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 | X113151.58-123158.6 | chandra | ccd7 | 134.179 | 789.276 | 31865.3 | 192.227 | 1.15788 | 0.00698485 | 1162.04 | 1 | 0.747285 | 0.455352 | 90 | 0.320883 | A | F | 3.42e+20 | 8.59515e-12 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 1 | X113151.37-123157.9 | chandra | ccd7 | 140.008 | 790.272 | 4343.37 | 66.7009 | 0.157823 | 0.00242368 | 158.391 | 1 | 0.492 | 0.492 | 61.6621 | 0.301614 | F | F | 3.42e+20 | 1.17178e-12 | 1 | dbpx | ||||
Report | srcpi bgdpi arf | 10 | X113145.68-123458.0 | chandra | ccd7 | 309.688 | 424.624 | 60.0314 | 8.77283 | 0.00218133 | 0.000318774 | 2.18918 | 0.984207 | 0.622496 | 0.622496 | 0 | 3.57816 | F | F | 3.43e+20 | 2.16214e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 7 | X113150.70-123154.6 | chandra | ccd7 | 160.3 | 797.499 | 60.5696 | 12.3406 | 0.00220089 | 0.000448414 | 2.20881 | 0.985561 | 1.40404 | 1.40404 | 0 | 0.280427 | T | F | 3.42e+20 | 1.6373e-14 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 2 | X113156.61-122826.9 | chandra | ccd6 | 298.536 | 223.613 | 23.441 | 5.41034 | 0.000851765 | 0.000196593 | 10.9653 | 1 | 1.12515 | 1.12515 | 0 | 3.46459 | F | F | 3.38e+20 | 9.05415e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 8 | X113150.43-123153.5 | chandra | ccd7 | 168.485 | 799.704 | 114.088 | 10.6812 | 0.00414555 | 0.000388116 | 4.16048 | 0.999978 | 2.24178 | 2.24178 | 0 | 0.323365 | T | F | 3.41e+20 | 3.08322e-14 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 3 | X113152.45-123202.7 | chandra | ccd7 | 108.193 | 780.998 | 51.3206 | 9.21779 | 0.00186481 | 0.000334943 | 1.87152 | 0.968892 | 1.49 | 1.49 | 0 | 0.494751 | T | F | 3.42e+20 | 1.38491e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X113149.73-123149.5 | chandra | ccd7 | 189.235 | 807.765 | 60.5593 | 7.9635 | 0.00220051 | 0.000289366 | 2.20843 | 0.985561 | 1.5 | 1.5 | 0 | 0.401584 | T | F | 3.41e+20 | 1.7608e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X113222.91-123838.4 | chandra | ccd3 | 703.786 | 285.928 | 16.6572 | 5.56793 | 0.000605281 | 0.000202324 | 9.5311 | 1 | 0.886831 | 0.821692 | 133.569 | 10.3992 | F | F | 3.48e+20 | 8.27321e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X113154.06-122949.5 | chandra | ccd6 | 373.833 | 55.1665 | 7.86382 | 3.00003 | 0.000285744 | 0.000109011 | 3.67856 | 0.999076 | 0.770226 | 0.492 | 25.3553 | 1.95776 | A | F | 3.4e+20 | 3.03065e-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