Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for PDS 456 |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
0.309 |
0.137 |
0.428 |
| ACIS-I |
0.359 |
0.397 |
0.662 |
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 |
1.000 |
0.007 |
1.555 |
0.007 |
2.723 |
0.014 |
| Q-norm |
0.091 |
0.001 |
0.163 |
0.001 |
0.315 |
0.002 |
| ACIS-I |
keV |
1.205 |
0.007 |
1.716 |
0.007 |
3.132 |
0.018 |
| Q-norm |
0.117 |
0.001 |
0.184 |
0.001 |
0.368 |
0.002 |
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.
| 1.4788 |
5.0240 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
| 0.0320 |
0.0023 |
0.0018 |
0.0008 |
0.0340 |
0.0024 |
0.0365 |
0.0002 |
0.0405 |
0.0002 |
9.1379 |
0.0290 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of PDS 456.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.025 |
|
36.135 |
|
1.000 |
|
0.01 |
|
3.3463e-12 |
0.00608869 |
1.04 |
355 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of PDS 456. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
6.069 |
|
1.000 |
|
0.31 |
|
9.54508e-14 |
0 |
1.08 |
75 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of PDS 456. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.038 |
|
30.000 |
|
1.000 |
|
0.32 |
|
1.21627e-13 |
0 |
1.64 |
78 |
HETG Light Curve
 |
| Odds | 1.662 |
| Prob. | 0.979 |
| Var. Index | 6 |
|
HETG light curve for PDS 456, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for PDS 456
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for PDS 456
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR