Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for SU UMA |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.035 |
0.125 |
0.091 |
| ACIS-I |
0.022 |
0.361 |
0.380 |
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 |
0.869 |
0.006 |
1.190 |
0.008 |
1.862 |
0.013 |
| Q-norm |
0.074 |
0.001 |
0.116 |
0.001 |
0.203 |
0.002 |
| ACIS-I |
keV |
0.986 |
0.007 |
1.351 |
0.009 |
2.037 |
0.025 |
| Q-norm |
0.089 |
0.001 |
0.136 |
0.001 |
0.226 |
0.003 |
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.
| 0.7055 |
0.9258 |
0.0000 |
0.0000 |
0.0832 |
0.2799 |
0.7130 |
1.3307 |
0.3576 |
0.8703 |
1.1653 |
2.4882 |
0.2447 |
1.8446 |
| 0.2579 |
0.0632 |
0.0257 |
0.3625 |
0.2862 |
0.3679 |
0.2279 |
0.0036 |
0.3129 |
0.0063 |
2.6815 |
0.0525 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of SU UMA.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
7.706 |
|
0.707 |
|
0.96 |
|
3.6487e-12 |
0 |
1.17 |
92 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of SU UMA. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
18.285 |
|
0.663 |
|
0.28 |
|
4.56289e-13 |
0.205227 |
1.03 |
75 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of SU UMA. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.010 |
|
7.473 |
|
0.787 |
|
0.95 |
|
6.49186e-13 |
0.134862 |
1.33 |
75 |
HETG Light Curve
 |
| Odds | -1.522 |
| Prob. | 0.029 |
| Var. Index | 0 |
|
HETG light curve for SU UMA, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for SU UMA
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for SU UMA
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR