| 1. |
- Feuerbacher, M., et al.
(författare)
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The Samson phase, β-Mg2Al3, Revisited
- 2007
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Ingår i: Zeitschrift für Kristallographie. - 0044-2968. ; 222:6, s. 259-288
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Tidskriftsartikel (refereegranskat)
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| 2. |
- Martin-Carrillo, A., et al.
(författare)
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INTEGRAL detection and follow-up observations of GRBs 080414 and 080603
- 2008
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Ingår i: Proc. Sci..
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Konferensbidrag (refereegranskat)abstract
- INTEGRAL detected GRB 080414 during an open time observation of the Galactic disk. The long (duration ∼10 s) GRB occurred at an off-axis angle of 11.5 degrees with a peak 20-200 keV flux of 1 ph cm-2 s -1 as reported by [1]. The Watcher robotic telescope started observations of GRB 080414 33 sec post GCN trigger. Initial analysis of the first images shows no new source down to 14 magnitude [2]. The burst location was coincidentally very close (30 arcminutes) to XTE J1810-189, which was active at the time. A common origin has been ruled out. GRB 080603 was detected by INTEGRAL during the Key Programme Observation of the North Ecliptic Pole. The burst occurred at about 3 degrees off-axis with a peak 20-200 keV flux of 0.5 ph cm-2 s-1 [3] and a fluence over the same energy range of ∼10-6 erg cm-2. The GRB was within the JEM-X field of view and is well detected between 3 and 35 keV, with a lightcurve consisting of 2 main pulses of emission. Detailed spectral and temporal analyses of the γ-ray emission from both bursts, along with the X-ray characteristics of GRB 080603 and the results of the search for an optical afterglow of GRB 080414 in the Watcher data are presented.
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| 3. |
- McGlynn, Sinéad, et al.
(författare)
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High energy emission and polarisation limits for the INTEGRAL burst GRB061122
- 2009
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 499:2, s. 465-472
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Tidskriftsartikel (refereegranskat)abstract
- Context. GRB061122 is one of the brightest GRBs detected within INTEGRAL's field of view to date, with a peak flux (20-200 keV) of 32 photons cm(-2) s(-1) and fluence of 2 x 10(-5) erg cm(-2). The Spectrometer aboard INTEGRAL, SPI, can measure linear polarisation in bright GRBs through the process of Compton scattering in the Germanium detectors. Polarisation measurements of the prompt emission are relatively rare. The spectral and polarisation results can be combined to provide vital information about the circumburst region. Aims. The two gamma-ray detectors on INTEGRAL were used to investigate the spectral characteristics of GRB061122. A search for linear polarisation in the prompt emission was carried out on GRB061122 using the SPI multiple event data in the energy range 100 keV-1 MeV. The X-ray properties were examined using data from the X-Ray Telescope (XRT) on Swift. Methods. The gamma-ray spectral and temporal properties of GRB061122 were determined using IBIS and SPI. The afterglow properties were obtained using XRT. The multiple event data of GRB061122 from SPI were analysed and compared with the predicted instrument response obtained from Monte-Carlo simulations using the GEANT 4 INTEGRAL mass model. The chi(2) distributions between the real and simulated data as a function of the percentage polarisation and polarisation angle were calculated and limits on the level and angle of polarisation were obtained from the best-fit value of chi(2). Results. The prompt spectrum was best fit by a combination of a blackbody and a power-law model (the quasithermal model), with evidence for high energy emission continuing above 8 MeV. A pseudo-redshift value of pz = 0.95 +/- 0.18 was determined using the spectral fit parameters. The isotropic energy at this pseudo-redshift is 8.5 x 10(52) erg. The jet opening angle was estimated to be smaller than 2.8 degrees or larger than 11.9 degrees from the X-ray lightcurve. An upper limit of 60% polarisation was determined for the prompt emission of GRB061122, using the multiple event data from the spectrometer on INTEGRAL. Conclusions. The high energy emission observed in the spectrum may be due to the reverse shock interacting with the GRB ejecta when it is decelerated by the circumburst medium. This behaviour has been observed in a small fraction of GRBs to date, but is expected to be more commonly observed by the Fermi Gamma-ray Space Telescope. The conditions for polarisation are met if the jet opening angle is less than 2.8 degrees, but further constraints on the level of polarisation are not possible.
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| 4. |
- Tellez, Luis A., et al.
(författare)
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Thermal unfolding of triosephosphate isomerase from Entamoeba histolytica : dimer dissociation leads to extensive unfolding
- 2008
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Ingår i: Biochemistry. - : American Chemical Society (ACS). - 0006-2960 .- 1520-4995. ; 47:44, s. 11665-11673
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Tidskriftsartikel (refereegranskat)abstract
- In mesophiles, triosephosphate isomerase (TIM) is an obligated homodimer. We have previously shown that monomeric folding intermediates are common in the chemical unfolding of TIM, where dissociation provides 75% of the overall conformational stability of the dimer. However, analysis of the crystallographic structure shows that, during unfolding, intermonomeric contacts contribute to only 5% of the overall increase in accessible surface area. In this work several methodologies were used to characterize the thermal dissociation and unfolding of the TIM from Entamoeba histolytica (EhTIM) and a monomeric variant obtained by chemical derivatization (mEhTIM). During EhTIM unfolding, sequential transitions corresponding to dimer dissociation into a compact monomeric intermediate followed by unfolding and further aggregation of the intermediate occurred. In the case of mEhTIM, a single transition, analogous to the second transition of EhTIM, was observed. Calorimetric, spectroscopic, hydrodynamic, and functional evidence shows that dimer dissociation is not restricted to localized interface reorganization. Dissociation represents 55% (DeltaH(Diss) = 146.8 kcal mol(-1)) of the total enthalpy change (DeltaH(Tot) = 266 kcal mol(-1)), indicating that this process is linked to substantial unfolding. We propose that, rather than a rigid body process, subunit assembly is best represented by a fly-casting mechanism. In TIM, catalysis is restricted to the dimer; therefore, the interface can be viewed as the final nucleation motif that directs assembly, folding, and function.
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| 5. |
- Feuerbacher, Michael, et al.
(författare)
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The Samson phase, β-Mg2Al3, revisited
- 2007
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Ingår i: Zeitschrift fur Kristallographie. - : Walter de Gruyter GmbH. - 0044-2968. ; 222:6, s. 259-288
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Forskningsöversikt (refereegranskat)abstract
- The Al-Mg phase diagram has been reinvestigated in the vicinity of the stability range of the Samson phase, β-Mg2Al3 (cF1168). For the composition Mg38.5Al61.5, this cubic phase, space group Fd3̄m (no 227), a = 28.242(1) Å, V = 22526(2) Å3, undergoes at 214°C a first-order phase transition to rhombohedral β′-Mg2Al3, (hR293), a = 19.968(1) Å, c = 48.9114(8) Å, V = 16889(2) Å3, (i.e. 22519 Å3 for the equivalent cubic unit cell) space group R3m (no 160), a subgroup of index four of Fd3̄m. The structure of the β-phase has been redetermined at ambient temperature as well as in situ at 400°C. It essentially agrees with Samson's model, even in most of the many partially occupied and split positions. The structure of β′-Mg 2Al3 is closely related to that of the β-phase. Its atomic sites can be derived from those of the β-phase by group-theoretical considerations. The main difference between the two structures is that all atomic sites are fully occupied in case of the β′-phase. The reciprocal space, Bragg as well as diffuse scattering, has been explored as function of temperature and the β- to β′-phase transition was studied in detail. The microstructures of both phases have been analyzed by electron microscopy and X-ray topography showing them highly defective. Finally, the thermal expansion coefficients and elastic parameters have been determined. Their values are somewhere in between those of Al and Mg.
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| 6. |
- Foley, S., et al.
(författare)
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Global Characteristics Of Gamma-Ray Bursts Observed With Integral
- 2009
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Ingår i: Baltic Astronomy. - 1392-0049. ; 18:3-4, s. 279-283
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Tidskriftsartikel (refereegranskat)abstract
- The gamma-ray instruments on board INTEGRAL have detected and localized 62 gamma-ray bursts (GRBs) to date. The peak flux distribution of these bursts shows that INTEGRAL detects proportionally more weak GRBs than Swift because of its higher sensitivity in a smaller field of view. Spectral lags, i.e., the time delay in the arrival of low-energy gamma rays with respect to high-energy gamma rays, are measured for 31 of the GRBs. Two groups are identified in the spectral lag distribution of INTEGRAL GRBs, one with short lags < 0.75 s (between 25-50 keV and 50-300 keV) and one with long lags > 0.75 s. Most of the long-lag GRBs are inferred to have low redshifts because of their long spectral lags. They are mainly observed in the direction of the supergalactic plane and hence reflect the local large-scale structure of the Universe. This low-luminosity population appears to be distinct from typical cosmological GRBs.
