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 | 2 | X024015.47+192103.5 | chandra | ccd7 | 944.42 | 961.935 | 38.9225 | 6.23879 | 0.0123814 | 0.00198458 | 55.0961 | 1 | 2.3616 | 2.3616 | 0 | 6.49948 | F | F | 6.75e+20 | 1.02023e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X024028.23+192156.5 | chandra | ccd7 | 576.763 | 1069.18 | 18.0062 | 4.35891 | 0.00572776 | 0.00138656 | 25.4884 | 1 | 1.52628 | 0.90674 | 13.4492 | 6.34736 | A | F | 6.7e+20 | 4.61205e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 9 | X024039.70+191613.0 | chandra | ccd7 | 247.279 | 371.56 | 15.9425 | 3.99281 | 0.00507137 | 0.00127013 | 22.5671 | 1 | 0.583929 | 0.583929 | 0 | 2.24055 | F | F | 6.63e+20 | 3.73706e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X023929.09+191309.4 | chandra | ccd3 | 924.548 | 69.0239 | 16.248 | 4.58266 | 0.00516845 | 0.00145774 | 35.7909 | 1 | 6.96431 | 2.76584 | 32.0215 | 14.7159 | A | F | 6.86e+20 | 7.22006e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X024012.87+192121.7 | chandra | ccd7 | 1018.61 | 998.611 | 8.25031 | 3.00002 | 0.00262441 | 0.000954301 | 11.6786 | 1 | 1.19258 | 1.09856 | 27.9069 | 7.09924 | F | F | 6.76e+20 | 2.26102e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X024022.32+191719.5 | chandra | ccd7 | 747 | 506.125 | 7.89489 | 2.82843 | 0.00251135 | 0.000899718 | 11.1755 | 1 | 0.635149 | 0.492 | 30.9735 | 2.58638 | F | F | 6.7e+20 | 1.89613e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X024020.86+191835.4 | chandra | ccd7 | 788.833 | 660.5 | 5.91368 | 2.44949 | 0.00188113 | 0.000779179 | 8.37101 | 0.999999 | 0.61997 | 0.492 | 72.6524 | 3.75014 | F | F | 6.71e+20 | 1.41687e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X024025.78+191753.9 | chandra | ccd7 | 647.333 | 576.167 | 5.90444 | 2.44949 | 0.00187819 | 0.000779179 | 8.35793 | 0.999999 | 0.492 | 0.492 | 11.9812 | 2.54381 | F | F | 6.69e+20 | 1.4006e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X024050.29+190521.8 | chandra | ccd5 | 407.333 | 1079.5 | 4.9144 | 2.44952 | 0.00156326 | 0.000779187 | 5.63437 | 0.999859 | 1.86133 | 0.854373 | 153.593 | 11.2646 | A | F | 6.62e+20 | 1.42002e-14 | 1 | dx | ||||
Report | 5 | X024033.31+191512.2 | chandra | ccd7 | 430.5 | 247.5 | 3.93881 | 2 | 0.00125293 | 0.000636197 | 5.57552 | 0.999829 | 0.492 | 0.492 | 76.7175 | 0.772303 | F | F | 6.65e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 6 | X024018.83+191601.2 | chandra | ccd7 | 847.5 | 347 | 3.90691 | 2 | 0.00124278 | 0.000636198 | 5.53036 | 0.999829 | 0.492 | 0.492 | 73.155 | 2.79652 | F | F | 6.71e+20 | 9.36069e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X024022.74+190738.1 | chandra | ccd6 | 1000 | 331.5 | 1.82843 | 1.41422 | 0.000581621 | 0.000449861 | 3.99705 | 0.998694 | 0.492 | 0.492 | 180 | 8.19314 | F | F | 6.67e+20 | 7.06897e-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