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 rmf | 1 | X202208.46+100111.6 | chandra | ccd7 | 975.172 | 562.296 | 1660.33 | 42.7577 | 0.139292 | 0.00358712 | 338.142 | 1 | 0.343104 | 0.315912 | 68.6249 | 0.174131 | 932.395 | 751.049 | -0.107723 | 0.025166 | F | F | 1.06e+21 | 1.54658e-12 | 1 | dsxf |
| Report | srcpi bgdpi arf rmf | 14 | X202223.49+095916.7 | chandra | ccd7 | 523.887 | 328.889 | 175.24 | 13.786 | 0.0147016 | 0.00115656 | 35.6893 | 1 | 1.19147 | 0.492988 | 55.3385 | 4.12243 | 140.825 | 27.7197 | -0.67107 | 0.100308 | A | F | 1.03e+21 | 1.44442e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X202225.39+095922.6 | chandra | ccd7 | 466.883 | 340.795 | 42.762 | 6.53927 | 0.00358748 | 0.000548606 | 8.70888 | 1 | 1.35243 | 0.704039 | 51.1707 | 4.51402 | 31.7796 | 9.33884 | -0.545759 | 0.209387 | F | F | 1.03e+21 | 3.15252e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 12 | X202215.84+100611.6 | chandra | ccd7 | 753.51 | 1172.14 | 18.468 | 5.1394 | 0.00154936 | 0.000431165 | 3.76118 | 0.999673 | 1.21628 | 0.370369 | 96.9143 | 5.50049 | 10.9227 | 7.79375 | -0.167175 | 0.296429 | F | T | 1.06e+21 | 1.4004e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X202154.51+101252.6 | chandra | ccd3 | 940.227 | 667.591 | 30.0213 | 7.46142 | 0.00251861 | 0.000625969 | 9.06052 | 1 | 5.83077 | 4.27127 | 122.677 | 12.3309 | 18.9607 | 11.3087 | -0.252797 | 0.254913 | F | F | 1.12e+21 | 3.46992e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X202135.56+100941.6 | chandra | ccd2 | 582.495 | 726.2 | 23.3996 | 8.08518 | 0.00196309 | 0.000678299 | 3.6119 | 0.999634 | 7.30881 | 1.57974 | 327.982 | 11.8986 | 11.5359 | 8.81566 | -0.133664 | 0.302348 | A | F | 1.13e+21 | 2.70876e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X202222.64+100004.4 | chandra | ccd7 | 549.461 | 425.692 | 16.5437 | 4.33233 | 0.00138792 | 0.000363457 | 3.36928 | 0.998928 | 0.767127 | 0.276694 | 65.0283 | 3.65252 | 12.9084 | 1.9084 | -0.7424 | 0.420285 | F | F | 1.03e+21 | 1.16817e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X202137.02+100607.9 | chandra | ccd2 | 538.4 | 291.2 | 17.7356 | 5.66369 | 0.00148791 | 0.00047515 | 9.81626 | 1 | 3.38834 | 2.14153 | 61.5281 | 9.24403 | 5.35783 | 11.5383 | 0.365794 | 0.351816 | A | F | 1.12e+21 | 2.07896e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 6 | X202216.98+100518.6 | chandra | ccd7 | 719.446 | 1064.28 | 19.7442 | 4.44344 | 0.00165642 | 0.000372779 | 4.02109 | 0.999825 | 1.3449 | 0.510425 | 94.5431 | 4.77769 | 7.80719 | 11.5822 | 0.194697 | 0.293325 | F | T | 1.06e+21 | 1.37684e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 7 | X202231.53+100110.5 | chandra | ccd7 | 281.967 | 559.767 | 17.3433 | 5.33013 | 0.001455 | 0.000447166 | 21.4015 | 1 | 0.930058 | 0.65577 | 85.033 | 5.71775 | 10.7612 | 6.70149 | -0.232479 | 0.315061 | F | F | 1.02e+21 | 1.21362e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X202214.53+100103.4 | chandra | ccd7 | 792.838 | 545.603 | 14.7919 | 3.84602 | 0.00124095 | 0.000322659 | 3.01251 | 0.99679 | 0.222599 | 0.222599 | 0 | 1.53085 | 12.9155 | 1 | -0.856275 | 0.461022 | F | F | 1.05e+21 | 9.61363e-15 | 1 | dsx |
| Report | srcpi bgdpi arf | 5 | X202202.94+095943.6 | chandra | ccd6 | 196.713 | 802.405 | 12.5759 | 3.54647 | 0.00105532 | 0.000297606 | 6.13695 | 0.999998 | 0.284858 | 0.284858 | 0 | 1.85152 | 2 | 10.9152 | 0.690287 | 0.446114 | F | F | 1.06e+21 | 1.62287e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 10 | X202157.12+100407.7 | chandra | ccd7 | 1315.33 | 920.332 | 17.8386 | 4.22358 | 0.00149655 | 0.000354334 | 3.633 | 0.999401 | 1.26494 | 0.696597 | 311.825 | 4.16413 | 9.67362 | 7.76687 | -0.109329 | 0.309099 | F | F | 1.09e+21 | 1.43017e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X202149.42+095932.6 | chandra | ccd6 | 602.893 | 780.11 | 7.82152 | 4.02722 | 0.000656353 | 0.000337949 | 3.81684 | 0.99957 | 0.618955 | 0.618955 | 0 | 4.87872 | 4.66098 | 5.74574 | 0.104236 | 0.431288 | F | F | 1.08e+21 | 7.24073e-15 | 1 | dsx |
| Report | srcpi bgdpi arf | 11 | X202219.67+100431.3 | chandra | ccd7 | 638 | 967.8 | 9.61932 | 4.27872 | 0.000807004 | 0.000358959 | 15.5907 | 1 | 0.98498 | 0.492 | 70.7651 | 4.47963 | 5 | 4.70392 | -0.0305117 | 0.44504 | A | T | 1.05e+21 | 6.47331e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X202151.57+101120.4 | chandra | ccd3 | 1028.5 | 480.318 | 9.38626 | 4.42783 | 0.000787451 | 0.000371468 | 7.38882 | 1 | 2.4236 | 1.35858 | 121.904 | 11.1105 | 8.0982 | 1.33552 | -0.716863 | 0.582235 | A | F | 1.12e+21 | 1.15317e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X202156.74+100158.9 | chandra | ccd6 | 382.5 | 1077 | 7.93536 | 3.95804 | 0.000665903 | 0.000332142 | 31.2113 | 1 | 0.644454 | 0.492 | 26.0625 | 3.00668 | 5 | 2.93536 | -0.260182 | 0.520855 | F | F | 1.08e+21 | 7.08525e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X202152.02+100314.8 | chandra | ccd6 | 524.1 | 1231.3 | 4.87932 | 3.39792 | 0.000409452 | 0.000285139 | 14.0456 | 1 | 0.690278 | 0.492 | 58.2825 | 4.5863 | 2.93966 | 1.93966 | -0.204947 | 0.721656 | F | F | 1.09e+21 | 4.79724e-15 | 1 | dx |
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