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 | 1 | X000900.04+192348.1 | chandra | ccd7 | 556.86 | 903.278 | 68.4706 | 8.86917 | 0.0112872 | 0.00146206 | 28.7722 | 1 | 0.723451 | 0.723451 | 0 | 3.2882 | F | F | 3.36e+20 | 7.73487e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 2 | X000935.38+192959.4 | chandra | ccd3 | 457.343 | 601.665 | 127.773 | 17.2857 | 0.00899094 | 0.00121634 | 9.77039 | 1 | 7.58567 | 6.98441 | 90 | 13.2359 | F | F | 3.32e+20 | 7.75763e-14 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 5 | X000836.82+192154.7 | chandra | ccd7 | 1224.58 | 672.663 | 37.3073 | 6.61755 | 0.00615003 | 0.00109089 | 15.677 | 1 | 0.928325 | 0.588271 | 20.059 | 2.80828 | F | F | 3.38e+20 | 4.20064e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X000927.60+193120.5 | chandra | ccd3 | 680.685 | 765.754 | 62.3942 | 11.4022 | 0.00439045 | 0.000802333 | 4.77108 | 0.999997 | 6.75825 | 5.43772 | 101.205 | 12.4285 | F | F | 3.31e+20 | 5.93321e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X000909.71+193118.4 | chandra | ccd3 | 1194.68 | 761.029 | 54.2674 | 8.54415 | 0.0038186 | 0.00060122 | 4.14965 | 0.999966 | 1.61999 | 0.980574 | 125.035 | 9.44581 | A | F | 3.32e+20 | 4.90523e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X000909.35+193108.5 | chandra | ccd3 | 1205.16 | 740.888 | 52.7244 | 8.18546 | 0.00371002 | 0.000575981 | 4.03167 | 0.999939 | 3.08693 | 1.91901 | 153.324 | 9.26176 | A | T | 3.32e+20 | 4.76162e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X000859.15+192341.1 | chandra | ccd7 | 582.434 | 888.954 | 16.3965 | 4.04926 | 0.00270292 | 0.000667511 | 6.89002 | 1 | 0.631338 | 0.631338 | 0 | 3.07109 | F | F | 3.36e+20 | 1.84637e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X000921.28+193317.9 | chandra | ccd3 | 862.536 | 1004.12 | 29.5824 | 7.41646 | 0.00208161 | 0.000521869 | 2.26207 | 0.986305 | 5.75863 | 4.17824 | 103.941 | 12.7023 | F | F | 3.3e+20 | 2.79031e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X000819.74+192456.2 | chandra | ccd6 | 833.494 | 456.858 | 24.6101 | 5.28766 | 0.00176309 | 0.000378812 | 13.9081 | 1 | 1.87531 | 1.87531 | 0 | 6.34208 | F | F | 3.38e+20 | 1.84796e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X000908.59+192142.7 | chandra | ccd7 | 310.759 | 648.43 | 24.985 | 4.9985 | 0.00411873 | 0.000823992 | 10.499 | 1 | 2.25196 | 2.25196 | 0 | 5.62216 | F | F | 3.37e+20 | 2.9366e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X000837.64+192839.7 | chandra | ccd6 | 318.29 | 910.447 | 17.99 | 4.35891 | 0.00126589 | 0.000306721 | 10.1668 | 1 | 0.662235 | 0.567305 | 2.7816 | 5.37333 | F | F | 3.35e+20 | 1.34271e-14 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 1 | X000905.37+193249.7 | chandra | ccd2 | 447.417 | 403.667 | 8.11117 | 3.46417 | 0.000570754 | 0.000243761 | 5.50435 | 0.999982 | 2.18355 | 0.918696 | 111.03 | 10.2201 | A | F | 3.31e+20 | 7.30258e-15 | 1 | dx | ||||
| Report | 2 | X000851.77+192231.8 | chandra | ccd7 | 794.056 | 747.5 | 5.93573 | 3.00006 | 0.000417676 | 0.000211103 | 2.49427 | 0.986488 | 0.492 | 0.492 | 149.527 | 1.75892 | F | F | 3.37e+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