| 6287 |
2006-04-07 07:40:41 |
WR 140 |
HD 193793 |
Wolf-Rayet Star |
WC7pd+O4-5 |
0.2700 |
305.116570 |
43.854500 |
49256.29 |
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 |
0.069 |
0.657 |
0.695 |
| ACIS-I |
0.112 |
0.742 |
0.789 |
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 |
0.004 |
1.482 |
0.002 |
2.095 |
0.007 |
| Q-norm |
0.104 |
0.001 |
0.153 |
0.000 |
0.233 |
0.001 |
| ACIS-I |
keV |
1.175 |
0.004 |
1.540 |
0.002 |
2.256 |
0.010 |
| Q-norm |
0.114 |
0.001 |
0.161 |
0.000 |
0.254 |
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 |
5.5868 |
0.0000 |
5.2507 |
0.0000 |
0.7760 |
0.0000 |
| 0.0077 |
0.0002 |
0.0003 |
0.0001 |
0.0081 |
0.0002 |
0.0041 |
0.0000 |
0.0042 |
0.0000 |
45.1130 |
0.0894 |
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) |
0.422 |
|
13.962 |
|
1.104 |
|
0.48 |
|
1.00436e-11 |
0.456232 |
1.37 |
356 |

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) |
0.608 |
|
30.000 |
|
2.363 |
|
0.32 |
|
2.20041e-13 |
0.868373 |
1.25 |
72 |

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) |
0.465 |
|
3.130 |
|
1.000 |
|
0.37 |
|
2.54884e-13 |
0.425227 |
1.08 |
71 |
HETG Light Curve
 |
| Odds | -2.176 |
| 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