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 | 3 | X041247.41+102142.5 | chandra | ccd3 | 535.723 | 236.718 | 28.3773 | 5.39512 | 0.00402919 | 0.000766033 | 16.2974 | 1 | 0.436477 | 0.436477 | 0 | 2.29043 | F | F | 1.31e+21 | 4.46615e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X041234.39+101657.7 | chandra | ccd1 | 577.416 | 646.043 | 17.2141 | 4.43386 | 0.00244416 | 0.000629547 | 4.82783 | 0.999975 | 1.05376 | 1.05376 | 0 | 6.03897 | F | F | 1.28e+21 | 2.93143e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X041304.49+102302.0 | chandra | ccd2 | 1024.56 | 721.431 | 13.5833 | 3.68555 | 0.00192952 | 0.000523535 | 10.6333 | 1 | 1.0673 | 0.567076 | 121.605 | 3.60862 | F | F | 1.32e+21 | 2.20839e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X041234.69+102156.0 | chandra | ccd3 | 917.212 | 264.237 | 11.1977 | 4.06588 | 0.00158992 | 0.0005773 | 6.43094 | 0.999999 | 0.668358 | 0.668358 | 0 | 5.20619 | F | F | 1.3e+21 | 1.89048e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X041228.84+102505.8 | chandra | ccd3 | 1092.12 | 649.577 | 12.1692 | 3.60557 | 0.00172786 | 0.000511939 | 6.98891 | 1 | 1.31268 | 1.02078 | 47.5788 | 7.97728 | F | F | 1.31e+21 | 2.28673e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X041316.74+102401.0 | chandra | ccd2 | 656.885 | 840.808 | 11.4856 | 3.60558 | 0.0016315 | 0.000512166 | 8.99118 | 1 | 1.05833 | 0.715725 | 14.9478 | 6.53447 | F | F | 1.33e+21 | 2.01529e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 12 | X041253.32+102032.8 | chandra | ccd3 | 358.2 | 94.6001 | 9.87671 | 3.16228 | 0.00140235 | 0.000448999 | 5.67229 | 0.999982 | 0.492 | 0.492 | 130.787 | 0.434277 | F | F | 1.31e+21 | 1.5262e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X041244.03+101735.9 | chandra | ccd1 | 287.786 | 723.072 | 6.91797 | 2.64575 | 0.000982254 | 0.000375659 | 1.9402 | 0.96461 | 0.492 | 0.492 | 177.801 | 3.8023 | F | F | 1.29e+21 | 1.10426e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X041302.40+102650.6 | chandra | ccd3 | 85.75 | 862.375 | 6.74447 | 2.82845 | 0.000957618 | 0.0004016 | 3.87341 | 0.998809 | 1.30731 | 0.975939 | 62.4036 | 6.78306 | F | F | 1.34e+21 | 1.23635e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X041316.56+102117.4 | chandra | ccd2 | 662.214 | 508.214 | 6.72742 | 2.64576 | 0.000955618 | 0.000375825 | 5.26639 | 0.999947 | 0.62195 | 0.539634 | 72.2312 | 5.43184 | F | F | 1.32e+21 | 1.12143e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X041307.52+101922.9 | chandra | ccd2 | 933.333 | 275.5 | 5.91645 | 2.44949 | 0.000840421 | 0.000347946 | 4.63154 | 0.999703 | 0.492 | 0.492 | 71.1266 | 3.25962 | F | F | 1.31e+21 | 9.22689e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X041255.17+102115.7 | chandra | ccd3 | 302.5 | 181.833 | 5.89947 | 2.44949 | 0.000837641 | 0.000347793 | 3.38812 | 0.995932 | 0.492 | 0.492 | 75.6948 | 0.945563 | F | T | 1.31e+21 | 9.16196e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X041246.98+102428.8 | chandra | ccd3 | 548.333 | 574.333 | 5.86459 | 2.44949 | 0.000832688 | 0.000347793 | 3.36809 | 0.995932 | 0.754037 | 0.492 | 138.113 | 4.58591 | A | F | 1.32e+21 | 9.9157e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X041238.26+102354.9 | chandra | ccd3 | 809.833 | 505.333 | 5.85867 | 2.44949 | 0.000831848 | 0.000347793 | 3.36469 | 0.995932 | 0.873476 | 0.492 | 39.8305 | 5.43296 | A | F | 1.31e+21 | 1.00702e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 11 | X041241.55+102736.0 | chandra | ccd3 | 711.1 | 954.7 | 4.61474 | 2.23608 | 0.000655227 | 0.000317491 | 2.65029 | 0.987393 | 1.05256 | 0.492 | 132.376 | 7.97762 | A | F | 1.33e+21 | 8.7531e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X041323.42+102227.5 | chandra | ccd2 | 456.5 | 650.9 | 4.5464 | 2.23608 | 0.000645809 | 0.000317631 | 3.55904 | 0.998508 | 0.492 | 0.492 | 90 | 7.34976 | F | T | 1.33e+21 | 8.10108e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X041236.54+102342.5 | chandra | ccd3 | 861.25 | 480.25 | 3.97292 | 2 | 0.000564098 | 0.000283972 | 2.28168 | 0.987393 | 0.492 | 0.492 | 45 | 5.62973 | F | T | 1.31e+21 | 6.86159e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X041236.29+101519.0 | chandra | ccd1 | 520.44 | 445.413 | 22.4067 | 6.73711 | 0.00318144 | 0.000956578 | 6.28413 | 1 | 0.984298 | 0.387703 | 56.3613 | 6.77793 | F | F | 1.28e+21 | 3.8899e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 9 | X041238.34+102431.9 | chandra | ccd3 | 807.25 | 580.5 | 3.9126 | 2 | 0.000555533 | 0.000283972 | 2.24704 | 0.96486 | 0.492 | 0.492 | 27.7457 | 5.84428 | F | F | 1.31e+21 | 6.82201e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X041246.74+102546.8 | chandra | ccd3 | 555.5 | 732.75 | 3.87333 | 2 | 0.000549958 | 0.000283972 | 2.22449 | 0.96486 | 0.565617 | 0.492 | 48.5625 | 5.81003 | F | F | 1.32e+21 | 6.79098e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X041309.01+101951.4 | chandra | ccd2 | 888.5 | 333.5 | 2.9455 | 1.73205 | 0.000418403 | 0.000246035 | 2.30581 | 0.974522 | 0.492 | 0.492 | 90 | 3.51973 | F | T | 1.31e+21 | 4.64715e-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