| 6247 |
2006-01-31 02:39:30 |
15 Mon |
HD 47839 |
Double or multiple star |
O7V((f))+O9.5Vn |
-0.2480 |
100.244330 |
9.895750 |
37471.43 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for 15 Mon |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.842 |
-0.672 |
-0.967 |
| ACIS-I |
-0.816 |
-0.456 |
-0.927 |
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 |
0.577 |
0.003 |
0.679 |
0.006 |
0.840 |
0.002 |
| Q-norm |
0.036 |
0.000 |
0.049 |
0.001 |
0.070 |
0.000 |
| ACIS-I |
keV |
0.635 |
0.004 |
0.781 |
0.007 |
0.942 |
0.007 |
| Q-norm |
0.044 |
0.000 |
0.062 |
0.001 |
0.083 |
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.
| 0.3082 |
0.8248 |
0.0000 |
0.0000 |
0.5604 |
2.1289 |
0.2211 |
0.2685 |
0.2252 |
0.1611 |
0.0000 |
0.0000 |
0.0325 |
0.1737 |
| 0.2525 |
0.1651 |
0.4648 |
2.6313 |
0.7223 |
2.6365 |
16.1859 |
7.1194 |
20.0382 |
10.9056 |
4.2016 |
2.3059 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of 15 Mon.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.150 |
|
0.229 |
|
0.017 |
|
0.06 |
|
0 |
0 |
1.01 |
38 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of 15 Mon. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.047 |
|
0.584 |
|
0.208 |
|
0.39 |
|
2.0542e-13 |
8.86376 |
1.80 |
43 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of 15 Mon. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.047 |
|
0.924 |
|
0.222 |
|
0.05 |
|
5.25783e-13 |
27.4603 |
1.44 |
50 |
HETG Light Curve
 |
| Odds | -1.707 |
| Prob. | 0.019 |
| Var. Index | 0 |
|
HETG light curve for 15 Mon, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for 15 Mon
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for 15 Mon
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR