| 1927 |
2001-02-07 09:57:17 |
VELA X-1 |
GP Vel |
High Mass X-ray Binary |
B0Ia |
0.3750 |
135.528360 |
-40.554810 |
29430.47 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for VELA 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 |
0.930 |
0.696 |
0.987 |
| ACIS-I |
0.943 |
0.734 |
0.991 |
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 |
3.701 |
0.003 |
4.694 |
0.000 |
5.716 |
0.001 |
| Q-norm |
0.442 |
0.000 |
0.571 |
0.000 |
0.703 |
0.000 |
| ACIS-I |
keV |
3.818 |
0.001 |
4.811 |
0.002 |
5.833 |
0.006 |
| Q-norm |
0.457 |
0.000 |
0.586 |
0.000 |
0.719 |
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.
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of VELA X-1.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
10.000 |
|
30.000 |
|
0.010 |
|
1.93 |
|
3.98369e-11 |
0 |
9.77 |
377 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of VELA X-1. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
1.000 |
|
1.49 |
|
9.16679e-14 |
0 |
15.42 |
83 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of VELA X-1. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
30.000 |
|
1.000 |
|
1.50 |
|
1.19688e-13 |
0 |
15.12 |
83 |
HETG Light Curve
 |
| Odds | 9999.999 |
| Prob. | 1.000 |
| Var. Index | 10 |
|
HETG light curve for VELA X-1, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for VELA X-1
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for VELA X-1
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR