XMM_299.png

XMM_299_E1.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

299

1147

0

2

false

false

606

6.7

-1.0

1.56E03

3.0

1

1

299_606

true

.5

.2

.997

7.78E-16

1.18E-16

6.46E-16

9.8E-17

2.69E-15

6.28E-16

2.61E-15

.4

.733

AGN

.733

.733

false

03:32:46

-27:42:14

2.3

03:32:46

-27:42:13

.2

.997

299_606

Notes

• -- Shares SNR=6 hard contours with XMM\#292 35arcsec to SE and SNR=5 with XMM\#308 40arcsec to NE. Prob. blend ,

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.