The spectra of short gamma-ray bursts

We present the results of the spectral analysis of a sample of short bright γ--ray bursts (GRB) detected by BATSE and compare them with the average and time resolved spectral properties of long bright bursts. While the spectral parameters of short GRBs confirm, as expected from previous works based on the hardness ratio, that they are harder than long events, we find that this difference is mainly due to a harder low energy spectral component present in short bursts, rather than to a (marginally) different peak energy. Intriguingly our analysis also reveals that the emission properties of short GRBs are similar to the first 2 s of long events. This might suggest that the central engine of long and short GRBs is the same, just working for a longer time for long GRBs. We find that short bursts do not obey the correlation between peak frequency and isotropic emitted energy for any assumed redshift, while they can obey the similar correlation between the peak frequency and isotropic emitted luminosity. This is consistent with (although not a proof of) the idea that short GRBs emit a γ--ray luminosity similar to long GRBs. If they indeed obey the peak frequency -- isotropic luminosity relation, we can estimate the redshift distribution of short bursts, which turns out to be consistent with that of long bursts just with a slightly smaller average redshift

Fermi/GBM and Batse Gamma-Ray Bursts: comparison of the spectral properties

The Gamma-ray Burst Monitor (GBM) on board Fermi allows to study the spectra of Gamma Ray Bursts (GRBs) over an unprecedented wide energy range (8 keV - 35 MeV). We compare the spectral properties of short and long GRBs detected by the GBM (up to March 2010) with those of GRBs detected by the BATSE instrument on board the CGRO. GBM and BATSE long bursts have similar distributions of fluence (F), Epeak and peak flux (P) but GBM bursts have a slightly harder low-energy spectral index \alpha with respect to BATSE GRBs. GBM and BATSE short bursts have similar distributions of fluence, \alpha and peak flux, with GBM bursts having slightly larger Epeak. We discuss these properties in light of the found correlations between Epeak and the fluence and the peak flux. GBM bursts confirm that these correlations are not determined by instrumental selection effects. Indeed, GBM bursts extend the Epeak-Fluence and Epeak-P correlations both in fluence/peak flux and in peak energy. No GBM long burst with Epeak exceeding a few MeV is found, despite the possibility of detecting it. Similarly to what found with BATSE, there are 3% of GBM long bursts (and almost all short ones) that are outliers at more than 3\sigma of the Epeak-Eiso correlation. Instead there is no outlier of the Epeak-Lp,iso correlation, for both long and short GBM bursts.Comment: The subject of this work is similar to our paper arXiv:1004.1410, that was rejected because based on Fermi/GBM spectral preliminary results reported in GCN Circulars. The present work is based on our own analysis of Fermi/GBM bursts detected up to March 2010 (presented in arXiv:1012.2863). Submitted to A&

The radio-loud AGN population at z 73 1 in the COSMOS field. I. selection and spectral energy distributions

