| 5955 |
2005-03-28 13:16:48 |
Capella |
HD 34029 |
Non-eclipsing spectroscopic binary |
G5IIIe+... |
0.8000 |
79.172500 |
45.997340 |
28676.74 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for Capella |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.786 |
-0.173 |
-0.845 |
| ACIS-I |
-0.757 |
-0.022 |
-0.766 |
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 |
0.781 |
0.001 |
0.883 |
7.117 |
1.029 |
6.971 |
| Q-norm |
0.062 |
0.000 |
0.076 |
0.924 |
0.095 |
0.905 |
| ACIS-I |
keV |
0.810 |
0.000 |
0.913 |
7.088 |
1.102 |
0.000 |
| Q-norm |
0.066 |
0.000 |
0.080 |
0.920 |
0.104 |
0.000 |
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.
| 2.3218 |
1.4717 |
0.0000 |
0.0000 |
0.0201 |
5.2431 |
0.0606 |
0.0293 |
0.1093 |
0.0534 |
0.0251 |
0.0138 |
0.0000 |
0.0000 |
| 0.0079 |
0.0008 |
0.0113 |
0.0027 |
0.0202 |
0.0028 |
0.0536 |
0.0001 |
0.0537 |
0.0001 |
808.8021 |
4.3360 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of Capella.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
50.000 |
|
0.655 |
|
0.40 |
|
1.17101e-11 |
0.960343 |
2.08 |
213 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of Capella. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.087 |
|
30.000 |
|
0.595 |
|
0.37 |
|
1.95225e-13 |
0 |
1.23 |
47 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of Capella. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.102 |
|
1.074 |
|
0.595 |
|
0.43 |
|
3.13082e-13 |
0 |
2.02 |
48 |
HETG Light Curve
 |
| Odds | -2.261 |
| Prob. | 0.005 |
| Var. Index | 0 |
|
HETG light curve for Capella, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for Capella
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for Capella
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR