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 | 3 | X130342.24-241455.6 | chandra | ccd7 | 629.24 | 429.035 | 60.4561 | 27.4716 | 0.00618085 | 0.00280862 | 3.97028 | 0.999937 | 1.97091 | 1.97091 | 0 | 1.02516 | F | F | 8.88e+20 | 4.03906e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X130347.82-241846.9 | chandra | ccd6 | 256.5 | 964.375 | 7.5738 | 2.82844 | 0.000774321 | 0.00028917 | 7.17811 | 0.999997 | 0.602173 | 0.492 | 102.131 | 3.29761 | F | F | 8.92e+20 | 7.38164e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X130332.45-242306.3 | chandra | ccd6 | 683.5 | 437.269 | 11.5919 | 3.60558 | 0.00118512 | 0.000368623 | 10.9863 | 1 | 1.47911 | 0.827829 | 169.373 | 7.47572 | A | F | 8.88e+20 | 1.22289e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X130324.92-242524.9 | chandra | ccd6 | 892.5 | 155.5 | 12.352 | 4.24275 | 0.00126283 | 0.000433765 | 11.7067 | 1 | 0.492 | 0.492 | 90 | 10.2056 | F | F | 8.86e+20 | 1.38771e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X130327.65-242509.2 | chandra | ccd6 | 816.808 | 187.346 | 9.83132 | 3.60561 | 0.00100512 | 0.000368626 | 9.31768 | 1 | 3.38076 | 1.34696 | 105.498 | 9.75213 | A | F | 8.87e+20 | 1.09118e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X130323.85-242425.6 | chandra | ccd6 | 922.192 | 276.039 | 9.63616 | 3.60561 | 0.00098517 | 0.000368627 | 9.13272 | 1 | 2.02825 | 1.52909 | 58.0267 | 9.38727 | F | F | 8.86e+20 | 1.06662e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X130347.05-242325.6 | chandra | ccd6 | 278 | 398 | 3.77863 | 2.00001 | 0.000386315 | 0.000204474 | 3.58121 | 0.99429 | 0.492 | 0.492 | 90 | 7.67171 | F | F | 8.91e+20 | 4.04638e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X130334.69-242136.7 | chandra | ccd6 | 621.79 | 619.938 | 26.7596 | 5.17297 | 0.00273583 | 0.00052887 | 25.3615 | 1 | 2.29287 | 0.9981 | 11.8471 | 5.92031 | F | F | 8.89e+20 | 2.72752e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X130327.01-242041.3 | chandra | ccd6 | 834.833 | 731.833 | 2.79464 | 1.73206 | 0.000285715 | 0.00017708 | 2.64863 | 0.973266 | 0.492 | 0.492 | 106.845 | 5.7589 | F | F | 8.87e+20 | 2.9751e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X130322.31-241737.9 | chandra | ccd6 | 965.5 | 1104.5 | 2.88553 | 1.73205 | 0.000295007 | 0.00017708 | 2.73478 | 0.973266 | 0.492 | 0.492 | 90 | 4.59045 | F | F | 8.86e+20 | 3.11463e-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