| 7253 |
2006-01-07 12:42:16 |
Lambda Ori X-1 |
HD 245059 |
Weak-lined T Tauri-type Star |
K1 |
0.7000 |
83.645430 |
10.118340 |
20887.32 |
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 |
-0.404 |
0.043 |
-0.367 |
| ACIS-I |
-0.346 |
0.265 |
-0.090 |
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 |
0.796 |
0.006 |
0.986 |
0.004 |
1.321 |
0.008 |
| Q-norm |
0.064 |
0.001 |
0.089 |
0.000 |
0.133 |
0.001 |
| ACIS-I |
keV |
0.883 |
0.004 |
1.073 |
0.006 |
1.467 |
0.011 |
| Q-norm |
0.076 |
0.001 |
0.100 |
0.001 |
0.152 |
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.
| 2.0804 |
3.6669 |
0.0000 |
0.0000 |
0.1744 |
0.8389 |
0.3423 |
0.5804 |
0.3457 |
0.4734 |
0.1380 |
0.2164 |
0.1660 |
0.4103 |
| 0.2478 |
0.0619 |
0.0670 |
0.3958 |
0.3234 |
0.4007 |
0.4272 |
0.0076 |
0.5353 |
0.0115 |
3.9493 |
0.0892 |
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 |
|
2.709 |
|
0.767 |
|
0.26 |
|
3.54161e-12 |
1.27012 |
1.37 |
73 |

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) |
0.039 |
|
2.095 |
|
0.602 |
|
0.29 |
|
3.5146e-13 |
0.558796 |
1.01 |
70 |

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 |
|
4.109 |
|
0.786 |
|
0.14 |
|
5.49811e-13 |
1.28035 |
1.15 |
63 |
HETG Light Curve
 |
| Odds | 0.436 |
| Prob. | 0.732 |
| Var. Index | 5 |
|
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