Fossil groups in the Millennium simulation Their environment and its evolution

Context. Fossil systems are defined to be X- ray bright galaxy groups ( or clusters) with a two- magnitude difference between their two brightest galaxies within half the projected virial radius, and represent an interesting extreme of the population of galaxy agglomerations. However, the physical conditions and processes leading to their formation are still poorly constrained. Aims. We compare the outskirts of fossil systems with that of normal groups to understand whether environmental conditions play a significant role in their formation. We study the groups of galaxies in both, numerical simulations and observations. Methods. We use a variety of statistical tools including the spatial cross- correlation function and the local density parameter Delta(5) to probe differences in the density and structure of the environments of "" normal"" and "" fossil"" systems in the Millennium simulation. Results. We find that the number density of galaxies surrounding fossil systems evolves from greater than that observed around normal systems at z = 0.69, to lower than the normal systems by z = 0. Both fossil and normal systems exhibit an increment in their otherwise radially declining local density measure (Delta(5)) at distances of order 2.5 r(vir) from the system centre. We show that this increment is more noticeable for fossil systems than normal systems and demonstrate that this difference is linked to the earlier formation epoch of fossil groups. Despite the importance of the assembly time, we show that the environment is different for fossil and non- fossil systems with similar masses and formation times along their evolution. We also confirm that the physical characteristics identified in the Millennium simulation can also be detected in SDSS observations. Conclusions. Our results confirm the commonly held belief that fossil systems assembled earlier than normal systems but also show that the surroundings of fossil groups could be responsible for the formation of their large magnitude gap.

THE SLOAN NEARBY CLUSTER WEAK LENSING SURVEY

We describe and present initial results of a weak lensing survey of nearby (z less than or similar to 0.1) galaxy clusters in the Sloan Digital Sky Survey (SDSS). In this first study, galaxy clusters are selected from the SDSS spectroscopic galaxy cluster catalogs of Miller et al. and Berlind et al. We report a total of seven individual low-redshift cluster weak lensing measurements that include A2048, A1767, A2244, A1066, A2199, and two clusters specifically identified with the C4 algorithm. Our program of weak lensing of nearby galaxy clusters in the SDSS will eventually reach similar to 200 clusters, making it the largest weak lensing survey of individual galaxy clusters to date.

DECISION TREE CLASSIFIERS FOR STAR/GALAXY SEPARATION

We study the star/galaxy classification efficiency of 13 different decision tree algorithms applied to photometric objects in the Sloan Digital Sky Survey Data Release Seven (SDSS-DR7). Each algorithm is defined by a set of parameters which, when varied, produce different final classification trees. We extensively explore the parameter space of each algorithm, using the set of 884,126 SDSS objects with spectroscopic data as the training set. The efficiency of star-galaxy separation is measured using the completeness function. We find that the Functional Tree algorithm (FT) yields the best results as measured by the mean completeness in two magnitude intervals: 14 <= r <= 21 (85.2%) and r >= 19 (82.1%). We compare the performance of the tree generated with the optimal FT configuration to the classifications provided by the SDSS parametric classifier, 2DPHOT, and Ball et al. We find that our FT classifier is comparable to or better in completeness over the full magnitude range 15 <= r <= 21, with much lower contamination than all but the Ball et al. classifier. At the faintest magnitudes (r > 19), our classifier is the only one that maintains high completeness (> 80%) while simultaneously achieving low contamination (similar to 2.5%). We also examine the SDSS parametric classifier (psfMag - modelMag) to see if the dividing line between stars and galaxies can be adjusted to improve the classifier. We find that currently stars in close pairs are often misclassified as galaxies, and suggest a new cut to improve the classifier. Finally, we apply our FT classifier to separate stars from galaxies in the full set of 69,545,326 SDSS photometric objects in the magnitude range 14 <= r <= 21.

