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 | X195437.91+282912.2 | chandra | ccd0 | 385.091 | 502.115 | 110.73 | 11.2006 | 0.0112516 | 0.00113813 | 40.8098 | 1 | 4.20272 | 2.61127 | 81.104 | 8.65717 | 81.527 | 33.7379 | -0.414603 | 0.112274 | F | F | 9.97e+21 | 1.71716e-13 | 1 | dsxf |
Report | srcpi bgdpi arf | 3 | X195402.85+283450.2 | chandra | ccd1 | 414.024 | 739.229 | 37.6865 | 6.44189 | 0.00382941 | 0.000654575 | 19.3036 | 1 | 0.931634 | 0.493932 | 63.125 | 4.33574 | 26.8653 | 12.9102 | -0.350847 | 0.197246 | F | F | 1.02e+22 | 5.88758e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X195452.58+283518.0 | chandra | ccd2 | 461.674 | 320.898 | 44.0178 | 6.64768 | 0.00447273 | 0.000675483 | 56.1428 | 1 | 3.89994 | 1.94453 | 116.238 | 7.29339 | 32.9423 | 8.1385 | -0.603781 | 0.219184 | F | F | 1.01e+22 | 7.51201e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 4 | X195434.33+283836.5 | chandra | ccd2 | 950.598 | 724.135 | 26.2865 | 5.12704 | 0.00267102 | 0.000520968 | 33.5273 | 1 | 0.635107 | 0.635107 | 0 | 3.53502 | 19.9152 | 6.91523 | -0.484524 | 0.260566 | F | F | 1.03e+22 | 4.26781e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X195527.83+284820.0 | chandra | ccd6 | 310.305 | 792.671 | 37.2143 | 8.19375 | 0.00378136 | 0.000832569 | 10.0229 | 1 | 4.81948 | 4.58864 | 73.5746 | 18.717 | 23.3241 | 13.2126 | -0.276749 | 0.231204 | F | F | 1.02e+22 | 8.86531e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X195424.31+284251.3 | chandra | ccd3 | 286.741 | 783.934 | 19.4218 | 4.40702 | 0.00197348 | 0.000447805 | 24.6069 | 1 | 1.27806 | 1.27806 | 0 | 5.99525 | 11.8306 | 6.98382 | -0.257611 | 0.306405 | F | F | 1.04e+22 | 3.4202e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 3 | X195428.90+284250.0 | chandra | ccd3 | 163.567 | 780.7 | 14.5273 | 4.96863 | 0.00147613 | 0.000504868 | 21.1285 | 1 | 1.08425 | 0.672523 | 33.7343 | 6.21201 | 3.84242 | 10.6848 | 0.471006 | 0.380448 | A | F | 1.04e+22 | 2.57366e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X195408.04+284647.5 | chandra | ccd3 | 721 | 1263.5 | 5.63792 | 3.59808 | 0.000572876 | 0.000365605 | 9.36953 | 1 | 1.37082 | 0.651338 | 27.1013 | 10.2201 | 0.879307 | 4.79885 | 0.690284 | 0.780181 | A | F | 1.05e+22 | 1.66429e-14 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X195432.05+283910.7 | chandra | ccd2 | 1011.17 | 793.056 | 8.83127 | 4.1225 | 0.000897359 | 0.000418894 | 21.4991 | 1 | 0.742179 | 0.492 | 35.7825 | 3.44667 | 7.88751 | 0.943755 | -0.78627 | 0.599552 | A | F | 1.03e+22 | 1.40637e-14 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X195405.28+283917.4 | chandra | ccd3 | 795.214 | 348.786 | 6.83061 | 3.78388 | 0.000694066 | 0.000384485 | 16.5966 | 1 | 0.492 | 0.492 | 147.152 | 4.03363 | 7 | -0.169387 | -1 | 0.773459 | F | F | 1.04e+22 | 1.05666e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X195355.42+283358.4 | chandra | ccd1 | 612.5 | 633.5 | 8.91531 | 4.1225 | 0.000905902 | 0.000418895 | 30.6346 | 1 | 0.492 | 0.492 | 31.7175 | 6.18079 | 0 | 8.91531 | 1 | 0.660252 | F | F | 1.02e+22 | 1.50059e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X195440.30+283756.0 | chandra | ccd2 | 790.167 | 641.333 | 5.84795 | 3.59808 | 0.000594219 | 0.000365606 | 14.9972 | 1 | 0.8218 | 0.492 | 57.002 | 4.5327 | 2.94932 | 2.89863 | -0.00866681 | 0.623447 | A | F | 1.02e+22 | 9.59782e-15 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X195425.74+283258.7 | chandra | ccd0 | 710.7 | 961.9 | 4.92965 | 3.39792 | 0.000500914 | 0.00034527 | 18.5863 | 1 | 0.592292 | 0.492 | 36.0906 | 4.13062 | 2 | 2.92965 | 0.188584 | 0.712077 | F | F | 1.01e+22 | 7.95892e-15 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X195427.57+283313.3 | chandra | ccd0 | 661.643 | 991.643 | 6.84032 | 3.78388 | 0.000695061 | 0.000384489 | 17.1177 | 1 | 0.521845 | 0.492 | 68.1986 | 4.04277 | 1.92016 | 4.92016 | 0.438576 | 0.611147 | F | F | 1.01e+22 | 1.06192e-14 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X195422.15+283328.5 | chandra | ccd0 | 806.786 | 1022.5 | 6.83061 | 3.78388 | 0.000694075 | 0.000384489 | 16.5966 | 1 | 0.492 | 0.492 | 77.4916 | 3.4756 | 5.83061 | 1 | -0.707201 | 0.686476 | F | F | 1.02e+22 | 1.09948e-14 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X195411.23+283109.1 | chandra | ccd0 | 1099.5 | 739.25 | 7.73353 | 3.95804 | 0.000785823 | 0.000402186 | 14.9815 | 1 | 1.25056 | 0.492 | 167.127 | 6.09577 | 3.93338 | 2.80015 | -0.168297 | 0.576557 | A | F | 1.01e+22 | 1.24207e-14 | 1 | dx |
Report | 6 | X195425.10+283310.3 | chandra | ccd0 | 728.313 | 986.063 | 14.6743 | 3.8307 | 0.0014911 | 0.000389249 | 5.40825 | 0.999997 | 0.639998 | 0.639998 | 0 | 3.90438 | F | F | 1.01e+22 | 0 | 1 | ds | |||||
Report | 1 | X195411.95+283555.0 | chandra | ccd1 | 170 | 870.25 | 3.91105 | 2 | 0.000397409 | 0.000203224 | 2.00329 | 0.959305 | 0.492 | 0.492 | 60.1282 | 2.06581 | F | F | 1.03e+22 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 6 | X195451.64+283554.8 | chandra | ccd2 | 486.5 | 395.25 | 3.91531 | 3.17945 | 0.00039784 | 0.000323069 | 13.4537 | 1 | 0.492 | 0.492 | 55.278 | 6.98144 | 3.91531 | 0 | -1 | 1.16887 | F | F | 1.01e+22 | 6.64342e-15 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X195423.70+283735.0 | chandra | ccd2 | 1234.5 | 598.5 | 3.91531 | 3.17945 | 0.00039784 | 0.000323069 | 13.4537 | 1 | 0.492 | 0.492 | 90 | 1.01794 | 1 | 2.91531 | 0.489184 | 0.920111 | F | F | 1.03e+22 | 6.06271e-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