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 | X143106.42+353138.4 | chandra | ccd2 | 209.609 | 908.721 | 19.902 | 4.46117 | 0.00431366 | 0.000966935 | 41.5345 | 1 | 0.557482 | 0.557482 | 0 | 2.54208 | F | F | 1.17e+20 | 0 | 1 | ds | |||||
| Report | 3 | X143126.88+352453.3 | chandra | ccd3 | 530.356 | 765.327 | 24.2646 | 4.92591 | 0.00525923 | 0.00106767 | 49.5323 | 1 | 1.3685 | 0.96259 | 355.265 | 5.51685 | F | F | 1.16e+20 | 0 | 1 | ds | |||||
| Report | 1 | X143044.86+352713.4 | chandra | ccd2 | 744.7 | 370.033 | 14.5706 | 3.87299 | 0.00315811 | 0.000839451 | 30.4082 | 1 | 1.27615 | 0.845359 | 25.753 | 6.76156 | A | F | 1.17e+20 | 0 | 1 | d | |||||
| Report | 8 | X143110.67+353000.8 | chandra | ccd2 | 103.611 | 709.722 | 8.95981 | 3 | 0.00194199 | 0.000650235 | 18.6987 | 1 | 0.492 | 0.492 | 138.637 | 0.974112 | F | F | 1.16e+20 | 0 | 1 | d | |||||
| Report | 1 | X143138.69+353535.3 | chandra | ccd1 | 861.833 | 1204.83 | 8.26567 | 3.00002 | 0.00179154 | 0.000650238 | 17.1129 | 1 | 1.58479 | 0.920373 | 166.485 | 7.41952 | A | F | 1.16e+20 | 0 | 1 | d | |||||
| Report | 2 | X143152.67+353349.1 | chandra | ccd1 | 514.722 | 989.389 | 8.14869 | 3.00002 | 0.00176619 | 0.000650238 | 16.8707 | 1 | 1.60141 | 1.37482 | 83.2244 | 8.54543 | F | F | 1.15e+20 | 0 | 1 | d | |||||
| Report | 6 | X143037.69+352850.6 | chandra | ccd2 | 922.333 | 567.833 | 5.67988 | 2.4495 | 0.00123109 | 0.000530916 | 11.8536 | 1 | 1.14449 | 0.610942 | 20.125 | 7.74623 | A | F | 1.17e+20 | 0 | 1 | d | |||||
| Report | 5 | X143102.23+352832.2 | chandra | ccd2 | 313.1 | 529.7 | 4.96098 | 2.23607 | 0.00107527 | 0.000484656 | 10.3533 | 1 | 0.539019 | 0.492 | 130.067 | 2.9979 | F | F | 1.17e+20 | 0 | 1 | d | |||||
| Report | 3 | X143104.04+353208.6 | chandra | ccd2 | 267.9 | 969.5 | 4.93909 | 2.23607 | 0.00107052 | 0.000484657 | 10.3076 | 1 | 0.492 | 0.492 | 62.496 | 3.23791 | F | F | 1.17e+20 | 0 | 1 | d | |||||
| Report | 4 | X143043.22+352556.3 | chandra | ccd2 | 785.5 | 213.3 | 4.9221 | 2.23607 | 0.00106684 | 0.000484657 | 10.2722 | 1 | 0.58559 | 0.492 | 52.8211 | 7.64543 | F | F | 1.17e+20 | 0 | 1 | d | |||||
| Report | 2 | X143118.67+352147.0 | chandra | ccd3 | 733.9 | 386.1 | 4.77263 | 2.23607 | 0.00103444 | 0.000484657 | 9.74255 | 1 | 1.13737 | 0.492 | 28.725 | 8.11986 | A | F | 1.15e+20 | 0 | 1 | d | |||||
| Report | 7 | X143051.50+353237.9 | chandra | ccd2 | 579 | 1029.25 | 3.93853 | 2 | 0.000853657 | 0.00043349 | 8.21952 | 0.999996 | 0.967768 | 0.492 | 80.3674 | 5.58993 | A | F | 1.17e+20 | 0 | 1 | d | |||||
| Report | 1 | X143130.76+352535.3 | chandra | ccd3 | 433.5 | 850.25 | 3.92804 | 2 | 0.000851383 | 0.00043349 | 8.01846 | 0.999995 | 0.543962 | 0.492 | 146.055 | 5.30667 | F | F | 1.16e+20 | 0 | 1 | d | |||||
| Report | 3 | X143128.79+353504.5 | chandra | ccd0 | 287.563 | 488.573 | 10.87 | 4.16569 | 0.00235918 | 0.000904104 | 4.26917 | 0.999853 | 1.08152 | 0.391691 | 85.656 | 5.87189 | F | F | 1.16e+20 | 0 | 1 | ds |
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