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 | 3 | X171419.23+611944.8 | chandra | ccd7 | 461.173 | 595.112 | 51.2789 | 7.21111 | 0.0110938 | 0.00156006 | 35.0919 | 1 | 0.492 | 0.492 | 161.27 | 0.570809 | F | F | 2.17e+20 | 7.49677e-14 | 1 | dpx | ||||
| Report | srcpi bgdpi arf | 1 | X171431.19+612242.7 | chandra | ccd7 | 286.879 | 957.324 | 17.6617 | 4.20258 | 0.00416237 | 0.000990431 | 12.0865 | 1 | 0.826763 | 0.826763 | 0 | 3.44074 | F | F | 2.16e+20 | 3.14131e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X171347.79+612519.3 | chandra | ccd7 | 920.104 | 1276.03 | 11.6138 | 4.70786 | 0.00273706 | 0.00110951 | 7.94773 | 1 | 1.82304 | 0.883887 | 30.0331 | 7.26112 | F | F | 2.15e+20 | 2.20619e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X171412.71+611942.8 | chandra | ccd7 | 557.1 | 591.656 | 18.8596 | 4.34276 | 0.00444469 | 0.00102347 | 12.9063 | 1 | 0.379792 | 0.379792 | 0 | 1.2799 | F | F | 2.17e+20 | 3.01123e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X171353.29+611900.1 | chandra | ccd7 | 841.316 | 505.192 | 11.6547 | 3.4139 | 0.00274669 | 0.00080456 | 7.97572 | 1 | 0.94489 | 0.94489 | 0 | 3.59545 | F | F | 2.17e+20 | 1.92667e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X171449.35+612216.7 | chandra | ccd7 | 21.1365 | 904.136 | 10.3382 | 3.31665 | 0.00223657 | 0.000717529 | 7.07477 | 1 | 0.920081 | 0.492 | 67.0724 | 4.26042 | A | F | 2.16e+20 | 2.377e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X171326.64+611950.4 | chandra | ccd7 | 1230.33 | 607.917 | 9.8315 | 3.46414 | 0.00212696 | 0.000749438 | 6.72804 | 0.999997 | 1.28058 | 0.953108 | 107.153 | 6.78216 | F | F | 2.16e+20 | 1.6248e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X171406.28+612009.1 | chandra | ccd7 | 650.625 | 644.625 | 7.55639 | 2.82844 | 0.00163476 | 0.000611909 | 5.17111 | 0.999921 | 0.492 | 0.492 | 17.8533 | 2.14684 | F | F | 2.17e+20 | 1.11866e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X171411.76+611833.2 | chandra | ccd7 | 570.5 | 449.643 | 6.59301 | 2.64576 | 0.00142634 | 0.000572388 | 4.51183 | 0.99962 | 0.556385 | 0.492 | 159.047 | 1.60437 | F | T | 2.17e+20 | 9.67017e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X171401.59+612320.0 | chandra | ccd7 | 718.667 | 1032.67 | 5.45066 | 2.4495 | 0.0011792 | 0.000529929 | 3.73008 | 0.998353 | 0.762437 | 0.492 | 11.5352 | 4.69272 | A | F | 2.16e+20 | 8.46686e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 12 | X171358.91+611813.1 | chandra | ccd7 | 758.7 | 409.1 | 4.66368 | 2.23608 | 0.00100895 | 0.000483757 | 3.19152 | 0.993606 | 0.492 | 0.492 | 58.2825 | 3.13429 | F | F | 2.18e+20 | 7.10319e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 11 | X171356.73+612226.6 | chandra | ccd7 | 789.75 | 924.25 | 3.67125 | 2.00001 | 0.000794245 | 0.000432685 | 2.51237 | 0.978043 | 0.492 | 0.492 | 159.407 | 4.37851 | F | F | 2.16e+20 | 5.60025e-15 | 1 | dx | ||||
| Report | 2 | X171447.35+612009.2 | chandra | ccd6 | 939.928 | 1081.93 | 6.91654 | 2.64575 | 0.00149633 | 0.000572387 | 10.422 | 1 | 0.492 | 0.492 | 45 | 3.00554 | F | F | 2.17e+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