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 | 2 | X175011.55-304703.0 | chandra | ccd2 | 411 | 605.889 | 17.9182 | 5.33013 | 0.00919981 | 0.00273667 | 62.6376 | 1 | 1.43712 | 0.694437 | 93.4305 | 6.16521 | 1 | 16.9182 | 0.888381 | 0.40005 | A | F | 6.71e+21 | 1.47879e-13 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X175024.12-304644.4 | chandra | ccd2 | 81.6667 | 643.333 | 5.9531 | 3.59808 | 0.00305653 | 0.00184738 | 27.49 | 1 | 1.77666 | 0.492 | 113.393 | 8.11116 | 3.9531 | 2 | -0.328082 | 0.644529 | A | F | 6.57e+21 | 4.86406e-14 | 1 | dx |
Report | 3 | X174958.53-304316.7 | chandra | ccd2 | 751.9 | 1066.1 | 4.94434 | 2.23607 | 0.0025386 | 0.00114808 | 12.6968 | 1 | 0.492 | 0.492 | 177.145 | 1.62646 | F | F | 6.98e+21 | 0 | 1 | d | |||||
Report | 1 | X174938.04-303907.9 | chandra | ccd1 | 373 | 412.75 | 3.95586 | 2 | 0.00203112 | 0.00102689 | 10.3314 | 1 | 0.684144 | 0.492 | 26.5651 | 4.54452 | F | F | 7.46e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X175024.61-304033.1 | chandra | ccd3 | 193.75 | 376 | 3.90879 | 3.17945 | 0.00200687 | 0.00163241 | 12.9429 | 1 | 0.914314 | 0.492 | 115.381 | 7.38755 | 4 | -0.0912053 | -1 | 1.14412 | A | F | 6.71e+21 | 3.11014e-14 | 1 | dx |
Report | 1 | X174939.68-304306.4 | chandra | ccd0 | 205.833 | 948.833 | 2.97886 | 1.73205 | 0.00152951 | 0.000889333 | 7.73709 | 0.999982 | 0.492 | 0.492 | 45 | 2.61225 | F | F | 7.28e+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