Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for YY Draconis |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
0.075 |
0.245 |
0.315 |
| ACIS-I |
0.136 |
0.475 |
0.574 |
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 |
0.942 |
0.007 |
1.336 |
0.006 |
2.066 |
0.010 |
| Q-norm |
0.083 |
0.001 |
0.135 |
0.001 |
0.229 |
0.001 |
| ACIS-I |
keV |
1.073 |
0.003 |
1.497 |
0.007 |
2.489 |
0.023 |
| Q-norm |
0.100 |
0.000 |
0.155 |
0.001 |
0.284 |
0.003 |
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.
| 1.1755 |
1.1129 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
19.1101 |
342.7862 |
41.1917 |
738.8569 |
36.2850 |
650.6086 |
6.6420 |
119.1641 |
| 0.0431 |
0.0039 |
0.0009 |
0.0008 |
0.0446 |
0.0040 |
0.0423 |
0.0003 |
0.0471 |
0.0003 |
8.8452 |
0.0349 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of YY Draconis.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
10.685 |
|
0.017 |
|
1.31 |
|
8.78073e-12 |
0 |
1.36 |
239 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of YY Draconis. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
0.836 |
|
1.39 |
|
3.84967e-13 |
0.0606335 |
1.34 |
72 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of YY Draconis. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
20.915 |
|
1.028 |
|
1.20 |
|
5.05146e-13 |
0.0386955 |
1.29 |
73 |
HETG Light Curve
 |
| Odds | -0.096 |
| Prob. | 0.445 |
| Var. Index | 0 |
|
HETG light curve for YY Draconis, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for YY Draconis
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for YY Draconis
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR