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 | 4 | X143500.54+535953.6 | chandra | ccd7 | 612.239 | 886.379 | 33.3473 | 5.85029 | 0.0214143 | 0.00375682 | 35.577 | 1 | 0.37871 | 0.37871 | 0 | 0.211333 | F | F | 1.1e+20 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 1 | X143459.59+540859.0 | chandra | ccd6 | 451.833 | 963.333 | 5.88544 | 3.59808 | 0.0037793 | 0.00231048 | 17.3882 | 1 | 2.31935 | 0.784525 | 91.8208 | 8.99828 | 2.94272 | 2.94272 | 0 | 0.449542 | A | F | 1.13e+20 | 5.03744e-14 | 1 | dx |
| Report | 1 | X143501.50+535732.2 | chandra | ccd7 | 594.5 | 598.5 | 4.95764 | 2.23607 | 0.00318352 | 0.00143588 | 5.28913 | 0.999697 | 0.492 | 0.492 | 45 | 2.47013 | F | F | 1.1e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X143525.62+535851.4 | chandra | ccd7 | 162.1 | 759.9 | 6.83547 | 3.78388 | 0.00438935 | 0.0024298 | 16.8517 | 1 | 0.506784 | 0.492 | 169.099 | 4.03746 | 2.91773 | 2.91773 | 0 | 0.453391 | F | F | 1.1e+20 | 3.83941e-14 | 1 | dx |
| Report | 2 | X143433.08+540132.8 | chandra | ccd6 | 926.5 | 56.8335 | 2.97588 | 1.73205 | 0.00191094 | 0.00111223 | 10.2123 | 0.999998 | 0.550073 | 0.492 | 18.4349 | 4.14818 | F | F | 1.11e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X143454.20+535758.1 | chandra | ccd7 | 725.5 | 651.167 | 2.94482 | 2.93649 | 0.001891 | 0.00188565 | 12.5362 | 1 | 0.755039 | 0.492 | 37.2379 | 2.14809 | 1 | 2 | 0.333333 | 1.05409 | A | F | 1.1e+20 | 1.4337e-14 | 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