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 | X161414.12+544251.4 | chandra | ccd1 | 176.768 | 625.469 | 244.034 | 16.5906 | 0.0530487 | 0.00360652 | 43.6784 | 1 | 3.58378 | 2.64079 | 4.83081 | 9.43238 | F | F | 1.12e+20 | 6.80313e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 6 | X161340.21+543828.2 | chandra | ccd1 | 772.591 | 88.4092 | 40.5656 | 6.48075 | 0.00881822 | 0.0014088 | 7.26063 | 1 | 1.2194 | 0.892562 | 23.0504 | 8.27481 | F | F | 1.07e+20 | 1.25951e-13 | 1 | dx | ||||
| Report | 3 | X161303.47+544316.8 | chandra | ccd3 | 391.6 | 876.5 | 9.98852 | 3.16228 | 0.00217132 | 0.000687421 | 19.9802 | 1 | 0.492 | 0.492 | 141.34 | 2.64622 | F | F | 1.05e+20 | 0 | 1 | d | |||||
| Report | 4 | X161306.28+544855.6 | chandra | ccd2 | 138.8 | 527.1 | 9.93812 | 3.16228 | 0.00216187 | 0.0006879 | 20.1121 | 1 | 0.576818 | 0.492 | 124.83 | 3.37166 | F | F | 1.07e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X161226.62+544330.8 | chandra | ccd3 | 1040.33 | 906.167 | 5.79321 | 2.44949 | 0.00125934 | 0.000532475 | 11.5883 | 1 | 1.0263 | 0.492 | 68.1447 | 6.84281 | A | F | 1.03e+20 | 1.71716e-14 | 1 | dx | ||||
| Report | 1 | X161313.57+544355.4 | chandra | ccd3 | 213.7 | 955.1 | 4.93449 | 2.23607 | 0.00107267 | 0.000486081 | 9.87055 | 1 | 0.492 | 0.492 | 161.565 | 1.7427 | F | F | 1.06e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X161251.13+544812.1 | chandra | ccd2 | 405.1 | 438.9 | 4.92405 | 2.23607 | 0.00107114 | 0.000486419 | 9.96496 | 1 | 0.495065 | 0.492 | 45 | 3.91265 | F | F | 1.06e+20 | 1.29857e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X161327.16+545254.9 | chandra | ccd0 | 784.5 | 813.7 | 4.85921 | 2.23607 | 0.00105704 | 0.000486419 | 9.80317 | 1 | 1.3489 | 0.492 | 89.1161 | 7.60414 | A | F | 1.11e+20 | 1.41388e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X161400.83+544732.3 | chandra | ccd0 | 192.072 | 159.071 | 6.60667 | 2.64576 | 0.00143717 | 0.00057554 | 13.3286 | 1 | 1.3709 | 0.722164 | 110.924 | 7.33535 | A | F | 1.13e+20 | 1.92188e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X161322.30+545044.3 | chandra | ccd0 | 869.5 | 548.25 | 3.93453 | 2 | 0.000855891 | 0.000435067 | 7.93769 | 0.999994 | 0.668034 | 0.492 | 100.205 | 5.31885 | F | F | 1.09e+20 | 1.06571e-14 | 1 | dx | ||||
| Report | 4 | X161336.76+544657.5 | chandra | ccd0 | 615 | 87.5 | 3.94902 | 2 | 0.000859041 | 0.000435066 | 7.96691 | 0.999994 | 0.492 | 0.492 | 16.845 | 3.84825 | F | F | 1.1e+20 | 0 | 1 | d | |||||
| Report | 1 | X161243.49+544626.0 | chandra | ccd2 | 539.75 | 223.5 | 3.91687 | 2 | 0.00085205 | 0.000435067 | 7.92671 | 0.999994 | 0.521845 | 0.492 | 90 | 4.14145 | F | F | 1.05e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X161239.31+544527.4 | chandra | ccd2 | 613.5 | 104.5 | 0.977312 | 1 | 0.000212598 | 0.000217533 | 1.97782 | 0.974626 | 0.492 | 0.492 | 90 | 4.67354 | F | F | 1.04e+20 | 2.72442e-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