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 |
0.065 |
0.188 |
0.249 |
| ACIS-I |
0.126 |
0.427 |
0.524 |
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 |
0.913 |
0.003 |
1.307 |
0.005 |
1.993 |
0.008 |
| Q-norm |
0.080 |
0.000 |
0.131 |
0.001 |
0.220 |
0.001 |
| ACIS-I |
keV |
1.059 |
0.004 |
1.467 |
0.005 |
2.343 |
0.021 |
| Q-norm |
0.099 |
0.001 |
0.152 |
0.001 |
0.265 |
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.
| 3.3229 |
6.5249 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.2003 |
0.3726 |
0.6389 |
0.4064 |
1.2603 |
0.9349 |
0.1078 |
0.1342 |
| 0.0386 |
0.0031 |
0.0014 |
0.0010 |
0.0407 |
0.0033 |
0.0446 |
0.0002 |
0.0489 |
0.0003 |
10.2064 |
0.0398 |
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 |
|
10.690 |
|
0.014 |
|
1.08 |
|
7.3249e-12 |
0 |
1.79 |
278 |

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 |
|
0.807 |
|
1.50 |
|
2.5284e-13 |
0.0227476 |
0.96 |
69 |

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 |
|
20.309 |
|
0.895 |
|
0.80 |
|
3.55167e-13 |
0.0609547 |
1.07 |
70 |
HETG Light Curve
 |
| Odds | -1.030 |
| Prob. | 0.085 |
| 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