| 1706 |
2000-05-18 09:41:14 |
EX HYA |
RX J1252.4-2914 |
Cataclysmic Var. DQ Her type |
M5/M6:... |
1.8000 |
193.100890 |
-29.249000 |
59146.24 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for EX HYA |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
0.022 |
0.234 |
0.255 |
| ACIS-I |
0.088 |
0.436 |
0.505 |
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 |
0.927 |
7.073 |
1.263 |
0.000 |
2.008 |
0.007 |
| Q-norm |
0.081 |
0.919 |
0.125 |
0.000 |
0.222 |
0.001 |
| ACIS-I |
keV |
1.029 |
0.000 |
1.424 |
0.007 |
2.373 |
0.007 |
| Q-norm |
0.095 |
0.000 |
0.146 |
0.001 |
0.269 |
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.
| 2.2666 |
1.0345 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.1523 |
0.0576 |
0.4576 |
0.1197 |
0.4661 |
0.1214 |
0.2152 |
0.0613 |
| 0.0025 |
0.0001 |
0.0005 |
0.0000 |
0.0031 |
0.0001 |
0.0044 |
0.0000 |
0.0044 |
0.0000 |
155.9110 |
0.1462 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of EX HYA.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.019 |
|
30.000 |
|
0.010 |
|
3.05 |
|
8.0388e-12 |
0 |
2.44 |
376 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of EX HYA. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
0.802 |
|
1.49 |
|
2.01739e-13 |
0.116788 |
1.16 |
75 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of EX HYA. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
27.280 |
|
0.730 |
|
1.18 |
|
2.90164e-13 |
0.101735 |
0.90 |
73 |
HETG Light Curve
 |
| Odds | 1954.849 |
| Prob. | 1.000 |
| Var. Index | 10 |
|
HETG light curve for EX HYA, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for EX HYA
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for EX HYA
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR