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 | 5 | X235905.68+050343.0 | chandra | ccd7 | 260.206 | 504.333 | 91.5442 | 9.76675 | 0.022152 | 0.00236337 | 46.6841 | 1 | 1.91332 | 1.1268 | 354.877 | 5.46983 | F | F | 4.33e+20 | 1.72016e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X235927.00+050736.0 | chandra | ccd3 | 919.441 | 663.559 | 13.5957 | 4.12315 | 0.00328986 | 0.000997713 | 30.4047 | 1 | 3.49257 | 1.92972 | 90.2134 | 9.51572 | A | F | 4.33e+20 | 4.51338e-14 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 1 | X235822.11+051635.8 | chandra | ccd5 | 838.335 | 145.255 | 11.1281 | 4.43868 | 0.00269279 | 0.00107408 | 3.80044 | 0.999406 | 2.99899 | 2.99899 | 0 | 11.4529 | F | F | 4.4e+20 | 2.54714e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X235937.59+050352.9 | chandra | ccd3 | 597.633 | 210.233 | 10.7844 | 3.87307 | 0.00260959 | 0.0009372 | 24.1177 | 1 | 6.36216 | 3.81288 | 17.1109 | 12.599 | A | F | 4.3e+20 | 3.75201e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X235849.22+050406.4 | chandra | ccd7 | 759.625 | 551.375 | 7.74784 | 2.82843 | 0.00187481 | 0.00068442 | 3.95111 | 0.999345 | 0.773434 | 0.492 | 34.181 | 3.12277 | A | F | 4.34e+20 | 1.38531e-14 | 1 | dx | ||||
Report | 3 | X235832.09+050803.5 | chandra | ccd6 | 908 | 65.3335 | 5.89774 | 2.44949 | 0.00142713 | 0.000592724 | 11.9147 | 1 | 0.615629 | 0.492 | 132.072 | 4.24767 | F | F | 4.36e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X235850.78+050334.9 | chandra | ccd7 | 712.333 | 487.333 | 5.84337 | 2.44949 | 0.00141397 | 0.000592725 | 2.9799 | 0.993725 | 0.655694 | 0.492 | 70.0972 | 3.67895 | F | F | 4.33e+20 | 1.05366e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X235852.38+050913.9 | chandra | ccd7 | 663.667 | 1176.33 | 5.81381 | 2.4495 | 0.00140682 | 0.000592725 | 2.96482 | 0.993725 | 0.49779 | 0.492 | 174.116 | 2.19164 | F | F | 4.36e+20 | 1.28032e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X235856.73+050700.5 | chandra | ccd7 | 531.667 | 905.333 | 5.78211 | 2.44949 | 0.00139915 | 0.000592725 | 2.94866 | 0.993725 | 0.492 | 0.492 | 15.1282 | 1.98283 | F | F | 4.35e+20 | 1.0128e-14 | 1 | dx | ||||
Report | 1 | X235927.30+050737.4 | chandra | ccd3 | 910.5 | 666.5 | 5.30761 | 2.64578 | 0.00128433 | 0.000640222 | 11.8697 | 1 | 0.492 | 0.492 | 90 | 9.58995 | F | F | 4.33e+20 | 0 | 1 | dc | |||||
Report | 1 | X235918.52+051314.4 | chandra | ccd2 | 791 | 394.25 | 3.87062 | 2 | 0.000936606 | 0.000483958 | 8.87298 | 0.999998 | 0.492 | 0.492 | 104.872 | 9.53198 | F | F | 4.36e+20 | 0 | 1 | d | |||||
Report | 2 | X235844.01+051447.5 | chandra | ccd6 | 546 | 886.5 | 3.80655 | 2.00001 | 0.000921103 | 0.000483958 | 7.69002 | 0.999994 | 1.08852 | 0.695059 | 142.018 | 7.65865 | A | F | 4.39e+20 | 0 | 1 | d | |||||
Report | 1 | X235823.83+051443.8 | chandra | ccd6 | 1158.5 | 879 | 3.78235 | 2.00001 | 0.000915246 | 0.000483958 | 7.64113 | 0.999994 | 0.492 | 0.492 | 31.7175 | 9.74575 | F | F | 4.39e+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