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 | X142558.70+343824.9 | chandra | ccd3 | 937.302 | 1055.57 | 43.2054 | 6.57308 | 0.00916403 | 0.00139418 | 100.312 | 1 | 0.516601 | 0.516601 | 0 | 2.96619 | F | F | 1.22e+20 | 0 | 1 | ds | |||||
Report | srcpi bgdpi arf | 1 | X142635.56+344214.9 | chandra | ccd1 | 717.317 | 680.398 | 35.3195 | 6.32464 | 0.00749141 | 0.00134148 | 16.3237 | 1 | 1.61633 | 0.893921 | 59.9654 | 6.22448 | F | F | 1.22e+20 | 9.64974e-14 | 1 | dsx | ||||
Report | 2 | X142549.08+344247.9 | chandra | ccd2 | 409.367 | 907.299 | 13.9267 | 4.09184 | 0.0029539 | 0.000867894 | 8.29842 | 1 | 0.557793 | 0.557793 | 0 | 3.89657 | F | F | 1.24e+20 | 0 | 1 | ds | |||||
Report | srcpi bgdpi arf | 1 | X142526.93+343725.0 | chandra | ccd2 | 965 | 251.188 | 13.7147 | 4.00004 | 0.00290894 | 0.000848422 | 8.17212 | 1 | 3.50011 | 1.46406 | 36.7691 | 8.76898 | A | F | 1.23e+20 | 6.22536e-14 | 1 | dx | ||||
Report | 5 | X142549.38+344228.2 | chandra | ccd2 | 401.167 | 866.611 | 8.96172 | 3 | 0.00190081 | 0.00063631 | 5.33997 | 0.99996 | 0.610087 | 0.492 | 72.1908 | 3.69753 | F | F | 1.24e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 4 | X142520.03+344244.3 | chandra | ccd2 | 1136.88 | 900.375 | 7.12664 | 2.82845 | 0.00151158 | 0.000599924 | 4.24651 | 0.99931 | 2.52504 | 1.55542 | 150.973 | 9.58338 | A | F | 1.26e+20 | 2.15934e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X142553.27+344156.8 | chandra | ccd2 | 303.786 | 802.786 | 6.92468 | 2.64575 | 0.00146875 | 0.000561173 | 4.12617 | 0.99931 | 0.894122 | 0.492 | 49.6231 | 2.76085 | A | F | 1.24e+20 | 1.66844e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X142549.20+345031.7 | chandra | ccd0 | 1078 | 1030.5 | 1.75039 | 1.41423 | 0.000371264 | 0.000299964 | 4.24419 | 0.987075 | 0.492 | 0.492 | 63.4349 | 10.135 | F | F | 1.28e+20 | 7.41134e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X142601.48+344413.4 | chandra | ccd0 | 771 | 261.5 | 2.96295 | 1.73205 | 0.000628451 | 0.000367374 | 7.18427 | 0.99997 | 0.492 | 0.492 | 180 | 3.3583 | F | F | 1.24e+20 | 7.10344e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X142552.50+343558.5 | chandra | ccd3 | 1092.5 | 757.5 | 0.974461 | 1 | 0.000206686 | 0.000212104 | 2.26244 | 0.98478 | 0.492 | 0.492 | 90 | 5.71942 | F | F | 1.22e+20 | 2.57641e-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