| 609 |
1999-12-17 04:05:25 |
LAMBDA AND |
HD 222107 |
Variable of RS CVn type |
G8III+... |
1.0800 |
354.390930 |
46.458210 |
81900.03 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for LAMBDA AND |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.530 |
0.119 |
-0.438 |
| ACIS-I |
-0.485 |
0.328 |
-0.186 |
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 |
7.190 |
0.986 |
0.003 |
1.278 |
0.001 |
| Q-norm |
0.066 |
0.934 |
0.089 |
0.000 |
0.127 |
0.000 |
| ACIS-I |
keV |
0.883 |
0.000 |
1.059 |
6.942 |
1.394 |
0.001 |
| Q-norm |
0.076 |
0.000 |
0.099 |
0.901 |
0.142 |
0.000 |
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.
| 2.7873 |
1.8568 |
0.0000 |
0.0000 |
0.0729 |
0.0581 |
0.3390 |
0.1626 |
0.5808 |
0.2760 |
0.1283 |
0.0539 |
0.0547 |
0.0211 |
| 0.0048 |
0.0003 |
0.0027 |
0.0003 |
0.0084 |
0.0006 |
0.0194 |
0.0000 |
0.0195 |
0.0000 |
273.7716 |
0.6552 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of LAMBDA AND.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
3.864 |
|
0.900 |
|
0.21 |
|
9.98104e-12 |
0.202579 |
2.46 |
354 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of LAMBDA AND. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
1.054 |
|
1.020 |
|
0.16 |
|
8.42321e-14 |
0 |
1.63 |
63 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of LAMBDA AND. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
1.091 |
|
1.048 |
|
0.25 |
|
1.28489e-13 |
0.417942 |
1.01 |
61 |
HETG Light Curve
 |
| Odds | 14.781 |
| Prob. | 1.000 |
| Var. Index | 9 |
|
HETG light curve for LAMBDA AND, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for LAMBDA AND
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for LAMBDA AND
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR