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 | 10 | X192429.44+510129.7 | chandra | ccd7 | 557.057 | 381.843 | 41.4935 | 6.44154 | 0.0111909 | 0.0017373 | 48.4883 | 1 | 0.479674 | 0.479674 | 0 | 0.384742 | F | F | 8.24e+20 | 8.48825e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X192422.76+510513.0 | chandra | ccd7 | 684.5 | 835.1 | 9.76705 | 3.16228 | 0.00263419 | 0.000852874 | 11.4136 | 1 | 0.524512 | 0.492 | 46.4312 | 3.8685 | F | F | 8.33e+20 | 2.06342e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X192438.65+510432.0 | chandra | ccd7 | 380.167 | 751.833 | 8.74797 | 3.00001 | 0.00235935 | 0.000809108 | 10.2227 | 1 | 0.576921 | 0.492 | 45 | 3.11165 | F | F | 8.43e+20 | 1.86707e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X192406.56+510110.9 | chandra | ccd7 | 995.5 | 343.5 | 7.79458 | 2.82843 | 0.00210221 | 0.000762834 | 9.10857 | 1 | 0.70356 | 0.492 | 147.222 | 3.988 | F | F | 8.04e+20 | 1.80451e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X192406.50+510039.8 | chandra | ccd7 | 996.75 | 280.25 | 7.68855 | 2.82843 | 0.00207362 | 0.000762834 | 8.98466 | 1 | 0.831524 | 0.494646 | 20.1823 | 4.0867 | A | F | 8.03e+20 | 1.81878e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X192502.48+505908.6 | chandra | ccd6 | 394.643 | 1038.93 | 6.8532 | 2.64575 | 0.00184834 | 0.000713573 | 12.5653 | 1 | 1.08054 | 0.600645 | 85.0417 | 5.4268 | A | F | 8.37e+20 | 2.23916e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X192343.51+505758.4 | chandra | ccd3 | 141.5 | 372.072 | 6.08943 | 2.64578 | 0.00164237 | 0.000713588 | 11.3537 | 1 | 1.98353 | 0.675362 | 173.537 | 8.42084 | A | F | 7.84e+20 | 2.79342e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X192434.85+510217.6 | chandra | ccd7 | 452.833 | 478.667 | 5.87992 | 2.44949 | 0.00158583 | 0.000660633 | 6.87114 | 0.999988 | 0.589148 | 0.492 | 56.2081 | 0.8336 | T | F | 8.31e+20 | 1.20887e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X192425.73+510454.3 | chandra | ccd7 | 627.7 | 797.1 | 4.89774 | 2.23607 | 0.00132093 | 0.000603073 | 5.72338 | 0.999885 | 0.492 | 0.492 | 13.2825 | 3.42312 | F | F | 8.34e+20 | 1.03036e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X192423.70+510349.5 | chandra | ccd7 | 666.5 | 665.5 | 3.90216 | 2 | 0.00105242 | 0.000539405 | 4.55998 | 0.999041 | 0.492 | 0.492 | 90 | 2.54729 | F | F | 8.28e+20 | 8.57375e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X192427.59+510611.4 | chandra | ccd7 | 592 | 953.75 | 3.88358 | 2 | 0.00104741 | 0.000539405 | 4.53826 | 0.999041 | 0.492 | 0.492 | 97.4657 | 4.62036 | F | F | 8.4e+20 | 8.32122e-15 | 1 | dx | ||||
| Report | 7 | X192423.20+510434.0 | chandra | ccd7 | 676.167 | 755.833 | 2.91776 | 1.73205 | 0.000786927 | 0.000467138 | 3.40963 | 0.99328 | 0.492 | 0.492 | 45 | 3.24321 | F | F | 8.3e+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