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 | 7 | X095702.82+563136.1 | chandra | ccd7 | 452.636 | 320.99 | 83.0486 | 9.24286 | 0.0307414 | 0.00342136 | 76.1013 | 1 | 1.22114 | 0.671953 | 48.0341 | 4.21328 | 43 | 14.8602 | -0.486342 | 0.16684 | F | F | 9.44e+19 | 2.4737e-13 | 1 | dsx |
| Report | 1 | X095631.51+563202.9 | chandra | ccd7 | 979.197 | 375.191 | 11.3047 | 3.36225 | 0.00418458 | 0.00124458 | 10.359 | 1 | 0.325175 | 0.325175 | 0 | 1.304 | F | F | 9.42e+19 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 6 | X095629.73+563656.1 | chandra | ccd7 | 1008.38 | 970.625 | 7.7596 | 3.95804 | 0.00287229 | 0.00146511 | 15.8262 | 1 | 1.03966 | 0.492 | 35.4956 | 3.72711 | 1.95993 | 4.83974 | 0.423521 | 0.611445 | A | F | 9.49e+19 | 2.52694e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X095635.09+563217.0 | chandra | ccd7 | 918.5 | 403.214 | 6.83061 | 3.78388 | 0.00252842 | 0.00140064 | 16.5966 | 1 | 0.492 | 0.492 | 90 | 0.991469 | 4 | -0.169387 | -1 | 1.14412 | F | F | 9.43e+19 | 1.91235e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X095706.27+563110.4 | chandra | ccd7 | 394.072 | 268.357 | 6.93428 | 3.78388 | 0.00256679 | 0.00140064 | 27.0492 | 1 | 0.634339 | 0.492 | 62.8769 | 4.82462 | 4 | 2.93428 | -0.153689 | 0.558584 | F | F | 9.44e+19 | 2.18315e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X095634.37+563205.5 | chandra | ccd7 | 930.667 | 380 | 5.66123 | 3.59808 | 0.00209556 | 0.00133186 | 9.72649 | 1 | 0.492 | 0.492 | 59.0362 | 1.18206 | 3.91531 | 0.830613 | -0.649967 | 0.86687 | F | F | 9.43e+19 | 1.59016e-14 | 1 | dx |
| Report | 1 | X095622.12+563212.4 | chandra | ccd6 | 126.5 | 630 | 3.94574 | 2 | 0.00146056 | 0.000740321 | 8.38245 | 0.999996 | 0.492 | 0.492 | 116.565 | 2.04271 | F | F | 9.42e+19 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X095556.48+562859.3 | chandra | ccd6 | 558.5 | 238.25 | 3.85675 | 3.17945 | 0.00142761 | 0.0011769 | 10.19 | 1 | 1.21069 | 0.682657 | 84.1059 | 6.79959 | 1.95225 | 1.9045 | -0.0123809 | 0.83913 | A | F | 9.37e+19 | 1.76547e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X095601.73+563202.8 | chandra | ccd6 | 469.25 | 611 | 3.8525 | 3.17945 | 0.00142604 | 0.0011769 | 10.0309 | 0.999999 | 0.564966 | 0.492 | 45.7956 | 4.71413 | 2.92625 | 0.926248 | -0.519144 | 0.946441 | F | F | 9.42e+19 | 1.63033e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X095554.51+562949.4 | chandra | ccd6 | 591.3 | 340.1 | 4.97266 | 3.39792 | 0.00184068 | 0.00125777 | 30.0729 | 1 | 1.52361 | 0.492 | 129.122 | 6.53459 | 3 | 0.972658 | -0.510324 | 0.914526 | A | F | 9.38e+19 | 2.20423e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X095604.00+563002.5 | chandra | ccd6 | 431.7 | 366.5 | 6.88091 | 3.78388 | 0.00254704 | 0.00140064 | 19.9391 | 1 | 0.700128 | 0.492 | 90 | 5.33224 | 4.94045 | 1.94045 | -0.435989 | 0.606965 | F | F | 9.39e+19 | 2.97194e-14 | 1 | dx |
| Report | 5 | X095707.70+563135.3 | chandra | ccd7 | 370.167 | 319.167 | 2.92079 | 1.73205 | 0.00108116 | 0.000641137 | 2.67645 | 0.992488 | 0.615 | 0.492 | 45 | 4.84208 | F | F | 9.44e+19 | 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