| 5419 |
2006-03-31 03:21:37 |
WR 140 |
HD 193793 |
Wolf-Rayet Star |
WC7pd+O4-5 |
0.2700 |
305.116560 |
43.854510 |
45101.57 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for WR 140 |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
0.054 |
0.657 |
0.687 |
| ACIS-I |
0.094 |
0.746 |
0.785 |
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 |
1.102 |
0.000 |
1.467 |
0.006 |
2.051 |
0.007 |
| Q-norm |
0.104 |
0.000 |
0.152 |
0.001 |
0.227 |
0.001 |
| ACIS-I |
keV |
1.175 |
0.001 |
1.526 |
0.001 |
2.168 |
0.011 |
| Q-norm |
0.114 |
0.000 |
0.159 |
0.000 |
0.243 |
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 |
65.7216 |
0.0000 |
55.2263 |
0.0000 |
10.0948 |
0.0000 |
| 0.0041 |
0.0001 |
0.0001 |
0.0000 |
0.0044 |
0.0001 |
0.0065 |
0.0000 |
0.0067 |
0.0000 |
34.7020 |
0.0476 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of WR 140.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.371 |
|
45.428 |
|
1.227 |
|
0.36 |
|
1.02586e-11 |
0.530238 |
1.38 |
344 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of WR 140. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.494 |
|
29.997 |
|
1.605 |
|
0.14 |
|
2.03259e-13 |
0.614065 |
1.35 |
71 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of WR 140. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.697 |
|
2.575 |
|
1.000 |
|
0.27 |
|
2.52951e-13 |
1.10466 |
1.07 |
72 |
HETG Light Curve
 |
| Odds | -2.163 |
| Prob. | 0.007 |
| Var. Index | 0 |
|
HETG light curve for WR 140, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for WR 140
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for WR 140
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR