| 2538 |
2002-07-10 11:27:42 |
CPD-66 3080B |
HD 155555C |
Star in Double System |
M4.5 |
1.5400 |
259.380360 |
-66.951610 |
94218.76 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for CPD-66 3080B |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.640 |
0.083 |
-0.588 |
| ACIS-I |
-0.598 |
0.232 |
-0.425 |
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 |
0.810 |
0.007 |
0.956 |
0.000 |
1.132 |
0.006 |
| Q-norm |
0.066 |
0.001 |
0.085 |
0.000 |
0.108 |
0.001 |
| ACIS-I |
keV |
0.854 |
0.002 |
1.000 |
0.001 |
1.219 |
0.008 |
| Q-norm |
0.072 |
0.000 |
0.091 |
0.000 |
0.119 |
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.
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of CPD-66 3080B.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.017 |
|
0.784 |
|
0.010 |
|
0.11 |
|
1.89564e-12 |
0 |
1.75 |
105 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of CPD-66 3080B. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
0.760 |
|
1.20 |
|
7.44725e-14 |
1.82688 |
1.71 |
54 |
HETG Light Curve
 |
| Odds | 160.438 |
| Prob. | 1.000 |
| Var. Index | 10 |
|
HETG light curve for CPD-66 3080B, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for CPD-66 3080B
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for CPD-66 3080B
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR