| 6265 |
2005-08-09 07:22:10 |
V4046 Sgr |
HD 319139 |
Classical T Tauri-type Star |
K5 |
0.9000 |
273.543650 |
-32.792980 |
45869.33 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for V4046 Sgr |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.558 |
-0.112 |
-0.631 |
| ACIS-I |
-0.493 |
0.134 |
-0.384 |
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 |
0.708 |
0.002 |
0.913 |
0.003 |
1.117 |
0.006 |
| Q-norm |
0.053 |
0.000 |
0.080 |
0.000 |
0.106 |
0.001 |
| ACIS-I |
keV |
0.825 |
0.006 |
0.986 |
0.003 |
1.263 |
0.009 |
| Q-norm |
0.068 |
0.001 |
0.089 |
0.000 |
0.125 |
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.
| 3.3298 |
4.0456 |
0.3133 |
3.6677 |
0.7002 |
1.3671 |
0.3069 |
0.3156 |
0.1160 |
0.2057 |
0.2057 |
0.3969 |
0.1595 |
0.1748 |
| 0.2677 |
0.0740 |
0.1245 |
0.0730 |
0.4155 |
0.1054 |
0.6961 |
0.0157 |
0.8816 |
0.0246 |
3.7538 |
0.1112 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of V4046 Sgr.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
4.515 |
|
0.757 |
|
0.21 |
|
2.00847e-12 |
4.17143 |
1.13 |
72 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of V4046 Sgr. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.218 |
|
1.006 |
|
0.198 |
|
0.30 |
|
1.27059e-13 |
3.00822 |
0.87 |
59 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of V4046 Sgr. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
7.791 |
|
0.681 |
|
0.19 |
|
2.44574e-13 |
2.95739 |
1.65 |
60 |
HETG Light Curve
 |
| Odds | 13.822 |
| Prob. | 1.000 |
| Var. Index | 9 |
|
HETG light curve for V4046 Sgr, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for V4046 Sgr
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for V4046 Sgr
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR