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 | 2 | X151402.71-493720.0 | chandra | ccd6 | 812.871 | 913.565 | 249.553 | 16.2008 | 0.0251843 | 0.00163494 | 69.4471 | 1 | 4.94664 | 3.55483 | 38.4975 | 8.49605 | 209.666 | 34.7636 | -0.715553 | 0.0853638 | F | F | 2.1e+21 | 2.33074e-13 | 1 | dsxf |
Report | srcpi bgdpi arf | 1 | X151410.33-494501.8 | chandra | ccd7 | 499.545 | 1021.01 | 29.4791 | 5.42947 | 0.00297495 | 0.000547926 | 21.1634 | 1 | 0.444251 | 0.444251 | 0 | 0.893578 | 15.8307 | 12.9153 | -0.101417 | 0.226482 | F | F | 2.12e+21 | 2.47245e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X151400.30-493717.8 | chandra | ccd6 | 860 | 917.553 | 32.7142 | 7.30476 | 0.00330142 | 0.000737176 | 13.0484 | 1 | 3.4883 | 2.69931 | 121.409 | 8.57912 | 30.8299 | 1.40811 | -0.912643 | 0.304258 | F | F | 2.1e+21 | 4.09111e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X151513.05-494740.1 | chandra | ccd3 | 570.605 | 1082.5 | 18.8611 | 5.55522 | 0.00190342 | 0.000560619 | 17.6736 | 1 | 2.00881 | 1.35102 | 3.72624 | 10.7487 | 17.7722 | 1.08888 | -0.884537 | 0.395158 | F | F | 2.14e+21 | 3.26798e-14 | 1 | dx |
Report | srcpi bgdpi arf | 8 | X151403.63-494912.9 | chandra | ccd7 | 631.314 | 510.75 | 20.5947 | 4.53814 | 0.00207836 | 0.000457977 | 14.7852 | 1 | 1.13012 | 0.359095 | 314.525 | 3.47507 | 9.81014 | 7.81014 | -0.113506 | 0.306085 | A | F | 2.12e+21 | 1.75116e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 5 | X151420.71-495156.2 | chandra | ccd7 | 295.222 | 178.222 | 18.682 | 5.55522 | 0.00188532 | 0.000560615 | 16.2727 | 1 | 1.101 | 0.891109 | 120.971 | 6.499 | 16.5144 | 3.37567 | -0.660568 | 0.342876 | F | T | 2.13e+21 | 1.71356e-14 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X151419.75-494509.9 | chandra | ccd7 | 313.904 | 1004.55 | 15.2523 | 3.90542 | 0.00153922 | 0.000394124 | 10.9498 | 1 | 0.753544 | 0.753544 | 0 | 2.07965 | 6 | 7.74593 | 0.127014 | 0.357352 | F | F | 2.12e+21 | 1.2907e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 6 | X151420.33-495153.5 | chandra | ccd7 | 302.633 | 183.567 | 18.3758 | 5.4441 | 0.00185442 | 0.000549401 | 23.2583 | 1 | 0.769262 | 0.696722 | 20.6543 | 6.43782 | 16.8217 | 1.64331 | -0.822008 | 0.383625 | F | T | 2.13e+21 | 1.68045e-14 | 1 | dbpx |