We select a sample of radio galaxies at high redshifts (z 73 1) in the COSMOS field by cross-matching optical and infrared (IR) images with the FIRST radio data. The aim of this study is to explore the high-z radio-loud (RL) active galactic nuclei (AGN) population at much lower luminosities than the classical samples of distant radio sources, which are similar to those of the local population of radio galaxies. Precisely, we extended a previous analysis focused on low-luminosity radio galaxies. The wide multiwavelength coverage provided by the COSMOS survey allows us to derive their spectral energy distributions (SEDs). We model them with our own developed technique 2SPD that includes old and young stellar populations and dust emission. When added to those previously selected, we obtain a sample of 74 RL AGN. The SED modeling returns several important quantities associated with the AGN and host properties. The resulting photometric redshifts range from z ~ 0.7 to 3. The sample mostly includes compact radio sources but also 21 FR IIs sources; the radio power distribution of the sample covers ~1031.5 - 1034.3 erg s-1 Hz-1, thus straddling the local FR I/FR II break. The inferred range of stellar mass of the hosts is ~1010 - 1011.5M 99. The SEDs are dominated by the contribution from an old stellar population with an age of ~1 - 3 Gyr for most of the sources. However, UV and mid-IR (MIR) excesses are observed for half of the sample. The dust luminosities inferred from the MIR excesses are in the range, Ldust ~ 1043 - 1045.5 erg s-1, which are associated with temperatures approximately of 350-1200 K. Estimates of the UV component yield values of ~1041.5 - 1045.5 erg s-1 at 2000 \uc5. The UV emission is significantly correlated with both IR and radio luminosities; the former being the stronger link. However, the origin of UV and dust emission, whether it is produced by the AGN of by star formation, is still unclear. Our results show that this RL AGN population at high redshifts displays a wide variety of properties. Low-power radio galaxies, which are associated with UV- and IR-faint hosts are generally similar to red massive galaxies of the local FR Is. At the opposite side of the radio luminosity distribution, large MIR and UV excesses are observed in objects consistent with quasar-like AGN, as also proved by their high dust temperatures, which are more similar to local FR IIs

Re-born fireballs in Gamma-Ray Bursts

We consider the interaction between a relativistic fireball and material assumed to be still located just outside the progenitor star. Only a small fraction of the expected mass is sufficient to decelerate the fireball efficiently, leading to dissipation of most of its kinetic energy. Since the scattering optical depths are still large at distances comparable to the progenitor radius, the dissipated energy is trapped in the system, accelerating it to relativistic velocities. The process resembles the birth of another fireball at radii R similar to 10(11) cm, not far from the transparency radius, and with starting bulk Lorentz factors Gamma(c) similar to 10. As seen in the observer frame, this `re- generated' fireball appears collimated within an angle theta = 1/Gamma(c). If the central engine works intermittently, the funnel can, at least partially, refill and the process can repeat itself. We discuss how this idea can help to solve some open issues of the more conventional internal shock scenario for interpreting gamma-ray burst propertie

Constraints on the bulk Lorentz factor of gamma-ray burst jets from Fermi/LAT upper limits

It is largely recognized that gamma-ray burst (GRB) jets involve ultrarelativistic motion. However, the value of the Lorentz factor Γ0 is still not clear and only lower limits are known for most bursts. We suggest here a new method to obtain upper limits on Γ0. The early highenergy synchrotron afterglow flux depends strongly on Γ0. Upper limits on GeV emission therefore provide upper limits on Γ0. Applying this method to 190 Fermi GRBs which have not been detected by the Fermi-LAT, we place upper limits on the high-energy afterglow flux, and in turn on Γ0. For bursts at a typical redshift z = 2, we find values of the order of 200 (and above) for a homogeneous density medium, and in the range 100-400 for a wind-like medium. These upper limits are consistent with (and are very close to) lower limits and direct estimates inferred using other methods, suggesting that the typical Lorentz factors of GRB jets are of the order of a few hundred. © 2016 The Authors

Coronal properties of the luminous radio-quiet quasar QSO B2202–209

We present an analysis of the joint $XMM$-$Newton$ and $NuSTAR$ observations of the radio-quiet quasar QSO B2202$-$209. Using an optical observation from the Hale Telescope at the Palomar Observatory, we revise the redshift of the source from the previously reported $z=1.77$ to $z=0.532$, and we estimate the mass of the central black hole, \log (M_\rm BH/M_\odot) = 9.08 \pm 0.18. The X-ray spectrum of this source can be well described by a power-law of photon index $\Gamma = 1.82 \pm 0.05$ with E_\rm cut = 152_-54^+103\,\rm keV, in the rest frame of the source. Assuming a Comptonisation model, we estimate the coronal temperature to be kT_\rm e=42\pm 3 \,\rm keV and kT_\rm e= 56 \pm 3\,\rm keV for a spherical and a slab geometry, respectively. The coronal properties are comparable to the ones derived for local AGN, despite a difference of around one order of magnitude in black hole mass and X-ray luminosity ($L_2-10 = 1.93\times 10^45\,\rm erg\,s^-1$). The quasar is X-ray loud, with an unusually flat observed optical-to-X-ray spectral slope \alpha_\rm OX = 1.00 \pm 0.02, and has an exceptionally strong optical [O III] line. Assuming that both the X-ray emission and the [O III] line are isotropic, these two extreme properties can be explained by a nearly edge-on disk, leading to a reduction in the observed UV continuum light

