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 | X003344.48-094001.1 | chandra | ccd7 | 935.955 | 814.932 | 60.2731 | 7.76358 | 0.0122998 | 0.0015843 | 59.4526 | 1 | 1.24749 | 0.771868 | 16.5202 | 4.56361 | F | F | 2.58e+20 | 9.56389e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X003328.32-094608.1 | chandra | ccd3 | 387.796 | 938.463 | 24.0711 | 5.19619 | 0.00491212 | 0.00106037 | 39.2404 | 1 | 2.40002 | 1.87939 | 143.737 | 8.73717 | F | F | 2.54e+20 | 6.87415e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X003426.28-094831.3 | chandra | ccd6 | 468.939 | 414.987 | 8.34173 | 4.4239 | 0.00170228 | 0.000902779 | 3.52044 | 0.997972 | 1.6059 | 1.6059 | 0 | 8.87593 | F | F | 2.61e+20 | 2.09781e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X003407.72-094002.5 | chandra | ccd7 | 237.491 | 812.158 | 12.2071 | 3.49387 | 0.00249108 | 0.000712986 | 12.0409 | 1 | 1.04399 | 0.3796 | 138.756 | 2.96042 | F | F | 2.62e+20 | 2.02438e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 6 | X003410.88-094316.0 | chandra | ccd6 | 931.656 | 1055.84 | 10.8431 | 3.29289 | 0.00221273 | 0.000671973 | 4.57608 | 0.999919 | 0.816136 | 0.409523 | 93.0976 | 2.74638 | F | T | 2.61e+20 | 2.39665e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X003358.13-094222.0 | chandra | ccd7 | 525.25 | 528.125 | 7.79705 | 2.82843 | 0.00159112 | 0.000577189 | 7.69091 | 0.999999 | 0.492 | 0.492 | 172.534 | 0.543328 | F | F | 2.59e+20 | 1.2443e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X003429.96-094851.4 | chandra | ccd6 | 357.944 | 373.611 | 7.30431 | 3.00004 | 0.00149057 | 0.000612208 | 3.08262 | 0.994748 | 2.8327 | 1.1586 | 147.406 | 9.7608 | A | F | 2.61e+20 | 2.02203e-14 | 1 | dx | ||||
Report | 12 | X003349.75-094426.0 | chandra | ccd7 | 777.071 | 276.072 | 6.84749 | 2.64575 | 0.00139735 | 0.000539911 | 6.75427 | 0.999988 | 0.492 | 0.492 | 72.2312 | 3.32211 | F | F | 2.57e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 4 | X003404.37-094248.1 | chandra | ccd7 | 337.786 | 475.214 | 6.73697 | 2.64576 | 0.00137479 | 0.000539912 | 6.64526 | 0.999988 | 0.492 | 0.492 | 173.953 | 1.08087 | F | F | 2.6e+20 | 1.04147e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 10 | X003405.71-094035.8 | chandra | ccd7 | 297.5 | 744 | 5.81613 | 2.44949 | 0.00118688 | 0.000499861 | 5.73695 | 0.999902 | 0.518405 | 0.492 | 52.0181 | 2.21812 | F | F | 2.61e+20 | 9.13859e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X003418.44-094651.5 | chandra | ccd6 | 704.167 | 617.333 | 5.38587 | 2.44951 | 0.00109908 | 0.000499863 | 2.27298 | 0.987281 | 1.32086 | 0.626335 | 88.3968 | 6.32304 | A | F | 2.6e+20 | 1.28033e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 8 | X003408.36-094140.2 | chandra | ccd7 | 217.9 | 613.1 | 4.87231 | 2.23607 | 0.000994277 | 0.000456308 | 4.80598 | 0.999316 | 0.492 | 0.492 | 45 | 2.0993 | F | F | 2.61e+20 | 7.64482e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X003352.89-094358.9 | chandra | ccd7 | 682.7 | 331.3 | 4.84854 | 2.23607 | 0.000989426 | 0.000456308 | 4.78253 | 0.999316 | 0.492 | 0.492 | 160.67 | 2.43721 | F | T | 2.58e+20 | 7.55906e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X003355.59-094449.4 | chandra | ccd7 | 601.5 | 228.5 | 4.77981 | 2.23607 | 0.000975401 | 0.000456309 | 4.71474 | 0.999316 | 0.836657 | 0.492 | 125.008 | 2.71231 | A | F | 2.58e+20 | 7.62042e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X003404.60-094239.3 | chandra | ccd7 | 330.9 | 493.1 | 4.75028 | 2.23607 | 0.000969374 | 0.000456309 | 4.68561 | 0.999316 | 0.556234 | 0.492 | 152.769 | 1.08658 | F | F | 2.6e+20 | 7.33573e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 9 | X003402.81-094219.5 | chandra | ccd7 | 384.7 | 533.3 | 4.72404 | 2.23608 | 0.000964021 | 0.000456309 | 4.65973 | 0.999316 | 0.492 | 0.492 | 160.67 | 0.611447 | F | F | 2.6e+20 | 7.25344e-15 | 1 | dx | ||||
Report | 2 | X003340.34-094737.2 | chandra | ccd3 | 26.75 | 757.5 | 3.86817 | 2.00001 | 0.000789365 | 0.000408135 | 6.30583 | 0.999954 | 0.492 | 0.492 | 118.997 | 7.19482 | F | F | 2.54e+20 | 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