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 | 4 | X093241.17+530633.8 | chandra | ccd7 | 725.057 | 860.757 | 428.051 | 21.13 | 0.0727613 | 0.00359175 | 99.7151 | 1 | 0.439592 | 0.439592 | 0 | 0.582663 | F | F | 1.49e+20 | 5.37561e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 6 | X093251.88+531207.4 | chandra | ccd6 | 189.011 | 551.261 | 86.7244 | 9.38084 | 0.0147416 | 0.00159458 | 136.399 | 1 | 0.863405 | 0.681523 | 113.897 | 5.27393 | F | F | 1.48e+20 | 1.66127e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X093206.10+531508.1 | chandra | ccd6 | 1024.29 | 919.125 | 20.0132 | 4.89903 | 0.00340191 | 0.000832751 | 31.4766 | 1 | 3.80262 | 1.74845 | 68.0384 | 9.5101 | A | F | 1.44e+20 | 4.00184e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X093331.60+531353.2 | chandra | ccd2 | 807.262 | 496.738 | 13.4576 | 4.58268 | 0.00228756 | 0.000778977 | 21.6944 | 1 | 3.88648 | 2.39955 | 114.069 | 10.2157 | A | F | 1.48e+20 | 3.08492e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X093215.02+531206.1 | chandra | ccd6 | 862.039 | 548.885 | 12.2081 | 3.60556 | 0.00207516 | 0.000612884 | 19.2007 | 1 | 1.40763 | 1.10761 | 103.802 | 6.25799 | F | F | 1.44e+20 | 2.27565e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X093344.63+530250.2 | chandra | ccd3 | 900.409 | 143.045 | 9.53595 | 3.31665 | 0.00162095 | 0.000563774 | 15.8404 | 1 | 2.1957 | 0.918507 | 52.9304 | 10.5548 | A | F | 1.51e+20 | 2.43201e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X093232.24+530212.3 | chandra | ccd7 | 888.278 | 328.833 | 8.77665 | 3 | 0.00149188 | 0.000509949 | 2.04453 | 0.977492 | 0.629734 | 0.492 | 130.269 | 5.08125 | F | F | 1.5e+20 | 1.129e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X093223.77+530610.0 | chandra | ccd7 | 1043 | 812 | 7.77398 | 2.82843 | 0.00132144 | 0.000480784 | 1.81096 | 0.964074 | 0.618449 | 0.492 | 148.283 | 2.68165 | F | F | 1.44e+20 | 9.46712e-15 | 1 | dx | ||||
| Report | 1 | X093235.12+531049.4 | chandra | ccd6 | 495 | 392.75 | 5.93461 | 2.44949 | 0.00100878 | 0.000416371 | 9.33388 | 1 | 0.492 | 0.492 | 97.4657 | 3.77275 | F | F | 1.48e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X093220.09+531154.0 | chandra | ccd6 | 769.5 | 524.333 | 5.84048 | 2.44949 | 0.000992781 | 0.000416372 | 9.18584 | 1 | 0.788897 | 0.492 | 133.915 | 5.65717 | A | F | 1.44e+20 | 1.07374e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X093248.32+531207.6 | chandra | ccd6 | 253.9 | 551.7 | 4.87104 | 2.23607 | 0.000827993 | 0.000380094 | 7.66111 | 0.999996 | 0.666749 | 0.492 | 17.3476 | 5.1293 | F | F | 1.48e+20 | 9.07136e-15 | 1 | dx | ||||
| Report | 8 | X093227.36+531126.1 | chandra | ccd6 | 636.75 | 467.5 | 3.94994 | 2 | 0.000671421 | 0.000339966 | 6.21241 | 0.999936 | 0.492 | 0.492 | 180 | 4.72552 | F | F | 1.47e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 7 | X093220.02+531151.0 | chandra | ccd6 | 770.833 | 518.167 | 2.91668 | 1.73205 | 0.000495785 | 0.000294419 | 4.58732 | 0.999193 | 0.492 | 0.492 | 45 | 5.62057 | F | F | 1.44e+20 | 5.35712e-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