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 | X014730.54-264324.0 | chandra | ccd5 | 470.528 | 367.658 | 164.723 | 15.9064 | 0.030294 | 0.00292534 | 128.186 | 1 | 7.47931 | 5.68899 | 117.446 | 11.2896 | F | F | 1.49e+20 | 2.94252e-13 | 1 | dx | ||||
| Report | srcpi bgdpi arf rmf | 1 | X014800.42-265301.8 | chandra | ccd7 | 695.473 | 1002.08 | 109.372 | 10.631 | 0.0201147 | 0.00195516 | 67.8645 | 1 | 0.426702 | 0.426702 | 0 | 1.44722 | F | F | 1.51e+20 | 1.33576e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 2 | X014755.27-265331.5 | chandra | ccd7 | 835.677 | 941.699 | 15.0402 | 4.38016 | 0.00276604 | 0.000805556 | 9.33233 | 1 | 0.329738 | 0.329738 | 0 | 0.293139 | F | F | 1.51e+20 | 2.05961e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X014806.21-265334.8 | chandra | ccd7 | 538.1 | 934.792 | 16.3658 | 4.04547 | 0.00300984 | 0.000744004 | 10.1549 | 1 | 0.739825 | 0.472665 | 40.9316 | 2.69976 | F | F | 1.51e+20 | 2.28381e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X014730.16-265137.0 | chandra | ccd6 | 984 | 258.5 | 11.4882 | 3.46411 | 0.00211279 | 0.000637082 | 17.1681 | 1 | 1.15732 | 0.714239 | 53.3496 | 5.63086 | A | F | 1.52e+20 | 2.80572e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X014752.89-265421.9 | chandra | ccd7 | 899.833 | 838.611 | 8.81326 | 3 | 0.00162084 | 0.000551728 | 5.46856 | 0.999982 | 0.514647 | 0.492 | 76.9523 | 1.01754 | F | F | 1.52e+20 | 1.35879e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X014806.72-265652.0 | chandra | ccd7 | 524.056 | 533.5 | 8.69167 | 3.00001 | 0.00159848 | 0.000551729 | 5.39312 | 0.999982 | 0.641592 | 0.536336 | 51.2644 | 4.46976 | F | F | 1.52e+20 | 1.23836e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X014745.03-265714.6 | chandra | ccd7 | 1113.5 | 487.722 | 8.48794 | 3.00001 | 0.00156101 | 0.00055173 | 5.2667 | 0.999982 | 1.06533 | 0.492 | 77.0085 | 4.35772 | A | F | 1.53e+20 | 1.46019e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X014808.27-265340.0 | chandra | ccd7 | 481.5 | 923.786 | 6.7252 | 2.64576 | 0.00123683 | 0.000486579 | 4.17294 | 0.999627 | 0.492 | 0.492 | 114.699 | 3.16536 | F | F | 1.51e+20 | 9.58398e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X014752.73-265340.9 | chandra | ccd7 | 904.167 | 922 | 5.89219 | 2.44949 | 0.00108363 | 0.000450484 | 3.65606 | 0.998523 | 0.492 | 0.492 | 166.224 | 0.430221 | F | F | 1.52e+20 | 8.10723e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X014749.16-265417.8 | chandra | ccd7 | 1001.1 | 847.1 | 4.83006 | 2.23607 | 0.000888292 | 0.000411234 | 2.99701 | 0.994698 | 0.492 | 0.492 | 2.8553 | 1.43326 | F | F | 1.52e+20 | 6.70141e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X014741.96-265204.2 | chandra | ccd6 | 663 | 203.5 | 3.94433 | 2 | 0.000725398 | 0.000367819 | 5.89444 | 0.999896 | 0.492 | 0.492 | 70.6701 | 3.01646 | F | F | 1.51e+20 | 7.99201e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X014756.24-265829.2 | chandra | ccd7 | 808.75 | 336 | 3.55907 | 2.00001 | 0.000654546 | 0.000367821 | 2.20838 | 0.982915 | 0.927194 | 0.492 | 171.789 | 5.12196 | A | F | 1.53e+20 | 6.08917e-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