| 6241 |
2005-12-30 11:55:59 |
Lambda Ori X-1 |
HD 245059 |
Weak-lined T Tauri-type Star |
K1 |
0.7000 |
83.645420 |
10.118300 |
17724.68 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for Lambda Ori X-1 |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.374 |
0.002 |
-0.372 |
| ACIS-I |
-0.316 |
0.229 |
-0.094 |
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 |
0.781 |
0.007 |
0.986 |
0.007 |
1.336 |
0.010 |
| Q-norm |
0.062 |
0.001 |
0.089 |
0.001 |
0.135 |
0.001 |
| ACIS-I |
keV |
0.869 |
0.006 |
1.073 |
0.007 |
1.482 |
0.011 |
| Q-norm |
0.074 |
0.001 |
0.100 |
0.001 |
0.153 |
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.
| 1.7585 |
2.8650 |
0.0000 |
0.0000 |
0.2908 |
0.5848 |
0.6795 |
1.2643 |
0.6089 |
0.8665 |
0.5104 |
1.0976 |
0.4384 |
0.7336 |
| 0.2713 |
0.0745 |
0.0769 |
0.0721 |
0.3572 |
0.1040 |
0.4622 |
0.0103 |
0.6019 |
0.0168 |
3.3093 |
0.0961 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of Lambda Ori X-1.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
5.004 |
|
0.991 |
|
0.15 |
|
3.46063e-12 |
2.88473 |
1.15 |
62 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of Lambda Ori X-1. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
2.616 |
|
0.618 |
|
0.31 |
|
4.01864e-13 |
0.658548 |
1.38 |
60 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of Lambda Ori X-1. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
2.374 |
|
0.643 |
|
0.28 |
|
6.62653e-13 |
0.641098 |
0.88 |
68 |
HETG Light Curve
 |
| Odds | 39.983 |
| Prob. | 1.000 |
| Var. Index | 10 |
|
HETG light curve for Lambda Ori X-1, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for Lambda Ori X-1
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for Lambda Ori X-1
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR