| 3410 |
2001-12-18 19:24:18 |
Mu Vel |
HD 93497 |
Double or multiple star |
G5IIIa |
0.9140 |
161.692560 |
-49.420280 |
57003.33 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for Mu Vel |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.747 |
-0.158 |
-0.809 |
| ACIS-I |
-0.710 |
0.003 |
-0.708 |
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 |
7.234 |
0.883 |
7.117 |
1.044 |
0.003 |
| Q-norm |
0.061 |
0.939 |
0.076 |
0.924 |
0.097 |
0.000 |
| ACIS-I |
keV |
0.810 |
0.000 |
0.927 |
7.073 |
1.117 |
0.001 |
| Q-norm |
0.066 |
0.000 |
0.081 |
0.919 |
0.106 |
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.
| 2.9872 |
2.5054 |
0.6306 |
2.1254 |
0.2153 |
0.1966 |
0.0442 |
0.0293 |
0.0630 |
0.0474 |
0.0265 |
0.0154 |
0.0063 |
0.0110 |
| 0.0272 |
0.0029 |
0.0362 |
0.0050 |
0.0669 |
0.0061 |
0.1875 |
0.0004 |
0.1887 |
0.0004 |
151.2817 |
1.4888 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of Mu Vel.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.011 |
|
1.828 |
|
0.672 |
|
0.38 |
|
7.51633e-12 |
2.00708 |
4.46 |
177 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of Mu Vel. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.088 |
|
30.000 |
|
0.566 |
|
0.30 |
|
9.46313e-14 |
0 |
1.29 |
46 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of Mu Vel. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
|
0.000 |
|
0.000 |
|
0.000 |
|
0.00 |
|
9.46313e-14 |
0 |
0.00 |
0 |
HETG Light Curve
 |
| Odds | -0.639 |
| Prob. | 0.187 |
| Var. Index | 0 |
|
HETG light curve for Mu Vel, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for Mu Vel
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for Mu Vel
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR