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 | 1 | X013644.12+154818.7 | chandra | ccd7 | 501.702 | 636.37 | 32.089 | 5.70372 | 0.00607385 | 0.00107961 | 31.7021 | 1 | 0.937779 | 0.489299 | 348.427 | 3.53412 | F | F | 4.66e+20 | 0 | 1 | ds | |||||
| Report | 1 | X013646.10+154120.4 | chandra | ccd6 | 657 | 787.7 | 9.8433 | 3.16228 | 0.00186315 | 0.000598561 | 15.9056 | 1 | 0.889741 | 0.492 | 103.002 | 4.06102 | A | F | 4.59e+20 | 0 | 1 | d | |||||
| Report | 3 | X013641.73+154701.1 | chandra | ccd7 | 571.389 | 478.278 | 8.7948 | 3 | 0.00166469 | 0.000567844 | 8.68877 | 1 | 0.59969 | 0.492 | 168.203 | 2.90455 | F | F | 4.6e+20 | 0 | 1 | d | |||||
| Report | 2 | X013647.47+154744.9 | chandra | ccd7 | 402.833 | 567.167 | 8.68313 | 3.00001 | 0.00164355 | 0.000567845 | 8.57845 | 1 | 0.492 | 0.492 | 45 | 2.68766 | F | F | 4.66e+20 | 0 | 1 | d | |||||
| Report | 3 | X013650.63+154011.5 | chandra | ccd6 | 524.125 | 647.75 | 7.86394 | 2.82843 | 0.0014885 | 0.000535369 | 12.7072 | 1 | 0.900938 | 0.492 | 108.883 | 5.02219 | A | F | 4.59e+20 | 0 | 1 | d | |||||
| Report | 10 | X013646.04+154423.2 | chandra | ccd7 | 444.75 | 157.25 | 7.86095 | 2.82843 | 0.00148793 | 0.000535369 | 7.76618 | 0.999999 | 0.492 | 0.492 | 13.2825 | 1.48681 | F | F | 4.6e+20 | 0 | 1 | d | |||||
| Report | 4 | X013651.06+154547.4 | chandra | ccd7 | 297.625 | 328.5 | 7.7674 | 2.82843 | 0.00147022 | 0.000535369 | 7.67375 | 0.999999 | 0.492 | 0.492 | 41.879 | 0.578864 | F | F | 4.61e+20 | 0 | 1 | d | |||||
| Report | 8 | X013646.18+154842.1 | chandra | ccd7 | 440.625 | 683.5 | 7.70988 | 2.82843 | 0.00145934 | 0.000535369 | 7.61694 | 0.999999 | 0.704765 | 0.492 | 29.8313 | 3.69045 | F | F | 4.67e+20 | 0 | 1 | d | |||||
| Report | 9 | X013650.01+154931.2 | chandra | ccd7 | 328.357 | 783.214 | 6.71395 | 2.64576 | 0.00127083 | 0.000500792 | 6.63301 | 0.999988 | 0.657474 | 0.492 | 77.9272 | 4.31596 | F | F | 4.68e+20 | 0 | 1 | d | |||||
| Report | 5 | X013641.70+154552.8 | chandra | ccd7 | 572.167 | 339.5 | 5.87359 | 2.44949 | 0.00111176 | 0.000463643 | 5.80278 | 0.999903 | 0.492 | 0.492 | 180 | 2.37685 | F | F | 4.6e+20 | 0 | 1 | d | |||||
| Report | 6 | X013644.93+154546.2 | chandra | ccd7 | 477.5 | 325.9 | 4.7228 | 2.23608 | 0.000893937 | 0.000423247 | 4.66586 | 0.999327 | 0.580128 | 0.492 | 169.838 | 1.60441 | F | F | 4.6e+20 | 0 | 1 | d | |||||
| Report | 2 | X013659.55+154015.6 | chandra | ccd6 | 262.25 | 656 | 3.90249 | 2 | 0.000738669 | 0.000378563 | 6.30597 | 0.99995 | 0.492 | 0.492 | 57.1139 | 5.34706 | F | F | 4.6e+20 | 0 | 1 | d | |||||
| Report | 7 | X013652.34+154737.7 | chandra | ccd7 | 260 | 552.5 | 3.81166 | 2.00001 | 0.000721476 | 0.000378564 | 3.76571 | 0.99595 | 0.521845 | 0.492 | 90 | 2.43094 | F | F | 4.67e+20 | 0 | 1 | d | |||||
| Report | 2 | X013621.48+153711.8 | chandra | ccd2 | 190.572 | 200.18 | 13.8135 | 4.47347 | 0.00261465 | 0.000846746 | 5.54835 | 0.999998 | 2.66099 | 2.66099 | 0 | 10.7456 | F | F | 4.55e+20 | 0 | 1 | ds | |||||
| Report | 4 | X013655.34+153740.5 | chandra | ccd6 | 385.833 | 340.833 | 2.86889 | 1.73206 | 0.000543027 | 0.000327846 | 4.63579 | 0.999339 | 0.492 | 0.492 | 90 | 7.60345 | F | F | 4.58e+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