| 3015 |
2001-12-21 10:59:59 |
3C 120 |
4C 05.20 |
Seyfert 1 Galaxy |
S0 D ~ |
0.6200 |
68.296220 |
5.354320 |
57215.63 |
Chandra Configuration for the Observation
Zeroth-Order Image
 | |
| The zeroth-order image for 3C 120 |
Hardness Ratios and Quantiles
Hardness ratios and quantiles are calculated from the predicted ACIS-S or ACIS-I aimpoint spectra, as indicated.
| ACIS-S |
0.096 |
0.258 |
0.346 |
| ACIS-I |
0.148 |
0.486 |
0.592 |
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 |
0.971 |
0.000 |
1.380 |
0.001 |
2.066 |
0.004 |
| Q-norm |
0.087 |
0.000 |
0.140 |
0.000 |
0.229 |
0.000 |
| ACIS-I |
keV |
1.117 |
0.003 |
1.511 |
0.007 |
2.416 |
0.008 |
| Q-norm |
0.106 |
0.000 |
0.157 |
0.001 |
0.275 |
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.
| 0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
0.0000 |
8.6717 |
38.0952 |
47.3944 |
208.3303 |
2.5568 |
11.2334 |
| 0.0014 |
0.0000 |
0.0000 |
0.0000 |
0.0014 |
0.0000 |
0.0060 |
0.0000 |
0.0061 |
0.0000 |
83.6670 |
0.0620 |
Spectral Fits

Mewe-Kaastra-Liedahl 2-temperature fit of the low-resolution zeroth-order spectrum of 3C 120.
Warning: The zeroth-order spectrum may be subject to distortions from pileup.
| zeroth-order |
xswabs*(xsmekal1+xsmekal2) |
0.102 |
|
50.000 |
|
0.579 |
|
1.50 |
|
1.36049e-11 |
0.0435006 |
2.41 |
472 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-S Aimpoint spectrum of 3C 120. The predicted spectrum was scaled to 1500 counts.
| ACIS-S |
xswabs*(xsmekal1+xsmekal2) |
0.069 |
|
29.993 |
|
1.658 |
|
0.18 |
|
1.94823e-13 |
0.374061 |
1.31 |
69 |

Mewe-Kaastra-Liedahl 2-temperature fit of the predicted low-resolution ACIS-I Aimpoint spectrum of 3C 120. The predicted spectrum was scaled to 1500 counts.
| ACIS-I |
xswabs*(xsmekal1+xsmekal2) |
0.022 |
|
9.010 |
|
1.354 |
|
0.39 |
|
2.77233e-13 |
0.0609623 |
0.85 |
75 |
HETG Light Curve
 |
| Odds | 29.171 |
| Prob. | 1.000 |
| Var. Index | 9 |
|
HETG light curve for 3C 120, constructed from all ±1st, ±2nd, and ±3rd order HETG events.
HETG HEG Spectrum
High-Resolution 1st Order HEG Spectrum for 3C 120
HETG MEG Spectrum
High-Resolution 1st Order MEG Spectrum for 3C 120
X-Atlas Data Products
Retrieve observation data from the Chandra Data Archive:
WebChaSeR