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 | 7 | X123128.55+254457.1 | chandra | ccd7 | 490.607 | 525.168 | 25.8097 | 5.08032 | 0.0146924 | 0.00289202 | 47.1023 | 1 | 0.649557 | 0.425985 | 129.297 | 3.01653 | A | F | 1.42e+20 | 7.82285e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X123124.07+254630.4 | chandra | ccd7 | 613.496 | 714.837 | 20.7973 | 4.56041 | 0.0118391 | 0.00259605 | 37.9548 | 1 | 0.459261 | 0.459261 | 0 | 1.73127 | F | F | 1.42e+20 | 6.32193e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X123107.82+254733.9 | chandra | ccd7 | 1059.57 | 844.23 | 19.2444 | 4.38684 | 0.0109551 | 0.00249725 | 35.1208 | 1 | 1.20301 | 0.704285 | 93.1679 | 4.59666 | F | F | 1.43e+20 | 6.57454e-14 | 1 | dsx | ||||
| Report | arf | 1 | X123135.76+255744.8 | chandra | ccd6 | 770.458 | 1149.17 | 19.5474 | 4.89904 | 0.0111275 | 0.00278882 | 57.3886 | 1 | 3.61187 | 2.17633 | 60.2735 | 9.92789 | A | F | 1.43e+20 | 1.1526e-13 | 1 | dx | ||||
| Report | arf | 2 | X123142.80+255401.4 | chandra | ccd6 | 577.709 | 695.599 | 14.5872 | 3.81932 | 0.00830387 | 0.00217418 | 42.8261 | 1 | 2.29327 | 2.29327 | 0 | 6.89945 | F | F | 1.42e+20 | 8.10074e-14 | 1 | dsx | ||||
| Report | 1 | X123129.57+254621.3 | chandra | ccd7 | 462.1 | 695.9 | 9.92268 | 3.16228 | 0.00564857 | 0.00180015 | 18.1088 | 1 | 0.492 | 0.492 | 121.862 | 1.64267 | F | F | 1.42e+20 | 0 | 1 | d | |||||
| Report | arf | 1 | X123209.69+254827.4 | chandra | ccd2 | 944 | 779.9 | 9.16667 | 3.16229 | 0.00521821 | 0.00180016 | 27.3854 | 1 | 2.52006 | 1.98194 | 76.2782 | 9.35822 | F | F | 1.41e+20 | 5.84353e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X123134.17+254516.6 | chandra | ccd7 | 335.75 | 564.375 | 7.90349 | 2.82843 | 0.00449913 | 0.00161011 | 14.4238 | 1 | 0.677387 | 0.492 | 36.0453 | 3.01114 | F | F | 1.41e+20 | 2.5085e-14 | 1 | dx | ||||
| Report | arf | 2 | X123227.06+255043.2 | chandra | ccd2 | 467.643 | 1056.79 | 6.49203 | 2.64576 | 0.00369564 | 0.00150612 | 19.395 | 1 | 2.79213 | 0.492 | 82.1963 | 13.5368 | A | F | 1.41e+20 | 4.50523e-14 | 1 | dx | ||||
| Report | 1 | X123158.26+253944.0 | chandra | ccd3 | 864.667 | 660.833 | 5.85369 | 2.44949 | 0.00333226 | 0.0013944 | 18.5025 | 1 | 0.543447 | 0.492 | 36.419 | 10.6638 | F | F | 1.4e+20 | 0 | 1 | d | |||||
| Report | arf | 3 | X123138.70+254958.0 | chandra | ccd6 | 689.5 | 200.3 | 4.94188 | 2.23607 | 0.00281321 | 0.0012729 | 14.5087 | 1 | 0.492 | 0.492 | 129.345 | 3.10143 | F | F | 1.42e+20 | 2.53637e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X123123.47+254558.3 | chandra | ccd7 | 629.5 | 649.25 | 3.91954 | 2 | 0.00223123 | 0.00113852 | 7.1531 | 0.999984 | 0.492 | 0.492 | 90 | 2.25709 | F | F | 1.42e+20 | 1.22847e-14 | 1 | dx | ||||
| Report | 3 | X123125.94+254452.5 | chandra | ccd7 | 561.833 | 515.5 | 2.97178 | 1.73205 | 0.00169171 | 0.000985985 | 5.42346 | 0.999733 | 0.492 | 0.492 | 180 | 3.13171 | F | F | 1.42e+20 | 0 | 1 | d | |||||
| Report | 4 | X123147.10+255544.4 | chandra | ccd6 | 459.5 | 904.5 | 2.94207 | 1.73205 | 0.0016748 | 0.000985986 | 8.63754 | 0.999993 | 0.492 | 0.492 | 90 | 8.86302 | F | F | 1.42e+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