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 | X175748.70-275214.4 | chandra | ccd3 | 219.731 | 602.505 | 154.173 | 12.735 | 0.0791089 | 0.00653454 | 54.4863 | 1 | 2.83459 | 1.76907 | 110.047 | 7.74267 | 115.577 | 44.4187 | -0.444752 | 0.093905 | F | F | 5.96e+21 | 1.154e-12 | 1 | dsxf |
Report | srcpi bgdpi arf | 1 | X175710.07-275753.6 | chandra | ccd0 | 160.333 | 874 | 5.80858 | 3.59808 | 0.00298044 | 0.00184621 | 13.2764 | 1 | 0.653336 | 0.492 | 160.239 | 2.49261 | 2.93619 | 2.87239 | -0.0109847 | 0.627687 | F | F | 6.21e+21 | 3.90896e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X175700.10-280113.0 | chandra | ccd0 | 429 | 469.178 | 17.5028 | 4.18363 | 0.00898103 | 0.00214671 | 44.7429 | 1 | 1.7966 | 1.7966 | 0 | 6.35719 | 1.91533 | 14.9153 | 0.7724 | 0.393593 | F | F | 6.2e+21 | 1.31522e-13 | 1 | dsx |
Report | 3 | X175721.26-275826.5 | chandra | ccd2 | 893.833 | 851.167 | 2.9863 | 1.73205 | 0.0015323 | 0.000888733 | 7.65046 | 0.99998 | 0.492 | 0.492 | 106.845 | 1.96572 | F | F | 6.06e+21 | 0 | 1 | d | |||||
Report | 2 | X175745.79-280244.3 | chandra | ccd2 | 233.833 | 326.833 | 2.94021 | 1.73205 | 0.00150865 | 0.000888733 | 7.53239 | 0.99998 | 1.06521 | 0.615 | 90 | 8.51314 | A | F | 5.58e+21 | 0 | 1 | d | |||||
Report | 1 | X175740.83-275717.1 | chandra | ccd2 | 367 | 992 | 1.98163 | 1.41421 | 0.0010168 | 0.000725648 | 5.07665 | 0.999474 | 0.492 | 0.492 | 45 | 4.77759 | F | F | 5.88e+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