2009A&A...496..557L


Query : 2009A&A...496..557L

2009A&A...496..557L - Astronomy and Astrophysics, volume 496557-576 (2009/3-3)

Analysis of extremely low signal-to-noise ratio data from INTEGRAL/PICsIT.

LUBINSKI P.

Abstract (from CDS):

The PICsIT detector onboard the INTEGRAL satellite was designed to provide information about emission in the soft γ-ray band for many bright sources. Due to strong and variable instrumental background, only 4 objects have been detected so far using standard software. The moderate sensitivity of PICsIT can be compensated for in the case of many objects by adopting a long exposure time, thanks to INTEGRAL's large field of view and an observing strategy focused on the Galactic plane. With angular resolution far higher than that of all other instruments operating in a similar energy band, PICsIT is suitable for fields too crowded or too significantly affected by Galactic diffuse emission. Therefore, it is desirable to improve the spectral extraction software to both obtain more reliable results and enlarge the number of objects that can be studied. The new PICsIT spectral extraction method is based on three elements: careful modelling of the background, an energy-dependent pixel-illumination function, and the computation of the probability density of the source count rate. Background maps of the detector plane are prepared for short periods and relatively narrow energy bands to insure that the background dependence on time and energy is modelled well. The most important element of the new spectral extraction method is the proper treatment of the Poisson-distributed data, developed within a Bayesian framework. The new method was tested extensively on both a large true data set and simulated data.
Result. assumed in simulations were reproduced perfectly, without any bias and with high precision. Count rates measured for Crab were far more stable than those obtained with the standard software. For weaker sources, the new method produced spectra of far higher quality and allows us to detect at least 8 additional objects. Comparison with other INTEGRAL instruments demonstrated that PICsIT is well calibrated and provides valuable information about the continuum emission in the 250keV-1MeV band, detectable currently only by INTEGRAL.

Abstract Copyright: ∼

Journal keyword(s): gamma rays: observations - instrumentation: detectors - methods: data analysis - methods: statistical

Simbad objects: 21

goto Full paper

goto View the references in ADS

Number of rows : 21
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
2 NGC 4051 Sy1 12 03 09.6101337312 +44 31 52.682601288   11.08 12.92 9.94   ~ 2270 1
3 NGC 4151 Sy1 12 10 32.5759813872 +39 24 21.063527532   12.18 11.48     ~ 3938 2
4 NAME Centaurus A BLL 13 25 27.61521044 -43 01 08.8050291   8.18 6.84 6.66   ~ 4774 3
5 PSR B1509-58 Psr 15 13 47.6 -59 07 54     13.06     ~ 879 1
6 V* V381 Nor HXB 15 50 58.6637920704 -56 28 35.258385000           K3III 1254 0
7 V* V1033 Sco HXB 16 54 00.1423963019 -39 50 44.761701340       16.14   F3-6IV 1980 0
8 V* V821 Ara LXB 17 02 49.3876391280 -48 47 23.087954544         15.322 ~ 2237 0
9 HD 153919 HXB 17 03 56.7725629224 -37 50 38.913331452 6.06 6.78 6.51 6.08 5.90 O6Iafcp 851 0
10 2E 3938 HXB 17 43 54.7 -29 44 44           ~ 693 1
11 [KRL2007b] 270 gam 17 45 38.5 -29 01 15           ~ 27 0
12 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
13 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 4970 3
14 [CHM2006] Candidate 1b LXB 17 49 38.039 -28 21 17.50           ~ 82 0
15 2MAXI J1753-013 LXB 17 53 28.2898766424 -01 27 06.256555272 15.30 16.73 16.46 16.15 15.64 ~ 384 0
16 2CXO J180112.3-254436 HXB 18 01 12.4783119670 -25 44 35.694663099           AV 417 1
17 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2810 0
18 HD 226868 HXB 19 58 21.6757355952 +35 12 05.784512688 9.38 9.72 8.91 8.42   O9.7Iabpvar 4590 0
19 NAME Cyg Complex reg 20 32 +45.0           ~ 667 0
20 NAME Cas A SNR 23 23 26.0 +58 48 41     14.30     ~ 3033 1
21 NAME Galactic Bulge reg ~ ~           ~ 4794 0

To bookmark this query, right click on this link: simbad:objects in 2009A&A...496..557L and select 'bookmark this link' or equivalent in the popup menu