| 601 |
2001-01-03 02:25:32 |
TY Pyx |
HD 77137 |
Eclipsing variable of RS CVn type |
G5IV+G5IV |
0.6640 |
134.928070 |
-27.816330 |
49126.75 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for TY Pyx |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.531 |
0.116 |
-0.442 |
| ACIS-I |
-0.478 |
0.304 |
-0.203 |
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 |
0.825 |
0.000 |
0.986 |
7.015 |
1.248 |
0.002 |
| Q-norm |
0.068 |
0.000 |
0.089 |
0.911 |
0.123 |
0.000 |
| ACIS-I |
keV |
0.883 |
7.117 |
1.044 |
0.000 |
1.380 |
0.007 |
| Q-norm |
0.076 |
0.924 |
0.097 |
0.000 |
0.140 |
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.
| 3.6036 |
2.5072 |
1.1650 |
3.9529 |
0.0882 |
0.1247 |
0.1734 |
0.0979 |
0.2735 |
0.1363 |
0.1667 |
0.0736 |
0.0943 |
0.0421 |
| 0.0150 |
0.0010 |
0.0085 |
0.0010 |
0.0256 |
0.0017 |
0.0562 |
0.0001 |
0.0571 |
0.0001 |
59.5246 |
0.2272 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of TY Pyx.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.001 |
|
2.694 |
|
0.826 |
|
0.45 |
|
9.16626e-12 |
0.461617 |
1.51 |
250 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of TY Pyx. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.052 |
|
1.477 |
|
0.649 |
|
0.31 |
|
1.26693e-13 |
1.1903 |
0.93 |
59 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of TY Pyx. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
1.029 |
|
1.000 |
|
0.14 |
|
2.05411e-13 |
0 |
2.02 |
61 |
HETG Light Curve
 |
| Odds | 50.257 |
| Prob. | 1.000 |
| Var. Index | 10 |
|
HETG light curve for TY Pyx, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for TY Pyx
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for TY Pyx
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR