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 | X034716.94+502952.8 | chandra | ccd7 | 55.2097 | 781.64 | 133.863 | 13.0631 | 0.013374 | 0.00130511 | 38.2298 | 1 | 2.37269 | 2.37269 | 0 | 7.59325 | F | F | 6.88e+21 | 7.29912e-14 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 2 | X034611.84+502754.9 | chandra | ccd7 | 1317.91 | 541.006 | 19.3143 | 4.3948 | 0.00192965 | 0.000439076 | 5.51596 | 0.999998 | 0.887182 | 0.887182 | 0 | 3.83203 | F | F | 6.69e+21 | 2.19132e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X034637.68+502753.3 | chandra | ccd7 | 816.438 | 537.49 | 13.9413 | 3.73381 | 0.00139284 | 0.000373036 | 3.98148 | 0.999814 | 1.36606 | 0.588762 | 25.7953 | 2.96704 | T | F | 6.77e+21 | 1.56758e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X034716.03+503426.3 | chandra | ccd3 | 973.7 | 300 | 8.2494 | 3.16231 | 0.000824179 | 0.00031594 | 9.4066 | 1 | 2.01427 | 0.904798 | 120.004 | 8.37255 | A | F | 6.9e+21 | 1.2411e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf rmf | 2 | X034618.69+504141.8 | chandra | ccd2 | 1207.97 | 616.514 | 222.806 | 16.086 | 0.02226 | 0.00160712 | 37.1582 | 1 | 4.95689 | 4.01974 | 101.969 | 11.2821 | F | F | 6.83e+21 | 5.50477e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 4 | X034706.39+503822.6 | chandra | ccd3 | 1161.38 | 779.875 | 6.61471 | 2.82846 | 0.000660861 | 0.000282585 | 7.54261 | 0.999998 | 1.6422 | 0.492 | 100.12 | 9.79142 | A | F | 6.89e+21 | 1.02583e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X034708.26+503549.7 | chandra | ccd3 | 1124.5 | 469.071 | 6.56136 | 2.64576 | 0.000655531 | 0.000264332 | 7.48177 | 0.999998 | 0.664397 | 0.492 | 13.0148 | 8.12741 | F | F | 6.89e+21 | 9.8351e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X034717.11+503737.1 | chandra | ccd3 | 953.928 | 687.929 | 5.34377 | 2.64579 | 0.000533884 | 0.000264335 | 6.09338 | 0.999984 | 1.87978 | 1.13107 | 164.821 | 10.3672 | A | F | 6.91e+21 | 8.33731e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X034608.30+502927.4 | chandra | ccd6 | 508.9 | 167.5 | 4.90658 | 2.23607 | 0.000490206 | 0.000223401 | 5.46635 | 0.999809 | 0.492 | 0.492 | 155.457 | 3.52462 | F | F | 6.69e+21 | 6.37923e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X034602.25+503237.3 | chandra | ccd6 | 625.7 | 553.7 | 4.82037 | 2.23607 | 0.000481592 | 0.000223401 | 5.3703 | 0.999809 | 0.603223 | 0.528017 | 115.097 | 4.78647 | F | F | 6.7e+21 | 6.41552e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X034622.89+503432.9 | chandra | ccd6 | 225.7 | 788.3 | 4.76809 | 2.23607 | 0.000476369 | 0.000223401 | 5.31205 | 0.999809 | 0.592224 | 0.492 | 174.345 | 4.1346 | F | F | 6.77e+21 | 6.28898e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X034618.57+503206.5 | chandra | ccd6 | 309.5 | 490.75 | 3.90254 | 2 | 0.000389894 | 0.000199816 | 4.34776 | 0.998545 | 0.492 | 0.492 | 161.348 | 2.3233 | F | F | 6.74e+21 | 4.93614e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X034627.34+503453.9 | chandra | ccd6 | 139.5 | 831 | 3.88992 | 2 | 0.000388633 | 0.000199816 | 4.3337 | 0.998545 | 0.492 | 0.492 | 148.283 | 4.36623 | F | F | 6.79e+21 | 5.21678e-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