series of line-line, line-continuum, and continuum-continuum ratios calculated from the high-resolution 1st order MEG or LEG spectrum.
| 0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
| 0.0011 |
199.8768 |
0.0000 |
0.0000 |
0.0011 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
3.6242 |
0.0018 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of IGR J17497-2821.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
5.191 |
|
30.000 |
|
0.011 |
|
0.74 |
|
2.20156e-11 |
0 |
1.18 |
303 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of IGR J17497-2821. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
1.000 |
|
1.50 |
|
1.33857e-13 |
0 |
16.13 |
81 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of IGR J17497-2821. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
1.000 |
|
1.50 |
|
6.44379e-13 |
0 |
11.10 |
78 |
HETG Light Curve
 |
| Odds | -1.842 |
| Prob. | 0.014 |
| Var. Index | 0 |
|
HETG light curve for IGR J17497-2821, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for IGR J17497-2821
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for IGR J17497-2821
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR