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 |
0.024 |
0.228 |
0.250 |
| ACIS-I |
0.082 |
0.457 |
0.520 |
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 |
0.927 |
0.001 |
1.263 |
0.007 |
1.964 |
0.008 |
| Q-norm |
0.081 |
0.000 |
0.125 |
0.001 |
0.216 |
0.001 |
| ACIS-I |
keV |
1.044 |
0.002 |
1.424 |
0.007 |
2.197 |
0.019 |
| Q-norm |
0.097 |
0.000 |
0.146 |
0.001 |
0.246 |
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.
| 0.8326 |
0.4981 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
1.2699 |
1.0566 |
1.1818 |
0.9392 |
1.9550 |
1.6337 |
1.2072 |
1.1844 |
| 0.0203 |
0.0012 |
0.0009 |
0.0004 |
0.0218 |
0.0013 |
0.0379 |
0.0002 |
0.0407 |
0.0002 |
13.6727 |
0.0412 |
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) |
0.000 |
|
7.207 |
|
0.010 |
|
1.36 |
|
7.54998e-12 |
0 |
1.62 |
286 |

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 |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
0.825 |
|
1.23 |
|
2.377e-13 |
0.092889 |
1.80 |
71 |

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 |
|
6.098 |
|
0.743 |
|
1.50 |
|
3.16316e-13 |
0.0652502 |
1.11 |
74 |
HETG Light Curve
 |
| Odds | 25.668 |
| 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