cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Διαχείριση χρηματοοικονομικών επενδύσεων στο πλαίσιο της χρηματοοικονομικής τεχνολογίας (FinTech)
Creators: name: Κολιάκος, Χρήστος
Publisher: name: Πανεπιστήμιο Πειραιώς
Year: 2023
Subjects: subject: FinTech
subject: Διαχείριση χαρτοφυλακίου
subject: Blockchain

description: Αντικείμενο της διπλωματικής εργασίας αποτελεί η σύγκριση αμοιβαίων κεφαλαίων που επενδύουν βασισμένα στις παραδοσιακές μεθόδους και σε αμοιβαία κεφάλαια και επενδυτικά χρηματοπιστωτικά ιδρύματα που επενδύουν βασισμένα στην τεχνολογία. Στο πρώτο μέρος της διπλωματικής εργασίας παρουσιάζονται τα προηγμένα εργαλεία του συμπλέγματος οικονομίας και τεχνολογίας (FinTech) που είναι διαθέσιμα στους επενδυτές και πως χρησιμοποιούνται από τα μεγάλα fund και τα χρηματοπιστωτικά ιδρύματα. Στην συνέχεια αναπτύσσετε η μεθοδολογία που ακολουθήθηκε για την σύγκριση των Hedge Funds μέσω συγκεκριμένων δεικτών. Για την πραγματοποίηση της ανάλυσης, σχετικά με την απόδοση των ‘έξυπνων’ αμοιβαίων κεφαλαίων, πραγματοποιήθηκε η συλλογή δεδομένων από σχετικές αξιόπιστες πηγές. Τα επονομαζόμενα ‘έξυπνα’ Ηedge Fund μπορεί να περιλαμβάνουν μια ευρεία γκάμα από περιουσιακά στοιχεία, το καθένα με τα δικά του ευφυή χαρακτηριστικά. Παρ’ όλα αυτά, έγινε επιλογή εκείνων των Ηedge Fund, τα οποία σχετίζονται με την τεχνολογία και ειδικότερα με την Τεχνητή Νοημοσύνη. Επιπλέον, για την αξιολόγηση αυτών των ‘έξυπνων’ Ηedge Fund, επιλέχθηκαν στατιστικά και χρηματοοικονομικά μέτρα, τα οποία χρησιμοποιούνται κατά κόρον στην ανάλυση απόδοσης χρηματοοικονομικών και χρηματιστηριακών στοιχείων. Οι δυο αυτές κατηγορίες μέτρων προσφέρουν μια συνολική εικόνα ενός περιουσιακού στοιχείου και δίνουν μια ολοκληρωμένη πληροφόρηση σχετικά με την απόδοση του. Η ανάλυση των ‘έξυπνων’ Ηedge Fund είναι μια διαχρονική εργασία, και θα πρέπει να περιλαμβάνει στοιχεία απόδοσης του κι από περιόδους κρίσεις. Σε κάθε περίπτωση, θα πρέπει να συγκρίνεται με σημαντικούς χρηματοοικονομικούς δείκτες, καθώς επίσης κι άλλες κατηγορίες από Ηedge Fund. Από τα δεδομένα της εργασίας προκύπτει ότι ολοένα και ενισχύεται ο αριθμός των επενδυτών, οι οποίοι προτιμούν τα Ηedge Fund, σε σύγκριση με παραδοσιακά στοιχεία όπως μετοχές και δείκτες. 3 Παρ’ όλα αυτά, η απόδοση τους δεν αντικατοπτρίζει πάντα αυτήν την προτίμηση. Οι αποδόσεις μεταξύ Fund σε μακρο-οικονομικά στοιχεία και σε αυτά με υποκείμενο τίτλο μετοχές έχουν πολύ μικρό βαθμό συσχέτισης, ενδεχομένως λόγω της φύσης του υποκείμενου τίτλου. Κάτι τέτοιο παρατηρείται και με τα ‘έξυπνα’ Ηedge Fund. Βάσει των χρηματοοικονομικών και στατιστικών μέτρων, είναι ασφαλές να υποθέσουμε ότι τα ‘έξυπνα’ Ηedge Fund προσφέρουν μια ελκυστική επενδυτική λύση, με ικανοποιητικές αποδόσεις, αλλά ταυτόχρονα κι ελεγχόμενο επίπεδο κινδύνου.
ESPRESSO vede la luce in fondo al “tunnel”
Creators: Massimo Ramella
Publisher: name: Media Inaf
Year: 2016