Hubble parameter reconstruction from a principal component analysis: minimizing the bias

Aims. A model-independent reconstruction of the cosmic expansion rate is essential to a robust analysis of cosmological observations. Our goal is to demonstrate that current data are able to provide reasonable constraints on the behavior of the Hubble parameter with redshift, independently of any cosmological model or underlying gravity theory. Methods. Using type Ia supernova data, we show that it is possible to analytically calculate the Fisher matrix components in a Hubble parameter analysis without assumptions about the energy content of the Universe. We used a principal component analysis to reconstruct the Hubble parameter as a linear combination of the Fisher matrix eigenvectors (principal components). To suppress the bias introduced by the high redshift behavior of the components, we considered the value of the Hubble parameter at high redshift as a free parameter. We first tested our procedure using a mock sample of type Ia supernova observations, we then applied it to the real data compiled by the Sloan Digital Sky Survey (SDSS) group. Results. In the mock sample analysis, we demonstrate that it is possible to drastically suppress the bias introduced by the high redshift behavior of the principal components. Applying our procedure to the real data, we show that it allows us to determine the behavior of the Hubble parameter with reasonable uncertainty, without introducing any ad-hoc parameterizations. Beyond that, our reconstruction agrees with completely independent measurements of the Hubble parameter obtained from red-envelope galaxies.

THE SLOAN BRIGHT ARCS SURVEY: DISCOVERY OF SEVEN NEW STRONGLY LENSED GALAXIES FROM z=0.66-2.94

We report the discovery of seven new, very bright gravitational lens systems from our ongoing gravitational lens search, the Sloan Bright Arcs Survey (SBAS). Two of the systems are confirmed to have high source redshifts z = 2.19 and z = 2.94. Three other systems lie at intermediate redshift with z = 1.33, 1.82, 1.93 and two systems are at low redshift z = 0.66, 0.86. The lensed source galaxies in all of these systems are bright, with i-band magnitudes ranging from 19.73 to 22.06. We present the spectrum of each of the source galaxies in these systems along with estimates of the Einstein radius for each system. The foreground lens in most systems is identified by a red sequence based cluster finder as a galaxy group; one system is identified as a moderately rich cluster. In total, SBAS has now discovered 19 strong lens systems in the SDSS imaging data, 8 of which are among the highest surface brightness z similar or equal to 2-3 galaxies known.

Factors determining normal adult height in girls with gonadotropin-dependent precocious puberty treated with depot gonadotropin-releasing hormone analogs

Context: Several factors can affect adult height (AH) of patients with gonadotropin-dependent precocious puberty (GDPP) treated with depot GnRH analogs. Objective: Our objective was to determine factors influencing AH in patients with GDPP treated with depot GnRH analogs. Patients: A total of 54 patients (45 girls) with GDPP treated with depot GnRH analog who reached AH was included in the study. Design: Univariate and multivariate analyses of the factors potentially associated with AH were performed in all girls with GDPP. In addition, clinical features of the girls who attained target height (TH) range were compared with those who did not. Predicted height using Bayley and Pinneau tables was compared with attained AH. Results: In girls the mean AH was 155.3 +/- 6.9 cm (-1.2 +/- 1 SD) with TH range achieved by 81% of this group. Multiple regression analysis revealed that the interval between chronological age at onset of puberty and at the start of GnRH analog therapy, height SD scores (SDSs) at the start and end of therapy, and TH explained 74% of AH variance. The predicted height at interruption of GnRH therapy, obtained from Bayley and Pinneau tables for average bone age, was more accurate than for advanced bone age in both sexes. In boys the mean AH was 170.6 +/- 9.2 cm (-1 +/- 1.3 SDS), whereas TH was achieved by 89% of this group. Conclusions: The major factors determining normal AH in girls with GDPP treated with depot GnRH analogs were shorter interval between the onset of puberty and start of therapy, higher height SDS at the start and end of therapy, and TH. Therefore, prompt depot GnRH analog therapy in properly selected patients with GDPP is critical to obtain normal AH.

