Galaxy triplets in Sloan Digital Sky Survey Data Release 7-I. Catalogue

We present a new catalogue of galaxy triplets derived from the Sloan Digital Sky Survey (SDSS) Data Release 7. The identification of systems was performed considering galaxies brighter than Mr=-20.5 and imposing constraints over the projected distances, radial velocity differences of neighbouring galaxies and isolation. To improve the identification of triplets, we employed a data pixelization scheme, which allows us to handle large amounts of data as in the SDSS photometric survey. Using spectroscopic and photometric data in the redshift range 0.01 =z= 0.40, we obtain 5901 triplet candidates. We have used a mock catalogue to analyse the completeness and contamination of our methods. The results show a high level of completeness ( 80 per cent) and low contamination ( 5 per cent). By using photometric and spectroscopic data, we have also addressed the effects of fibre collisions in the spectroscopic sample. We have defined an isolation criterion considering the distance of the triplet brightest galaxy to the closest neighbour cluster, to describe a global environment, as well as the galaxies within a fixed aperture, around the triplet brightest galaxy, to measure the local environment. The final catalogue comprises 1092 isolated triplets of galaxies in the redshift range 0.01 =z= 0.40. Our results show that photometric redshifts provide very useful information, allowing us to complete the sample of nearby systems whose detection is affected by fibre collisions, as well as extending the detection of triplets to large distances, where spectroscopic redshifts are not available.

THE SLOAN DIGITAL SKY SURVEY CO-ADD: A GALAXY PHOTOMETRIC REDSHIFT CATALOG

We present and describe a catalog of galaxy photometric redshifts (photo-z) for the Sloan Digital Sky Survey (SDSS) Co-add Data. We use the artificial neural network (ANN) technique to calculate the photo-z and the nearest neighbor error method to estimate photo-z errors for similar to 13 million objects classified as galaxies in the co-add with r < 24.5. The photo-z and photo-z error estimators are trained and validated on a sample of similar to 83,000 galaxies that have SDSS photometry and spectroscopic redshifts measured by the SDSS Data Release 7 (DR7), the Canadian Network for Observational Cosmology Field Galaxy Survey, the Deep Extragalactic Evolutionary Probe Data Release 3, the VIsible imaging Multi-Object Spectrograph-Very Large Telescope Deep Survey, and the WiggleZ Dark Energy Survey. For the best ANN methods we have tried, we find that 68% of the galaxies in the validation set have a photo-z error smaller than sigma(68) = 0.031. After presenting our results and quality tests, we provide a short guide for users accessing the public data.

Galaxy triplets in Sloan Digital Sky Survey Data Release 7: II. A connection with compact groups?

We analyse a sample of 71 triplets of luminous galaxies derived from the work of O’Mill et al. We compare the properties of triplets and their members with those of control samples of compact groups, the 10 brightest members of rich clusters and galaxies in pairs. The triplets are restricted to have members with spectroscopic redshifts in the range 0.01 ≤ z ≤ 0.14 and absolute r-band luminosities brighter than Mr = −20.5. For these member galaxies, we analyse the stellar mass content, the star formation rates, the Dn(4000) parameter and (Mg − Mr) colour index. Since galaxies in triplets may finally merge in a single system, we analyse different global properties of these systems. We calculate the probability that the properties of galaxies in triplets are strongly correlated. We also study total star formation activity and global colours, and define the triplet compactness as a measure of the percentage of the system total area that is filled by the light of member galaxies. We concentrate in the comparison of our results with those of compact groups to assess how the triplets are a natural extension of these compact systems. Our analysis suggests that triplet galaxy members behave similarly to compact group members and galaxies in rich clusters. We also find that systems comprising three blue, star-forming, young stellar population galaxies (blue triplets) are most probably real systems and not a chance configuration of interloping galaxies. The same holds for triplets composed of three red, non-star-forming galaxies, showing the correlation of galaxy properties in these systems. From the analysis of the triplet as a whole, we conclude that, at a given total stellar mass content, triplets show a total star formation activity and global colours similar to compact groups. However, blue triplets show a high total star formation activity with a lower stellar mass content. From an analysis of the compactness parameter of the systems we find that light is even more concentrated in triplets than in compact groups. We propose that triplets composed of three luminous galaxies, should not be considered as an analogous of galaxy pairs with a third extra member, but rather they are a natural extension of compact groups.

