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 | arf | 7 | X033841.41-353133.7 | chandra | ccd2 | 1010.56 | 666.518 | 163.221 | 12.8063 | 0.0453562 | 0.00355863 | 166.863 | 1 | 0.584865 | 0.492 | 98.2212 | 3.63466 | F | F | 1.51e+20 | 4.60169e-13 | 1 | dbx | ||||
Report | arf | 1 | X033828.98-352701.7 | chandra | ccd3 | 802.354 | 331.391 | 75.1825 | 17.5135 | 0.0209104 | 0.004871 | 4.94088 | 0.999999 | 1.5 | 1.5 | 0 | 2.40132 | T | F | 1.5e+20 | 2.11367e-13 | 1 | dsx | ||||
Report | arf | 2 | X033852.15-353540.1 | chandra | ccd2 | 744.606 | 165.479 | 125.874 | 12.57 | 0.0349782 | 0.00349297 | 128.683 | 1 | 0.681906 | 0.606424 | 154.903 | 8.08383 | F | F | 1.52e+20 | 3.90508e-13 | 1 | dx | ||||
Report | arf | 6 | X033908.53-353121.4 | chandra | ccd2 | 337.654 | 690.731 | 10.184 | 3.6056 | 0.00282996 | 0.00100193 | 10.4113 | 1 | 2.79948 | 1.61088 | 26.6302 | 8.66567 | A | F | 1.54e+20 | 3.27482e-14 | 1 | dbx | ||||
Report | arf | 1 | X033832.20-353343.1 | chandra | ccd0 | 324.072 | 938.643 | 6.85903 | 2.64575 | 0.001906 | 0.000735208 | 5.00124 | 0.999848 | 0.636603 | 0.492 | 40.1901 | 4.44178 | F | F | 1.5e+20 | 1.97277e-14 | 1 | dx | ||||
Report | arf | 2 | X033825.17-353944.4 | chandra | ccd0 | 498.5 | 204.25 | 6.81433 | 2.82846 | 0.00189358 | 0.000785979 | 4.96865 | 0.999848 | 2.48137 | 0.711472 | 71.2631 | 10.3452 | A | F | 1.44e+20 | 4.45683e-14 | 1 | dx | ||||
Report | arf | 3 | X033808.78-353418.6 | chandra | ccd0 | 905.393 | 862.031 | 90.1272 | 9.59209 | 0.025067 | 0.00266783 | 65.7159 | 1 | 1.76331 | 1.40029 | 220.748 | 6.15983 | F | F | 1.44e+20 | 2.69762e-13 | 1 | dsx | ||||
Report | arf | 4 | X033821.98-352928.2 | chandra | ccd1 | 63.6431 | 572.643 | 6.80594 | 2.64576 | 0.00189125 | 0.000735208 | 8.39408 | 1 | 0.492 | 0.492 | 62.496 | 1.03255 | F | F | 1.49e+20 | 1.86691e-14 | 1 | dx | ||||
Report | arf | 1 | X033812.74-352856.9 | chandra | ccd1 | 293.167 | 636.333 | 5.82194 | 2.44949 | 0.00161781 | 0.000680671 | 7.18046 | 0.999994 | 0.492 | 0.492 | 164.675 | 2.9475 | F | F | 1.45e+20 | 1.61016e-14 | 1 | dx | ||||
Report | arf | 1 | X033843.61-353348.6 | chandra | ccd2 | 956 | 392.333 | 5.79731 | 2.4495 | 0.00161097 | 0.000680671 | 5.92666 | 0.999937 | 0.888276 | 0.492 | 48.519 | 5.54945 | A | F | 1.51e+20 | 1.68163e-14 | 1 | dx | ||||
Report | arf | 3 | X033800.30-352332.2 | chandra | ccd1 | 602.667 | 1295.83 | 5.15707 | 2.44951 | 0.00143306 | 0.000680676 | 6.36045 | 0.999936 | 1.72913 | 0.571972 | 174.928 | 8.00401 | A | F | 1.44e+20 | 1.57614e-14 | 1 | dx | ||||
Report | arf | 3 | X033843.58-353308.4 | chandra | ccd2 | 956.9 | 474.1 | 4.86101 | 2.23607 | 0.00135079 | 0.000621365 | 4.96948 | 0.999527 | 0.492 | 0.492 | 70.6701 | 5.02832 | F | F | 1.51e+20 | 1.39501e-14 | 1 | dx | ||||
Report | arf | 5 | X033848.70-352833.2 | chandra | ccd2 | 829.25 | 1033.25 | 3.91156 | 2 | 0.00108695 | 0.000555765 | 3.99884 | 0.99696 | 0.492 | 0.492 | 90 | 4.49009 | F | F | 1.52e+20 | 1.19723e-14 | 1 | dx | ||||
Report | arf | 2 | X033807.01-352805.4 | chandra | ccd1 | 435.5 | 740.833 | 2.89015 | 1.73205 | 0.00080312 | 0.000481307 | 3.56455 | 0.995373 | 0.492 | 0.492 | 90 | 4.28487 | F | F | 1.44e+20 | 8.32244e-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