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 | X194246.67+452003.6 | chandra | ccd7 | 991.978 | 978.64 | 40.5878 | 6.37123 | 0.0148343 | 0.0023286 | 56.6679 | 1 | 0.408275 | 0.408275 | 0 | 0.810046 | F | F | 1.37e+21 | 1.13134e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X194254.61+451530.2 | chandra | ccd7 | 821.595 | 422.923 | 18.891 | 4.34638 | 0.00690442 | 0.00158855 | 26.3753 | 1 | 2.04443 | 0.737255 | 1.67956 | 4.15441 | T | F | 1.39e+21 | 5.57159e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X194227.75+452244.1 | chandra | ccd6 | 678.043 | 560.101 | 17.1455 | 4.14071 | 0.00626645 | 0.00151337 | 37.4951 | 1 | 1.71273 | 0.975994 | 89.7582 | 5.06686 | F | F | 1.35e+21 | 6.65974e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X194256.85+451841.0 | chandra | ccd7 | 773.167 | 810.389 | 8.83939 | 3 | 0.00323064 | 0.00109645 | 12.3414 | 1 | 0.517477 | 0.492 | 103.675 | 1.44917 | F | F | 1.38e+21 | 2.48621e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X194334.67+452221.4 | chandra | ccd3 | 1079.3 | 467.3 | 4.74842 | 2.23608 | 0.00173546 | 0.000817246 | 10.7871 | 0.999998 | 1.02871 | 0.633567 | 177.145 | 8.25142 | A | F | 1.37e+21 | 2.2685e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X194224.74+452511.4 | chandra | ccd6 | 741.75 | 859.25 | 3.87315 | 2 | 0.00141557 | 0.000730966 | 8.4701 | 0.999997 | 0.492 | 0.492 | 100.278 | 7.19106 | F | F | 1.34e+21 | 1.57542e-14 | 1 | dx | ||||
Report | 1 | X194314.95+452523.6 | chandra | ccd2 | 772.167 | 76.8335 | 2.64713 | 1.73207 | 0.00096748 | 0.000633042 | 6.03956 | 0.998976 | 0.563657 | 0.492 | 45 | 7.22568 | F | F | 1.36e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X194221.66+452605.9 | chandra | ccd6 | 807.5 | 970 | 1.95547 | 1.41422 | 0.000714689 | 0.000516871 | 4.27636 | 0.998696 | 1.44099 | 0.492 | 39.8056 | 8.23794 | A | F | 1.34e+21 | 8.18779e-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