Codici di distillazione per la mitigazione d’attacchi di tipo Denial of Service in comunicazioni Multicast

Si descrivono dei codici di distillazione per la mitigazione degli effetti di un DoS nelle comunicazioni multicast. Si fa uso di una tecnica di signature amortization basata sul Merkle tree, ulteriormente ottimizzato. Le comunicazioni dei dati sono su multi-channel: si prevede uno scheduling adeguato dei pacchetti sui diversi canali

On the accuracy of the S/N estimates obtained with the exposure time calculator of the Wide Field Planetary Camera 2 on board the Hubble Space Telescope

We have studied the accuracy and reliability of the exposure time calculator (ETC) of the Wide Field Planetary Camera 2 (WFPC2) on board the Hubble Space Telescope (HST) with the objective of determining how well it represents actual observations and, therefore, how much confidence can be invested in it and in similar software tools. We have found, for example, that the ETC gives, in certain circumstances, very optimistic values for the signal-to-noise ratio (SNR) of point sources. These values overestimate by up to a factor of 2 the HST performance when simulations are needed to plan deep imaging observations, thus bearing serious implications on observing time allocation. For this particular case, we calculate the corrective factors to compute the appropriate SNR and detection limits and we show how these corrections vary with field crowding and sky background. We also compare the ETC of the WFPC2 with a more general ETC tool, which takes into account the real effects of pixel size and charge diffusion. Our analysis indicates that similar problems may afflict other ETCs in general showing the limits to which they are bound and the caution with which their results must be taken.Comment: 14 pages, 13 figures, to be published in PASP on July 200

Interferometry of chemically peculiar stars: theoretical predictions vs. modern observing facilities

By means of numerical experiments we explore the application of interferometry to the detection and characterization of abundance spots in chemically peculiar (CP) stars using the brightest star eps~Uma as a case study. We find that the best spectral regions to search for spots and stellar rotation signatures are in the visual domain. The spots can clearly be detected already at a first visibility lobe and their signatures can be uniquely disentangled from that of rotation. The spots and rotation signatures can also be detected in NIR at low spectral resolution but baselines longer than 180~m are needed for all potential CP candidates. According to our simulations, an instrument like VEGA (or its successor e.g., FRIEND) should be able to detect, in the visual, the effect of spots and spots+rotation, provided that the instrument is able to measure $V^2\approx10^{-3}$, and/or closure phase. In infrared, an instrument like AMBER but with longer baselines than the ones available so far would be able to measure rotation and spots. Our study provides necessary details about strategies of spot detection and the requirements for modern and planned interferometric facilities essential for CP star research.Comment: Accepted by NMRAS, 18 pages, 11 figures, 2 table

SFADI: the Speckle-Free Angular Differential Imaging method

We present a new processing technique aimed at significantly improving the angular differential imaging method (ADI) in the context of high-contrast imaging of faint objects nearby bright stars in observations obtained with extreme adaptive optics (EXAO) systems. This technique, named "SFADI" for "Speckle-Free ADI", allows to improve the achievable contrast by means of speckles identification and suppression. This is possible in very high cadence data, which freeze the atmospheric evolution. Here we present simulations in which synthetic planets are injected into a real millisecond frame rate sequence, acquired at the LBT telescope at visible wavelength, and show that this technique can deliver low and uniform background, allowing unambiguous detection of $10^{-5}$ contrast planets, from $100$ to $300$ mas separations, under poor and highly variable seeing conditions ($0.8$ to $1.5$ arcsec FWHM) and in only $20$ min of acquisition. A comparison with a standard ADI approach shows that the contrast limit is improved by a factor of $5$. We extensively discuss the SFADI dependence on the various parameters like speckle identification threshold, frame integration time, and number of frames, as well as its ability to provide high-contrast imaging for extended sources, and also to work with fast acquisitions.Comment: Accepted for publication in Ap

De-biasing interferometric visibilities in VLTI-AMBER data of low SNR observations

AIMS: We have found that the interferometric visibilities of VLTI-AMBER observations, extracted via the standard reduction package, are significantly biased when faint targets are concerned. The visibility biases derive from a time variable fringing effect (correlated noise) appearing on the detector. METHODS: We have developed a method to correct this bias that consists in a subtraction of the extra power due to such correlated noise, so that the real power spectrum at the spatial frequencies of the fringing artifact can be restored. RESULTS: This pre-processing procedure is implemented in a software, called AMDC and available to the community, to be run before the standard reduction package. Results obtained on simulated and real observations are presented and discussed.Comment: 7 pages, 9 figure

