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 | X062706.72-352915.3 | chandra | ccd7 | 828.734 | 558.625 | 3272.62 | 62.5365 | 0.165333 | 0.00315935 | 349.422 | 1 | 0.714802 | 0.714802 | 0 | 0.303422 | T | F | 6.36e+20 | 2.29784e-12 | 1 | dsxf | ||||
Report | srcpi bgdpi arf rmf | 6 | X062655.54-353130.2 | chandra | ccd6 | 63.1594 | 245.539 | 195.233 | 14.3498 | 0.0098632 | 0.000724953 | 49.1553 | 1 | 0.776838 | 0.776838 | 0 | 2.90404 | F | F | 6.34e+20 | 1.06916e-13 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 8 | X062717.36-353131.1 | chandra | ccd7 | 564.782 | 282.686 | 70.7847 | 8.41336 | 0.00357605 | 0.000425044 | 7.55778 | 1 | 0.656871 | 0.656871 | 0 | 3.21141 | F | F | 6.42e+20 | 3.06452e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 5 | X062719.75-352546.0 | chandra | ccd7 | 505.255 | 983.929 | 56.8906 | 8.305 | 0.00287412 | 0.00041957 | 6.07429 | 1 | 1.27248 | 0.751753 | 63.2166 | 4.66541 | A | F | 6.38e+20 | 2.52278e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X062726.26-353040.6 | chandra | ccd7 | 344.049 | 385.039 | 56.3805 | 7.99943 | 0.00284835 | 0.000404132 | 6.01983 | 1 | 1.35366 | 0.565387 | 51.1099 | 4.41952 | F | F | 6.44e+20 | 2.22947e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X062631.05-352708.9 | chandra | ccd6 | 671.646 | 776.074 | 36.5339 | 8.55427 | 0.0018457 | 0.000432163 | 9.19842 | 1 | 1.55744 | 1.55744 | 0 | 7.36921 | F | F | 6.26e+20 | 2.3285e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X062659.71-352937.1 | chandra | ccd7 | 1002.79 | 514.484 | 41.101 | 7.03398 | 0.00207643 | 0.000355358 | 4.38841 | 0.999978 | 0.44143 | 0.44143 | 0 | 1.18451 | F | F | 6.33e+20 | 1.58497e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X062738.38-352056.6 | chandra | ccd3 | 271.494 | 215.698 | 38.284 | 9.3973 | 0.00193411 | 0.000474753 | 5.41281 | 1 | 3.45687 | 3.45687 | 0 | 10.8116 | F | F | 6.42e+20 | 2.89003e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 7 | X062733.28-352601.2 | chandra | ccd7 | 168.5 | 952.417 | 33.647 | 6.32462 | 0.00169985 | 0.00031952 | 3.59254 | 0.99969 | 0.916586 | 0.752278 | 177.626 | 6.6064 | F | F | 6.44e+20 | 1.50858e-14 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 6 | X062733.24-352603.4 | chandra | ccd7 | 170.073 | 948.351 | 41.5621 | 8.28767 | 0.00209972 | 0.000418694 | 4.43764 | 0.999985 | 1.5 | 1.5 | 0 | 6.56046 | F | F | 6.44e+20 | 1.86373e-14 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 1 | X062742.38-352046.8 | chandra | ccd3 | 171.583 | 235.111 | 27.2184 | 6.0001 | 0.00137507 | 0.000303125 | 3.84829 | 0.999849 | 3.40192 | 3.09185 | 166.016 | 11.4519 | F | F | 6.44e+20 | 2.0197e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X062712.90-353131.1 | chandra | ccd7 | 675.471 | 282.659 | 24.1016 | 5.69796 | 0.00121761 | 0.000287861 | 2.57336 | 0.992914 | 0.528876 | 0.528876 | 0 | 2.59777 | F | F | 6.4e+20 | 9.40911e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 26 | X062711.35-353148.4 | chandra | ccd7 | 714.051 | 247.578 | 26.2326 | 5.12178 | 0.00132528 | 0.000258753 | 2.80089 | 0.995966 | 1.40889 | 0.546923 | 36.5789 | 2.67787 | A | F | 6.4e+20 | 1.03401e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 5 | X062641.00-352737.6 | chandra | ccd6 | 423.961 | 717.5 | 23.0864 | 5.09905 | 0.00116632 | 0.000257604 | 5.81263 | 0.999999 | 1.92644 | 0.981126 | 40.3696 | 5.28699 | A | F | 6.28e+20 | 1.30088e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X062642.78-353035.3 | chandra | ccd6 | 379.906 | 356.805 | 9.7085 | 3.11585 | 0.000490475 | 0.000157413 | 2.44438 | 0.988825 | 0.885555 | 0.885555 | 0 | 4.75904 | F | F | 6.3e+20 | 5.52772e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X062642.13-351944.2 | chandra | ccd2 | 622.955 | 327.773 | 18.3237 | 5.29162 | 0.000925714 | 0.000267333 | 2.89448 | 0.996986 | 1.62634 | 0.952083 | 17.6783 | 10.7798 | A | F | 6.25e+20 | 1.29573e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X062734.17-352211.1 | chandra | ccd3 | 375.804 | 63.9346 | 17.2486 | 4.79591 | 0.000871399 | 0.000242289 | 2.4387 | 0.99103 | 2.85262 | 2.14054 | 48.5764 | 9.2994 | F | F | 6.41e+20 | 1.22396e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X062649.46-353132.3 | chandra | ccd6 | 213.74 | 240.7 | 13.7538 | 5.00013 | 0.00069484 | 0.000252607 | 3.46289 | 0.999086 | 4.10548 | 3.01035 | 120.961 | 3.88648 | T | F | 6.32e+20 | 7.59834e-15 | 1 | dbx | ||||
Report | srcpi bgdpi arf | 2 | X062640.26-351928.2 | chandra | ccd2 | 670.004 | 360.691 | 14.147 | 7.36363 | 0.00071471 | 0.000372013 | 2.23471 | 0.985517 | 2.83128 | 2.83128 | 0 | 11.2049 | F | F | 6.25e+20 | 1.02802e-14 | 1 | dbsx | ||||
Report | srcpi bgdpi arf | 3 | X062652.79-351644.1 | chandra | ccd2 | 358.071 | 694.054 | 27.6396 | 7.48361 | 0.00139635 | 0.000378072 | 4.36605 | 0.999963 | 8.4866 | 5.41338 | 116.178 | 12.9382 | A | F | 6.26e+20 | 1.93689e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X062645.90-351917.3 | chandra | ccd2 | 529.079 | 382.395 | 32.1019 | 6.32463 | 0.00162179 | 0.00031952 | 5.07093 | 0.999998 | 1.29643 | 0.54791 | 69.9048 | 10.8785 | A | F | 6.26e+20 | 2.29237e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X062647.75-352852.1 | chandra | ccd6 | 256.346 | 566.115 | 7.68499 | 3.60563 | 0.000388246 | 0.000182157 | 1.93491 | 0.967932 | 3.32653 | 1.02474 | 106.312 | 3.6432 | A | F | 6.3e+20 | 4.18299e-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