Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for WX HYI |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.038 |
0.234 |
0.198 |
| ACIS-I |
0.027 |
0.470 |
0.490 |
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 |
0.913 |
0.000 |
1.234 |
0.007 |
1.876 |
0.008 |
| Q-norm |
0.080 |
0.000 |
0.121 |
0.001 |
0.205 |
0.001 |
| ACIS-I |
keV |
1.029 |
0.002 |
1.394 |
0.005 |
2.081 |
0.016 |
| Q-norm |
0.095 |
0.000 |
0.142 |
0.001 |
0.231 |
0.002 |
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.
| 3.3952 |
3.0880 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.1369 |
0.1330 |
0.8771 |
0.5057 |
1.0742 |
0.6644 |
0.1635 |
0.2370 |
| 0.0275 |
0.0018 |
0.0025 |
0.0009 |
0.0304 |
0.0020 |
0.0413 |
0.0002 |
0.0441 |
0.0002 |
14.3215 |
0.0503 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of WX HYI.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.002 |
|
6.710 |
|
0.010 |
|
2.03 |
|
7.85453e-12 |
0 |
1.35 |
293 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of WX HYI. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
|
0.000 |
|
0.000 |
|
0.000 |
|
0.00 |
|
7.85453e-12 |
0 |
0.00 |
0 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of WX HYI. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
6.981 |
|
1.031 |
|
1.50 |
|
3.30474e-13 |
0.0682234 |
0.96 |
78 |
HETG Light Curve
 |
| Odds | 23.861 |
| Prob. | 1.000 |
| Var. Index | 9 |
|
HETG light curve for WX HYI, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for WX HYI
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for WX HYI
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR