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 | X042208.23+191521.8 | chandra | ccd7 | 333.348 | 785.271 | 3574.61 | 61.1284 | 0.143479 | 0.0024536 | 390.116 | 1 | 0.423288 | 0.393281 | 331.549 | 0.611033 | F | T | 1.68e+21 | 6.05905e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 2 | X042159.44+193204.7 | chandra | ccd5 | 333.459 | 759.135 | 3296.58 | 83.5739 | 0.106184 | 0.00269194 | 1182.93 | 1 | 6.72589 | 5.82803 | 126.516 | 16.2641 | F | T | 1.75e+21 | 1.12025e-12 | 1 | dx | ||||
| Report | srcpi bgdpi arf rmf | 1 | X042204.26+193430.3 | chandra | ccd5 | 195.127 | 1055.19 | 125.504 | 25.8478 | 0.00404251 | 0.000832566 | 45.0352 | 1 | 7.3381 | 5.01365 | 168.175 | 18.6031 | F | T | 1.76e+21 | 4.59064e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X042244.01+191225.5 | chandra | ccd3 | 889.709 | 219.895 | 66.3164 | 9.27375 | 0.00213607 | 0.00029871 | 40.0389 | 1 | 3.5954 | 2.73602 | 88.5675 | 9.38238 | F | T | 1.66e+21 | 2.7567e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X042308.71+191208.7 | chandra | ccd3 | 178.613 | 186.5 | 49.72 | 11.0005 | 0.0016015 | 0.00035433 | 30.0187 | 1 | 4.37433 | 4.26307 | 96.0685 | 15.0199 | F | T | 1.66e+21 | 2.26755e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X042213.24+191200.1 | chandra | ccd7 | 189.036 | 375.327 | 29.5132 | 5.94634 | 0.00118462 | 0.000238677 | 3.22093 | 0.998949 | 1.1722 | 0.609733 | 316.381 | 4.17291 | F | F | 1.66e+21 | 9.33894e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X042159.72+192209.2 | chandra | ccd6 | 449.29 | 577.351 | 19.1102 | 6.04497 | 0.000625634 | 0.000197902 | 6.6622 | 1 | 2.60371 | 0.794786 | 84.5809 | 6.4742 | F | T | 1.71e+21 | 6.66869e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X042204.24+191835.1 | chandra | ccd6 | 319.236 | 142.129 | 15.2762 | 4.38442 | 0.000500115 | 0.000143538 | 5.32559 | 0.999994 | 0.639833 | 0.639833 | 0 | 2.75509 | F | F | 1.69e+21 | 4.96795e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X042208.23+192055.5 | chandra | ccd6 | 204.407 | 427.553 | 17.4823 | 5.03432 | 0.000572337 | 0.000164814 | 6.09468 | 0.999999 | 1.09405 | 0.570663 | 50.0147 | 5.00898 | F | F | 1.7e+21 | 5.9138e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X042211.78+192106.0 | chandra | ccd6 | 102.251 | 448.883 | 7.88154 | 3.39899 | 0.000258027 | 0.000111277 | 2.74766 | 0.995129 | 0.903607 | 0.903607 | 0 | 5.29384 | F | F | 1.7e+21 | 2.69845e-15 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X042200.69+192240.0 | chandra | ccd6 | 420.682 | 639.5 | 8.84551 | 3.31666 | 0.000284917 | 0.000106831 | 3.08372 | 0.997855 | 1.01459 | 0.527456 | 159.383 | 6.92043 | A | T | 1.71e+21 | 3.06261e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X042246.17+191936.8 | chandra | ccd2 | 703.5 | 59.5 | 6.25022 | 2.82848 | 0.000201321 | 9.11061e-05 | 3.77018 | 0.997848 | 0.492 | 0.492 | 90 | 9.92879 | F | T | 1.69e+21 | 2.52803e-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