Collaudo pienamente riuscito per il sistema di ottiche che unisce uno dei telescopi del VLT dell’ESO, a Paranal, e il Coudé Combined Laboratory, dove nel 2017 verrà installato lo spettrografo ESPRESSO. Un risultato raggiunto grazie al contributo di ricercatori dell’INAF di Trieste e di Milano
Additional file 1 of Managing patients on extracorporeal membrane oxygenation support during the COVID-19 pandemic – a proposal for a nursing standard operating procedure
Creators: name: Puslecki, Mateusz
name: Dabrowski, Marek
name: Baumgart, Konrad
name: Ligowski, Marcin
name: Dabrowska, Agata
name: Ziemak, Piotr
name: Stefaniak, Sebastian
name: Szarpak, Lukasz
name: Friedrich, Tammy
name: Szlanga, Lidia
name: Skorupa, Paulina
name: Steliga, Aleksandra
name: Hebel, Kazimiera
name: Andrejanczyk, Blazej
name: Ladzinska, Malgorzata
name: Wieczorek, Magdalena
name: Puslecki, Lukasz
name: Smereka, Jacek
name: Tukacs, Monika
name: Swol, Justyna
name: Jemielity, Marek
name: Perek, Bartlomiej
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Appendices A. Organization of patient care environment. The normal font contains innovation suggestions, italic commentary as integrated part of discussion.
The Stellar Populations of Lyman Break Galaxies at z~5
Creators: name: Yabe, Kiyoto
name: Ohta, Kouji
name: Iwata, Ikuru
name: Sawicki, Marcin
name: Tamura, Naoyuki
name: Akiyama, Masayuki
name: Aoki, Kentaro
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of Spectral Energy Distribution(SED) fitting analysis for Lyman Break Galaxies(LBGs) at z~5 in the GOODS-N and its flanking fields (the GOODS-FF). With the publicly available IRAC images in the GOODS-N and IRAC data in the GOODS-FF, we constructed the rest-frame UV to optical SEDs for a large sample (~100) of UV-selected galaxies at z~5. Comparing the observed SEDs with model SEDs generated with a population synthesis code, we derived a best-fit set of parameters (stellar mass, age, color excess, and star formation rate) for each of sample LBGs. The derived stellar masses range from 10^8 to 10^11M_sun with a median value of 4.1x10^9M_sun. The comparison with z=2-3 LBGs shows that the stellar masses of z~5 LBGs are systematically smaller by a factor of 3-4 than those of z=2-3 LBGs in a similar rest-frame UV luminosity range. The star formation ages are relatively younger than those of the z=2-3 LBGs. We also compared the results for our sample with other studies for the z=5-6 galaxies. Although there seem to be similarities and differences in the properties, we could not conclude its significance. We also derived a stellar mass function of our sample by correcting for incompletenesses. Although the number densities in the massive end are comparable to the theoretical predictions from semi-analytic models, the number densities in the low-mass part are smaller than the model predictions. By integrating the stellar mass function down to 10^8 M_sun, the stellar mass density at z~5 is calculated to be (0.7-2.4)x10^7M_sun Mpc^-3. The stellar mass density at z~5 is dominated by massive part of the stellar mass function. Compared with other observational studies and the model predictions, the mass density of our sample is consistent with general trend of the increase of the stellar mass density with time.
description: 29 pages, 21 figures, accepted for publication in ApJ. For high-resolution figures, see http://www.kusastro.kyoto-u.ac.jp/~kiyoyabe/arXiv/ms_astroph_hr.pdf
Ανισότητες και τηλεκπαίδευση την περίοδο του Covid 19. Αντιλήψεις εκπαιδευτικών και συνέπειες στην εκπαιδευτική διαδικασία.
Creators: name: Φουρλά, Ελπίδα
Publisher: name: Πανεπιστήμιο Πελοποννήσου
Year: 2023
Subjects: subject: COVID-19 (Ασθένεια) -- Ελλάδα
subject: COVID-19 (Ασθένεια) -- Κοινωνικές απόψεις -- Ελλάδα
subject: Εκπαιδευτική ισότητα -- Ελλάδα
subject: Εκπαίδευση εξ' αποστάσεως -- Ελλάδα
subject: Διδασκαλία με τη βοήθεια υπολογιστή -- Ελλάδα
subject: Εκπαιδευτική τεχνολογία -- Ελλάδα
subject: Εκπαιδευτικοί -- Στάσεις -- Ελλάδα
subject: Ανισότητα στην εκπαίδευση
subject: Ανισότητες στην τηλεκπαίδευση
subject: Κοινωνικές και γνωστικές επιπτώσεις μαθητών δημοτικού μετά την τηλεκπαίδευση
subject: Inequality in education
subject: Inequalities in tele-education
subject: Social and cognitive impacts of primary school students after tele-education

description: Αριθμός Εισαγωγής: 013622 cd
description: Σκοπός της παρούσας διπλωματικής εργασίας είναι να διερευνήσει τις κοινωνικές και γνωστικές επιπτώσεις σε μαθητές δημοτικού μετά το διάστημα της τηλεκπαίδευσης κατά την περίοδο της πανδημίας του Covid-19. Στη συγκεκριμένη ακαδημαϊκή εργασία ωστόσο θα αναλυθούν και διάφορες διαστάσεις της ανισότητας στην εκπαίδευση κατά την τηλεκπαίδευση. Το πρώτο μέρος αποτελείται από τα ευρήματα της σύγχρονης βιβλιογραφίας. Συγκεκριμένα στο πρώτο κεφάλαιο αναφέρονται οι ανισότητες στην εκπαίδευση, η ιστορική ανασκόπηση της Εξ Αποστάσεως Εκπαίδευσης, η Σύγκριση της Εξ Αποστάσεως Εκπαίδευσης στην Τριτοβάθμια και την Πρωτοβάθμια Εκπαίδευση και οι Δυσκολίες της Τηλεκπαίδευσης στη Διδακτική Πράξη. Στο δεύτερο κεφάλαιο αναφέρεται η ανισότητα στην εκπαίδευση κατά την περίοδο της πανδημίας Covid-19, η επίδραση τηλεκπαίδευσης στις κοινωνικές δεξιότητες και στην ακαδημαϊκή επίδοση των μαθητών, οι συνέπειες της τηλεκπαίδευσης σε ευάλωτες κοινωνικές ομάδες και οι συνέπειες της τηλε-εκπαίδευσης στην Ειδική Αγωγή. Εν συνεχεία, στο τρίτο κεφάλαιο αναφέρεται η μεθοδολογία της παρούσας ερευνητικής εργασίας, ο σκοπός της έρευνας και τα ερευνητικά ερωτήματα, η μέθοδος που επιλέχθηκε, η δειγματοληψία, τα ερευνητικά εργαλεία που επιλέχθηκαν, η ερευνητική διαδικασία και η μέθοδος ανάλυσης των αποτελεσμάτων. Στο επόμενο κεφάλαιο θα παρουσιαστούν τα αποτελέσματα και θα ερμηνευθούν με βάση και σε σύγκριση με τα ευρήματα της επιστημονικής βιβλιογραφίας.
title: Ð£ÑÐµÑ Ð¸ Ð°ÑÐ´Ð¸Ñ ÐÐÐ ÐºÐ°Ðº ÑÐ»ÐµÐ¼ÐµÐ½Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð·Ð° Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¾Ð·, ÐÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÑÐµÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿Ð°ÑÐ¾Ð²
Ð°ÑÐ´Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿Ð°ÑÐ¾Ð²
Ð¸Ð½Ð²ÐµÐ½ÑÐ°ÑÐ¸Ð·Ð°ÑÐ¸Ñ

description: Ð Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿Ð°ÑÐ¾Ð², Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð°Ð²ÑÐ¾ÑÐ¾Ð² Ðº Ð¼ÐµÑÐ¾Ð´Ð°Ð¼ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¸ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿Ð°ÑÐ¾Ð². ÐÐ¾Ð¼Ð¸Ð¼Ð¾ ÑÑÐ¾Ð³Ð¾, Ð¾ÑÐ´ÐµÐ»ÑÐ½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¸ Ð°ÑÐ´Ð¸ÑÐ° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿Ð°ÑÐ¾Ð². ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾ÑÐ¼ÑÑÐ»ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¹, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ð¹ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ, Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¹ Ð¸ Ð½Ð°ÑÑÐ½ÑÑ ÑÑÐ°ÑÐµÐ¹ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¾ Ð¾Ð±ÑÐµÐµ Ð²Ð¸Ð´ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°ÑÐ¸ÐºÐ¸, Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ»Ð¾Ð¶Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÑÐµÑÐ° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð°Ð¿Ð°ÑÐ¾Ð².
Toccare il suolo marziano
Creators: Patrizia Caraveo
Publisher: name: Media Inaf
Year: 2016

Oggi domenica 16 ottobre, alle ore 16:42, esattamente come previsto, il lander della sonda ExoMars si è separato dall’orbiter TGO e ha spiccato il volo verso il suolo marziano. Il touchdown è atteso per mercoledì. Vi riproponiamo l’articolo di Patrizia Caraveo pubblicato oggi sul Sole24Ore
The effect of some environmental factors on the morphological characteristics of western hemlock seedlings (Tsuga heterophylla (Raf.) (Sarg.)
Creators: name: Soos, Joseph
Publisher: name: University of British Columbia
Year: 2012

description: The objective of the study reported in this thesis is to assess the influence of light and site quality on the morphology of western hemlock Tsuga heterophylla (Raf.) Sarg. seedlings. The importance of western hemlock to the present and future economy of British Columbia is emphasized. The silvical literature on the species is reviewed. The inadequate treatment given western hemlock in the technical literature is noted and the point is made that, as the hemlock forests are exploited and new forests regenerated, information on the silvical characteristics of the species will be needed. At the present time, knowledge of the silvics of western hemlock is very limited. This thesis attempts to add to knowledge in that field with particular reference to some factors (light, microsite and site) which influence the juvenile growth of western hemlock on the University of British Columbia Research Forest, near Haney, B.C. The effect of light intensity was studied through measurements of natural regeneration growing on 10 plots, under full light and under different degrees of canopy closure, in a 77-year-old stand. Measurements included height, diameter and number of green and dead branches. The influence of different microsites was studied on three-year-old wild seedlings and on 1 + 1 planted seedlings, with particular reference to height, stem diameter at ground level, number of branches, length of needles, angle of branches, diameter of branches, weight and depth of roots, and root/shoot ratio. Four-and five-year-old wildlings growing on plots with known site indices were studied with particular reference to maximum needle length and branch angle of last year's shoots. The results indicate that diameter and height growth increased directly with increased light and that seedlings cannot survive with less than ten per cent of full light (measured on cloudy days). The average minimum light intensity was found to be 117 foot-candles for a 12-hour period on bright days. Seedlings studied on five types of microsites showed significantly different external characteristics in height, diameter, maximum length of needles and angle of branches of the last internode. These characteristics were then studied on planted wildlings of local provenance on plots of known site indices. The results show that, after two years, the morphological characteristics of hemlock planted on different sites, were modified to levels associated with site quality. These modifications involved branch angle, maximum needle length, and height growth. It was concluded that, within a particular provenance, the influence of environment is of greater significance than hereditary factors, in superimposing modifications on the basic form of western hemlock seedlings. The possibility of using branch angle and maximum needle length to estimate site quality is noted.
Spherical cloaking using nonlinear transformations for improved segmentation into concentric isotropic coatings
Creators: name: Qiu, Cheng-Wei
name: Hu, Li
name: Zhang, Baile
name: Wu, Bae-Ian
name: Johnson, Steven G.
name: Joannopoulos, John D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Two novel classes of spherical invisibility cloaks based on nonlinear transformation have been studied. The cloaking characteristics are presented by segmenting the nonlinear transformation based spherical cloak into concentric isotropic homogeneous coatings. Detailed investigations of the optimal discretization (e.g., thickness control of each layer, nonlinear factor, etc.) are presented for both linear and nonlinear spherical cloaks and their effects on invisibility performance are also discussed. The cloaking properties and our choice of optimal segmentation are verified by the numerical simulation of not only near-field electric-field distribution but also the far-field radar cross section (RCS).
description: 12 pages, 8 figures
Estacionalidad en el Turismo
Creators: name: Dirección Nacional De Mercados Y Estadística
Publisher: name: Zenodo
Year: 2022

description: La estacionalidad turística se define como la concentración de las visitas a un destino en un período específico de tiempo, por ejemplo una estación del año, un mes o un conjunto de meses específicos, fechas de festividades o feriados.
Umani e robot, tutti insieme a Settimo Torinese
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Da oggi, sabato 15 ottobre, fino a domenica 23, una settimana di eventi per adulti, bambini e ragazzi dedicata all’affascinante mondo della robotica. Succede al Festival dell’Innovazione e della Scienza della città di Settimo Torinese. Previsti anche incontri sui robot spaziali
title: Ð¨Ð¸ÑÐ¾ÐºÐ¾Ð¿Ð¾Ð»Ð¾ÑÐ½ÑÐ¹ ÑÑÐ¸Ð»Ð¸ÑÐµÐ»Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ ÑÐ°Ð½ÑÐ¸Ð¼ÐµÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ð° Ð´Ð»Ð¸Ð½ Ð²Ð¾Ð»Ð½
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð ÑÐ·Ð°Ð½ÑÐµÐ², ÐÑÐ¸Ð³Ð¾ÑÐ¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð£ÑÐ¸Ð»Ð¸ÑÐµÐ»Ð¸ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¿Ð¾Ð»Ð¾ÑÐ½ÑÐµ
Ð£ÑÐ¸Ð»Ð¸ÑÐµÐ»Ð¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸
Ð Ð°Ð´Ð¸Ð¾Ð»Ð¾ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÑÐ°Ð½ÑÐ¸Ð¸

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¿Ð¾Ð»Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ð¸ÑÐµÐ»Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ ÑÐ°Ð½ÑÐ¸Ð¼ÐµÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ð° Ð´Ð»Ð¸Ð½ Ð²Ð¾Ð»Ð½, ÐºÐ¾ÑÐ¾ÑÑÐ¹ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÑÐ°Ð²Ð½Ð¾Ð¹ ÑÐ°ÑÑÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿Ð¾Ð¼ÐµÑ ÑÐ°Ð´Ð¸Ð¾Ð»Ð¾ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ ÑÑÐ°Ð½ÑÐ¸ÑÐ¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÑÐµÐ¼Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÑÐµÐ±ÑÐµÐ¼ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ ÑÐµÐ°Ð»ÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¿Ð¾Ð»Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ð¸ÑÐµÐ»Ñ. ÐÐ¾ ÑÐ¾Ð²Ð¾ÐºÑÐ¿Ð½Ð¾ÑÑÐ¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐ¹ ÑÑÐ¸Ð»Ð¸ÑÐµÐ»Ñ ÑÑÐ°Ð²Ð½Ð¸Ð¼ Ñ Ð»ÑÑÑÐ¸Ð¼Ð¸ Ð¼Ð¸ÑÐ¾Ð²ÑÐ¼Ð¸ Ð°Ð½Ð°Ð»Ð¾Ð³Ð°Ð¼Ð¸.
description: The work is dedicated to the development of broadband power amplifier centimeter range of wavelengths. This amplifier is an integral part of the jamming system. Circuit solutions have been developed to achieve the desired parameters using real elements models. Amplifier characteristics are calculated. A set of parameters of the amplifier comparable to the best world analogues.
SN 2003bg: The First Type IIb Hypernova
Creators: name: Hamuy, Mario
name: Deng, Jinsong
name: Mazzali, Paolo A.
name: Morrell, Nidia I.
name: Phillips, Mark M.
name: Roth, Miguel
name: Gonzalez, Sergio
name: Thomas-Osip, Joanna
name: Krzeminski, Wojtek
name: Contreras, Carlos
name: Maza, Jose
name: Gonzalez, Luis
name: Huerta, Leonor
name: Folatelli, Gaston
name: Chornock, Ryan
name: Filippenko, Alexei V.
name: Persson, S. E.
name: Freedman, W. L.
name: Koviak, Kathleen
name: Suntzeff, Nicholas B.
name: Krisciunas, Kevin
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Optical and near-infrared photometry and optical spectroscopy are reported for SN 2003bg, starting a few days after explosion and extending for a period of more than 300 days. Our early-time spectra reveal the presence of broad, high-velocity Balmer lines. The nebular-phase spectra, on the other hand, show a remarkable resemblance to those of Type Ib/c supernovae, without clear evidence for hydrogen. Near maximum brightness SN 2003bg displayed a bolometric luminosity comparable to that of other Type I hypernovae unrelated to gamma-ray bursts, implying a rather normal amount of 56Ni production (0.1-0.2 Msun) compared with other such objects. The bolometric light curve of SN 2003bg, on the other hand, is remarkably broad, thus suggesting a relatively large progenitor mass at the moment of explosion. These observations, together with the large value of the kinetic energy of expansion established in the accompanying paper (Mazzali et al. 2009), suggest that SN 2003bg can be regarded as a Type IIb hypernova.
description: 41 pages, 12 figures, accepted by The Astrophysical Journal
Batterie nucleari, è l’ora della skutterudite
Creators: Giuseppina Pulcrano
Publisher: name: Media Inaf
Year: 2016