Reduced probability of improving viro-immunological state in subjects with vertical transmission of HIV reaching adult age: A multicenter retrospective cohort study

Introduction: Young adults with vertical transmission (VT) of human immunodeficiency virus (HIV) represent a fragile population. This study evaluates factors associated with viro-immunological outcome of these patients. Methods: We performed a multicenter study including HIV-infected subjects with VT ≥ 18 years old from six Italian clinics. Subjects were observed from birth to death, lost to follow-up, or last visit until December 31, 2019. Condition of "optimal viro-immunological status" (OS) was defined as the simultaneous presence of HIV ribonucleic acid (RNA) < 50 copies/mL, CD4+ > 500 cells/mm3 , and CD4+/CD8+ ratio ≥ 1. Results: A total of 126 subjects were enrolled. At 18 years of age, 52/126 (44.4%) had HIV-RNA > 50 copies/mL, 47/126 (38.2%) had CD4+ < 500/mm3 , and 78/126 (67.2%) had CD4+/CD8+ < 1; 28 subjects (23.7%) presented in the condition of OS. Having a CD4+/CD8+ ratio ≥ 1 at 18 years of age was related with an increased probability of shift from suboptimal viro-immunological status (SOS) to OS (HR: 7.7, 95% confidence interval [CI]: 4.23-14.04), and a reduced risk of shift from the OS to the SOS (HR: 0.49, 95% CI: 0.26-0.92). Acquired immunodeficiency syndrome (AIDS) diagnosis significantly reduced the probability of shift from a viro-immunological SOS to OS (HR: 0.09, 95% CI: 0.03-0.30). Subjects who had not achieved an OS at 18 years of age had an increased risk of discontinuation of combination antiretroviral therapy (cART, p = .019). Conclusions: Only a small proportion of subjects with VT of HIV reached the adult age with "OS". Transition to the adult care with a compromised viro-immunological condition represents a negative driver for future optimal infection control, with a higher risk of discontinuation of cART and a reduced probability to improve the immunological status later in the years

Translating in the Environmental Field: The Case of the Website of the Stelvio National Park ​

reservedCe mémoire a pour objectif d’analyser les caractéristiques et les stratégies de la traduction et de la révision dans le domaine de l’environnement, notamment le tourisme de nature. Le cas d’étude est représenté par le site web d’un parc national italien : le parc du Stelvio, plus spécifiquement le secteur trentin du Parc, dont la traduction (IT > FR) et la révision (EN > EN) seront proposées. Pour cela, l’environnement en général et le domaine environnemental objet de l’analyse, à savoir l’environnement des Alpes, seront explorés, en se penchant surtout sur la terminologie. Ensuite, les discours caractérisant les pages du site, notamment le discours scientifique et le discours touristique, seront pris en examen, en présentant les publications qui ont été considérées comme particulièrement pertinentes pour ce travail ; des articles proposant une analyse terminologique et de traduction de textes sur les sciences naturelles et sur le tourisme seront illustrés, avec une attention particulière pour l’utilité des corpus comparables. Cette première partie de la recherche servira de base pour passer à examiner le travail terminologique, traductologique et de révision mené pour les textes du site. Les étapes de la compilation de fiches terminologiques, notamment la recherche et la rédaction de définitions terminologiques, seront illustrées. Finalement, nous verrons dans le détail les stratégies adoptées dans la traduction et dans la révision des textes