Observation details report
Detailed source parameters (including errors) in a comma-separated values file
Click on source number for detailed analysis, including spectral fits if applicable
| data | idnum | idradec | telescope | instrument | x | y | cnts | cntserr | rate | rateerr | SNR | poisprob | sigmaj | sigmin | incang | offax | cnts_soft | cnts_hard | hr | hr_err | ext | var | N_H | flux | vign | flags | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Report | srcpi bgdpi arf | 9 | X051408.36+005632.6 | chandra | ccd7 | 536.21 | 476.084 | 41.1469 | 6.43124 | 0.00518864 | 0.000810981 | 34.2788 | 1 | 0.40224 | 0.40224 | 0 | 0.341076 | F | F | 8.73e+20 | 3.88677e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X051423.29+005451.1 | chandra | ccd6 | 691.21 | 1093.75 | 18.539 | 4.30569 | 0.00233778 | 0.000542951 | 21.2536 | 1 | 0.941963 | 0.941963 | 0 | 3.75795 | F | F | 8.93e+20 | 2.44749e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X051359.71+005817.4 | chandra | ccd7 | 800.063 | 689.142 | 14.8788 | 4.12923 | 0.00187622 | 0.000520698 | 12.3953 | 1 | 0.661763 | 0.29055 | 348.069 | 3.10209 | F | F | 8.62e+20 | 1.46993e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X051423.04+005831.2 | chandra | ccd7 | 88.6492 | 717.165 | 15.6984 | 4.05947 | 0.00197958 | 0.000511901 | 13.0781 | 1 | 0.742381 | 0.742381 | 0 | 3.93792 | F | F | 8.91e+20 | 1.71947e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X051325.18+005749.2 | chandra | ccd3 | 641.564 | 1257.76 | 14.148 | 5.61037 | 0.00178688 | 0.000708583 | 3.39874 | 0.998989 | 3.55676 | 3.55676 | 0 | 11.2046 | F | F | 8.36e+20 | 2.66265e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X051354.80+010117.2 | chandra | ccd7 | 949.045 | 1054.05 | 9.25075 | 3.31666 | 0.00116652 | 0.00041823 | 7.70664 | 1 | 0.932898 | 0.795675 | 106.694 | 6.10658 | F | F | 8.59e+20 | 9.77327e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X051407.44+010227.0 | chandra | ccd7 | 563.7 | 1195.9 | 8.32123 | 3.16231 | 0.00104931 | 0.000398767 | 6.93228 | 0.999997 | 1.46471 | 0.704387 | 41.8717 | 6.03536 | A | F | 8.68e+20 | 8.90278e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X051406.10+005832.6 | chandra | ccd7 | 604.643 | 719.5 | 6.67148 | 2.64576 | 0.000841273 | 0.00033363 | 5.5579 | 0.99998 | 0.492 | 0.492 | 171.87 | 2.28419 | F | F | 8.69e+20 | 6.45696e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X051403.55+005540.6 | chandra | ccd7 | 682.5 | 369.833 | 5.64064 | 2.4495 | 0.000711284 | 0.000308882 | 4.69912 | 0.999871 | 0.575665 | 0.492 | 72.3912 | 1.7095 | F | F | 8.67e+20 | 5.36683e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X051421.88+005828.3 | chandra | ccd7 | 123.5 | 710.7 | 4.80334 | 2.23607 | 0.000605701 | 0.000281969 | 4.00158 | 0.999265 | 0.526281 | 0.492 | 28.4881 | 3.66817 | F | F | 8.89e+20 | 5.08538e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X051432.27+005310.9 | chandra | ccd6 | 416.9 | 889.5 | 4.47695 | 2.23608 | 0.000564544 | 0.00028197 | 5.1325 | 0.999859 | 0.993655 | 0.492 | 94.8912 | 6.52333 | A | F | 9.05e+20 | 6.28262e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X051352.96+005804.9 | chandra | ccd7 | 1005.25 | 663.25 | 3.7662 | 2.00001 | 0.000474917 | 0.000252201 | 3.13756 | 0.996323 | 0.492 | 0.492 | 18.4349 | 4.4871 | F | F | 8.56e+20 | 3.85879e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X051435.03+005429.6 | chandra | ccd6 | 332.75 | 1049.5 | 3.64972 | 2.00002 | 0.00046023 | 0.000252202 | 4.18414 | 0.998866 | 0.747485 | 0.492 | 78.3074 | 6.63299 | A | F | 9.08e+20 | 9.45314e-15 | 1 | dx | ||||
| Report | 4 | X051426.61+005712.9 | chandra | ccd6 | 589.5 | 1381.5 | 2.94017 | 1.73205 | 0.000370755 | 0.000218412 | 3.37069 | 0.992341 | 0.492 | 0.492 | 90 | 4.30561 | F | F | 8.96e+20 | 0 | 1 | d |
counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 7.99 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), T = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters,
b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters,
i = psf spatial fitting parameters, f = spectral fitting parameters,
c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest