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 | 2 | X083827.10+305215.1 | chandra | ccd1 | 1106.72 | 526.998 | 34.1692 | 5.84544 | 0.00697352 | 0.00119298 | 57.6098 | 1 | 0.71762 | 0.460244 | 351.183 | 3.87477 | F | F | 3.8e+20 | 8.2475e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X083745.53+305547.9 | chandra | ccd2 | 843.5 | 352.562 | 15.0461 | 4.00001 | 0.00307065 | 0.000816335 | 25.1021 | 1 | 1.30193 | 1.17327 | 85.3868 | 6.67439 | F | F | 3.76e+20 | 4.30115e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X083817.59+305453.4 | chandra | ccd3 | 390.125 | 1199.25 | 7.88707 | 2.82843 | 0.0016096 | 0.00057723 | 13.4171 | 1 | 0.52985 | 0.492 | 72.9839 | 0.556579 | F | F | 3.77e+20 | 1.84339e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X083843.84+305610.4 | chandra | ccd1 | 668.667 | 1005.17 | 5.80149 | 2.44949 | 0.001184 | 0.000499905 | 9.78141 | 1 | 0.914803 | 0.506168 | 23.4238 | 5.89195 | A | F | 3.81e+20 | 1.4752e-14 | 1 | dx | ||||
| Report | 6 | X083851.31+304928.8 | chandra | ccd1 | 472.167 | 189 | 5.77913 | 2.4495 | 0.00117943 | 0.000499905 | 9.74371 | 1 | 0.492 | 0.492 | 120.779 | 9.51787 | F | F | 3.83e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X083754.05+305828.0 | chandra | ccd2 | 620.5 | 677.75 | 4.93837 | 2.23607 | 0.00100784 | 0.000456344 | 8.23892 | 0.999998 | 0.492 | 0.492 | 124.722 | 5.72357 | F | F | 3.76e+20 | 1.40773e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X083826.12+305530.1 | chandra | ccd1 | 1132.1 | 922.9 | 4.9252 | 2.23607 | 0.00100516 | 0.000456348 | 8.30398 | 0.999998 | 0.492 | 0.492 | 115.097 | 2.04331 | F | F | 3.79e+20 | 1.14805e-14 | 1 | dx | ||||
| Report | 2 | X083749.83+305208.2 | chandra | ccd3 | 1116.5 | 863.9 | 4.67877 | 2.23608 | 0.00095485 | 0.000456342 | 7.9593 | 0.999998 | 0.492 | 0.492 | 180 | 6.6069 | F | F | 3.76e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X083823.51+310420.6 | chandra | ccd0 | 847.7 | 1047.1 | 4.34113 | 2.23608 | 0.000885967 | 0.000456354 | 7.46818 | 0.999972 | 1.78441 | 0.59671 | 158.358 | 9.06026 | A | F | 3.78e+20 | 1.30761e-14 | 1 | dx | ||||
| Report | 4 | X083804.37+305719.0 | chandra | ccd2 | 350.75 | 537.25 | 3.95111 | 2 | 0.000806355 | 0.000408166 | 6.59183 | 0.999963 | 0.492 | 0.492 | 90 | 3.24544 | F | F | 3.76e+20 | 0 | 1 | d | |||||
| Report | 5 | X083754.13+304906.4 | chandra | ccd3 | 1004.25 | 494.25 | 3.90522 | 2 | 0.000796982 | 0.000408163 | 6.64336 | 0.999969 | 0.492 | 0.492 | 45 | 7.93105 | F | F | 3.77e+20 | 0 | 1 | d | |||||
| Report | 3 | X083805.66+305345.2 | chandra | ccd3 | 702.25 | 1060.75 | 3.90125 | 2 | 0.000796173 | 0.000408163 | 6.63662 | 0.999969 | 0.513971 | 0.492 | 24.1832 | 2.8693 | F | F | 3.77e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X083820.52+304723.6 | chandra | ccd3 | 313.25 | 285 | 3.82614 | 2.00001 | 0.000780843 | 0.000408164 | 6.50884 | 0.999969 | 1.13801 | 0.731168 | 29.1332 | 8.05558 | A | F | 3.81e+20 | 1.07658e-14 | 1 | dx | ||||
| Report | 3 | X083756.99+310158.9 | chandra | ccd2 | 543.25 | 1106.25 | 3.82328 | 2.00001 | 0.000780267 | 0.000408167 | 6.37856 | 0.999963 | 0.884831 | 0.537905 | 156.801 | 7.80511 | A | F | 3.77e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X083852.37+305419.5 | chandra | ccd1 | 445.25 | 780 | 3.8018 | 2.00001 | 0.000775889 | 0.000408171 | 6.40989 | 0.999966 | 0.774901 | 0.492 | 143.045 | 7.74798 | A | F | 3.82e+20 | 1.07247e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X083753.26+305540.5 | chandra | ccd2 | 641.5 | 337.167 | 2.96959 | 1.73205 | 0.000606043 | 0.000353482 | 4.9543 | 0.999478 | 0.492 | 0.492 | 90 | 5.01348 | F | F | 3.76e+20 | 7.99259e-15 | 1 | dx | ||||
| Report | 3 | X083838.43+304952.0 | chandra | ccd1 | 809.5 | 235.833 | 2.90276 | 1.73205 | 0.00059241 | 0.000353486 | 4.89411 | 0.999518 | 0.492 | 0.492 | 90 | 7.25347 | F | F | 3.82e+20 | 0 | 1 | d | |||||
| Report | 2 | X083836.48+305952.6 | chandra | ccd0 | 508.5 | 502.5 | 2.81146 | 1.73206 | 0.00057378 | 0.000353489 | 4.83663 | 0.999585 | 0.492 | 0.492 | 180 | 6.177 | F | F | 3.79e+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