Estudos de impacte ambiental em infraestruturas rodoviárias com recurso a tecnologia SIG e avaliação multicritério

O Estudo de Impacte Ambiental (EIA) é uma peça fundamental no processo de Avaliação Ambiental a que têm de ser submetidos alguns projetos de engenharia. Este é o resultado de atividades e avaliações metodológicas conducentes a identificar/avaliar possíveis impactes, apresentando medidas de minimização e o plano de monitorização. Se existirem múltiplas alternativas, o EIA deve indicar a “ambientalmente mais favorável”. O presente trabalho apresenta uma proposta metodológica para apoio dessas atividades/avaliações, tendo como estrutura integradora um SIG ligado a modelos externos específicos, constituindo -se assim como uma contribuição para o desenvolvimento de um SADE -MC, no domínio ambiental. Essa proposta engloba a conceção duma rotina interativa, em Visual Basic® para suportar os processos de Screening/Scoping, Avaliação da Significância e Seleção dos Indicadores Ambientais. As funcionalidades do SIG, associadas aos módulos externos, são usadas para prever/quantificar os impactes e os indicadores ambientais. Estes indicadores são então utilizados como critérios, no módulo de avaliação multicritério que utiliza, nesta aplicação, o método ELECTRE III. Isso permite apresentar uma preordenação final das alternativas, desde a “ambientalmente mais favorável” até à mais adversa. Como caso de estudo, essa proposta metodológica é aplicada a um EIA referente ao projeto de um troço de autoestrada no Centro de Portugal.

Sistema de apoio à decisão espacial para análise do impacte ambiental da dispersão de poluentes atmosféricos

Neste artigo é apresentado um Sistema de Apoio à Decisão Espacial (SADE) onde os decisores podem facilmente definir diferentes tipos de problemas espaciais recorrendo a diferentes categorias de objetos, pré-definidas ou a definir, associando- lhes características com ou sem dependência espacial, e indicando formas de interferência (impactos) entre essas caracte- rísticas/propriedades. A análise espacial para determinação ou avaliação de configurações alternativas para a localização de diferentes tipos de ocorrências espaciais será feita através da utilização interativa do SADE de acordo com conjuntos de regras intrínsecas aos vários elementos gráficos (objetos, categorias, características, impactos) utilizados na definição dos problemas. O teste à generalidade representativa e analítica do SADE proposto é efectuado recorrendo a um problema concreto, suficientemente específico e complexo, relativo à aplicação de modelos gaussianos para o estudo da dispersão atmosférica de eventuais poluentes resultantes do tratamento de resíduos sólidos. A região em estudo está limitada, neste exemplo, ao município de Coimbra, Portugal. Para este município estão acessíveis, e são utilizados, os dados demográficos ao nível da secção de voto (censos oficiais) e, como tal, é possível a realização de um estudo realístico do impacto com populações humanas.

Hazardous substances in frequently used professional cleaning products.

A growing number of studies have identified cleaners as a group at risk for adverse health effects of the skin and the respiratory tract. Chemical substances present in cleaning products could be responsible for these effects. Currently, only limited information is available about irritant and health hazardous chemical substances found in cleaning products. We hypothesized that chemical substances present in cleaning products are known health hazardous substances that might be involved in adverse health effects of the skin and the respiratory tract. We performed a systematic review of cleaning products used in the Swiss cleaning sector. We surveyed Swiss professional cleaning companies (n = 1476) to identify the most used products (n = 105) for inclusion. Safety data sheets (SDSs) were reviewed and hazardous substances present in cleaning products were tabulated with current European and global harmonized system hazard labels. Professional cleaning products are mixtures of substances (arithmetic mean 3.5 +/- 2.8), and more than 132 different chemical substances were identified in 105 products. The main groups of chemicals were fragrances, glycol ethers, surfactants, solvents; and to a lesser extent, phosphates, salts, detergents, pH-stabilizers, acids, and bases. Up to 75% of products contained irritant (Xi), 64% harmful (Xn) and 28% corrosive (C) labeled substances. Hazards for eyes (59%) and skin (50%), and hazards by ingestion (60%) were the most reported. Cleaning products potentially give rise to simultaneous exposures to different chemical substances. As professional cleaners represent a large workforce, and cleaning products are widely used, it is a major public health issue to better understand these exposures. The list of substances provided in this study contains important information for future occupational exposure assessment studies.

