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 |
-0.019 |
0.231 |
0.213 |
| ACIS-I |
0.045 |
0.447 |
0.482 |
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 |
0.913 |
0.002 |
1.234 |
0.007 |
1.920 |
0.009 |
| Q-norm |
0.080 |
0.000 |
0.121 |
0.001 |
0.210 |
0.001 |
| ACIS-I |
keV |
1.015 |
0.004 |
1.394 |
0.007 |
2.154 |
0.023 |
| Q-norm |
0.093 |
0.000 |
0.142 |
0.001 |
0.241 |
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.
| 0.7219 |
0.7212 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.3776 |
0.2615 |
0.1941 |
0.1664 |
0.3776 |
0.1926 |
0.0744 |
0.1136 |
| 0.0500 |
0.0057 |
0.0075 |
0.0029 |
0.0581 |
0.0064 |
0.0723 |
0.0004 |
0.0808 |
0.0004 |
8.5379 |
0.0396 |
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) |
0.013 |
|
8.623 |
|
0.793 |
|
0.99 |
|
5.10857e-12 |
0 |
1.17 |
223 |

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 |
|
30.000 |
|
1.090 |
|
0.31 |
|
2.2953e-13 |
0.17513 |
1.06 |
72 |

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 |
|
12.913 |
|
0.848 |
|
1.50 |
|
3.08051e-13 |
0.106653 |
1.20 |
72 |
HETG Light Curve
 |
| Odds | 29.939 |
| Prob. | 1.000 |
| Var. Index | 9 |
|
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