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 | 3 | X143352.27+052729.9 | chandra | ccd3 | 366.302 | 940.315 | 298.259 | 17.8847 | 0.0594069 | 0.00356225 | 64.172 | 1 | 0.468808 | 0.468808 | 0 | 1.97183 | 26.7461 | 277.154 | 0.823981 | 0.0788482 | F | F | 2.48e+20 | 1.83548e-12 | 1 | dsxf |
| Report | srcpi bgdpi arf | 1 | X143324.70+053609.7 | chandra | ccd2 | 1046.89 | 986.096 | 61.2504 | 8.7471 | 0.0121999 | 0.00174225 | 22.1731 | 1 | 5.61521 | 2.8799 | 75.241 | 10.689 | 43.5657 | 22.9578 | -0.309785 | 0.146459 | F | F | 2.43e+20 | 2.05548e-13 | 1 | dsx |
| Report | 9 | X143357.15+052950.7 | chandra | ccd2 | 62.1461 | 215.608 | 28.4158 | 5.33065 | 0.00565988 | 0.00106176 | 10.2867 | 1 | 0.450441 | 0.450441 | 0 | 0.757188 | F | F | 2.48e+20 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 1 | X143431.61+052543.0 | chandra | ccd1 | 182.808 | 578.769 | 24.018 | 6.07445 | 0.00478397 | 0.00120992 | 24.2374 | 1 | 2.76687 | 1.78267 | 12.2178 | 9.26353 | 17.6727 | 6.3999 | -0.468283 | 0.279763 | A | F | 2.53e+20 | 6.82983e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X143357.29+053500.2 | chandra | ccd0 | 1071.02 | 682.7 | 21.5342 | 4.6405 | 0.00428926 | 0.000924312 | 38.4726 | 1 | 2.10821 | 0.478951 | 54.0406 | 5.93353 | -0.0384728 | 13.8461 | 1 | 0.497717 | A | F | 2.47e+20 | 6.69216e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X143403.86+052943.3 | chandra | ccd0 | 871.167 | 37.9443 | 8.93625 | 4.1225 | 0.00177996 | 0.000821136 | 35.3923 | 1 | 0.653722 | 0.492 | 6.04738 | 1.83267 | 5 | 3.93625 | -0.119038 | 0.469063 | T | F | 2.49e+20 | 2.07833e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X143408.93+052214.7 | chandra | ccd1 | 871.357 | 155.214 | 6.946 | 3.78388 | 0.00138352 | 0.000753683 | 29.8906 | 1 | 0.771567 | 0.492 | 102.548 | 7.46652 | 1 | 5.946 | 0.712064 | 0.676624 | A | F | 2.52e+20 | 1.86335e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X143351.46+053203.9 | chandra | ccd2 | 234.333 | 485.833 | 5.91531 | 3.59808 | 0.00117822 | 0.000716667 | 20.326 | 1 | 0.492 | 0.492 | 5.39215 | 3.27297 | 3 | 2.91531 | -0.0143177 | 0.616388 | F | F | 2.47e+20 | 1.46841e-14 | 1 | dx |
| Report | 2 | X143408.71+052606.7 | chandra | ccd1 | 877.833 | 626.833 | 2.94117 | 1.73205 | 0.00058583 | 0.000344994 | 5.38603 | 0.99974 | 0.492 | 0.492 | 16.845 | 4.17684 | F | F | 2.5e+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