| 3753 |
2003-12-12 12:06:50 |
EPSILON ORI |
HD 37128 |
Emission-line Star |
B0Ia |
-0.1900 |
84.053350 |
-1.201920 |
91647.03 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for EPSILON ORI |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.825 |
-0.477 |
-0.935 |
| ACIS-I |
-0.797 |
-0.254 |
-0.874 |
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 |
0.635 |
0.000 |
0.781 |
0.000 |
0.927 |
0.000 |
| Q-norm |
0.044 |
0.000 |
0.062 |
0.000 |
0.081 |
0.000 |
| ACIS-I |
keV |
0.723 |
0.000 |
0.854 |
0.000 |
1.000 |
0.005 |
| Q-norm |
0.055 |
0.000 |
0.072 |
0.000 |
0.091 |
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.
| 1.0172 |
0.3175 |
0.0000 |
0.0000 |
0.3756 |
0.1004 |
0.1044 |
0.0203 |
0.0264 |
0.0143 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
| 0.0261 |
0.0000 |
0.0464 |
0.0000 |
0.0770 |
0.0000 |
0.8544 |
0.0000 |
0.8544 |
0.0039 |
0.0000 |
0.0000 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of EPSILON ORI.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.173 |
|
0.251 |
|
0.026 |
|
0.03 |
|
0 |
0 |
4.99 |
122 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of EPSILON ORI. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.083 |
|
0.324 |
|
0.322 |
|
0.16 |
|
6.23221e-14 |
0 |
2.36 |
48 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of EPSILON ORI. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.083 |
|
0.735 |
|
0.280 |
|
0.12 |
|
1.32748e-13 |
8.67004 |
1.52 |
49 |
HETG Light Curve
 |
| Odds | -1.930 |
| Prob. | 0.012 |
| Var. Index | 0 |
|
HETG light curve for EPSILON ORI, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for EPSILON ORI
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for EPSILON ORI
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR