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 rmf | 3 | X185609.55+021743.9 | chandra | ccd7 | 466.636 | 807.841 | 190.618 | 14.122 | 0.13558 | 0.0100445 | 64.2067 | 1 | 0.402414 | 0.402414 | 0 | 0.896054 | F | F | 1.47e+22 | 6.54931e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X185625.63+022819.3 | chandra | ccd5 | 349.963 | 42.131 | 28.8055 | 7.04823 | 0.0204882 | 0.00501313 | 6.30512 | 1 | 5.79802 | 4.53821 | 16.9679 | 10.8153 | F | F | 1.48e+22 | 3.99894e-13 | 1 | dsx | ||||
| Report | 1 | X185605.53+021822.0 | chandra | ccd7 | 588.625 | 884.75 | 7.96071 | 2.82843 | 0.00566208 | 0.00201173 | 2.68144 | 0.990786 | 0.492 | 0.492 | 149.405 | 0.489496 | F | F | 1.47e+22 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X185622.57+022214.5 | chandra | ccd6 | 257.5 | 270.25 | 3.92758 | 2 | 0.0027935 | 0.00142251 | 10.4689 | 1 | 0.514845 | 0.492 | 30.7785 | 5.34456 | F | F | 1.47e+22 | 4.75786e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X185643.33+021920.6 | chandra | ccd2 | 906.25 | 413.75 | 3.38785 | 2.00002 | 0.00240962 | 0.00142252 | 9.50917 | 0.99999 | 2.20272 | 0.759911 | 156.613 | 9.00401 | A | F | 1.44e+22 | 4.60082e-14 | 1 | dcx | ||||
| Report | 2 | X185613.36+022209.5 | chandra | ccd6 | 538.167 | 260.167 | 2.98781 | 1.73205 | 0.00212509 | 0.00123193 | 7.964 | 0.999985 | 0.492 | 0.492 | 45 | 3.98263 | F | F | 1.47e+22 | 0 | 1 | d | |||||
| Report | 3 | X185613.93+022002.1 | chandra | ccd6 | 520.833 | 1.1665 | 2.96452 | 1.73205 | 0.00210852 | 0.00123193 | 7.90191 | 0.999985 | 0.569535 | 0.492 | 36.6504 | 2.25765 | F | F | 1.47e+22 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X185643.74+021920.9 | chandra | ccd2 | 893.833 | 414.5 | 2.59408 | 1.73207 | 0.00184505 | 0.00123194 | 7.28119 | 0.99969 | 0.952754 | 0.550073 | 18.4349 | 9.10594 | A | F | 1.44e+22 | 3.5063e-14 | 1 | dcx |
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