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 | 8 | X122626.10+084847.5 | chandra | ccd7 | 662.233 | 525.514 | 33.2019 | 5.76211 | 0.00655563 | 0.00113771 | 34.4347 | 1 | 1.02583 | 0.509936 | 132.769 | 3.96004 | F | F | 1.46e+20 | 4.94557e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X122622.16+085124.1 | chandra | ccd7 | 781.083 | 843.784 | 25.0369 | 5.20827 | 0.00494349 | 0.00102836 | 25.9666 | 1 | 0.521826 | 0.521826 | 0 | 2.30276 | F | F | 1.46e+20 | 3.66103e-14 | 1 | dsx | ||||
| Report | 2 | X122627.85+085145.0 | chandra | ccd7 | 609.482 | 886.181 | 20.789 | 4.59874 | 0.00410473 | 0.000908009 | 21.5609 | 1 | 0.361703 | 0.361703 | 0 | 1.03125 | F | F | 1.46e+20 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 1 | X122708.97+085415.5 | chandra | ccd2 | 985.583 | 1082.83 | 9.71616 | 3.46414 | 0.00191843 | 0.000683985 | 11.9851 | 1 | 2.1037 | 1.91607 | 39.6902 | 9.75109 | F | F | 1.44e+20 | 2.99933e-14 | 1 | dx | ||||
| Report | 5 | X122631.55+085433.3 | chandra | ccd6 | 1014.5 | 276.944 | 8.92334 | 3 | 0.00176189 | 0.000592342 | 13.586 | 1 | 0.563741 | 0.492 | 147.962 | 1.96234 | F | F | 1.46e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X122632.12+090102.9 | chandra | ccd6 | 997.375 | 1068.75 | 6.87464 | 2.82845 | 0.00135738 | 0.00055847 | 10.4668 | 1 | 2.89785 | 1.73561 | 71.4904 | 8.435 | A | F | 1.46e+20 | 1.77414e-14 | 1 | dx | ||||
| Report | 3 | X122631.61+085228.2 | chandra | ccd7 | 495.786 | 973.643 | 6.78261 | 2.64576 | 0.00133921 | 0.000522397 | 7.03446 | 0.999994 | 0.50026 | 0.492 | 91.7341 | 0.418433 | F | F | 1.46e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X122629.41+085541.8 | chandra | ccd6 | 1079.17 | 416 | 5.94484 | 2.44949 | 0.00117379 | 0.000483645 | 9.05119 | 1 | 0.492 | 0.492 | 102.821 | 3.07082 | F | F | 1.46e+20 | 1.27939e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X122711.45+084906.4 | chandra | ccd2 | 910.5 | 454.667 | 5.45009 | 2.4495 | 0.00107611 | 0.000483647 | 6.72278 | 0.999994 | 0.838166 | 0.492 | 10.8352 | 10.8184 | A | F | 1.44e+20 | 1.70363e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X122648.65+085339.2 | chandra | ccd6 | 499.7 | 166.9 | 4.88662 | 2.23607 | 0.000964849 | 0.000441506 | 7.44002 | 0.999994 | 0.585852 | 0.492 | 46.0227 | 4.70723 | F | F | 1.45e+20 | 1.14522e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X122642.87+085038.6 | chandra | ccd7 | 156.7 | 750.9 | 4.7053 | 2.23608 | 0.000929049 | 0.000441507 | 4.88002 | 0.999593 | 0.567373 | 0.492 | 21.4395 | 3.73834 | F | F | 1.45e+20 | 7.88415e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X122643.39+085601.8 | chandra | ccd6 | 658 | 456.75 | 3.91749 | 2 | 0.000773498 | 0.000394895 | 5.9645 | 0.999913 | 0.492 | 0.492 | 11.9812 | 4.73632 | F | F | 1.45e+20 | 8.88395e-15 | 1 | dx | ||||
| Report | 6 | X122619.17+085102.7 | chandra | ccd7 | 870.5 | 799.833 | 3.87483 | 2 | 0.000765075 | 0.000394895 | 4.01871 | 0.997309 | 0.492 | 0.492 | 90 | 3.11783 | F | F | 1.46e+20 | 0 | 1 | d | |||||
| Report | 4 | X122626.28+084733.5 | chandra | ccd7 | 656.5 | 374.5 | 2.80402 | 1.73206 | 0.000553646 | 0.00034199 | 2.90814 | 0.985024 | 0.521845 | 0.492 | 90 | 5.15639 | F | F | 1.46e+20 | 0 | 1 | d |
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