Suurnopeuskompressorin tekninen markkinoilletuonti

Diplomityössä tarkastellaan suurnopeuskompressorin kehityspolkua suurnopeusteknologian lähtökohdista prototyypiksi ja edelleen teolliseksi tuotteeksi. Työssä tarkastelun kohteena on sähköteholtaan 20….250 kW oleva, suurnopeussähkökoneella ja öljyttömillä magneettilaakereilla varustettu keskipainekompressori. Tyypillisesti kompressorin painesuhde on 1,2 … 2,4. Ko. kompressorin käyttökohteina on tarkasteltu mm. pienen kunnallisen jätevedenpuhdistamon käsittelyaltaiden ilmastusta, suuren kaupungin vastaavan puhdistuslaitoksen ilmastuskäyttöä ja teollista käyttöä lasivillatehtaan ns. linkokompressorina. Suurnopeuskompressori soveltuu hyvin rinnankytkentään ns. ryhmäohjaimen avulla, jolloin rinnan voi olla kytkettynä jopa 16 kompressoria, joiden päällä oloa optimoidaan säätöteknisesti niin, että koko laitos on kuin yksi kompressori. Työssä tarkastellaan myös kompressorin em. sovellutuksista yli kahdeksan vuoden ajalta kaupallista kohteista saatuja käyttökokemuksia. Pääsäätöisesti voi sanoa, että jokaisessa uudessa sovellutuksessa ilmenee uusia reunaehtoja ja järjestelmäkohtaisia vaatimuksia, jotka täytyy huomioida kompressorin säädössä ja ominaisparametreissa.

Paperin puhtauden parantaminen lajittelun ja muiden prosessiteknisten keinojen avulla

Tämä työ suoritettiin UPM- Kymmene Oyj:n Tervasaaren tehtaan PK 5:llä. PK 5 valmistaa tarrantaustapaperia. Tämän työn tarkoituksena oli löytää eri keinoja paperin puhtauden parantamiseksi. Puhtaamman paperin valmistaminen parantaa paperikoneen kilpailukykyä kilpailijoihinsa nähden sekä vähentää asiakasvalituskustannuksia. Työn kirjallinen osa koostuu kolmesta suuremmasta kokonaisuudesta, joiden tarkoituksena on luoda teoriapohjaa kokeellisen osan suoritusta varten. Kirjallisuusosan pääpaino on kohdistettu PK 5:llä esiintyviin saostumanaiheuttajiin, kuten uuteaineisiin, ASA- liimaan ja mikrobeihin. Tarkemmassa tarkastelussa on kirjallisuusosassa myös painelajittelu ja pyörrepuhdistus. Kokeellisessa osassa suoritettiin PK 5:n prosessissa syntyvien epäpuhtauksien karakterisointi. Suurimmat saostuman aiheuttajat analyysien perusteella olivat puuperäiset uuteaineet ja ASA- liima. Epäorgaanisista aineista päällystyskomponenttina toimiva kaoliini ja sellun mukana tuleva pihkatalkki esiintyi useimpien saostumien komponentteina. Selvityksessä havaittiin, että prosessille vieraita aineita ei löydetty muista, kuin kalanteroidusta paperista analysoiduista tummista täplistä. Tummista täplistä analysoitu styreenin alkuperä voi selittyä mm. prosessiin päässeellä kumilla tai muovilla. PK 5:n prosessissa selvityksen mukaan silikonipohjainen vaahdonestoaine aiheuttaa erittäin suuria tummia saostumia, joten sen pääsy prosessiin tulee estää sellutehtaalla tarkoin. Epäpuhtauksien määrä on suurin PK 5:n prosessissa hylkylinjassa ja lyhyessä kierrossa. Hylyn painelajittelu poistaa hyvin roskia syöttömassasta. Hylyn lajittelun toisen portaan lajittimen rejektin roskapitoisuus on suhteellisen suuri. Rejektin ohjaaminen ulos prosessista vähentää roskaisuuden rikastumista prosessiin. Sakeamassalajittelun sijoittaminen PK 5:n konekyypin jälkeen vähentää roskien päätymistä paperiin. Hylyn painelajittelun ja PP- laitoksen rejektin ohjaaminen sakeamassalajittelun toiseen portaaseen vähentäisi priimakuitutappiota ja roskien määrää käytetyissä massoissa. Seisokin aikaisen putkilinjojen pesujen lopputulos parani huomattavasti BA- pesuaineen käyttöönoton jälkeen. Kyseisen pesuaine soveltuu liuottamaan putkistosta mm. PK 5:llä esiintyvät uuteaine- ja ASA- saostumat. BSA- sellun pH- säädön lopettamisella oli suuri vähentävä vaikutus tummien täplien esiintymistiheyteen. pH- säädössä BSA- tornin pohjalaimennukseen annosteltu lipeä edesauttoi tummien saostumien syntymistä saippuoiden uuteaineita.

