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 | 4 | X005407.36+730308.8 | chandra | ccd7 | 879.122 | 225.675 | 364.918 | 19.2402 | 0.0254924 | 0.00134408 | 321.12 | 1 | 0.556993 | 0.431792 | 35.1726 | 1.91047 | 209.803 | 158.803 | -0.138359 | 0.0554201 | F | F | 2.2e+21 | 2.71027e-13 | 1 | dsxf |
| Report | srcpi bgdpi arf rmf | 1 | X005404.04+730506.1 | chandra | ccd7 | 908.55 | 464.085 | 163.695 | 12.7943 | 0.0114354 | 0.000893788 | 144.048 | 1 | 1.93996 | 1.45098 | 25.078 | 0.0783578 | 141.183 | 54.1442 | -0.445604 | 0.0850682 | T | F | 2.2e+21 | 9.48534e-14 | 1 | dsx |
| Report | srcpi bgdpi arf rmf | 5 | X005333.16+730401.5 | chandra | ccd6 | 530.796 | 1120.03 | 117.513 | 10.8403 | 0.00821106 | 0.000757454 | 38.7086 | 1 | 0.711072 | 0.569663 | 167.661 | 2.5153 | 71 | 48.5252 | -0.188034 | 0.102157 | F | F | 2.21e+21 | 8.03271e-14 | 1 | dsxf |
| Report | srcpi bgdpi arf | 3 | X005430.91+730539.5 | chandra | ccd7 | 670.359 | 532.126 | 66.1213 | 8.36163 | 0.0046191 | 0.000584127 | 58.1853 | 1 | 0.552608 | 0.366849 | 90.3494 | 1.99952 | 21.9437 | 44.7748 | 0.342201 | 0.146475 | F | F | 2.19e+21 | 3.84774e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X005401.79+730509.5 | chandra | ccd7 | 928.543 | 471.055 | 47.7558 | 6.91056 | 0.00333612 | 0.000482758 | 42.024 | 1 | 1.50453 | 0.705828 | 359.558 | 0.237981 | 35.0512 | 25.1867 | -0.163758 | 0.150342 | T | F | 2.2e+21 | 2.76989e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 4 | X005251.30+725847.8 | chandra | ccd6 | 905.773 | 483.752 | 30.2293 | 7.60777 | 0.00211223 | 0.000531582 | 9.95749 | 1 | 2.52159 | 2.52159 | 0 | 8.23082 | 30.0686 | 22.7985 | -0.137517 | 0.163245 | F | F | 2.23e+21 | 2.58818e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X005232.61+731126.6 | chandra | ccd3 | 778.179 | 242.571 | 29.0272 | 6.72276 | 0.00202823 | 0.000469742 | 16.8355 | 1 | 3.03042 | 2.1713 | 134.322 | 9.24839 | 16.3933 | 12.6946 | -0.127157 | 0.233735 | F | F | 2.21e+21 | 2.8487e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 14 | X005422.03+730250.3 | chandra | ccd7 | 748.691 | 188.059 | 20.2828 | 4.50364 | 0.00141692 | 0.000314616 | 17.8484 | 1 | 0.550543 | 0.550543 | 0 | 2.54404 | 16 | 4.91527 | -0.529983 | 0.307918 | F | F | 2.2e+21 | 1.22129e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 11 | X005442.50+730826.0 | chandra | ccd7 | 568.46 | 870.768 | 22.1042 | 4.70151 | 0.00154416 | 0.000328439 | 19.4512 | 1 | 0.963975 | 0.963975 | 0 | 4.35762 | 14.492 | 4.15326 | -0.554496 | 0.34236 | F | F | 2.18e+21 | 1.3226e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X005310.74+730506.9 | chandra | ccd6 | 729.384 | 1253.52 | 17.0496 | 4.12912 | 0.00119131 | 0.000288515 | 5.61611 | 0.999999 | 1.26273 | 0.412404 | 0.420302 | 3.92486 | 11.917 | 5.77868 | -0.346882 | 0.320539 | A | F | 2.21e+21 | 1.34704e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 7 | X005449.28+730653.5 | chandra | ccd7 | 507.943 | 682.997 | 19.0664 | 4.37159 | 0.00133194 | 0.00030539 | 16.778 | 1 | 1.04551 | 0.418206 | 100.103 | 3.72581 | 10.7967 | 5.62727 | -0.314749 | 0.334645 | F | F | 2.18e+21 | 1.13901e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 8 | X005448.86+730750.1 | chandra | ccd7 | 512.06 | 797.91 | 13.0009 | 3.60568 | 0.000908213 | 0.000251884 | 11.4405 | 1 | 0.917589 | 0.325316 | 80.8588 | 4.24889 | 10.9099 | 0.879916 | -0.850733 | 0.512873 | F | F | 2.18e+21 | 7.77619e-15 | 1 | dsx |
| Report | srcpi bgdpi arf | 12 | X005436.60+730834.9 | chandra | ccd7 | 620.2 | 888.2 | 10.5595 | 4.42783 | 0.000737664 | 0.000309318 | 15.91 | 1 | 0.661683 | 0.492 | 87.1447 | 4.22395 | 4.93707 | 5.62243 | 0.0649043 | 0.423646 | F | F | 2.18e+21 | 6.30554e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X005356.51+730147.5 | chandra | ccd6 | 323.125 | 847 | 7.69084 | 3.95804 | 0.000537383 | 0.000276561 | 13.8319 | 1 | 0.539491 | 0.492 | 26.1122 | 3.31016 | 1.92271 | 5.76813 | 0.5 | 0.581489 | F | F | 2.21e+21 | 5.90854e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 10 | X005404.75+730525.8 | chandra | ccd7 | 901.786 | 503.643 | 6.68146 | 3.78388 | 0.000466752 | 0.000264334 | 11.8382 | 1 | 0.523422 | 0.492 | 121.409 | 0.382477 | 1.68146 | 4 | 0.40809 | 0.693069 | F | F | 2.2e+21 | 3.84616e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 13 | X005416.43+730948.5 | chandra | ccd7 | 798.643 | 1037.64 | 6.46677 | 3.78388 | 0.000451754 | 0.000264334 | 8.85583 | 1 | 0.937949 | 0.492 | 60.6031 | 4.83612 | 3.82226 | 2.68895 | -0.174055 | 0.596815 | A | F | 2.19e+21 | 3.92616e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X005405.01+730320.9 | chandra | ccd7 | 899.5 | 249.667 | 5.91531 | 3.59808 | 0.00041323 | 0.000251354 | 20.326 | 1 | 0.492 | 0.492 | 140.502 | 1.70026 | 2.91531 | 3 | 0.0143177 | 0.616388 | F | F | 2.2e+21 | 3.4851e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 9 | X005333.83+730521.5 | chandra | ccd7 | 1176 | 495.167 | 5.74592 | 3.59808 | 0.000401397 | 0.000251354 | 11.3992 | 1 | 0.492 | 0.492 | 180 | 2.26849 | 4.91531 | 0.830613 | -0.710886 | 0.77848 | F | F | 2.21e+21 | 3.41508e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X005144.96+730823.3 | chandra | ccd2 | 562.9 | 653.3 | 4.66712 | 3.39792 | 0.000326038 | 0.000237374 | 8.08917 | 0.999999 | 1.67166 | 0.505531 | 7.07774 | 10.686 | 0.974394 | 3.74394 | 0.586975 | 0.847722 | A | F | 2.23e+21 | 4.58301e-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