XMM_146.png
XMM_146_E3.png
| ID210 |
ID510 |
SpuFlag |
BlendFlag |
MAIN210 |
MAIN510 |
ID |
Signif |
DET_ML |
EXPOSURE |
Offax |
nCCtparts |
nGoodCCtparts |
XCID |
Good |
angDist |
sigDist |
reliability |
FLUX |
FLUX_ERR |
FLUX28 |
FLUX28_ERR |
HFlux |
FXMM28 |
FChandra |
dCX |
zadopt |
Type |
zOABo |
zMerge |
zCheck |
RA_X |
Dec_X |
eRA_X |
RA_C |
Dec_C |
PosErr |
assocProba |
XCID |
| 146 |
1067 |
0 |
0 |
true |
true |
200 |
40.5 |
1038.8 |
1.6E03 |
8.3 |
1 |
1 |
146_200 |
true |
1.3 |
.9 |
1.000 |
1.05E-14 |
3.15E-16 |
8.72E-15 |
2.62E-16 |
1.17E-14 |
8.48E-15 |
1.13E-14 |
.1 |
.122 |
AGN |
.122 |
.122 |
false |
03:32:14 |
-27:51:00 |
1.4 |
03:32:14 |
-27:51:01 |
.1 |
1.000 |
146_200 |
Notes
- -- Mild blendingmay be with nearby XMM\#145 13arcsec to ESE ,
Finding charts contents:
- First row: XMM soft, hard and 5-10keV images
- Second row: Chandra soft, hard and total images (in XMM_*_E*.png are E-CDF-S images, otherwise 4Ms)
- Third row: MUSYC R, MUSYC K, SIMPLE 3.6um images
In all panels:
- blue square in soft XMM image: 10"x10" scale
- green circle: XMM 2-10keV position and positional error (truncated to 16arcsec if >16arcsec), source number in green in hard XMM image.
- red romboid: XMM 5-10keV position and positional error (truncated to 16arcsec if >16arcsec), source number in red in soft XMM image.
- green dashed contours in hard XMM image: 2-10sigma SNR contours in 2-10keV assuming a gaussian PSF with FWHM=8.5arcsec (Ranalli+13) and using Bayesian statistics (assuming Gauss-Poisson statistics)
- red dashed contours in 5-10keV XMM image: 2-10sigma SNR contours in 5-10keV
- cyan circle: Chandra 4Ms position and positional error, source number in cyan in soft Chandra image
- magenta square: E-CDF-S position and positional error (error circle inscribed in square), source number in magenta in soft Chandra image, only 4Ms Chandra source number shown in case of same source in Xue+11 and Lehmer+05
- cyan X: pos. of optical/NIR/MIR/VLA counterpart to 4Ms Chandra source from Xue+11
- magenta +: pos. of optical/NIR/MIR counterpart to E-CDF-S Chandra source from Silverman+10
The XMM images are shown in a local linear zscale scale, all other images with histeq scaling.