| 7186 |
2005-10-19 10:22:16 |
RT Cru |
IGR J12349-6434 |
Variable Star |
undef |
0.0000 |
188.723950 |
-64.565540 |
49344.95 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for RT Cru |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
0.980 |
0.301 |
0.989 |
| ACIS-I |
0.984 |
0.294 |
0.991 |
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 |
3.657 |
0.018 |
4.621 |
0.017 |
5.745 |
0.021 |
| Q-norm |
0.436 |
0.002 |
0.561 |
0.002 |
0.707 |
0.003 |
| ACIS-I |
keV |
3.774 |
0.014 |
4.752 |
0.016 |
5.906 |
0.018 |
| Q-norm |
0.451 |
0.002 |
0.578 |
0.002 |
0.728 |
0.002 |
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.
| 0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
| 0.2882 |
0.0965 |
0.0008 |
0.0043 |
0.2891 |
0.0966 |
0.0655 |
0.0009 |
1.9866 |
0.4685 |
0.0341 |
0.0080 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of RT Cru.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
10.000 |
|
50.000 |
|
1.000 |
|
1.50 |
|
7.77669e-12 |
0 |
1.97 |
254 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of RT Cru. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
1.000 |
|
1.50 |
|
8.43875e-14 |
0 |
14.64 |
83 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of RT Cru. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
1.000 |
|
1.50 |
|
6.34132e-14 |
0 |
16.30 |
79 |
HETG Light Curve
 |
| Odds | 2.197 |
| Prob. | 0.994 |
| Var. Index | 7 |
|
HETG light curve for RT Cru, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for RT Cru
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for RT Cru
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR