| 5420 |
2006-01-13 08:42:57 |
Lambda Ori X-1 |
HD 245059 |
Weak-lined T Tauri-type Star |
K1 |
0.7000 |
83.645510 |
10.118340 |
54766.42 |
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 |
-0.521 |
0.006 |
-0.516 |
| ACIS-I |
-0.469 |
0.230 |
-0.267 |
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 |
0.767 |
0.006 |
0.956 |
0.001 |
1.219 |
0.007 |
| Q-norm |
0.061 |
0.001 |
0.085 |
0.000 |
0.119 |
0.001 |
| ACIS-I |
keV |
0.854 |
0.005 |
1.029 |
0.004 |
1.351 |
0.007 |
| Q-norm |
0.072 |
0.001 |
0.095 |
0.000 |
0.136 |
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.
| 3.0785 |
3.1446 |
1.2451 |
5.9338 |
0.0395 |
0.2142 |
0.3256 |
0.3114 |
0.4514 |
0.4824 |
0.3540 |
0.4364 |
0.1565 |
0.1764 |
| 0.0976 |
0.0191 |
0.0368 |
0.0076 |
0.1442 |
0.0211 |
0.3613 |
0.0031 |
0.3994 |
0.0036 |
9.4661 |
0.1091 |
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 |
|
1.579 |
|
0.660 |
|
0.28 |
|
2.47006e-12 |
1.02232 |
1.52 |
100 |

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) |
0.000 |
|
0.990 |
|
0.986 |
|
0.15 |
|
1.1555e-13 |
0 |
1.98 |
58 |

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 |
|
0.979 |
|
0.978 |
|
0.15 |
|
2.01747e-13 |
0 |
1.56 |
65 |
HETG Light Curve
 |
| Odds | -1.831 |
| Prob. | 0.015 |
| Var. Index | 0 |
|
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