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 | X170745.17+783938.1 | chandra | ccd2 | 850.231 | 784.358 | 178.603 | 14.5255 | 0.0150465 | 0.0012237 | 31.3839 | 1 | 5.84777 | 4.13965 | 353.287 | 10.5196 | F | F | 4.31e+20 | 1.91595e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 2 | X170405.38+784303.1 | chandra | ccd6 | 1051.56 | 426.255 | 88.0639 | 9.68674 | 0.00741896 | 0.000816061 | 36.6647 | 1 | 1.05614 | 0.592859 | 48.0021 | 3.23272 | F | F | 4.24e+20 | 6.96049e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 7 | X170237.41+783733.7 | chandra | ccd7 | 1114.73 | 687.63 | 31.936 | 9.86466 | 0.00273412 | 0.000844537 | 6.09545 | 1 | 0.804218 | 0.804218 | 0 | 5.13526 | F | F | 4.2e+20 | 1.83184e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X170329.47+783755.1 | chandra | ccd7 | 801.618 | 729.6 | 27.8057 | 7.13463 | 0.00238051 | 0.000610812 | 5.30712 | 0.999999 | 0.665905 | 0.665905 | 0 | 2.80457 | F | F | 4.21e+20 | 1.48285e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X170419.06+783434.6 | chandra | ccd7 | 503.357 | 321.722 | 28.1826 | 7.08747 | 0.00241278 | 0.000606775 | 5.37906 | 0.999999 | 1.17845 | 1.17845 | 0 | 5.27351 | F | F | 4.19e+20 | 1.61799e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X170403.44+783722.1 | chandra | ccd7 | 597.511 | 662.07 | 14.5154 | 7.0158 | 0.0012427 | 0.000600639 | 2.77048 | 0.994145 | 0.543929 | 0.543929 | 0 | 2.49839 | F | F | 4.21e+20 | 7.76174e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X170439.08+783524.8 | chandra | ccd7 | 382.67 | 423.836 | 23.0865 | 6.35135 | 0.00197649 | 0.000543754 | 4.4064 | 0.999963 | 1.08711 | 1.08711 | 0 | 4.63492 | F | F | 4.21e+20 | 1.35472e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X170228.47+783526.3 | chandra | ccd7 | 1169.9 | 428.6 | 19.9825 | 5.47734 | 0.00168343 | 0.000461437 | 3.81396 | 0.99976 | 2.15496 | 0.996363 | 135.303 | 6.69972 | A | F | 4.18e+20 | 1.14688e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X170330.03+783954.4 | chandra | ccd7 | 797.56 | 971.998 | 14.3487 | 8.00306 | 0.00122843 | 0.000685162 | 2.73866 | 0.994145 | 0.606438 | 0.606438 | 0 | 2.02319 | F | F | 4.23e+20 | 7.55459e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X170541.27+783127.2 | chandra | ccd3 | 1122 | 719.964 | 17.4651 | 5.29163 | 0.00147134 | 0.000445792 | 12.907 | 1 | 2.9711 | 2.00746 | 28.0575 | 9.49106 | F | F | 4.2e+20 | 1.86891e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X170609.05+783230.7 | chandra | ccd3 | 954.58 | 850.34 | 16.0645 | 5.00011 | 0.00135335 | 0.000421234 | 11.872 | 1 | 3.2596 | 1.44314 | 119.463 | 9.35623 | A | F | 4.22e+20 | 1.68439e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X170515.39+783021.0 | chandra | ccd3 | 1278.35 | 584.7 | 12.4013 | 4.47225 | 0.00104474 | 0.000376764 | 9.16476 | 1 | 3.38142 | 2.22361 | 101.251 | 10.0004 | A | F | 4.18e+20 | 1.37213e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X170410.38+783734.0 | chandra | ccd7 | 555.763 | 686.254 | 11.0676 | 5.92796 | 0.000947521 | 0.000507505 | 2.11241 | 0.978156 | 0.517146 | 0.517146 | 0 | 2.26795 | F | F | 4.22e+20 | 5.88959e-15 | 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