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 | X093525.49+033756.4 | chandra | ccd7 | 203.386 | 591.719 | 86.3698 | 9.33696 | 0.0484706 | 0.00523988 | 96.0266 | 1 | 1.24717 | 0.611307 | 129.999 | 3.88515 | F | F | 2.7e+20 | 3.64308e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X093433.36+033330.7 | chandra | ccd2 | 488.068 | 987.182 | 37.274 | 6.63332 | 0.0209176 | 0.00372251 | 117.616 | 1 | 4.02699 | 3.41381 | 18.9553 | 10.3953 | F | F | 2.67e+20 | 2.76351e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X093530.18+033133.7 | chandra | ccd6 | 127 | 830.333 | 5.97114 | 2.44949 | 0.00335091 | 0.00137462 | 17.2017 | 1 | 0.496605 | 0.492 | 93.8826 | 5.34221 | F | F | 2.68e+20 | 3.7261e-14 | 1 | dx | ||||
| Report | 1 | X093459.20+033652.3 | chandra | ccd7 | 1002.83 | 461 | 5.93327 | 2.44949 | 0.00332966 | 0.00137462 | 6.59665 | 0.999978 | 0.550073 | 0.510857 | 180 | 4.16585 | F | F | 2.68e+20 | 0 | 1 | d | |||||
| Report | 4 | X093514.71+033545.6 | chandra | ccd7 | 530.9 | 325.3 | 4.95691 | 2.23607 | 0.00278174 | 0.00125485 | 5.51113 | 0.999804 | 0.492 | 0.492 | 76.7175 | 0.571233 | F | F | 2.69e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X093502.97+032929.4 | chandra | ccd6 | 955.25 | 577.75 | 3.77485 | 2.00001 | 0.00211839 | 0.00112237 | 10.8746 | 0.999992 | 1.41418 | 0.545719 | 20.2696 | 6.38362 | A | F | 2.66e+20 | 2.43989e-14 | 1 | dx | ||||
| Report | 3 | X093512.02+033526.5 | chandra | ccd7 | 612.833 | 286.5 | 2.97478 | 1.73205 | 0.0016694 | 0.000972 | 3.30738 | 0.990571 | 0.492 | 0.492 | 180 | 0.662644 | F | F | 2.69e+20 | 0 | 1 | d | |||||
| Report | 2 | X093441.95+033831.3 | chandra | ccd3 | 119.5 | 566.167 | 2.92692 | 1.73205 | 0.00164254 | 0.000972 | 9.17429 | 0.999996 | 1.42913 | 0.492 | 164.745 | 8.77086 | A | F | 2.69e+20 | 0 | 1 | d | |||||
| Report | 1 | X093443.56+034236.0 | chandra | ccd3 | 70.5 | 1063.5 | 0.999987 | 1 | 0.000561177 | 0.000561184 | 3.13441 | 0.995158 | 0.492 | 0.492 | 90 | 10.6942 | F | F | 2.7e+20 | 0 | 1 | d |
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