| 3454 |
2002-03-27 09:33:57 |
GK PER |
HD 21629 |
Cataclysmic Variable Star |
sd:Be+... |
-2.6800 |
52.799980 |
43.904290 |
31581.52 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for GK PER |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
0.880 |
-0.539 |
0.649 |
| ACIS-I |
0.907 |
-0.201 |
0.863 |
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 |
2.081 |
0.027 |
4.241 |
0.008 |
5.512 |
0.008 |
| Q-norm |
0.231 |
0.004 |
0.512 |
0.001 |
0.677 |
0.001 |
| ACIS-I |
keV |
3.409 |
0.010 |
4.650 |
0.008 |
5.818 |
0.008 |
| Q-norm |
0.404 |
0.001 |
0.565 |
0.001 |
0.717 |
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.
| 1.5360 |
1.8736 |
8.6813 |
37.4401 |
14.4818 |
10.8698 |
0.0799 |
0.0719 |
0.2133 |
0.2054 |
0.2598 |
0.1891 |
0.1895 |
0.2422 |
| 0.0672 |
0.0036 |
0.0040 |
0.0014 |
0.0714 |
0.0038 |
0.1612 |
0.0005 |
0.4303 |
0.0024 |
0.5988 |
0.0030 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of GK PER.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
10.000 |
|
30.000 |
|
0.109 |
|
2.37 |
|
1.15787e-11 |
0 |
5.50 |
275 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of GK PER. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
1.000 |
|
1.49 |
|
1.23352e-13 |
0 |
13.36 |
85 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of GK PER. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
1.000 |
|
1.50 |
|
1.29351e-13 |
0 |
13.47 |
86 |
HETG Light Curve
 |
| Odds | 745.238 |
| Prob. | 1.000 |
| Var. Index | 10 |
|
HETG light curve for GK PER, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for GK PER
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for GK PER
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR