| 5423 |
2005-08-06 19:42:58 |
V4046 Sgr |
HD 319139 |
Classical T Tauri-type Star |
K5 |
0.9000 |
273.543670 |
-32.792990 |
97729.02 |
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 |
-0.598 |
-0.094 |
-0.655 |
| ACIS-I |
-0.535 |
0.129 |
-0.435 |
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 |
0.000 |
0.913 |
0.000 |
1.088 |
0.006 |
| Q-norm |
0.053 |
0.000 |
0.080 |
0.000 |
0.102 |
0.001 |
| ACIS-I |
keV |
0.840 |
0.003 |
0.971 |
0.000 |
1.248 |
0.007 |
| Q-norm |
0.070 |
0.000 |
0.087 |
0.000 |
0.123 |
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.
| 2.7545 |
2.9665 |
4.1245 |
13.6529 |
0.1635 |
0.2659 |
0.7335 |
0.6815 |
0.3590 |
0.5087 |
0.2224 |
0.2795 |
0.0617 |
0.3423 |
| 0.1507 |
0.0321 |
0.1040 |
0.0259 |
0.2789 |
0.0443 |
0.4398 |
0.0046 |
0.4996 |
0.0057 |
7.3589 |
0.1018 |
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 |
|
8.952 |
|
0.750 |
|
0.26 |
|
1.7056e-12 |
6.65103 |
1.79 |
100 |

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) |
0.123 |
|
0.939 |
|
0.224 |
|
0.26 |
|
6.2315e-14 |
1.29603 |
1.39 |
58 |

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 |
|
0.975 |
|
0.252 |
|
0.27 |
|
1.12992e-13 |
0.51939 |
1.43 |
59 |
HETG Light Curve
 |
| Odds | 2.176 |
| Prob. | 0.993 |
| Var. Index | 7 |
|
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