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| 7. |
- Hanlon, L., et al.
(författare)
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Global characteristics of GRBs observed with INTEGRAL and the inferred large population of low-luminosity GRBs
- 2008
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Ingår i: Proc. Sci..
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Konferensbidrag (refereegranskat)abstract
- The g-ray instruments on board INTEGRAL have detected and localised 55 GRBs from launch in October 2002 up to July 2008, including 53 long-duration GRBs (T90 ≳ 2 s) and 2 short-duration GRBs (T90 ≲ 2 s). The spectra of the majority of INTEGRAL GRBs can be well described by single power-laws. In 11 cases, models with curvature, such as the Band model or the power law plus blackbody model, are required to fit the time-averaged burst spectra. INTEGRAL detects proportionally more weak GRBs than Swift because of its higher sensitivity in a smaller field of view. The all-sky rate of GRBs above ∼0.15phcm∼2 s-1 is ∼1400yr-1 in the fully coded field of view of IBIS. Spectral lags i.e. the time delay in the arrival of low-energy g-rays with respect to high-energy g-rays, can be measured for 31 of the GRBs in the sample. Two groups are identified in the spectral lag distribution of INTEGRAL GRBs, one with short lags <0.75 s (between 25-50 keV and 50-300 keV) and one with long lags > 0.75 s. Most of the long-lag GRBs are inferred to have low redshifts because of their tendency to have low peak energies and their faint optical and X-ray afterglows. They are mainly observed in the direction of the supergalactic plane with a quadrupole moment of Q = -0.225 ± 0.090 and hence reflect the local large-scale structure of the Universe. The rate of long-lag GRBs with inferred low luminosity is ∼25% of Type Ib/c SNe. Some of these bursts could be produced by the collapse of a massive star without a SN. Alternatively, they could result from a different progenitor, such as the merger of two white dwarfs or a white dwarf with a neutron star or black hole, possibly in the cluster environment without a host galaxy.
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| 8. |
- McGlynn, Sinead, et al.
(författare)
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GRB 070707 : the first short gamma-ray burst observed by INTEGRAL
- 2008
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 486:2, s. 405-410
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Tidskriftsartikel (refereegranskat)abstract
- Context. INTEGRAL has observed 47 long-duration GRBs (T-90 greater than or similar to 2 s) and 1 short-duration GRB (T-90 less than or similar to 2 s) in five years of observation since October 2002. Aims. This work presents the properties of the prompt emission of GRB 070707, which is the first short hard GRB observed by INTEGRAL. Methods. The spectral and temporal properties of GRB 070707 were determined using the two sensitive coded-mask gamma-ray instruments on board INTEGRAL, IBIS and SPI. Results. The T-90 duration was 0.8 s, and the spectrum of the prompt emission was obtained by joint deconvolution of IBIS and SPI data to yield a best fit power-law with photon index alpha = -1.19(-0.13)(+0.14) , which is consistent with the characteristics of short-hard gamma-ray bursts. The peak flux over 1 s was 1.79(-0.21)(+0.06) photons cm(-2) s(-1) and the fluence over the same interval was (2.07(-0.32)(+0.06) ) x 10(-7) erg cm(-2) in the energy range 20-200 keV. The spectral lag measured between 25-50 keV and 100-300 keV is 20 +/- 5 ms, consistent with the small or negligible lags measured for short bursts. Conclusions. The spectral and temporal properties of GRB 070707 are comparable to those of the short hard bursts detected by other gamma-ray satellites, including BATSE and Swift. We estimate a lower limit on the Lorentz factor Gamma greater than or similar to 25 for GRB 070707, assuming the typical redshift for short GRBs of z = 0.35. This limit is consistent with previous estimates for short GRBs and is smaller than the lower limits of Gamma greater than or similar to 100 calculated for long GRBs. If GRB 070707 is a member of the recently postulated class of short GRBs at z similar to 1, the lower limit on Gamma increases to Gamma greater than or similar to 35.
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