| 1921 |
2001-08-09 05:37:23 |
GX340+0 |
4U 1642-45 |
Low Mass X-ray Binary |
undef |
0.0000 |
251.448510 |
-45.611410 |
23358.85 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for GX340+0 |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
0.992 |
0.306 |
0.996 |
| ACIS-I |
0.994 |
0.229 |
0.996 |
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 |
3.219 |
0.000 |
4.095 |
0.000 |
5.103 |
0.000 |
| Q-norm |
0.379 |
0.000 |
0.493 |
0.000 |
0.624 |
0.000 |
| ACIS-I |
keV |
3.292 |
4.708 |
4.198 |
0.007 |
5.220 |
0.000 |
| Q-norm |
0.389 |
0.611 |
0.506 |
0.001 |
0.639 |
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.
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of GX340+0.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
6.690 |
|
30.000 |
|
0.010 |
|
0.25 |
|
1.77421e-10 |
0 |
2.05 |
451 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of GX340+0. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
7.619 |
|
9.475 |
|
0.010 |
|
0.00 |
|
1.46583e-12 |
0 |
0.09 |
72 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of GX340+0. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
7.577 |
|
11.921 |
|
0.010 |
|
0.00 |
|
1.54548e-12 |
0 |
0.11 |
73 |
HETG Light Curve
 |
| Odds | -2.313 |
| Prob. | 0.005 |
| Var. Index | 0 |
|
HETG light curve for GX340+0, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for GX340+0
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for GX340+0
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR