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 | 1 | X095146.07+594433.2 | chandra | ccd7 | 903.745 | 338.966 | 48.0378 | 6.93093 | 0.00937387 | 0.00135247 | 32.9984 | 1 | 0.434123 | 0.434123 | 0 | 1.00721 | F | F | 1.56e+20 | 5.97285e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X095130.36+594037.0 | chandra | ccd6 | 553.679 | 700.068 | 41.8254 | 6.46726 | 0.0081616 | 0.00126199 | 79.4113 | 1 | 2.02767 | 1.30614 | 8.46033 | 5.39454 | F | F | 1.54e+20 | 8.352e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X095151.55+594430.2 | chandra | ccd7 | 819.645 | 332.875 | 25.3895 | 5.0388 | 0.00495439 | 0.000983249 | 17.4407 | 1 | 0.510947 | 0.510947 | 0 | 1.12786 | F | F | 1.56e+20 | 3.16465e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 13 | X095157.97+594403.5 | chandra | ccd7 | 720.878 | 278.668 | 25.1385 | 5.01383 | 0.0049054 | 0.000978373 | 17.2683 | 1 | 0.527524 | 0.527524 | 0 | 1.94344 | F | F | 1.56e+20 | 3.15904e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 11 | X095144.95+595057.1 | chandra | ccd7 | 920.834 | 1119.29 | 18.5229 | 5.39173 | 0.00361447 | 0.00105212 | 12.7239 | 1 | 0.938241 | 0.938241 | 0 | 5.43217 | F | F | 1.6e+20 | 2.73105e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X095146.36+594038.2 | chandra | ccd6 | 307.445 | 702.413 | 28.0184 | 5.29324 | 0.00546737 | 0.0010329 | 53.1968 | 1 | 1.99269 | 0.625083 | 21.2082 | 4.89746 | A | F | 1.53e+20 | 5.59523e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X095230.37+594639.3 | chandra | ccd7 | 223.864 | 596.137 | 16.4516 | 4.06202 | 0.00321029 | 0.000792645 | 11.301 | 1 | 1.2244 | 1.2244 | 0 | 5.46213 | F | F | 1.58e+20 | 2.42207e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 10 | X095133.83+595006.7 | chandra | ccd7 | 1090.75 | 1016.33 | 11.7339 | 3.46411 | 0.00228969 | 0.000675966 | 8.06035 | 1 | 0.662991 | 0.492 | 172.053 | 4.90826 | F | F | 1.59e+20 | 1.84222e-14 | 1 | dpx | ||||
| Report | srcpi bgdpi arf | 3 | X095104.46+594255.8 | chandra | ccd6 | 951.056 | 982.389 | 8.33631 | 3.00001 | 0.0016267 | 0.000585406 | 15.8276 | 1 | 1.54173 | 1.01428 | 92.8624 | 6.06213 | A | F | 1.57e+20 | 1.75257e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X095141.75+594606.9 | chandra | ccd7 | 969.5 | 529 | 7.90818 | 2.82843 | 0.00154316 | 0.000551924 | 5.43233 | 0.999986 | 0.492 | 0.492 | 112.5 | 0.96924 | F | F | 1.57e+20 | 9.82186e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X095159.74+594740.6 | chandra | ccd7 | 693.5 | 719.375 | 7.84251 | 2.82843 | 0.00153034 | 0.000551924 | 5.38722 | 0.999925 | 0.492 | 0.492 | 69.444 | 2.60934 | F | F | 1.58e+20 | 1.00032e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X095103.91+593603.5 | chandra | ccd5 | 360.833 | 1006.5 | 6.23457 | 3.00006 | 0.00121658 | 0.000585415 | 6.26631 | 0.99999 | 1.73754 | 0.556166 | 75.2863 | 10.9821 | A | F | 1.53e+20 | 9.5745e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X095145.87+594749.9 | chandra | ccd7 | 906.3 | 738.3 | 4.90685 | 2.23607 | 0.000957495 | 0.000436334 | 3.37064 | 0.998428 | 0.492 | 0.492 | 174.345 | 2.31274 | F | F | 1.58e+20 | 6.24841e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X095149.74+594458.9 | chandra | ccd7 | 846.9 | 390.7 | 4.85652 | 2.23607 | 0.000947674 | 0.000436334 | 3.33607 | 0.993852 | 0.492 | 0.492 | 7.62756 | 0.598033 | F | F | 1.56e+20 | 6.00789e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X095130.71+593554.7 | chandra | ccd6 | 548.333 | 125.833 | 4.718 | 2.44953 | 0.000920643 | 0.000477986 | 8.95777 | 0.999989 | 2.70205 | 1.11151 | 25.3214 | 9.86294 | A | F | 1.51e+20 | 1.10623e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 12 | X095220.89+594421.6 | chandra | ccd7 | 368.25 | 315.5 | 3.9439 | 2 | 0.000769591 | 0.000390269 | 2.70917 | 0.993852 | 0.492 | 0.492 | 180 | 4.31652 | F | F | 1.56e+20 | 5.84955e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X095202.55+594054.6 | chandra | ccd6 | 57.75 | 735.25 | 3.93432 | 2 | 0.000767721 | 0.000390269 | 7.46985 | 0.999989 | 0.5535 | 0.492 | 161.565 | 4.97809 | F | F | 1.54e+20 | 8.51351e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X095151.18+594556.2 | chandra | ccd7 | 824.75 | 507.25 | 3.87296 | 2 | 0.000755747 | 0.000390269 | 2.66043 | 0.978738 | 0.492 | 0.492 | 45 | 0.576958 | F | F | 1.57e+20 | 4.8021e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X095047.52+595303.4 | chandra | ccd3 | 787.75 | 436.25 | 3.15558 | 2.00003 | 0.000615763 | 0.000390273 | 6.29161 | 0.999863 | 1.96707 | 0.821578 | 84.3151 | 10.6863 | A | F | 1.61e+20 | 8.09449e-15 | 1 | dx | ||||
| Report | 7 | X095203.91+594117.8 | chandra | ccd6 | 36.8333 | 782.5 | 2.9803 | 1.73205 | 0.000581559 | 0.000337983 | 5.65852 | 0.999802 | 0.492 | 0.492 | 180 | 4.69174 | F | F | 1.54e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 6 | X095139.95+594038.5 | chandra | ccd6 | 405.5 | 702.5 | 1.95318 | 1.41422 | 0.000381132 | 0.000275962 | 3.70838 | 0.997106 | 0.521845 | 0.492 | 45 | 4.99338 | F | F | 1.53e+20 | 3.88056e-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