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 | 1 | X135839.45+372736.5 | chandra | ccd7 | 692.741 | 1013.82 | 62.2596 | 7.92976 | 0.00397781 | 0.000506638 | 33.6742 | 1 | 0.521122 | 0.521122 | 0 | 2.13863 | F | F | 9.84e+19 | 3.01988e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X135837.97+372528.2 | chandra | ccd7 | 728.625 | 753.18 | 67.4046 | 8.81572 | 0.00430653 | 0.000563243 | 36.457 | 1 | 0.407498 | 0.407498 | 0 | 0.288046 | F | F | 9.83e+19 | 3.18592e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X135846.50+372336.4 | chandra | ccd7 | 521.375 | 525.375 | 7.5185 | 2.82844 | 0.000480361 | 0.00018071 | 4.06652 | 0.999154 | 0.492 | 0.492 | 11.8147 | 2.76732 | F | F | 9.73e+19 | 3.9361e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X135837.92+372440.7 | chandra | ccd7 | 729.278 | 656.056 | 8.59688 | 3.00001 | 0.000549259 | 0.000191672 | 4.64978 | 0.99994 | 0.492 | 0.492 | 87.6182 | 0.909237 | F | F | 9.83e+19 | 4.0743e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X135838.75+372531.9 | chandra | ccd7 | 709.709 | 760.571 | 13.6799 | 4.46144 | 0.000874021 | 0.000285045 | 7.39902 | 1 | 0.322839 | 0.322839 | 0 | 0.434248 | F | F | 9.83e+19 | 6.45656e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X135837.80+372533.2 | chandra | ccd7 | 732.045 | 762.682 | 9.73262 | 3.31665 | 0.000621822 | 0.000211902 | 5.26406 | 0.999986 | 0.735443 | 0.492 | 9.30644 | 0.245691 | T | F | 9.84e+19 | 4.60074e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X135839.61+372627.8 | chandra | ccd7 | 688.333 | 873.667 | 5.6127 | 2.4495 | 0.000358598 | 0.0001565 | 3.03573 | 0.997187 | 0.492 | 0.492 | 109.903 | 1.09697 | F | F | 9.83e+19 | 2.67255e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X135844.72+372058.3 | chandra | ccd7 | 564.375 | 204 | 7.22614 | 2.82845 | 0.000461682 | 0.000180712 | 3.90839 | 0.999154 | 1.0539 | 0.492 | 40.861 | 4.85409 | A | F | 9.73e+19 | 6.3545e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X135900.93+372201.9 | chandra | ccd7 | 171.633 | 333.7 | 12.3766 | 3.87302 | 0.000790745 | 0.00024745 | 6.69409 | 0.999999 | 1.39289 | 0.648986 | 179.863 | 5.9808 | A | F | 9.58e+19 | 6.27888e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X135839.23+372524.4 | chandra | ccd7 | 697.611 | 744.944 | 7.83154 | 3.00002 | 0.000500361 | 0.000191673 | 4.23583 | 0.999766 | 0.541848 | 0.492 | 55.0476 | 0.546198 | F | F | 9.82e+19 | 3.92498e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 11 | X135838.75+372707.4 | chandra | ccd7 | 709.1 | 954.3 | 4.54606 | 2.23608 | 0.000290451 | 0.000142864 | 2.45882 | 0.976281 | 0.492 | 0.492 | 155.301 | 1.63543 | F | F | 9.84e+19 | 2.17741e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 12 | X135847.18+372115.5 | chandra | ccd7 | 505.366 | 239.524 | 47.1235 | 6.86466 | 0.00301075 | 0.000438587 | 25.4876 | 1 | 1.50424 | 0.817211 | 359.656 | 4.77904 | F | F | 9.7e+19 | 2.34309e-14 | 1 | dsx |
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