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 | X102557.96+124109.9 | chandra | ccd3 | 485.907 | 703.107 | 160.982 | 24.2424 | 0.0180158 | 0.00271301 | 10.965 | 1 | 1.7331 | 1.7331 | 0 | 3.19473 | 318.663 | 116.793 | -0.463582 | 0.0641181 | T | F | 3.58e+20 | 1.92366e-13 | 1 | dsxf |
| Report | srcpi bgdpi arf | 4 | X102627.25+124001.0 | chandra | ccd1 | 566.805 | 885.237 | 37.8654 | 6.71722 | 0.00423761 | 0.000751739 | 14.0574 | 1 | 2.64261 | 1.43132 | 336.073 | 7.59413 | 27.679 | 14.8076 | -0.302951 | 0.18957 | F | F | 3.41e+20 | 5.45271e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X102609.91+125049.8 | chandra | ccd2 | 409.648 | 886.83 | 25.7706 | 6.07176 | 0.00288403 | 0.000679501 | 10.9411 | 1 | 1.90463 | 1.00491 | 18.2928 | 6.8948 | 18.9107 | 10.3746 | -0.291481 | 0.233602 | F | F | 3.65e+20 | 3.91421e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X102614.40+124649.4 | chandra | ccd2 | 276.149 | 398.174 | 30.0573 | 5.48245 | 0.00336377 | 0.000613552 | 12.7611 | 1 | 1.29803 | 0.578316 | 7.64197 | 4.0974 | 14.8868 | 17.8114 | 0.0894408 | 0.209743 | F | F | 3.61e+20 | 4.557e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X102519.62+125120.5 | chandra | ccd6 | 688.21 | 351 | 33.0723 | 7.61438 | 0.00370122 | 0.000852147 | 10.4964 | 1 | 5.32644 | 4.16338 | 50.2344 | 12.4104 | 18.7569 | 14.4477 | -0.129778 | 0.231813 | F | F | 3.71e+20 | 5.24103e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X102613.95+123625.1 | chandra | ccd1 | 961.731 | 445.808 | 11.2423 | 4.7081 | 0.00125815 | 0.000526892 | 8.47974 | 1 | 3.42998 | 1.06275 | 10.6895 | 8.40474 | 7.60649 | 4.71452 | -0.234718 | 0.406251 | A | F | 3.52e+20 | 1.6846e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X102622.98+124200.9 | chandra | ccd1 | 693.5 | 1128.36 | 7.72426 | 3.95804 | 0.000864436 | 0.000442952 | 14.7097 | 1 | 0.740418 | 0.602682 | 151.368 | 5.72003 | 4.86213 | 2.86213 | -0.258925 | 0.534926 | F | F | 3.43e+20 | 1.05216e-14 | 1 | dx |
| Report | 2 | X102546.52+124619.0 | chandra | ccd2 | 1104.5 | 335.833 | 5.89098 | 2.44949 | 0.000659268 | 0.000274126 | 2.50107 | 0.988313 | 0.516245 | 0.492 | 78.4007 | 4.17191 | F | F | 3.64e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 9 | X102600.56+124528.7 | chandra | ccd2 | 687.333 | 233.667 | 5.91531 | 3.59808 | 0.00066199 | 0.000402666 | 20.326 | 1 | 0.492 | 0.492 | 105.715 | 1.25147 | 2.91531 | 3 | 0.0143177 | 0.616388 | F | F | 3.61e+20 | 7.81692e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X102630.41+124245.8 | chandra | ccd0 | 815.333 | 237.667 | 5.51273 | 3.59808 | 0.000616943 | 0.000402669 | 7.89734 | 0.999999 | 0.940417 | 0.492 | 69.6691 | 7.2348 | 5.86711 | -0.354379 | -1 | 0.878776 | A | F | 3.43e+20 | 7.9529e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X102642.06+124646.3 | chandra | ccd0 | 469.278 | 726.833 | 7.94954 | 4.1225 | 0.000889653 | 0.000461359 | 7.75627 | 1 | 2.6439 | 0.964712 | 68.8717 | 10.2379 | 5.87642 | 2.07313 | -0.478429 | 0.580425 | A | F | 3.45e+20 | 1.28518e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X102621.28+124445.8 | chandra | ccd0 | 1087.68 | 482.132 | 14.6882 | 3.83252 | 0.0016438 | 0.000428908 | 21.0473 | 1 | 1.31861 | 0.581099 | 1.8517 | 4.87253 | 4.88806 | 9.7388 | 0.331633 | 0.360144 | F | F | 3.46e+20 | 1.99127e-14 | 1 | dsx |
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