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 | 5 | X014251.77+133352.5 | chandra | ccd6 | 1254.14 | 846.218 | 53.0307 | 7.28222 | 0.0104708 | 0.00143786 | 99.8435 | 1 | 1.55306 | 0.752731 | 54.5278 | 4.83741 | F | F | 4.62e+20 | 1.16729e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X014302.31+133843.6 | chandra | ccd7 | 543.976 | 466.84 | 28.267 | 8.87843 | 0.00558127 | 0.00175303 | 7.55634 | 1 | 1.5 | 0.700429 | 199.887 | 0.736978 | T | F | 4.64e+20 | 3.75615e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X014302.47+133853.6 | chandra | ccd7 | 539.03 | 487.291 | 17.5364 | 4.79084 | 0.00346253 | 0.000945943 | 4.68783 | 0.999975 | 0.398676 | 0.398676 | 0 | 0.89438 | F | F | 4.64e+20 | 2.33332e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X014303.84+133955.5 | chandra | ccd7 | 498.506 | 613.084 | 14.2296 | 3.77221 | 0.00280961 | 0.000744817 | 3.80386 | 0.999704 | 0.490563 | 0.490563 | 0 | 1.96502 | F | F | 4.65e+20 | 1.9161e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X014301.17+134003.2 | chandra | ccd7 | 577.667 | 628.678 | 13.2802 | 3.6442 | 0.00262216 | 0.000719543 | 3.55006 | 0.999369 | 0.525996 | 0.525996 | 0 | 2.06595 | F | F | 4.65e+20 | 1.80012e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X014232.38+133239.6 | chandra | ccd2 | 484.357 | 1014.79 | 12.3383 | 3.74169 | 0.00243615 | 0.000738785 | 23.3107 | 1 | 2.71356 | 2.05799 | 102.987 | 8.9991 | F | F | 4.59e+20 | 3.07268e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X014310.19+133114.9 | chandra | ccd6 | 707.625 | 525.5 | 7.7034 | 2.82843 | 0.00152102 | 0.000558466 | 14.5036 | 1 | 1.17683 | 0.840485 | 122.28 | 7.02764 | F | F | 4.64e+20 | 1.62195e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X014219.19+133435.0 | chandra | ccd3 | 506.25 | 318.625 | 6.59807 | 2.82846 | 0.00130277 | 0.000558471 | 12.9341 | 1 | 2.79903 | 2.07946 | 35.2829 | 10.9925 | F | F | 4.58e+20 | 1.70425e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X014307.06+133130.2 | chandra | ccd6 | 800.5 | 556.5 | 5.62854 | 2.4495 | 0.00111134 | 0.000483647 | 10.5971 | 0.999999 | 0.843037 | 0.492 | 141.047 | 6.60564 | A | F | 4.63e+20 | 1.18019e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X014309.44+133458.5 | chandra | ccd6 | 730.1 | 979.9 | 4.96147 | 2.23607 | 0.000979629 | 0.000441505 | 9.34121 | 0.999999 | 0.492 | 0.492 | 20.9936 | 3.50224 | F | F | 4.64e+20 | 9.77455e-15 | 1 | dx | ||||
| Report | 3 | X014226.14+133419.3 | chandra | ccd3 | 300.167 | 286.5 | 2.91249 | 1.73205 | 0.000575063 | 0.000341989 | 5.70932 | 0.999845 | 1.22304 | 0.492 | 118.155 | 9.49973 | A | F | 4.59e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X014313.87+133014.9 | chandra | ccd6 | 598.5 | 403.5 | 2.74049 | 1.73206 | 0.000541101 | 0.00034199 | 5.15965 | 0.999789 | 0.492 | 0.492 | 90 | 8.25733 | F | F | 4.64e+20 | 5.94086e-15 | 1 | dx | ||||
| Report | 2 | X014219.84+134026.2 | chandra | ccd3 | 486.5 | 1032.5 | 0.839993 | 1.00001 | 0.000165854 | 0.000197449 | 1.64663 | 0.971478 | 0.492 | 0.492 | 90 | 10.5722 | F | F | 4.6e+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