Generatori termoelettrici a radioisotopi in grado di convertire con più efficienza il calore sprigionato dal decadimento radioattivo del plutonio in energia elettrica per le missioni spaziali. Le stanno collaudando al JPL della NASA, e si basano su materiali dalle proprietà innovative
Constraints on Neutron Star Crusts From Oscillations in Giant Flares
Creators: name: Steiner, Andrew W.
name: Watts, Anna L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We show that the fundamental seismic shear mode, observed as a quasi-periodic oscillation in giant flares emitted by highly-magnetized neutron stars, is particularly sensitive to the nuclear physics of the crust. The identification of an oscillation at ~ 30 Hz as the fundamental crustal shear mode requires a nuclear symmetry energy that depends very weakly on density near saturation. If the nuclear symmetry energy varies more strongly with density, then lower frequency oscillations, previously identified as torsional Alfven modes of the fluid core, could instead be associated with the crust. If this is the case, then future observations of giant flares should detect oscillations at around 18 Hz. An accurate measurement of the neutron skin thickness of lead will also constrain the frequencies predicted by the model.
description: 5 pages, 3 figures; Version to appear in Phys. Rev. Lett
Additional file 2 of Managing patients on extracorporeal membrane oxygenation support during the COVID-19 pandemic – a proposal for a nursing standard operating procedure
Creators: name: Puslecki, Mateusz
name: Dabrowski, Marek
name: Baumgart, Konrad
name: Ligowski, Marcin
name: Dabrowska, Agata
name: Ziemak, Piotr
name: Stefaniak, Sebastian
name: Szarpak, Lukasz
name: Friedrich, Tammy
name: Szlanga, Lidia
name: Skorupa, Paulina
name: Steliga, Aleksandra
name: Hebel, Kazimiera
name: Andrejanczyk, Blazej
name: Ladzinska, Malgorzata
name: Wieczorek, Magdalena
name: Puslecki, Lukasz
name: Smereka, Jacek
name: Tukacs, Monika
name: Swol, Justyna
name: Jemielity, Marek
name: Perek, Bartlomiej
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Appendices B. Direct care of COVID-19 patients with ECMO – nurse daily routine activity. The normal font contains innovation suggestions, italic commentary as integrated part of discussion.
New Light in Star-Forming Dwarf Galaxies: The PMAS Integral Field View of the Blue Compact Dwarf Galaxy Mrk 409
Creators: name: Cairos, L. M.
name: Caon, N.
name: Papaderos, P.
name: Kehrig, C.
name: Weilbacher, P.
name: Roth, M. M.
name: Zurita, C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present an integral field spectroscopic study of the central 2x2 kpc^2 of the blue compact dwarf galaxy Mrk 409, observed with the Potsdam MultiAperture Spectrophotometer. This study focuses on the morphology, two-dimensional chemical abundance pattern, excitation properties and kinematics of the ionized interstellar medium in the starburst component. We also investigate the nature of the extended ring of ionized gas emission surrounding the bright nuclear starburst region of Mrk 409. PMAS spectra of selected regions along the ring, interpreted with evolutionary and population synthesis models, indicate that their ionized emission is mainly due to a young stellar population with a total mass of ~1.5x10^6 M_sun, which started forming almost coevally ~10 Myr ago. This stellar component is likely confined to the collisional interface of a spherically expanding, starburst-driven super-bubble with denser, swept-up ambient gas, ~600 pc away from the central starburst nucleus. The spectroscopic properties of the latter imply a large extinction (C_H-beta>0.9), and the presence of an additional non-thermal ionization source, most likely a low-luminosity Active Galactic Nucleus. Mrk 409 shows a relatively large oxygen abundance (12+log(O/H)~8.4) and no chemical abundance gradients out to R~600 pc. The ionized gas kinematics displays an overall regular rotation on a northwest-southwest axis, with a maximum velocity of 60 km/s; the total mass inside the star-forming ring is about 1.4x10^9 M_sun.
description: Accepted for publication in ApJ
Duemila miliardi di galassie per Hubble
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Un team di ricercatori ha estrapolato una nuova stima sul numero totale di galassie nell’Universo, che risulta superare di circa dieci volte i valori precedentemente conosciuti. Adriano Fontana (INAF Roma): «Il risultato conferma una cosa che già sapevamo: in epoca primordiale esisteva un grande numero di galassie molto piccole, che per ora sono invisibili ai nostri occhi»
Vuoti cosmici e superammassi, ecco la mappa
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

Un team di ricercatori dell'Università di Portsmouth ha pubblicato la più grande mappa mai realizzata dei vuoti cosmici e superammassi. Potrà essere utilizzata per misurare l'effetto dovuto all'energia oscura sull'espansione dell'Universo. I risultati sono riportati su ApJ Letters
Global warming preistorico, forse fu una cometa
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Il recente ritrovamento di minuscole sferule di vetro lungo la costa atlantica degli Stati Uniti offre una possibile spiegazione al cosiddetto “Massimo termico del Paleocene-Eocene”, un periodo d’intenso riscaldamento globale avvenuto 56 milioni di anni fa: potrebbe essere stato innescato dall’impatto con un oggetto extraterrestre
Le basi della vita? Nella luce delle stelle
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Grazie alle capacità osservative del telescopio spaziale Herschel dell’ESA, un team di ricercatori è riuscito a ricostruire un possibile canale attraverso cui nascono gli elementi base da cui si può formare la vita. La luce ultravioletta proveniente dalle stelle più massicce potrebbe essere responsabile della vita come la conosciamo
A worm algorithm for the fully-packed loop model
Creators: name: Zhang, Wei
name: Garoni, Timothy M.
name: Deng, Youjin
Publisher: name: arXiv
Year: 2008
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We present a Markov-chain Monte Carlo algorithm of worm type that correctly simulates the fully-packed loop model on the honeycomb lattice, and we prove that it is ergodic and has uniform stationary distribution. The fully-packed loop model on the honeycomb lattice is equivalent to the zero-temperature triangular-lattice antiferromagnetic Ising model, which is fully frustrated and notoriously difficult to simulate. We test this worm algorithm numerically and estimate the dynamic exponent z = 0.515(8). We also measure several static quantities of interest, including loop-length and face-size moments. It appears numerically that the face-size moments are governed by the magnetic dimension for percolation.
description: 31 pages, 10 figures. Several new figures added, and some minor typos corrected. Uses the following latex packages: algorithm.sty, algorithmic.sty, elsart-num.bst, elsart1p.cls, elsart.cls
Additional file 3 of Managing patients on extracorporeal membrane oxygenation support during the COVID-19 pandemic – a proposal for a nursing standard operating procedure
Creators: name: Puslecki, Mateusz
name: Dabrowski, Marek
name: Baumgart, Konrad
name: Ligowski, Marcin
name: Dabrowska, Agata
name: Ziemak, Piotr
name: Stefaniak, Sebastian
name: Szarpak, Lukasz
name: Friedrich, Tammy
name: Szlanga, Lidia
name: Skorupa, Paulina
name: Steliga, Aleksandra
name: Hebel, Kazimiera
name: Andrejanczyk, Blazej
name: Ladzinska, Malgorzata
name: Wieczorek, Magdalena
name: Puslecki, Lukasz
name: Smereka, Jacek
name: Tukacs, Monika
name: Swol, Justyna
name: Jemielity, Marek
name: Perek, Bartlomiej
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 3: Appendices C. Procedures with extracorporeal techniques. The normal font contains innovation suggestions, italic commentary as integrated part of discussion.
title: Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð»Ð°ÑÑÐ¸ÑÐ½Ð¾ÑÑÐ¸ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð². ÐÐ·ÑÑÐµÐ½Ð¸Ðµ ÑÐµÐºÑÑÑÑ Ð¼ÐµÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ð»Ð¸ÑÑÐ¾Ð² Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð¿ÑÑÐ¼ÑÑ Ð¿Ð¾Ð»ÑÑÐ½ÑÑ ÑÐ¸Ð³ÑÑ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¾Ð¼Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2018
Subjects: ÐÐµÑÐ°Ð»Ð»Ñ

