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 | 1 | X141224.54-620319.0 | chandra | ccd1 | 665.882 | 1087.58 | 27.1163 | 5.51992 | 0.00273243 | 0.000556225 | 20.942 | 1 | 1.50692 | 0.597831 | 35.7559 | 5.83069 | F | F | 1.88e+22 | 5.20882e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 11 | X141309.83-620008.9 | chandra | ccd3 | 392.886 | 500.182 | 19.7708 | 4.44644 | 0.00199224 | 0.000448054 | 13.6358 | 1 | 0.71813 | 0.71813 | 0 | 3.7051 | F | F | 1.87e+22 | 3.70032e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 5 | X141318.63-615647.2 | chandra | ccd3 | 266.364 | 909.545 | 20.5279 | 4.69043 | 0.00206853 | 0.000472639 | 14.158 | 1 | 1.76151 | 1.23441 | 146.249 | 7.05182 | F | F | 1.87e+22 | 4.20872e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X141243.21-620004.1 | chandra | ccd3 | 773.903 | 509.371 | 16.5997 | 4.56116 | 0.0016727 | 0.000459614 | 11.4487 | 1 | 0.659195 | 0.659195 | 0 | 5.21432 | F | F | 1.88e+22 | 3.12745e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 7 | X141242.74-615645.8 | chandra | ccd3 | 780.917 | 911.917 | 11.2489 | 3.46411 | 0.00113351 | 0.000349067 | 7.75828 | 1 | 1.69278 | 0.747887 | 174.875 | 7.95815 | A | F | 1.89e+22 | 2.30196e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X141237.25-620331.2 | chandra | ccd1 | 484.166 | 1063.3 | 10.9575 | 3.31021 | 0.00110415 | 0.000333558 | 8.4625 | 1 | 0.54437 | 0.54437 | 0 | 4.32879 | F | F | 1.87e+22 | 2.17819e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X141330.36-620454.6 | chandra | ccd2 | 1072.2 | 306.8 | 9.88974 | 3.16228 | 0.000996555 | 0.000318652 | 11.774 | 1 | 0.492 | 0.492 | 162.504 | 2.19223 | F | F | 1.84e+22 | 1.89437e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X141329.91-620002.8 | chandra | ccd2 | 1078.06 | 899.833 | 8.7946 | 3.00001 | 0.000886202 | 0.0003023 | 10.4702 | 1 | 0.633027 | 0.492 | 170.97 | 4.20123 | F | F | 1.86e+22 | 1.69264e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X141320.91-620535.3 | chandra | ccd0 | 821.072 | 1206.07 | 6.91467 | 2.64575 | 0.000696993 | 0.000266689 | 8.41257 | 0.999999 | 0.492 | 0.492 | 90 | 1.94082 | F | F | 1.84e+22 | 1.30963e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X141307.38-620303.0 | chandra | ccd3 | 427.357 | 145.643 | 6.72851 | 2.64576 | 0.000678009 | 0.000266604 | 4.64062 | 0.99966 | 0.749815 | 0.492 | 87.6666 | 1.10178 | A | F | 1.86e+22 | 1.19061e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 10 | X141239.76-620035.6 | chandra | ccd3 | 822.667 | 444.833 | 5.8186 | 2.44949 | 0.000586321 | 0.000246827 | 4.01306 | 0.998504 | 0.814802 | 0.492 | 37.3281 | 5.16049 | A | F | 1.88e+22 | 1.13473e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X141335.54-620311.0 | chandra | ccd2 | 998 | 517.333 | 5.80049 | 2.44949 | 0.000584496 | 0.000246827 | 6.90566 | 0.999991 | 0.583994 | 0.492 | 97.4132 | 2.58809 | F | F | 1.85e+22 | 1.10186e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X141215.48-620529.7 | chandra | ccd1 | 793.833 | 821 | 5.2816 | 2.44951 | 0.000532209 | 0.000246829 | 4.07899 | 0.998264 | 1.70912 | 0.492 | 47.8475 | 7.06689 | A | F | 1.88e+22 | 1.05957e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X141330.91-620639.1 | chandra | ccd0 | 678.5 | 1076.3 | 4.88498 | 2.23607 | 0.000492402 | 0.000225394 | 5.9432 | 0.999926 | 0.492 | 0.492 | 7.76206 | 3.44857 | F | F | 1.82e+22 | 8.85322e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X141330.22-620535.9 | chandra | ccd0 | 688.192 | 1204.88 | 12.6876 | 3.60556 | 0.0012789 | 0.000363437 | 15.4361 | 1 | 0.557224 | 0.492 | 54.0302 | 2.59243 | F | F | 1.83e+22 | 2.66075e-14 | 1 | dpx | ||||
Report | srcpi bgdpi arf | 1 | X141344.20-620302.4 | chandra | ccd2 | 874.1 | 534.5 | 4.88226 | 2.23607 | 0.000491969 | 0.000225321 | 5.81248 | 0.999906 | 0.607371 | 0.492 | 9.82691 | 3.60934 | F | F | 1.85e+22 | 9.07543e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X141257.64-620746.6 | chandra | ccd1 | 191.9 | 544.1 | 4.83298 | 2.23607 | 0.000487003 | 0.000225321 | 3.73252 | 0.998264 | 0.500717 | 0.492 | 178.093 | 4.40341 | F | F | 1.83e+22 | 9.36231e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X141251.59-620227.6 | chandra | ccd3 | 653.1 | 217.5 | 4.83195 | 2.23607 | 0.000486899 | 0.000225321 | 3.33257 | 0.994105 | 0.67381 | 0.492 | 65.9936 | 2.96947 | F | F | 1.87e+22 | 8.65471e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X141255.61-615614.7 | chandra | ccd3 | 596.5 | 975.5 | 4.70252 | 2.23608 | 0.000473857 | 0.000225322 | 3.24331 | 0.994105 | 0.984635 | 0.492 | 126.449 | 7.87944 | A | F | 1.88e+22 | 9.9012e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X141255.05-620608.6 | chandra | ccd1 | 229 | 743.25 | 3.89724 | 2 | 0.000392712 | 0.000201533 | 3.00985 | 0.992495 | 0.492 | 0.492 | 104.872 | 3.22311 | F | F | 1.85e+22 | 7.33948e-15 | 1 | dx | ||||
Report | 6 | X141242.61-615811.4 | chandra | ccd3 | 782.5 | 738 | 3.674 | 2.00001 | 0.000370217 | 0.000201534 | 2.53394 | 0.979457 | 0.810557 | 0.492 | 81.4486 | 6.73423 | A | F | 1.89e+22 | 0 | 1 | d | |||||
Report | 4 | X141305.61-620002.5 | chandra | ccd3 | 452.833 | 512.5 | 2.90844 | 1.73205 | 0.000293074 | 0.000174533 | 2.00594 | 0.979457 | 0.54799 | 0.492 | 33.0188 | 3.90602 | F | F | 1.87e+22 | 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