Report | srcpi bgdpi arf | 2 | X151351.11-494628.5 | chandra | ccd7 | 877.957 | 844.702 | 13.0933 | 3.61847 | 0.00132134 | 0.000365165 | 9.39983 | 1 | 0.936979 | 0.378933 | 114.69 | 2.73013 | 7.86307 | 4.76038 | -0.245788 | 0.386802 | F | F | 2.11e+21 | 1.12542e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 5 | X151426.68-494206.9 | chandra | ccd6 | 339.5 | 329.8 | 12.7435 | 4.7081 | 0.00128604 | 0.000475128 | 25.1617 | 1 | 0.974645 | 0.492 | 123.245 | 4.8142 | 6 | 6.74349 | 0.058343 | 0.372717 | A | T | 2.12e+21 | 1.48565e-14 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X151419.09-494616.0 | chandra | ccd7 | 326.5 | 869.7 | 9.32245 | 4.27872 | 0.000940792 | 0.000431795 | 11.3256 | 1 | 0.492 | 0.492 | 95.8841 | 1.93171 | 9 | 0.661227 | -0.863117 | 0.59021 | F | T | 2.12e+21 | 7.76371e-15 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X151437.33-494216.0 | chandra | ccd6 | 129.611 | 311.056 | 8.72849 | 4.1225 | 0.000880855 | 0.000416031 | 16.7513 | 1 | 1.36552 | 0.62551 | 132.841 | 5.97616 | 1.92243 | 6.80607 | 0.559506 | 0.546427 | A | F | 2.12e+21 | 1.45048e-14 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X151413.84-494029.4 | chandra | ccd6 | 592.75 | 528.125 | 10.7963 | 4.42783 | 0.00108953 | 0.000446844 | 23.9197 | 1 | 1.02259 | 0.492 | 45.1806 | 5.4049 | 4.95926 | 5.83702 | 0.0813028 | 0.41485 | A | T | 2.11e+21 | 1.25361e-14 | 1 | dx |
Report | srcpi bgdpi arf | 7 | X151346.60-494800.6 | chandra | ccd7 | 966.071 | 656.786 | 6.74592 | 3.78388 | 0.000680777 | 0.000381857 | 13.3831 | 1 | 0.492 | 0.492 | 67.5 | 4.03383 | 3.83061 | 3 | -0.121602 | 0.564609 | F | F | 2.11e+21 | 6.29323e-15 | 1 | dx |
Report | srcpi bgdpi arf | 13 | X151403.45-494918.4 | chandra | ccd7 | 634.333 | 499 | 5.70726 | 3.59808 | 0.000575959 | 0.000363106 | 10.5484 | 1 | 0.492 | 0.492 | 51.2644 | 3.56938 | 4.80484 | -0.0975792 | -1 | 1.01529 | F | F | 2.12e+21 | 4.85563e-15 | 1 | dx |
Report | srcpi bgdpi arf | 11 | X151352.54-495022.8 | chandra | ccd7 | 848.833 | 368 | 6.54807 | 3.78388 | 0.00066081 | 0.000381857 | 9.74045 | 1 | 0.645315 | 0.492 | 18.7253 | 5.17847 | 2.87088 | 3.74176 | 0.131699 | 0.583956 | F | F | 2.12e+21 | 5.98235e-15 | 1 | dx |
Report | srcpi bgdpi arf | 12 | X151408.77-494849.0 | chandra | ccd7 | 529.833 | 558.667 | 5.73169 | 3.59808 | 0.000578424 | 0.000363106 | 11.0654 | 1 | 0.620927 | 0.492 | 28.7412 | 3.02737 | 6 | -0.201229 | -1 | 0.859312 | F | F | 2.12e+21 | 4.84548e-15 | 1 | dx |
Report | srcpi bgdpi arf | 9 | X151418.81-494442.1 | chandra | ccd7 | 331.9 | 1060.5 | 4.49184 | 3.39792 | 0.000453302 | 0.000342907 | 6.30121 | 0.999984 | 0.492 | 0.492 | 55.9007 | 2.13194 | 1 | 3.57653 | 0.562988 | 0.864975 | F | F | 2.12e+21 | 5.41231e-15 | 1 | dx |
Report | srcpi bgdpi arf | 10 | X151407.87-494437.3 | chandra | ccd7 | 547.5 | 1070.3 | 4.23776 | 3.39792 | 0.000427661 | 0.000342907 | 4.8539 | 0.999858 | 0.492 | 0.492 | 172.238 | 1.17667 | 4.83061 | -0.338773 | -1 | 1.00987 | F | F | 2.11e+21 | 3.57541e-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