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¤ÐÐÐ¡ ÐÐÐ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 22.03.02 Â«ÐÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸ÑÂ» (Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°Ñ). Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐºÑÑÑÑ Ð¼ÐµÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ð»Ð¸ÑÑÐ¾Ð², Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¿ÑÑÐ¼ÑÑ Ð¿Ð¾Ð»ÑÑÐ½ÑÑ ÑÐ¸Ð³ÑÑ ÑÐµÐ½ÑÐ³ÐµÐ½Ð¾Ð²ÑÐºÐ¸Ð¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼, ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾ ÑÑÐµÑÐµÐ¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÐµÐ¹ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐµÑÐ¾Ðº ÐÐ¾Ð»Ð´ÑÑÐµÐ²Ð° Ð¸ ÐÑÐ»ÑÑÐ°, ÑÐ°ÑÑÐ¸ÑÑÐ¾Ð²ÐºÐ° Ð¿Ð¾Ð»ÑÑÐ½ÑÑ ÑÐ¸Ð³ÑÑ (ÐÐ¤) Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¸Ð´ÐµÐ°Ð»ÑÐ½ÑÑ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð¾Ðº. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¿Ð¾Ð»ÑÑÐ½ÑÑ ÑÐ¸Ð³ÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ð¸, Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ° (ÐÐÐÐ¸Ð¢) Ð¡ÐÐ±ÐÐ£ Ð¸ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð².
La caccia a ET svolta a Oriente
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Appena acceso, il radiotelescopio cinese FAST, il più grande al mondo come singola antenna, firma l’accordo di collaborazione con le Breaktrough Initiatives, un programma per la ricerca di civiltà aliene finanziato da un imprenditore russo. Lavorerà assieme ai radiotelescopi di Green Bank, negli Stati Uniti, e Parkes, in Australia
Dynamically Generated Anomalous Magnetic Moment in Massless QED
Creators: name: Ferrer, Efrain J.
name: de la Incera, Vivian
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this paper we investigate the non-perturbative generation of an anomalous magnetic moment for massless fermions in the presence of an external magnetic field. In the context of massless QED in a magnetic field, we prove that the phenomenon of magnetic catalysis of chiral symmetry breaking, which has been associated in the literature with dynamical mass generation, is also responsible for the generation of a dynamical anomalous magnetic moment. As a consequence, the degenerate energy of electrons in Landau levels higher than zero exhibits Zeeman splitting. We explicitly report the splitting for the first Landau level and find the non-perturbative Lande $\textit{g}$-factor and Bohr magneton. We anticipate that a dynamically generated anomalous magnetic moment will be a universal feature of theories with magnetic catalysis. Our findings can be important for condensed planar systems as graphene, as well as for highly magnetized dense systems as those forming the core of compact stars.
description: Version to appear in Nucl. Phys. B. A few misprints in the formulas were corrected and some references added
title: Ð¦Ð¸ÑÑÐ¾Ð²ÑÐµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¼Ð¸ÐºÑÐ¾Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÑ. Ð§. 2, ÐÐ¸ÐºÑÐ¾Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ½ÑÐµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¸ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
titleType: Subtitle
Creators: name: ÐÑÐ½ÑÐ¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ¾ÑÐ¾Ð·Ð¾Ð², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐÐ£
Year: 2004
Subjects: Ð Ð°Ð´Ð¸Ð¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð°Ñ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑÑÐ° Ð¼Ð¸ÐºÑÐ¾Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ½Ð°Ñ

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÐ¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÐ¼ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¾Ð¼ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð¦Ð¸ÑÑÐ¾Ð²ÑÐµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¼Ð¸ÐºÑÐ¾Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÑÂ» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 552500 Â«Ð Ð°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÐºÐ°Â» Ð¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² 654200 Â«Ð Ð°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÐºÐ°Â». ÐÐ°ÑÐµÑÐ¸Ð°Ð» Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ¾Ð³Ð»Ð°ÑÐ¾Ð²Ð°Ð» Ñ Ð»ÐµÐºÑÐ¸Ð¾Ð½Ð½ÑÐ¼ ÐºÑÑÑÐ¾Ð¼ Ð¸ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ. ÐÐ°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÑÑÑ Ð´Ð»Ñ Ð·Ð°ÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¸ Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÐµÐ½Ð¸Ñ Ð½Ð°Ð²ÑÐºÐ¾Ð² Ð² Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¼Ð¸ÐºÑÐ¾Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ½ÑÑ ÑÑÑÑÐ¾Ð¹ÑÑÐ². Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ¸ÑÑÐµÐ¼Ð° ÐºÐ¾Ð¼Ð°Ð½Ð´ Ð¼Ð¸ÐºÑÐ¾Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ° Ð580ÐÐ80Ð Ð¸ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ° Ð¼Ð¸ÐºÑÐ¾Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ° Ð580ÐÐ55. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð°Ð½Ð´ Ð¿ÐµÑÐµÑÑÐ»Ð¾Ðº, Ð±ÐµÐ·ÑÑÐ»Ð¾Ð²Ð½Ð¾Ð³Ð¾ Ð¸ ÑÑÐ»Ð¾Ð²Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÑÐ¾Ð´Ð¾Ð², Ð²ÑÐ·Ð¾Ð²Ð° Ð¿Ð¾Ð´Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼, ÑÐ°Ð±Ð¾ÑÑ ÑÐ¾ ÑÑÐµÐºÐ¾Ð¼, Ð°ÑÐ¸ÑÐ¼ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, Ð¾ÑÐ²Ð°Ð¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¼Ð¸ÐºÑÐ¾ÑÑÐµÐ¼Ñ Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ°. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ°Ð´Ð¸Ð¾ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°, Ð¸Ð½ÑÑÐ¸ÑÑÑÐ° Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, Ð²ÐµÑÐµÑÐ½ÐµÐ³Ð¾ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¸ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¾ÑÐºÑÑÑÐ¾Ð³Ð¾ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Due bronzi e un oro alle Olimpiadi d’astronomia
Creators: Gaetano Valentini
Publisher: name: Media Inaf
Year: 2016

