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 | 7 | X121942.49+104649.1 | chandra | ccd7 | 541.417 | 811.348 | 29.8325 | 5.46219 | 0.00643644 | 0.00117848 | 37.2182 | 1 | 0.676863 | 0.676863 | 0 | 3.31354 | F | F | 2.06e+20 | 0 | 1 | ds | |||||
Report | 7 | X121910.92+104908.5 | chandra | ccd6 | 621.883 | 452.693 | 30.7574 | 5.54594 | 0.00663599 | 0.00119655 | 57.2953 | 1 | 1.41099 | 0.876798 | 308.338 | 4.80052 | F | F | 2e+20 | 0 | 1 | ds | |||||
Report | 1 | X122000.30+105747.9 | chandra | ccd3 | 892.887 | 1156.05 | 20.563 | 5.56794 | 0.00443651 | 0.00120129 | 41.0203 | 1 | 6.60188 | 4.15895 | 96.8583 | 12.8688 | A | F | 2.13e+20 | 0 | 1 | d | |||||
Report | 1 | X121855.27+105423.3 | chandra | ccd5 | 270.131 | 519.688 | 19.4473 | 7.66371 | 0.0041958 | 0.00165346 | 3.10274 | 0.998018 | 5.82468 | 2.12301 | 127.05 | 10.8445 | F | F | 2.03e+20 | 0 | 1 | ds | |||||
Report | 2 | X121846.01+105138.4 | chandra | ccd5 | 547.18 | 184.34 | 16.8299 | 5.00011 | 0.00363107 | 0.00107878 | 2.68514 | 0.995347 | 3.95119 | 3.5885 | 126.194 | 11.4166 | F | F | 2.02e+20 | 0 | 1 | d | |||||
Report | 2 | X121947.04+104811.4 | chandra | ccd7 | 405.245 | 978.644 | 18.4658 | 4.29719 | 0.00398404 | 0.000927128 | 23.0374 | 1 | 1.21036 | 0.767611 | 37.7208 | 4.43262 | F | F | 2.07e+20 | 0 | 1 | ds | |||||
Report | 5 | X121908.10+105256.3 | chandra | ccd6 | 705.5 | 915.214 | 12.8907 | 3.74168 | 0.00278119 | 0.000807273 | 24.013 | 1 | 1.59763 | 1.06407 | 101.275 | 7.56263 | A | F | 2.05e+20 | 0 | 1 | d | |||||
Report | 3 | X121934.61+104855.9 | chandra | ccd7 | 776.8 | 1068.6 | 9.91093 | 3.16228 | 0.0021383 | 0.000682267 | 12.3646 | 1 | 0.492 | 0.492 | 122.819 | 1.99731 | F | F | 2.06e+20 | 0 | 1 | d | |||||
Report | 3 | X121904.43+104809.1 | chandra | ccd6 | 815.7 | 331.7 | 9.78954 | 3.16228 | 0.00211211 | 0.000682268 | 18.2361 | 1 | 1.17675 | 0.695257 | 79.7422 | 6.13245 | A | F | 2e+20 | 0 | 1 | d | |||||
Report | 1 | X121930.96+104700.1 | chandra | ccd7 | 886.167 | 833.167 | 5.90732 | 2.44949 | 0.00127451 | 0.000528482 | 7.36981 | 0.999995 | 0.492 | 0.492 | 45 | 0.606913 | F | F | 2.04e+20 | 0 | 1 | d | |||||
Report | 6 | X121925.21+104840.4 | chandra | ccd7 | 1058.5 | 1037.17 | 5.84139 | 2.44949 | 0.00126029 | 0.000528483 | 7.28756 | 0.999995 | 0.492 | 0.492 | 79.722 | 1.5852 | F | F | 2.05e+20 | 0 | 1 | d | |||||
Report | 1 | X121920.37+104946.7 | chandra | ccd6 | 338.3 | 529.9 | 4.95123 | 2.23607 | 0.00106824 | 0.000482436 | 9.22322 | 0.999999 | 0.492 | 0.492 | 108.014 | 3.19824 | F | F | 2.04e+20 | 0 | 1 | d | |||||
Report | 5 | X121936.69+105053.2 | chandra | ccd7 | 714.75 | 1307 | 3.91605 | 2 | 0.000844894 | 0.000431504 | 4.88555 | 0.999464 | 0.596688 | 0.492 | 140.502 | 3.90755 | F | F | 2.07e+20 | 0 | 1 | d | |||||
Report | 6 | X121902.73+105151.9 | chandra | ccd6 | 866.5 | 784.5 | 3.77497 | 2.00001 | 0.000814457 | 0.000431505 | 7.03208 | 0.999987 | 0.897473 | 0.492 | 74.5181 | 7.87278 | A | F | 2.01e+20 | 0 | 1 | d | |||||
Report | 4 | X121927.81+104351.8 | chandra | ccd7 | 980.5 | 450.5 | 2.9374 | 1.73205 | 0.000633749 | 0.000373693 | 3.66462 | 0.995729 | 0.492 | 0.492 | 45 | 3.58806 | F | F | 1.99e+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