| 1887 |
2001-03-29 03:34:42 |
ER Vul |
HD 200391 |
RS CVn (partial eclipse) |
G0V+G5V |
0.5700 |
315.607960 |
27.807370 |
112012.99 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for ER Vul |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
-0.615 |
0.076 |
-0.565 |
| ACIS-I |
-0.568 |
0.259 |
-0.363 |
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 |
0.810 |
0.000 |
0.956 |
7.044 |
1.175 |
0.000 |
| Q-norm |
0.066 |
0.000 |
0.085 |
0.915 |
0.114 |
0.000 |
| ACIS-I |
keV |
0.869 |
0.000 |
1.015 |
6.985 |
1.292 |
0.000 |
| Q-norm |
0.074 |
0.000 |
0.093 |
0.907 |
0.129 |
0.000 |
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.
| 4.3875 |
2.4028 |
0.1795 |
1.7580 |
0.1360 |
0.1070 |
0.0858 |
0.0364 |
0.1272 |
0.0493 |
0.1192 |
0.0602 |
0.0159 |
0.0093 |
| 0.0079 |
0.0004 |
0.0049 |
0.0004 |
0.0140 |
0.0007 |
0.0452 |
0.0001 |
0.0456 |
0.0001 |
114.8535 |
0.3577 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of ER Vul.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
2.027 |
|
0.749 |
|
0.31 |
|
8.1561e-12 |
0.776214 |
2.41 |
282 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of ER Vul. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.078 |
|
1.150 |
|
0.495 |
|
0.28 |
|
5.43867e-14 |
0.871478 |
1.07 |
58 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of ER Vul. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.000 |
|
1.759 |
|
0.730 |
|
0.27 |
|
9.27158e-14 |
1.95743 |
1.14 |
59 |
HETG Light Curve
 |
| Odds | 26.979 |
| Prob. | 1.000 |
| Var. Index | 9 |
|
HETG light curve for ER Vul, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for ER Vul
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for ER Vul
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR