| 6286 |
2006-03-23 04:59:01 |
WR 140 |
HD 193793 |
Wolf-Rayet Star |
WC7pd+O4-5 |
0.2700 |
305.116530 |
43.854520 |
46930.91 |
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 |
0.083 |
0.664 |
0.708 |
| ACIS-I |
0.124 |
0.751 |
0.800 |
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 |
1.117 |
0.007 |
1.497 |
0.001 |
2.110 |
0.007 |
| Q-norm |
0.106 |
0.001 |
0.155 |
0.000 |
0.235 |
0.001 |
| ACIS-I |
keV |
1.175 |
0.005 |
1.555 |
0.006 |
2.285 |
0.011 |
| Q-norm |
0.114 |
0.001 |
0.163 |
0.001 |
0.258 |
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 |
2.6560 |
0.0000 |
3.1523 |
0.0000 |
1.0134 |
0.0000 |
| 0.0077 |
0.0002 |
0.0001 |
0.0001 |
0.0080 |
0.0002 |
0.0042 |
0.0000 |
0.0043 |
0.0000 |
42.6013 |
0.0848 |
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) |
0.414 |
|
30.201 |
|
1.121 |
|
0.25 |
|
9.92883e-12 |
0.608993 |
1.35 |
349 |

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) |
0.396 |
|
30.000 |
|
1.967 |
|
0.23 |
|
2.36078e-13 |
0.342782 |
1.03 |
77 |

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) |
0.387 |
|
2.751 |
|
1.000 |
|
0.40 |
|
2.51687e-13 |
0.111587 |
1.31 |
73 |
HETG Light Curve
 |
| Odds | -1.777 |
| Prob. | 0.016 |
| 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