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 rmf | 1 | X110940.86+065027.4 | chandra | ccd3 | 103.487 | 195.453 | 112.182 | 15.3304 | 0.00582067 | 0.000795431 | 22.7953 | 1 | 9.5241 | 7.65372 | 139.99 | 15.2164 | F | F | 3.74e+20 | 8.52814e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X110851.05+065901.3 | chandra | ccd7 | 190.913 | 834.093 | 56.7255 | 8.01329 | 0.00294326 | 0.000415778 | 22.138 | 1 | 0.745659 | 0.745659 | 0 | 0.177624 | T | F | 3.58e+20 | 2.20095e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X110926.48+070000.1 | chandra | ccd2 | 900.699 | 366.788 | 37.6795 | 8.17957 | 0.00195515 | 0.000424429 | 6.96981 | 1 | 3.75064 | 1.92941 | 331.258 | 8.98154 | F | F | 3.61e+20 | 2.78127e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X110853.22+070123.0 | chandra | ccd6 | 473.193 | 137.25 | 33.901 | 5.82246 | 0.00175899 | 0.000302105 | 26.7335 | 1 | 0.560083 | 0.560083 | 0 | 2.36176 | F | F | 3.55e+20 | 1.84148e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X110916.61+065239.9 | chandra | ccd3 | 837.758 | 464.597 | 25.3347 | 5.56783 | 0.00131452 | 0.000288892 | 5.148 | 0.999997 | 2.73993 | 1.38618 | 12.0296 | 9.15345 | A | F | 3.67e+20 | 1.79445e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X110850.77+065958.6 | chandra | ccd7 | 199.53 | 950.591 | 17.3321 | 5.20087 | 0.000899292 | 0.000269852 | 6.76412 | 1 | 0.504855 | 0.101282 | 89.337 | 0.854094 | A | F | 3.57e+20 | 6.80047e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X110920.17+065212.3 | chandra | ccd3 | 730.394 | 409.045 | 30.2925 | 7.38318 | 0.00157176 | 0.000383084 | 6.15542 | 1 | 7.63123 | 2.22775 | 331.521 | 10.1458 | F | F | 3.67e+20 | 2.34527e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X110849.10+065952.7 | chandra | ccd7 | 249.977 | 938.531 | 18.3408 | 5.10886 | 0.000951631 | 0.000265078 | 7.15778 | 1 | 0.380221 | 0.380221 | 0 | 0.828798 | F | F | 3.57e+20 | 7.19501e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X110851.28+070108.6 | chandra | ccd6 | 531.947 | 107.912 | 13.6846 | 3.69927 | 0.000710038 | 0.00019194 | 10.7913 | 1 | 0.599702 | 0.599702 | 0 | 2.03074 | F | F | 3.56e+20 | 7.86356e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X110901.06+070306.5 | chandra | ccd6 | 235.956 | 347.598 | 9.81117 | 3.69529 | 0.000509063 | 0.000191734 | 7.73684 | 1 | 0.873012 | 0.324164 | 47.9539 | 4.7778 | F | F | 3.54e+20 | 9.05294e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X110843.51+065441.5 | chandra | ccd7 | 418.7 | 305.7 | 8.56866 | 3.1623 | 0.000444593 | 0.000164079 | 3.34405 | 0.998717 | 0.492 | 0.492 | 45 | 4.75543 | F | F | 3.63e+20 | 3.61523e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X110853.94+070343.9 | chandra | ccd6 | 450.944 | 422.944 | 8.36969 | 3.00002 | 0.000434269 | 0.000155659 | 6.60012 | 0.999993 | 0.639127 | 0.513729 | 33.6901 | 4.68778 | F | F | 3.52e+20 | 4.75415e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X110852.64+065953.0 | chandra | ccd7 | 142.357 | 938.786 | 6.05832 | 2.64577 | 0.000314342 | 0.000137278 | 2.36435 | 0.982768 | 0.492 | 0.492 | 151.138 | 0.931996 | F | F | 3.57e+20 | 2.37975e-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