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 | 2 | X025900.92+132609.9 | chandra | ccd2 | 882 | 185.333 | 5.62731 | 2.4495 | 0.00119357 | 0.000519547 | 4.5242 | 0.999792 | 0.492 | 0.492 | 145.427 | 7.00531 | F | F | 1.01e+21 | 1.74773e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X025951.50+132258.5 | chandra | ccd1 | 731 | 444.167 | 5.51946 | 2.4495 | 0.0011707 | 0.000519547 | 8.5219 | 0.999995 | 1.08165 | 0.869025 | 176.859 | 6.6007 | F | F | 1.03e+21 | 1.43287e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X025936.26+132100.7 | chandra | ccd3 | 192.167 | 524.5 | 5.43077 | 2.4495 | 0.00115188 | 0.000519548 | 7.42622 | 0.999979 | 1.54616 | 0.521612 | 179.386 | 6.07934 | A | F | 1.04e+21 | 1.411e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X025914.97+132115.0 | chandra | ccd3 | 823.5 | 553.667 | 5.42274 | 2.4495 | 0.00115018 | 0.000519548 | 7.41524 | 0.999979 | 1.11774 | 0.492 | 102.515 | 6.64961 | A | F | 1.03e+21 | 1.48512e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X025950.71+132607.1 | chandra | ccd1 | 754.7 | 827.5 | 4.94848 | 2.23607 | 0.00104959 | 0.000474278 | 7.64033 | 0.999995 | 0.492 | 0.492 | 119.518 | 5.19018 | F | F | 1.03e+21 | 1.23177e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X025922.90+132428.3 | chandra | ccd3 | 588.3 | 946.5 | 4.94256 | 2.23607 | 0.00104833 | 0.000474278 | 6.75864 | 0.999979 | 0.492 | 0.492 | 3.5414e-08 | 2.89774 | F | T | 1.02e+21 | 1.21564e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X025930.33+132605.4 | chandra | ccd3 | 368.1 | 1143.9 | 4.90429 | 2.23607 | 0.00104022 | 0.000474278 | 6.70629 | 0.999979 | 0.612151 | 0.492 | 153.784 | 0.800231 | T | F | 1.02e+21 | 1.15656e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X025928.19+133422.0 | chandra | ccd0 | 1078.5 | 845.25 | 3.75834 | 2.00001 | 0.00079768 | 0.000424487 | 5.28315 | 0.999818 | 0.492 | 0.492 | 90 | 7.50457 | F | F | 1e+21 | 1.04797e-14 | 1 | dx | ||||
| Report | 2 | X025938.45+132545.5 | chandra | ccd1 | 1118.17 | 783.5 | 2.95774 | 1.73205 | 0.000627346 | 0.000367374 | 4.56667 | 0.999075 | 0.492 | 0.492 | 180 | 2.42478 | F | F | 1.02e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X025940.30+132241.5 | chandra | ccd1 | 1063.17 | 409.5 | 2.95298 | 1.73205 | 0.000626338 | 0.000367374 | 4.55933 | 0.999075 | 0.492 | 0.492 | 180 | 4.92415 | F | F | 1.03e+21 | 7.34313e-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