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 | 6 | X122900.49+130824.2 | chandra | ccd7 | 434.431 | 73.7257 | 85.8565 | 9.80613 | 0.016868 | 0.00192658 | 27.657 | 1 | 1.84538 | 1.84538 | 0 | 6.41347 | F | F | 2.2e+20 | 1.34954e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X122843.57+132558.7 | chandra | ccd5 | 924.71 | 132.51 | 49.6032 | 10.0004 | 0.00974537 | 0.00196474 | 37.4326 | 1 | 7.50736 | 5.89373 | 79.2597 | 11.6838 | F | F | 2.48e+20 | 9.7395e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X122903.13+131058.5 | chandra | ccd7 | 355.87 | 387.223 | 15.2195 | 4.91829 | 0.00299013 | 0.000966281 | 4.90267 | 0.999974 | 1.13186 | 1.13186 | 0 | 4.06982 | F | F | 2.23e+20 | 2.27001e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X122847.13+131808.6 | chandra | ccd6 | 826.725 | 219.531 | 13.0927 | 4.01179 | 0.00257228 | 0.000788183 | 7.55687 | 1 | 2.0701 | 0.530524 | 87.1843 | 4.15328 | A | F | 2.37e+20 | 2.86534e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X122847.90+132014.4 | chandra | ccd6 | 803.318 | 474.591 | 10.6921 | 3.31663 | 0.00210064 | 0.000651607 | 6.17129 | 0.999997 | 0.511015 | 0.492 | 80.9979 | 5.90746 | F | F | 2.39e+20 | 2.62975e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X122900.80+132559.0 | chandra | ccd5 | 413.633 | 133.167 | 9.20136 | 3.87308 | 0.00180776 | 0.000760931 | 6.94372 | 0.999998 | 3.96522 | 1.1312 | 124.973 | 11.2663 | A | F | 2.43e+20 | 1.72296e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X122848.58+132224.1 | chandra | ccd6 | 783.056 | 738.278 | 8.29294 | 3.00001 | 0.00162929 | 0.000589403 | 4.78654 | 0.999928 | 1.5369 | 0.492 | 29.4249 | 7.91066 | A | F | 2.42e+20 | 1.9554e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X122844.98+131811.1 | chandra | ccd6 | 890.125 | 224 | 7.8074 | 2.82843 | 0.00153389 | 0.000555692 | 4.50629 | 0.999706 | 0.755123 | 0.492 | 153.927 | 4.49759 | A | F | 2.37e+20 | 1.74825e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X122840.26+132411.2 | chandra | ccd6 | 1029.9 | 956 | 7.43399 | 3.16236 | 0.00146053 | 0.000621298 | 4.29076 | 0.999706 | 2.40182 | 1.53581 | 96.4604 | 10.2661 | A | F | 2.46e+20 | 2.77522e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X122901.03+131926.2 | chandra | ccd6 | 413.9 | 376.7 | 4.89414 | 2.23607 | 0.000961535 | 0.000439313 | 2.82481 | 0.988058 | 0.492 | 0.492 | 69.1832 | 4.78394 | F | F | 2.35e+20 | 1.07403e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X122847.34+131824.2 | chandra | ccd6 | 820 | 250.75 | 3.91545 | 2 | 0.000769255 | 0.000392934 | 2.25993 | 0.966403 | 0.492 | 0.492 | 142.018 | 4.33149 | F | F | 2.37e+20 | 8.58739e-15 | 1 | dx | ||||
| Report | 1 | X122926.46+131541.3 | chandra | ccd2 | 1017.17 | 103.833 | 2.73156 | 1.73207 | 0.00053666 | 0.000340293 | 3.68758 | 0.997555 | 0.492 | 0.492 | 45 | 7.24224 | F | F | 2.23e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf rmf | 2 | X122926.50+132019.6 | chandra | ccd2 | 1016.81 | 670.011 | 224.3 | 14.9766 | 0.0440677 | 0.00294243 | 302.803 | 1 | 3.7649 | 2.97082 | 1.84531 | 9.09233 | F | F | 2.29e+20 | 6.76611e-13 | 1 | dsxf |
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