Due medaglie di bronzo, una a Pietro Benotto l'altra a Lorenzo Pica Ciamarra. E un oro a Jacopo Guoy Chen, vincitore sia della prova teorica e che di quella pratica. Per l’Italia, un successo senza precedenti alle Olimpiadi internazionali di astronomia, appena concluse in Bulgaria. Il resoconto di Gaetano Valentini dell'INAF di Teramo
Additional file 1 of Developing best practices for PPE Portraits across 25 sites: a systematic assessment of implementation and spread of adaptations using FRAME
Creators: name: Baratta, Juliana
name: Amano, Alexis
name: Parsons, Paige K
name: Vilendrer, Stacie
name: Winter, Shira G.
name: Verano, Mae-Richelle
name: Perez, Cynthia
name: Kalanithi, Lucy
name: Asch, Steven M
name: Heffernan, Mary Beth
name: Brown-Johnson, Cati
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Additional file 1:
Involutivity of field equations
Creators: name: Kruglikov, Boris
Publisher: name: arXiv
Year: 2009
Subjects: subject: Differential Geometry (math.DG)
subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 83C05, 83C22, 58H10, 58A15

description: We prove involutivity of Einstein, Einstein-Maxwell and other field equations by calculating the Spencer cohomology of these systems. Relation with Cartan method is traced in details. Basic implications through Cartan-Kahler theory are derived.
description: 13 pages; this version is updated with new field equations (radiation, dust etc) - they are proved involutive, Spencer cohomology calculated
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð¿Ð°ÑÐ¾Ð³Ð°Ð·Ð¾Ð²Ð¾Ð¹ Ð¢Ð­Ð¦ Ñ Ð±Ð»Ð¾ÐºÐ¾Ð¼ ÐÐÐ£-450 ÐÐÑ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð², ÐÐµÐ½Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¢Ð­Ð¦
ÑÑÐ°Ð½ÑÐ¸Ñ
ÑÐµÑÑÐµÐ¶Ð¸
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description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¢Ð­Ð¦ Ñ ÑÐ¸ÐºÐ»Ð¾Ð¼ ÐÐÐ£, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð¸ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²ÐºÐ¸ ÐµÐµ ÑÐ°ÑÑÐµÐ¹. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ Ð´Ð²ÑÑ ÑÑÐµÐ¼, Ð¸Ð· ÐºÐ¾ÑÐ¾ÑÑÑ Ð±ÑÐ»Ð° Ð²ÑÐ±ÑÐ°Ð½Ð° Ð»ÑÑÑÐ°Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð²ÑÐ±Ð¾Ñ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð³Ð¾ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ° Ð½Ð° ÐµÐ³Ð¾ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð¿ÑÐ¸ Ð·Ð°-Ð´Ð°Ð½Ð½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ°Ñ. Ð¢Ð°Ðº Ð¶Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ñ ÑÐµÑÑÐµÐ¶Ð¸ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹.
La superficie scabra della Luna
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

Grazie ai dati della Narrow Angle Camera, a bordo della sonda Lunar Reconnaissance Orbiter NASA, è stato possibile effettuare osservazioni comparate mettendo a confronto immagini riprese in differenti momenti della superficie della Luna, in particolare dei crateri che la caratterizzano. Lo scopo è quello di stabilire l’odierno tasso di formazione dei crateri stessi, e quali altri mutamenti avvengano attualmente sugli strati superficiali del suolo del nostro satellite. Lo studio è stato pubblicato sulla rivista Nature
title: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸. ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð² MS Access
title: Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ°Ð±Ð¾ÑÐ°Ð¼
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°ÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ
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description: ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ñ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» Ð´Ð½ÐµÐ²Ð½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ»ÑÑÐ°ÑÐµÐ»ÑÐ¼ Ð¿Ð¾ Ð²ÑÐ¾ÑÐ¾Ð¼Ñ Ð²ÑÑÑÐµÐ¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ½Ð¸ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð´ÑÑÐ³Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð±Ð°Ð· Ð´Ð°Ð½Ð½ÑÑ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ.
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Klonierung, Expression, Reinigung und Identifizierung putativer Acetolactatsynthasen aus Clostridium aceticum und Helicobacter canadensis
Creators: name: Malzacher, Stephan
Publisher: name: Zenodo
Year: 2022

