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 | X040924.88+075856.4 | chandra | ccd7 | 548.9 | 442.537 | 286.513 | 17.2209 | 0.0868627 | 0.00522091 | 90.3862 | 1 | 0.470918 | 0.385058 | 342.775 | 0.578047 | F | F | 9.53e+20 | 7.65814e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X040947.60+074805.4 | chandra | ccd5 | 727.108 | 1049.01 | 53.9589 | 8.88841 | 0.0163586 | 0.00269469 | 69.0619 | 1 | 8.017 | 4.65237 | 142.726 | 11.6575 | A | F | 9.35e+20 | 1.44346e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X040858.80+074815.6 | chandra | ccd2 | 436.917 | 471.833 | 10.2837 | 3.46414 | 0.00311768 | 0.00105022 | 25.122 | 1 | 4.75229 | 3.70107 | 48.0694 | 12.0868 | F | F | 9.43e+20 | 4.15275e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X040939.70+075357.1 | chandra | ccd6 | 514.625 | 806.875 | 7.87001 | 2.82843 | 0.00238594 | 0.000857491 | 17.6267 | 1 | 0.79807 | 0.492 | 163.089 | 5.65799 | A | F | 9.43e+20 | 2.45495e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X040936.57+075337.6 | chandra | ccd6 | 609.357 | 767.072 | 6.85229 | 2.64575 | 0.0020774 | 0.000802109 | 15.3473 | 1 | 0.596489 | 0.492 | 55.1413 | 5.49034 | F | F | 9.43e+20 | 2.12844e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X040929.05+080503.6 | chandra | ccd7 | 422.5 | 1188.36 | 6.43779 | 2.64576 | 0.00195173 | 0.000802112 | 2.03093 | 0.9719 | 1.07468 | 0.898271 | 80.2039 | 6.73566 | F | F | 9.61e+20 | 1.5988e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X040901.50+074924.4 | chandra | ccd2 | 355.357 | 611.5 | 6.0829 | 2.64577 | 0.00184414 | 0.000802115 | 14.86 | 1 | 1.48227 | 0.787758 | 29.8645 | 10.7624 | A | F | 9.44e+20 | 2.39614e-14 | 1 | dx | ||||
| Report | 1 | X040846.87+080201.7 | chandra | ccd3 | 394.9 | 1222.9 | 4.74878 | 2.23608 | 0.00143968 | 0.000677907 | 11.3622 | 0.999999 | 0.492 | 0.492 | 100.901 | 10.2328 | F | F | 9.61e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X040930.01+074941.8 | chandra | ccd6 | 807.3 | 287.9 | 4.6407 | 2.23608 | 0.00140691 | 0.000677909 | 10.3939 | 0.999998 | 1.66064 | 0.492 | 115.083 | 8.75666 | A | F | 9.4e+20 | 1.57656e-14 | 1 | dx | ||||
| Report | 6 | X040935.28+075239.6 | chandra | ccd6 | 648.25 | 649.25 | 3.93508 | 2 | 0.00119299 | 0.000606337 | 8.81354 | 0.999998 | 0.492 | 0.492 | 90 | 6.2143 | F | F | 9.42e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X040948.71+075345.9 | chandra | ccd6 | 242.5 | 784 | 3.75464 | 2.00001 | 0.00113829 | 0.000606339 | 8.40939 | 0.999944 | 0.574668 | 0.492 | 70.6701 | 7.37577 | F | F | 9.42e+20 | 1.24411e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X040939.95+075533.1 | chandra | ccd6 | 507.167 | 1001.83 | 2.91813 | 1.73205 | 0.000884684 | 0.000525104 | 6.53583 | 0.999944 | 0.774975 | 0.492 | 168.019 | 4.5653 | A | F | 9.45e+20 | 8.92323e-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