| 2575 |
2002-02-01 02:31:28 |
BETA CRU |
HD 111123 |
Variable Star of beta Cep type |
B0.5III |
-0.1520 |
191.930290 |
-59.688800 |
74380.47 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for BETA 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 |
-0.888 |
-0.711 |
-0.980 |
| ACIS-I |
-0.865 |
-0.525 |
-0.956 |
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 |
0.577 |
0.001 |
0.694 |
0.005 |
0.825 |
0.002 |
| Q-norm |
0.036 |
0.000 |
0.051 |
0.001 |
0.068 |
0.000 |
| ACIS-I |
keV |
0.635 |
0.002 |
0.767 |
0.002 |
0.913 |
0.007 |
| Q-norm |
0.044 |
0.000 |
0.061 |
0.000 |
0.080 |
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.
| 0.4082 |
0.5130 |
16.7181 |
58.5796 |
0.6285 |
0.5816 |
0.2100 |
0.1308 |
0.0200 |
0.0517 |
0.0061 |
0.0514 |
0.0000 |
0.0000 |
| 0.1635 |
0.0000 |
0.4247 |
0.0000 |
0.6019 |
0.0000 |
6.7698 |
0.0000 |
6.7698 |
0.6430 |
0.0000 |
0.0000 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of BETA CRU.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
0.309 |
|
0.088 |
|
0.16 |
|
4.91746e-12 |
1.07577 |
3.02 |
71 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of BETA CRU. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.088 |
|
1.033 |
|
0.248 |
|
0.30 |
|
8.83427e-14 |
0 |
3.29 |
41 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of BETA CRU. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
0.508 |
|
0.196 |
|
0.47 |
|
2.81315e-13 |
5.52352 |
1.83 |
44 |
HETG Light Curve
 |
| Odds | 1.722 |
| Prob. | 0.981 |
| Var. Index | 6 |
|
HETG light curve for BETA CRU, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for BETA CRU
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for BETA CRU
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR