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 | 2 | X063715.98+184103.1 | chandra | ccd3 | 141.212 | 329.798 | 44.5993 | 6.67827 | 0.00561317 | 0.000840513 | 70.3322 | 1 | 2.90304 | 1.79326 | 99.0479 | 7.28647 | F | F | 3.08e+21 | 7.24578e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X063632.33+184419.1 | chandra | ccd1 | 332.686 | 804 | 16.5684 | 5.31677 | 0.00208445 | 0.000668896 | 4.8439 | 0.999986 | 1.01515 | 1.01515 | 0 | 6.74612 | F | F | 3.1e+21 | 2.56173e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X063650.36+183607.0 | chandra | ccd2 | 931.025 | 769.601 | 12.5761 | 3.54628 | 0.00158219 | 0.000446154 | 20.3477 | 1 | 0.703405 | 0.357705 | 64.3122 | 2.5542 | F | F | 3.12e+21 | 1.93619e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X063712.16+184436.6 | chandra | ccd3 | 251.318 | 763.045 | 10.5039 | 3.31663 | 0.001322 | 0.000417424 | 16.5644 | 1 | 1.59083 | 1.06664 | 39.1272 | 8.48176 | F | F | 3.06e+21 | 1.79106e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X063650.66+183228.3 | chandra | ccd2 | 921.7 | 324.6 | 9.61849 | 3.16228 | 0.00121009 | 0.000397843 | 15.5624 | 1 | 1.14638 | 0.492 | 136.632 | 6.13821 | A | F | 3.14e+21 | 1.46975e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X063634.37+183948.0 | chandra | ccd1 | 273.5 | 252.278 | 8.90214 | 3 | 0.00111997 | 0.000377427 | 2.60261 | 0.991033 | 0.492 | 0.492 | 15.9137 | 3.26196 | F | T | 3.12e+21 | 1.256e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X063654.86+183006.5 | chandra | ccd2 | 800.389 | 36.5 | 8.03774 | 3.00002 | 0.00101122 | 0.000377429 | 13.0048 | 1 | 1.74816 | 1.59847 | 90 | 8.64048 | F | F | 3.15e+21 | 1.41803e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X063720.70+183345.5 | chandra | ccd2 | 53.625 | 482 | 7.05923 | 2.82845 | 0.000888113 | 0.000355844 | 11.4216 | 1 | 2.85687 | 1.00498 | 69.9194 | 9.29399 | A | F | 3.11e+21 | 1.21644e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X063706.77+183803.3 | chandra | ccd2 | 456.5 | 1005.67 | 5.88918 | 2.44949 | 0.00074091 | 0.000308168 | 9.52847 | 1 | 0.734667 | 0.492 | 28.3924 | 4.68788 | F | T | 3.09e+21 | 9.12478e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X063708.55+183701.0 | chandra | ccd2 | 405.1 | 879.1 | 4.88302 | 2.23607 | 0.000614327 | 0.000281317 | 7.90054 | 0.999997 | 0.51392 | 0.492 | 164.518 | 5.30919 | F | F | 3.1e+21 | 7.6484e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X063633.83+183521.1 | chandra | ccd0 | 372.1 | 724.9 | 4.83887 | 2.23607 | 0.000608772 | 0.000281318 | 7.83802 | 0.999997 | 0.780386 | 0.492 | 164.518 | 4.48341 | A | F | 3.14e+21 | 7.10904e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X063636.59+183138.2 | chandra | ccd0 | 292.5 | 271.9 | 4.65091 | 2.23608 | 0.000585125 | 0.000281318 | 7.53357 | 0.999997 | 0.89916 | 0.492 | 109.572 | 7.34772 | A | F | 3.16e+21 | 7.35892e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X063700.33+184220.6 | chandra | ccd3 | 592.75 | 486.5 | 3.93342 | 2 | 0.000495052 | 0.000251716 | 6.20293 | 0.999937 | 0.492 | 0.492 | 180 | 4.92015 | F | F | 3.08e+21 | 5.87812e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X063645.38+184022.5 | chandra | ccd3 | 1024.5 | 246.5 | 3.9264 | 2 | 0.000494168 | 0.000251716 | 6.19185 | 0.999937 | 0.492 | 0.492 | 45 | 1.86911 | F | F | 3.1e+21 | 5.55804e-15 | 1 | dx | ||||
| Report | 3 | X063647.81+184432.7 | chandra | ccd3 | 954.25 | 755 | 3.88535 | 2 | 0.000489002 | 0.000251716 | 6.12711 | 0.999937 | 0.492 | 0.492 | 127.982 | 5.99661 | F | T | 3.08e+21 | 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