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 | X075619.62-413742.2 | chandra | ccd3 | 1202.56 | 830.691 | 634.261 | 26.139 | 0.1972 | 0.00812696 | 121.171 | 1 | 0.473025 | 0.473025 | 0 | 0.92499 | F | F | 3.89e+21 | 4.16193e-12 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 1 | X075611.89-413358.5 | chandra | ccd1 | 854.885 | 427.396 | 30.8513 | 5.81948 | 0.00959205 | 0.00180935 | 22.5266 | 1 | 1.20429 | 0.444991 | 294.046 | 4.22015 | A | F | 3.92e+21 | 1.17622e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 6 | X075640.25-413845.2 | chandra | ccd3 | 732.738 | 702.385 | 24.2691 | 5.48454 | 0.00754558 | 0.00170521 | 4.63645 | 0.999982 | 0.685841 | 0.685841 | 0 | 4.70401 | F | F | 3.97e+21 | 9.65907e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X075654.87-413745.3 | chandra | ccd3 | 398.909 | 823.091 | 21.364 | 4.69042 | 0.00664232 | 0.00145831 | 4.08145 | 0.999874 | 1.30935 | 0.728021 | 118.54 | 7.40722 | A | F | 4.03e+21 | 9.20466e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X075549.09-413332.9 | chandra | ccd0 | 476.429 | 1018.43 | 12.8406 | 3.74167 | 0.00399229 | 0.00116333 | 29.8002 | 1 | 1.61017 | 1.22892 | 55.532 | 6.717 | F | F | 3.81e+21 | 5.20858e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X075538.53-413933.1 | chandra | ccd0 | 716.227 | 286 | 21.1937 | 4.69043 | 0.00658936 | 0.00145831 | 49.1859 | 1 | 1.46391 | 1.01849 | 33.3155 | 7.00864 | F | F | 3.68e+21 | 8.56119e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X075642.67-415319.2 | chandra | ccd6 | 428.342 | 713.237 | 12.5912 | 4.35901 | 0.00391476 | 0.00135526 | 27.4001 | 1 | 4.56683 | 3.14701 | 75.5965 | 16.0095 | F | F | 3.77e+21 | 6.06673e-14 | 1 | dx | ||||
Report | 6 | X075607.28-413427.9 | chandra | ccd1 | 960.12 | 367.632 | 11.9026 | 3.55513 | 0.00370068 | 0.00110534 | 8.69089 | 1 | 0.702857 | 0.386463 | 300.547 | 3.97609 | F | F | 3.89e+21 | 0 | 1 | ds | |||||
Report | srcpi bgdpi arf | 3 | X075646.27-414103.1 | chandra | ccd3 | 595.5 | 421.409 | 10.7628 | 3.31663 | 0.00334626 | 0.00103118 | 2.05615 | 0.978693 | 1.04939 | 0.608835 | 129.674 | 6.4747 | A | F | 3.95e+21 | 4.53137e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X075544.76-414213.2 | chandra | ccd2 | 1192.79 | 829.786 | 6.64687 | 2.64576 | 0.00206659 | 0.000822597 | 14.5504 | 1 | 1.58829 | 0.492 | 18.1374 | 7.00584 | A | F | 3.67e+21 | 2.67163e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X075638.21-413201.4 | chandra | ccd1 | 253.833 | 664.5 | 5.73134 | 2.4495 | 0.00178194 | 0.000761576 | 4.18484 | 0.999269 | 0.829466 | 0.492 | 145.068 | 7.4749 | A | F | 4.05e+21 | 2.42265e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X075603.23-412953.0 | chandra | ccd1 | 1052.17 | 925.667 | 5.67871 | 2.4495 | 0.00176558 | 0.000761577 | 4.14641 | 0.999269 | 0.492 | 0.492 | 110.817 | 8.5654 | F | F | 3.95e+21 | 2.43387e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X075612.32-413013.4 | chandra | ccd1 | 844.7 | 884.3 | 4.71539 | 2.23608 | 0.00146607 | 0.000695221 | 3.44302 | 0.996786 | 1.39047 | 0.492 | 57.0833 | 7.94308 | A | F | 3.98e+21 | 1.98203e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X075603.48-413633.0 | chandra | ccd0 | 148 | 652.75 | 3.96954 | 2 | 0.00123417 | 0.000621823 | 9.21242 | 0.999998 | 0.492 | 0.492 | 60.1282 | 2.7232 | F | F | 3.82e+21 | 1.46834e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X075559.86-413434.5 | chandra | ccd0 | 230.667 | 893.5 | 5.92386 | 2.44949 | 0.0018418 | 0.000761575 | 13.748 | 1 | 0.492 | 0.492 | 11.2397 | 4.59002 | F | F | 3.84e+21 | 2.2871e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X075550.03-413928.4 | chandra | ccd0 | 454.1 | 295.9 | 4.97787 | 2.23607 | 0.00154768 | 0.000695219 | 11.5525 | 1 | 0.492 | 0.492 | 70.6701 | 4.89957 | F | F | 3.72e+21 | 1.90519e-14 | 1 | dx | ||||
Report | 3 | X075636.11-412915.2 | chandra | ccd1 | 301.25 | 1002.5 | 3.87578 | 2.00001 | 0.00120502 | 0.000621825 | 2.82996 | 0.987517 | 0.492 | 0.492 | 118.997 | 9.71095 | F | F | 4.07e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 6 | X075548.66-413328.1 | chandra | ccd0 | 486.25 | 1028.25 | 3.60159 | 2.00001 | 0.00111978 | 0.000621826 | 8.35849 | 0.999957 | 0.661064 | 0.492 | 35.4105 | 6.83084 | F | F | 3.81e+21 | 1.46762e-14 | 1 | dx | ||||
Report | 7 | X075537.18-413737.0 | chandra | ccd0 | 747.25 | 522 | 7.94625 | 2.82843 | 0.00247058 | 0.000879391 | 18.4415 | 1 | 0.492 | 0.492 | 24.407 | 7.13897 | F | T | 3.69e+21 | 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