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 | 2 | X111411.60+564304.6 | chandra | ccd1 | 973.838 | 929.1 | 15.3612 | 3.91934 | 0.00308408 | 0.000786888 | 24.953 | 1 | 0.927586 | 0.500078 | 89.997 | 5.58492 | F | F | 7.36e+19 | 0 | 1 | ds | |||||
Report | 3 | X111438.78+565009.6 | chandra | ccd2 | 867.75 | 333.125 | 7.84516 | 2.82843 | 0.00157604 | 0.000568214 | 13.1214 | 1 | 0.493158 | 0.492 | 160.67 | 2.643 | F | T | 7.34e+19 | 0 | 1 | d | |||||
Report | 1 | X111420.00+563937.5 | chandra | ccd1 | 833.25 | 507.5 | 7.57722 | 2.82844 | 0.00152127 | 0.000567861 | 12.3085 | 1 | 1.13425 | 0.71352 | 65.947 | 8.21919 | A | T | 7.35e+19 | 0 | 1 | d | |||||
Report | 2 | X111459.84+565557.4 | chandra | ccd2 | 517.5 | 1040.38 | 7.14024 | 2.82844 | 0.00143443 | 0.000568216 | 11.9424 | 1 | 2.79342 | 0.829288 | 158.039 | 9.0195 | A | F | 7.3e+19 | 0 | 1 | d | |||||
Report | 1 | X111452.13+565033.0 | chandra | ccd2 | 645.1 | 380.9 | 4.94166 | 2.23607 | 0.000992748 | 0.000449212 | 8.26517 | 0.999998 | 0.59963 | 0.492 | 179.045 | 3.72524 | F | T | 7.33e+19 | 0 | 1 | d | |||||
Report | 3 | X111403.37+564736.7 | chandra | ccd3 | 602.9 | 572.9 | 4.93298 | 2.23607 | 0.000991005 | 0.000449212 | 7.92402 | 0.999997 | 0.492 | 0.492 | 53.677 | 4.47697 | F | T | 7.38e+19 | 0 | 1 | d | |||||
Report | 1 | X111429.86+564900.3 | chandra | ccd3 | 160.5 | 742.25 | 3.93231 | 2 | 0.000789977 | 0.000401788 | 6.31661 | 0.999947 | 0.492 | 0.492 | 90 | 1.69018 | F | T | 7.35e+19 | 0 | 1 | d | |||||
Report | 5 | X111414.12+564033.4 | chandra | ccd1 | 931.5 | 621.25 | 3.92797 | 2 | 0.000788613 | 0.000401537 | 6.38065 | 0.999952 | 0.492 | 0.492 | 90 | 7.60673 | F | F | 7.35e+19 | 0 | 1 | d | |||||
Report | 4 | X111401.54+563955.7 | chandra | ccd1 | 1142.5 | 545 | 3.80121 | 2.00001 | 0.000763164 | 0.000401539 | 6.17475 | 0.999952 | 0.492 | 0.492 | 148.283 | 8.96709 | F | F | 7.36e+19 | 0 | 1 | d | |||||
Report | 2 | X111357.08+565141.8 | chandra | ccd3 | 706.75 | 1071.25 | 3.77601 | 2.00001 | 0.000758576 | 0.000401788 | 6.06554 | 0.999947 | 0.829419 | 0.492 | 162.92 | 6.7593 | A | F | 7.39e+19 | 0 | 1 | d | |||||
Report | 1 | X111457.86+564810.4 | chandra | ccd0 | 1067.17 | 964.167 | 2.96141 | 1.73205 | 0.000594559 | 0.000347742 | 5.0569 | 0.999561 | 0.492 | 0.492 | 45 | 3.0498 | F | T | 7.33e+19 | 0 | 1 | d | |||||
Report | 6 | X111446.71+564958.3 | chandra | ccd2 | 735.5 | 310.167 | 2.94992 | 1.73205 | 0.000592621 | 0.000347958 | 4.9339 | 0.999488 | 0.492 | 0.492 | 151.845 | 2.83133 | F | F | 7.34e+19 | 0 | 1 | d | |||||
Report | 3 | X111422.47+564008.0 | chandra | ccd1 | 791.833 | 569.5 | 2.85868 | 1.73206 | 0.000573933 | 0.000347742 | 4.64368 | 0.999364 | 0.561105 | 0.492 | 115.097 | 7.64062 | F | T | 7.35e+19 | 0 | 1 | d | |||||
Report | 5 | X111505.68+565149.7 | chandra | ccd2 | 419.5 | 537 | 1.94151 | 1.41422 | 0.000390036 | 0.000284107 | 3.24727 | 0.994163 | 0.492 | 0.492 | 153.435 | 5.89643 | F | F | 7.31e+19 | 0 | 1 | d | |||||
Report | 4 | X111505.86+565148.7 | chandra | ccd2 | 416.5 | 535 | 1.93885 | 1.41422 | 0.000389502 | 0.000284107 | 3.24282 | 0.994163 | 0.492 | 0.492 | 153.435 | 5.90146 | F | F | 7.31e+19 | 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