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 | X115250.15+395114.4 | chandra | ccd2 | 1152.3 | 476.1 | 4.97989 | 2.23607 | 0.00245502 | 0.00110236 | 12.7624 | 1 | 0.492 | 0.492 | 82.3724 | 4.64064 | F | F | 1.9e+20 | 0 | 1 | d | |||||
| Report | 3 | X115240.43+394601.9 | chandra | ccd3 | 573.5 | 449 | 3.96554 | 2 | 0.00195497 | 0.000985977 | 9.66289 | 0.999999 | 0.492 | 0.492 | 90 | 4.81982 | F | F | 2.01e+20 | 0 | 1 | d | |||||
| Report | 1 | X115239.98+394804.9 | chandra | ccd3 | 583.75 | 699 | 3.95484 | 2 | 0.00194969 | 0.000985977 | 9.6368 | 0.999999 | 0.554428 | 0.492 | 10.5806 | 4.71828 | F | F | 1.97e+20 | 0 | 1 | d | |||||
| Report | 1 | X115331.82+394603.4 | chandra | ccd0 | 863.167 | 636.167 | 2.9851 | 1.73205 | 0.00147387 | 0.000855188 | 7.6488 | 0.99998 | 0.492 | 0.492 | 45 | 5.46848 | F | F | 1.98e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X115243.20+395125.9 | chandra | ccd3 | 507.833 | 1107.5 | 2.98896 | 1.73205 | 0.00147352 | 0.000853881 | 7.28323 | 0.999971 | 0.492 | 0.492 | 180 | 5.66158 | F | F | 1.9e+20 | 2.05901e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X115257.93+394222.3 | chandra | ccd1 | 819.5 | 854.5 | 2.96128 | 1.73205 | 0.00145988 | 0.000853881 | 7.39242 | 0.999976 | 0.492 | 0.492 | 180 | 5.25953 | F | F | 2.08e+20 | 1.78563e-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