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 | 1 | X142607.74+340425.9 | chandra | ccd2 | 1242.07 | 679.963 | 251.222 | 16.3341 | 0.0532855 | 0.00346454 | 63.6468 | 1 | 5.33765 | 3.31512 | 112.671 | 10.3986 | F | F | 1.08e+20 | 8.60964e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X142708.80+340218.6 | chandra | ccd3 | 521.4 | 1082.5 | 9.89362 | 3.16228 | 0.00209847 | 0.00067073 | 20.9103 | 1 | 0.569253 | 0.492 | 167.334 | 3.01977 | F | F | 1.06e+20 | 2.41245e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X142639.16+340137.0 | chandra | ccd2 | 448.25 | 335 | 7.87512 | 2.82843 | 0.00167034 | 0.000599919 | 1.99515 | 0.971567 | 0.746626 | 0.492 | 45.5509 | 4.74909 | A | T | 1.07e+20 | 2.01861e-14 | 1 | dx | ||||
| Report | 5 | X142722.86+340026.9 | chandra | ccd3 | 166 | 855.75 | 7.86223 | 2.82843 | 0.0016676 | 0.000599919 | 16.6169 | 1 | 0.492 | 0.492 | 113.424 | 6.45464 | F | T | 1.06e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X142631.07+341056.0 | chandra | ccd0 | 1319.5 | 713.375 | 6.99457 | 2.82845 | 0.00148357 | 0.000599924 | 12.6769 | 1 | 2.68506 | 1.70743 | 115.486 | 8.63531 | A | F | 1.09e+20 | 1.98119e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X142659.65+341159.0 | chandra | ccd0 | 598.688 | 841.188 | 14.0054 | 4.00003 | 0.00297059 | 0.00084842 | 25.3833 | 1 | 1.61339 | 1.25812 | 44.761 | 7.66 | F | F | 1.09e+20 | 3.81528e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X142705.78+340321.4 | chandra | ccd3 | 597.786 | 1210.07 | 6.95494 | 2.64575 | 0.00147517 | 0.000561173 | 14.6994 | 1 | 0.492 | 0.492 | 22.5 | 1.88845 | F | F | 1.07e+20 | 1.65097e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X142645.49+335729.9 | chandra | ccd3 | 1110.79 | 495.643 | 6.58841 | 2.64576 | 0.00139742 | 0.000561175 | 13.9247 | 1 | 0.97996 | 0.749972 | 69.4823 | 7.30769 | F | F | 1.06e+20 | 1.88365e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X142729.03+340223.3 | chandra | ccd1 | 648.333 | 278.5 | 5.69166 | 2.4495 | 0.00120722 | 0.000519547 | 11.4648 | 1 | 0.923125 | 0.506003 | 161.238 | 6.72017 | A | F | 1.06e+20 | 1.52937e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X142638.46+340928.8 | chandra | ccd0 | 1133.33 | 536 | 5.61799 | 2.4495 | 0.00119159 | 0.000519547 | 10.182 | 0.999999 | 1.23574 | 0.691046 | 51.6676 | 6.54346 | A | F | 1.08e+20 | 1.48e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X142659.90+340955.8 | chandra | ccd0 | 592.3 | 590.7 | 5.89348 | 2.44949 | 0.00125003 | 0.000519545 | 10.6813 | 1 | 0.492 | 0.492 | 5.65497 | 5.61237 | F | F | 1.08e+20 | 1.50671e-14 | 1 | dx | ||||
| Report | 4 | X142700.12+335907.9 | chandra | ccd3 | 740.833 | 694.833 | 2.95955 | 1.73205 | 0.000627729 | 0.000367374 | 6.25504 | 0.999912 | 0.543766 | 0.492 | 55.278 | 5.2191 | F | F | 1.06e+20 | 0 | 1 | d | |||||
| Report | 2 | X142731.64+340232.8 | chandra | ccd1 | 582.5 | 297.833 | 2.92277 | 1.73205 | 0.00061993 | 0.000367374 | 5.88738 | 0.999874 | 0.492 | 0.492 | 90 | 7.19786 | F | F | 1.06e+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