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 | 2 | X144932.71+002236.6 | chandra | ccd7 | 278.835 | 578.952 | 414.859 | 20.5264 | 0.1931 | 0.00955419 | 230.616 | 1 | 1.57748 | 0.827772 | 96.0413 | 4.49922 | A | T | 3.51e+20 | 0 | 1 | ds | |||||
| Report | 1 | X144913.51+002407.2 | chandra | ccd7 | 864.38 | 763.076 | 44.5542 | 6.67489 | 0.0207382 | 0.0031069 | 24.7673 | 1 | 0.765791 | 0.388895 | 303.725 | 3.09939 | F | F | 3.5e+20 | 0 | 1 | ds | |||||
| Report | 3 | X144907.71+001748.2 | chandra | ccd6 | 559.625 | 907.25 | 7.9277 | 2.82843 | 0.00368997 | 0.0013165 | 22.6146 | 1 | 0.879817 | 0.492 | 158.598 | 3.84461 | A | F | 3.5e+20 | 0 | 1 | d | |||||
| Report | 1 | X144856.86+001511.8 | chandra | ccd6 | 890.5 | 589.5 | 6.68911 | 2.64576 | 0.00311346 | 0.00123148 | 19.0814 | 1 | 1.25063 | 0.492 | 162.231 | 7.54613 | A | F | 3.49e+20 | 0 | 1 | d | |||||
| Report | 2 | X144859.13+001159.1 | chandra | ccd6 | 821.214 | 197.786 | 6.41233 | 2.64577 | 0.00298464 | 0.00123148 | 18.2919 | 1 | 2.80952 | 1.85582 | 70.9495 | 9.99735 | A | T | 3.49e+20 | 0 | 1 | d | |||||
| Report | 7 | X144919.36+002158.1 | chandra | ccd7 | 685.333 | 500.333 | 5.96575 | 2.44949 | 0.00277677 | 0.00114012 | 3.31631 | 0.998091 | 0.492 | 0.492 | 92.3818 | 1.26403 | F | F | 3.5e+20 | 0 | 1 | d | |||||
| Report | 7 | X144910.85+001909.5 | chandra | ccd6 | 463.9 | 1072.5 | 4.98065 | 2.23607 | 0.00231826 | 0.00104078 | 14.2078 | 1 | 0.492 | 0.492 | 150.482 | 2.27973 | F | F | 3.5e+20 | 0 | 1 | d | |||||
| Report | 6 | X144915.18+001951.7 | chandra | ccd7 | 812.9 | 243.3 | 4.92705 | 2.23607 | 0.00229331 | 0.00104078 | 2.7389 | 0.993874 | 0.543498 | 0.492 | 94.4863 | 1.22102 | F | F | 3.5e+20 | 0 | 1 | d | |||||
| Report | 4 | X144920.32+002243.6 | chandra | ccd7 | 656.25 | 592.75 | 3.9343 | 2 | 0.00183123 | 0.000930906 | 2.18704 | 0.982145 | 0.492 | 0.492 | 161.565 | 2.00319 | F | F | 3.5e+20 | 0 | 1 | d | |||||
| Report | 3 | X144919.74+002253.3 | chandra | ccd7 | 673.75 | 612.5 | 3.9276 | 2 | 0.00182811 | 0.000930906 | 2.18331 | 0.982145 | 0.492 | 0.492 | 2.35031e-08 | 2.0667 | F | F | 3.5e+20 | 0 | 1 | d | |||||
| Report | 6 | X144857.99+001534.5 | chandra | ccd6 | 855.833 | 635.5 | 2.94979 | 1.73205 | 0.00137299 | 0.000806188 | 8.4146 | 0.999991 | 0.492 | 0.492 | 61.845 | 7.07408 | F | F | 3.49e+20 | 0 | 1 | d | |||||
| Report | 1 | X144807.53+001952.2 | chandra | ccd2 | 1287.5 | 363.5 | 1.99985 | 1.41421 | 0.000930838 | 0.000658249 | 5.95186 | 0.99978 | 0.521845 | 0.492 | 45 | 17.1105 | F | F | 3.46e+20 | 0 | 1 | d | |||||
| Report | 4 | X144910.83+001841.7 | chandra | ccd6 | 464.5 | 1016 | 1.99322 | 1.41421 | 0.000927749 | 0.00065825 | 5.68587 | 0.999718 | 0.492 | 0.492 | 90 | 2.68294 | F | F | 3.5e+20 | 0 | 1 | d | |||||
| Report | 5 | X144857.55+001800.1 | chandra | ccd6 | 869.5 | 931.5 | 1.95774 | 1.41422 | 0.000911236 | 0.00065825 | 5.58467 | 0.999718 | 0.492 | 0.492 | 90 | 5.50038 | F | F | 3.49e+20 | 0 | 1 | d | |||||
| Report | 1 | X144833.11+003346.9 | chandra | ccd3 | 940.5 | 1123 | 1.95576 | 1.41422 | 0.000910312 | 0.000658251 | 5.8645 | 0.999789 | 2.58958 | 0.492 | 4.08562 | 16.5964 | A | F | 3.52e+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