Riccardo Lombardi nel socialismo italiano (1947-1964)

Il primo capitolo della tesi verte sull’ultimo anno di vita del Partito d’Azione, sulle modalità di partecipazione di Lombardi allo scontro elettorale del 1948 nelle liste del Fronte democratico popolare, e sul breve periodo di direzione ‘centrista’ del Psi a cavallo tra il 1948 e il 1949, quando Lombardi, appena entratovi, fu magna pars nel gruppo dirigente del partito. Il secondo capitolo abbraccia il periodo in cui Lombardi agì all’interno del Psi ‘morandiano’, o frontista: si è cercato di dare ragione sia dell’inserimento di Lombardi nelle logiche del frontismo socialista, sia della peculiarità di quell’inserimento negli ambiti privilegiati della politica economica e della politica estera. Oggetto del terzo capitolo è il ruolo giocato da Lombardi nella definizione delle linee guida dell’autonomismo socialista, un ruolo fattosi via via più pregnante a partire dal 1956, che ebbe la sua massima consacrazione col XXXIV Congresso del Psi, celebrato a Milano nel 1961: centrale in questo periodo la riflessione lombardiana sulle «riforme di struttura», un argomento che ci si è sforzati di inquadrare storicamente, sfuggendo dai luoghi comuni storiografici di cui spesso – con lodevoli eccezioni – è caduto vittima. Tali «riforme di struttura» Lombardi avrebbe voluto alla base dei governi di centro-sinistra. La tesi si chiude con un ultimo capitolo dedicato ad illustrare l’apporto di Lombardi al quarto Governo Fanfani e al primo Governo Moro, il ruolo da lui giocato nella loro nascita e il suo progressivo allontanamento da quell’esperimento che era stato, in gran parte, sua creatura.

Morbus Hunter : Neutralisationskapazität von Antikörpern unter Enzymersatztherapie und deren klinischen Auswirkungen

Morbus Hunter, eine lysosomale Speicherkrankheit, ist eine seltene, progrediente, x-chromosomal vererbte Stoffwechselkrankheit, die durch ein Defizit an Iduronat-2-sulfatase (IDS) hervorgerufen wird. Als Folge daraus erfolgt kein Abbau von Heparan- und Dermatansulfat und die Glykosaminoglykane reichern sich in de Lysosomen der Zelle an. M. Hunter ist eine Multisystemerkrankung und weist ein breites klinisches Spektrum mit interindividuell unterschiedlichem Krankheitsbeginn, Ausprägungen und Progression der Symptome auf. Seit 2007 besteht die Therapieoption einer Enzymersatztherapie (ERT) mit Elaprase®. Einige Patienten entwickeln Antikörper gegen das substituierte Enzym, welche partiell neutralisierende Eigenschaften besitzen. Ziel dieser Untersuchung war es zu klären, ob die Neutralisationskapazität der gebildeten Antikörper mittels einer Bestimmung im Mischserum festgestellt werden kann und ob persistierende Antikörper mit Neutralisationskapazität zu einer Einschränkung der Wirksamkeit der Enzymersatztherapie führen. Es sollte weiterhin untersucht werden, ob sich mittels Messung der neuronenspezifischen Enolase (NSE) und S-100 Rückschlüsse auf eine neuropathische Beteiligung ziehen lassen, da bis jetzt noch keine klinische oder biochemische Messmethode existiert, die für M. Hunter-Patienten eine verlässliche Vorhersage für eine neuropathische Beteiligung bietet. 30 Patienten wurden in die retrospektive/prospektive Kohortenstudie eingeschlossen. Bei der Bestimmung der IDS-Aktivität im Mischserum mit einem gesunden Menschen zeigten fünf der Patienten (17%) in zwölf Mischseren eine um ≥ 40% reduzierte Aktivität. Zwei (7%) der 30 untersuchten Patienten wurden mit dieser Methode als positiv für persistierende neutralisierende Antikörper identifiziert. Zum gleichen Ergebnis bezüglich der persistierenden neutralisierenden Antikörper führten die Anti-Elaprase®-Immunglobulin-Bestimmungen unter Berücksichtigung des Bestimmungszeitpunkts, die bei Shire Pharmaceuticals durchgeführt wurden. Die Untersuchungsergebnisse lassen den Schluss zu, dass die gebildeten Antikörper auch intraindividuell unterschiedlich sind. Zudem interagieren sie mit den verschiedensten Epitopen des Enzyms der ERT und besitzen nicht alle neutralisierende Eigenschaften. Aufgrund der heterogenen Zusammensetzung folgt die Hemmung der Enzymaktivität vermutlich keiner eindeutigen Kinetik. Anti-Elaprase®-Immunglobulin G spielt für die Neutralisationskapazität jedoch eine wichtige Rolle. Die Auswertung und Beurteilung der Einschränkung der Wirksamkeit der Therapie hervorgerufen durch die Antikörper mit Neutralisationskapazität gestaltete sich kompliziert. Im Ergebnis zeigte sich, dass sich die beiden Patienten mit persistierenden neutralisierenden Antikörpern in der Entwicklung der klinischen Parameter interindividuell stark unterschieden. Um einen Zusammenhang zwischen klinischem Verlauf und Antikörperbildung gegen die ERT zu finden, müssen in einem größeren Patientenkollektiv mehr Patienten mit persistierenden neutralisierenden Antikörpern identifiziert werden und der Einfluss der Antikörper untersucht werden. Die Untersuchung der NSE und S-100 ergab, dass weder die Konzentration der NSE noch der S-100 Rückschlüsse auf die neuropathische Beteiligung des Patienten zulässt.

