| 16 |
1999-10-09 11:22:12 |
AB DOR |
HD 36705 |
Rotationally variable Star |
K1IIIp... |
0.8000 |
82.186880 |
-65.448710 |
52333.62 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for AB DOR |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.517 |
0.002 |
-0.516 |
| ACIS-I |
-0.464 |
0.232 |
-0.260 |
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 |
0.767 |
7.234 |
0.956 |
0.000 |
1.205 |
0.005 |
| Q-norm |
0.061 |
0.939 |
0.085 |
0.000 |
0.117 |
0.001 |
| ACIS-I |
keV |
0.854 |
0.005 |
1.029 |
6.971 |
1.365 |
0.007 |
| Q-norm |
0.072 |
0.001 |
0.095 |
0.905 |
0.138 |
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.
| 2.2957 |
1.3755 |
0.8168 |
0.9402 |
0.1047 |
0.0777 |
0.2727 |
0.1152 |
0.1200 |
0.0372 |
0.0939 |
0.0392 |
0.0059 |
0.0033 |
| 0.0054 |
0.0003 |
0.0046 |
0.0004 |
0.0111 |
0.0007 |
0.0302 |
0.0000 |
0.0304 |
0.0000 |
160.2537 |
0.4277 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of AB DOR.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
6.356 |
|
0.823 |
|
0.21 |
|
9.86571e-12 |
0.222321 |
1.85 |
326 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of AB DOR. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
1.004 |
|
0.964 |
|
0.12 |
|
1.27966e-13 |
0 |
1.79 |
61 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of AB DOR. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
2.424 |
|
0.802 |
|
0.15 |
|
2.08905e-13 |
2.39708 |
1.03 |
64 |
HETG Light Curve
 |
| Odds | 184.655 |
| Prob. | 1.000 |
| Var. Index | 10 |
|
HETG light curve for AB DOR, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for AB DOR
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for AB DOR
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR