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 | X135644.06-621549.3 | chandra | ccd5 | 703.548 | 872.937 | 183.726 | 15.5703 | 0.0537119 | 0.00455195 | 23.9784 | 1 | 9.47506 | 7.01192 | 55.3984 | 13.439 | 179.418 | 10.4967 | -0.889458 | 0.112517 | F | F | 1.89e+22 | 2.73709e-13 | 1 | dsxf |
| Report | srcpi bgdpi arf | 4 | X135509.16-620035.2 | chandra | ccd7 | 648.72 | 1186.78 | 41.3159 | 6.59391 | 0.0120785 | 0.0019277 | 28.0873 | 1 | 2.36193 | 1.08796 | 355.84 | 5.93132 | 38.532 | 2.45398 | -0.880253 | 0.245652 | F | F | 1.84e+22 | 1.9248e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 1 | X135438.91-620258.3 | chandra | ccd7 | 1080.23 | 894.591 | 10.4493 | 4.42783 | 0.00305479 | 0.00129445 | 14.081 | 1 | 1.79436 | 0.729398 | 168.983 | 6.11356 | 5.86233 | 4.6214 | -0.118367 | 0.428785 | A | F | 1.84e+22 | 4.94392e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X135557.72-621245.5 | chandra | ccd6 | 682.722 | 451.389 | 9.79962 | 4.27872 | 0.00286493 | 0.00125089 | 21.8919 | 1 | 1.58964 | 0.752393 | 88.1322 | 7.6449 | 8.91985 | -0.120227 | -1 | 0.659916 | A | F | 1.87e+22 | 5.59674e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X135423.34-620344.8 | chandra | ccd7 | 1302.33 | 799.333 | 5.45932 | 3.59808 | 0.001596 | 0.00105187 | 7.4245 | 0.999998 | 0.539806 | 0.492 | 92.3818 | 7.40436 | 4.69104 | 0.768279 | -0.718544 | 0.822322 | F | F | 1.83e+22 | 2.76954e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X135523.29-620129.3 | chandra | ccd7 | 446 | 1076.5 | 3.83061 | 3.17945 | 0.00111986 | 0.000929492 | 9.30741 | 0.999999 | 0.492 | 0.492 | 121.717 | 4.80975 | 1 | 2.83061 | 0.47789 | 0.936301 | F | F | 1.85e+22 | 1.75964e-14 | 1 | dx |
| Report | 6 | X135524.57-620408.2 | chandra | ccd7 | 427.75 | 753.5 | 3.92776 | 2 | 0.00114826 | 0.000584688 | 2.67016 | 0.993151 | 0.562592 | 0.492 | 164.675 | 2.1714 | F | F | 1.85e+22 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X135510.93-620219.8 | chandra | ccd7 | 622.75 | 973.75 | 3.92783 | 3.17945 | 0.00114828 | 0.000929492 | 14.6213 | 1 | 0.578157 | 0.492 | 21.2552 | 4.20117 | 4 | -0.0721658 | -1 | 1.14412 | F | F | 1.85e+22 | 1.76914e-14 | 1 | dx |
| Report | 7 | X135514.02-620309.1 | chandra | ccd7 | 578.5 | 873.5 | 3.92075 | 2 | 0.00114621 | 0.000584688 | 2.66539 | 0.993151 | 0.492 | 0.492 | 45 | 3.30626 | F | F | 1.85e+22 | 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