The Body of Margaret Atwood: Sex Work and Prostitution within Margaret Atwood's The Handmaid's Tale, Oryx and Crake, and The Year of the Flood

In this paper, I will argue that Canadian author Margaret Atwood uses fiscal and socially conservative dystopias to show how sex work and prostitution are choices that women would never have to make in a world with true gender equality. In these radically different worlds, women have no agency beyond their sexuality and no ability to express themselves as equals within either society. And while the structures of both societies, the society of The Handmaid’s Tale and that of both Oryx and Crake and The Year of the Flood, are inherently different, they both stem from modern conservative philosophies: for example, the country of Gilead in The Handmaid’s Tale holds Christian conservative beliefs on the role of religion in the state and the culturally designated roles of women. I define social conservatism as the idea that government organizations are used to pursue an agenda promoting traditional religious values such as “public morality” and opposing “immoralities” such as abortion, prostitution, and homosexuality. I define fiscal conservatism as an agenda promoting privatization of the market, deregulation and lower taxes. In this paper I argue that because these philosophies are incompatible with gender equality, they drive women to occupations such as sex work. Women find that they have no choices and sex work provides something to “trade.” For Offred, this “trading” is more limited, because she is a sex slave. For Oryx, this trading allows her to travel to the West, yet not before her childhood is marked by prostitution and pornography. Sex work allows for Ren to reclaim some agency over her life, yet she only chooses sex work because she is presented with few other options. All of these issues stem from the philosophies that define these dystopias.

[Alban Köhler (1874-1947): Inventor of grid therapy]

Grid (or sieve) therapy ("Gitter-" oder "Siebtherapie"), spatially fractionated kilo- and megavolt X-ray therapy, was invented in 1909 by Alban Köhler, a radiologist in Wiesbaden, Germany. He tested it on several patients before 1913 using approximately 60-70kV Hittorf-Crookes tubes. Köhler pushed the X-ray tube's lead-shielded housing against a stiff grid of 1 mm-square iron wires woven 3.0-3.5mm on center, taped tightly to the skin over a thin chamois. Numerous islets unshielded by iron in the pressure-blanched skin were irradiated with up to about 6 erythema doses (ED). The skin was then thoroughly cleansed, disinfected, and bandaged; delayed punctate necrosis healed in several weeks. Although grid therapy was disparaged or ignored until the 1930s, it has been used successfully since then to shrink bulky malignancies. Also, advanced cancers in rats and mice have been mitigated or ablated using Köhler's concept since the early 1990s by unidirectional or stereotactic exposure to an array of nearly parallel microplanar (25-75μm-wide) beams of very intense, moderately hard (median energy approximately 100 keV) synchrotron-generated X rays spaced 0.1-0.4mm on center. Such beams maintain sharp edges at high doses well beneath the skin yet confer little toxicity. They could palliate some otherwise intractable malignancies, perhaps in young children too, with tolerable sequelae. There are plans for such studies in larger animals.