description: Acetohydroxyacid synthases (AHAS) sind Enyzme im Aminosäurestoffwechsel von Bakterien, Pflanzen, Pilzen und Archaeen. Durch eine Carboligation von zwei Pyruvatmolekülen zu Acetolactat oder einem Pyruvatmolekül und einem α – Ketobutyratmolekül zu 2-Aceto-2 Hydroxybutyrat leiten sie den Biosyntheseweg der verzweigtkettigen Aminosäuren Valin, Leucin und Isoleucin ein. Die Enzyme sind Thiamindiphosphat (ThDP), Flavinadenindinukelotid (FAD) und Mg2+ abhängig. Einzigartig unter den ThDP abhängigen Enzymen ist, dass sie aus zwei verschiedenen Polypetidketten bestehen, einer mit katalytischer und einer mit regulatorischer Funktion.
 Im Rahmen dieser Arbeit wurden zwei putative AHAS (regulatorische und katalytische Untereinheit) aus Clostridium aceticum und Helicobacter canadensis kloniert, produziert und gereinigt. Mittels Aktivitätsanalyse sollte zudem ihre Annotation als AHAS überprüft werden. Zur Reinigung wurde zunächst an die katalytischen Untereinheiten ein His-Tag, je C- und N-terminal ein His-tag fusioniert. Die regulatorischen Untereinheiten wurden C-terminal mit einem His-tag fusioniert. Dies wurde durch die Klonierung der Gene in verschiedene pET-Vektorsysteme erreicht. Die Produktion wurde in einem Autoinduktionsmedium mit Laktose als Induktor durchgeführt. Die anschließEnde Reinigung erfolgte mittels Ni-NTA- Affinitätschromatographie. Die Aktivität der Enzyme wurde photometrisch durch die physiologische Reaktion der Carboligation zweier Pyruvatmoleküle zu Acetolactat gemessen. Nach der Auswertung zeigte die AHAS aus Clostridium aceticum unter den getesteten Bedingungen keine Aktivität, wohingegen für die Helicobacter canadensis AHAS eine hohe Aktivität nachgewiesen werden konnte. Für dieses Enzym konnte die Annotation somit bestätigt werden.
Magnetically Regulated Gas Accretion in High-Redshift Galactic Disks
Creators: name: Birnboim, Yuval
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Disk galaxies are in hydrostatic equilibrium along their vertical axis. The pressure allowing for this configuration consists of thermal, turbulent, magnetic and cosmic ray components. For the Milky Way(MW) the thermal pressure contributes ~10% of the total pressure near the plane, with this fraction dropping towards higher altitudes. Out of the rest, magnetic fields contribute ~1/3 of the pressure to distances of ~3kpc above the disk plane. In this letter we attempt to extrapolate these local values to high redshift, rapidly accreting, rapidly star forming disk galaxies and study the effect of the extra pressure sources on the accretion of gas onto the galaxies. In particular, magnetic field tension may convert a smooth cold-flow accretion to clumpy, irregular star formation regions and rates. The infalling gas accumulates on the edge of the magnetic fields, supported by magnetic tension. When the mass of the infalling gas exceeds some threshold mass, its gravitational force cannot be balanced by magnetic tension anymore, and it falls toward the disk's plane, rapidly making stars. Simplified estimations of this threshold mass are consistent with clumpy star formation observed in SINS, UDF, GOODS and GEMS surveys. We discuss the shortcomings of pure hydrodynamic codes in simulating the accretion of cold flows into galaxies, and emphasize the need for magneto-hydrodynamic simulations
description: 12 pages, 3 figures, accepted to ApJL
Anelli contromano attorno a J1407b
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Sorpresa: gli estesi anelli che circondano J1407b devono ruotare nel verso opposto al moto orbitale del pianeta per non venire disgragati dalle forze mareali della stella madre. Questi i risultati di uno studio teorico in pubblcazione sulla rivista Astronomy & Astrophysics
Additional file 1 of Concentrations of oligosaccharides in human milk and child growth
Creators: name: Menzel, Philipp
name: Vogel, Mandy
name: Austin, Sean
name: Sprenger, Norbert
name: Grafe, Nico
name: Hilbert, Cornelia
name: Jurkutat, Anne
name: Kiess, Wieland
name: Binia, Aristea
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Computational Biology

description: Additional file 1: Supplementary Table S1. Associations between Human Milk Oligosaccharides at 3 months and maternal and birth parameter are presented as ratio, 95% confidence interval, and p-value. If the effects differed between the secretor and the non-secretor group, both effects are given. Otherwise the overall effect is reported. Supplementary Table S2. Associations between Human Milk Oligosaccharides at 3 months and height-SDS at the different time points are presented as ratio, 95% confidence interval, and p-value. If the effects differed between the secretor and the non-secretor group, both effects are given. Otherwise the overall effect is reported. Supplementary Table S3. Associations between Human Milk Oligosaccharides at 3 months and growth velocity at the different time points are presented as ratio, 95% confidence interval, and p-value. If the effects differed between the secretor and the non-secretor group, both effects are given. Otherwise the overall effect is reported. Supplementary Table S4. Associations between Human Milk Oligosaccharides at 3 months and BMI-SDS at the different time points are presented as ratio, 95% confidence interval, and p-value. If the effects differed between the secretor and the non-secretor group, both effects are given. Otherwise the overall effect is reported. Supplementary Table S5. Associations between Human Milk Oligosaccharides at 3 months and Head Circumference SDS at the different time points are presented as ratio, 95% confidence interval, and p-value. If the effects differed between the secretor and the non-secretor group, both effects are given. Otherwise the overall effect is reported.
Macchie stellari su Proxima Centauri
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Un ipotetico abitante del pianeta Proxima b, recentemente scoperto, potrebbe ammirare sulla propria stella Proxima Centauri delle macchie, come quelle solari ma molto più grandi. Macchie che si presentano con una periodicità di sette anni, un ciclo di attività stellare che gli astronomi non pensavano possibile per una stella piccola
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ ÑÑÑÐ´Ð° Ð´Ð»Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ·Ð½ÐµÑÐ¾Ð²Ð°, ÐÐ»Ð¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ñ
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