On the binarity of the classical Cepheid X Sgr from interferometric observations

Optical-infrared interferometry can provide direct geometrical measurements of the radii of Cepheids and/or reveal unknown binary companions of these stars. Such information is of great importance for a proper calibration of Period-Luminosity relations and for determining binary fraction among Cepheids. We observed the Cepheid X Sgr with VLTI/AMBER in order to confirm or disprove the presence of the hypothesized binary companion and to directly measure the mean stellar radius, possibly detecting its variation along the pulsation cycle. From AMBER observations in MR mode we performed a binary model fitting on the closure phase and a limb-darkened model fitting on the visibility. Our analysis indicates the presence of a point-like companion at a separation of 10.7 mas and 5.6 magK fainter than the primary, whose flux and position are sharply constrained by the data. The radius pulsation is not detected, whereas the average limb-darkened diameter results to be 1.48+/-0.08 mas, corresponding to 53+/-3 R_sun at a distance of 333.3 pc.Comment: 5 pages, 3 figures, research not

Stavroula Pipyrou, The grecanici of southern Italy: Governance, violence, and minority politics, Philadelphia, University of Pennsylvania Press, 2016, pp. 246

Book review of Stavroula Pipyrou, The grecanici of southern Italy: Governance, violence, and minority politics, Philadelphia, University of Pennsylvania Press, 2016, pp. 246.Recensione di Stavroula Pipyrou, The grecanici of southern Italy: Governance, violence, and minority politics, Philadelphia, University of Pennsylvania Press, 2016, pp. 246

Generazione di ibridi, generazione di donne. Costruzioni dell’umano in Aristotele e Galeno (e Palefato)

Denying or rationalizing the mythical monstrous hybrids in Aristotle, Palaephatus and Galen is also making use of the animal as a keystone for the construction of human. In such sense, through the reflection on centaurs and monsters, the three authors build the sphere of human as tendentially separated from animal’s. This sphere also tends to include the woman seen as a “dimensional door to theriomorfic alterity”, then as a threat to identity

Aleksander Bošković, Günther Schlee, a cura di, African political systems revisited: Changing perspectives on statehood and power, New York-Oxford, Berghahn Books, 2022, pp. 256

Book review of Aleksander Bošković, Günther Schlee, edited by, African political systems revisited: Changing perspectives on statehood and power, New York-Oxford, Berghahn Books, 2022, pp. 256.Recensione di Aleksander Bošković, Günther Schlee, a cura di, African political systems revisited: Changing perspectives on statehood and power, New York-Oxford, Berghahn Books, 2022, pp. 256

The role of CX3CR1 in pancreatic cancer

PhDPancreatic adenocarcinoma (PDAC) is the fourth leading cause of cancer death in Western countries. The PDAC tumour microenvironment (TME) is characterized by a dense stromal reaction, consisting of many cell types including fibroblasts and immune cells. The chemokine receptor, CX3CR1 forms a high-affinity axis with its unique ligand CX3CL1 and is expressed on monocytes, macrophages and T cells. CX3CR1 is also present on pancreatic malignant cells, where it has been associated with metastasis formation. The aim of my project is to investigate the role of CX3CR1 in the progression and development of pancreatic cancer in a genetically engineered mouse model of PDAC, the CX3CR1GFP/GFPLSL-KRASG12D/+LSL-Trp53R172H/+Pdx1-Cre (CKPC) mouse. In these mice, the CX3CR1 protein is not functional but they express GFP. I have found that the absence of CX3CR1 in KPC mice has no effect in their lifespan and response to chemotherapy. Comparison of the immune infiltrate of the tumours revealed that the lack of CX3CR1 causes a significant decrease in T cells and a possible increase in myeloid cells in CKPC mice compared to KPC mice. Expression analysis of several inflammatory cytokines in the TME showed a significant difference in IL-10 between KPC and CKPC mice. There was also a significant increase in levels of, CX3CL1, both locally and in the plasma. Finally, we performed RNA-seq on KPC and CKPC tumours. My analysis revealed 607 differentially-expressed genes, some of which encoded other chemokines or protein regulating the immune system. In particular, I observed the upregulation of Cxcl10 and Cxcl12, and the downregulation of Gata3 and S100a4, which could explain the decrease in T cells in the TME of CKPC mice. In conclusion, although the lack of CX3CR1 modifies the TME in this genetic model of PDAC, these changes do not affect the lifespan or the response to chemotherapy