Kenttätietojen hyödyntäminen taajuusmuuttajan luotettavuuden suunnittelussa

Taajuusmuuttaja on yhä yleisempi laite perinteisten oikosulkumoottoreiden nopeuden säädössä, niin teollisuudessa kuin muilla käyttökohteissa. Ensimmäiset laitetyypit olivat mekaanisesti suurikokoisia ja vaativat laitteen tekniseltä tuelta ja kunnossapidolta hyvää teknistä perehtyneisyyttä laitteisiin. Teknologian kehittymisen myötä laitteiden teho/kokosuhde on pienentynyt ja tarjolla on useita eri sovelluskohteisiin suoraan soveltuvia taajuusmuuttajia varustettuna helppokäyttöisillä ja kaupallisilla käyttöliittymillä. Laitteen elinkaaren aikainen luotettavuusjohtaminen edellyttää valmistajalta varsinaisen laitesuunnittelun lisäksi tarkoituksenmukaisia testausmenetelmiä ja kokemusperäistä luotettavuustietoa myös asennetusta laitekannasta. Työssä on käyty taajuusmuuttajan suunnittelun kannalta läpi luotettavuuden käsitteistö sekä yleisimpiä luotettavuusmenetelmiä. Luotettavuusnäkökohtia verrataan asennetusta laitekannasta saatuihin kokemuksiin laitteen valmistajan ja tuotetuen kannalta. Työssä on esitetty luokittelun perusteita ja menetelmät, miten käytön aikana voidaan arvioida laitteen teknistä tilaa sekä huomioida se kunnossapidon suunnittelussa. Johtopäätöksenä huomataan, että asennuspaikka ja käyttösovellus määrittävät taajuusmuuttajan käytettävyyden. Kenttätietoja voidaan hyödyntää paikallisen kunnossapidon kannalta kunnossapidon ja investointien suunnittelussa. Toisaalta valmistajan tuotekehitys saa asennetuista laitteista kokemuksia seuraavan sukupolven tyypin suunnittelun perustaksi. Tekniikan voimakkaan kehittymisen seurauksena uusien taajuusmuuttajatyyppien valmistus kestää yhä lyhyemmän ajanjakson, jolloin asennetusta laitekannasta saatu kenttäkokemus on arvokasta tietoa laitevalmistajalle. Yhteenvetona valmistajan laiterekistereitä voidaan kehittää siten, että niihin on tallennettavissa laitekartoitusten perusteella kerättyä informaatiota, jota niin valmistajan myynti, tuotetuki kuin laitesuunnittelu voi omassa toiminnassaan hyödyntää.

Environments of Acitive Galaxies

This dissertation presents studies on the environments of active galaxies. Paper I is a case study of a cluster of galaxies containing BL Lac object RGB 1745+398. We measured the velocity dispersion, mass, and richness of the cluster. This was one of the most thorough studies of the environments of a BL Lac object. Methods used in the paper could be used in the future for studying other clusters as well. In Paper II we studied the environments of nearby quasars in the Sloan Digital Sky Survey (SDSS). We found that quasars have less neighboring galaxies than luminous inactive galaxies. In the large-scale structure, quasars are usually located at the edges of superclusters or even in void regions. We concluded that these low-redshift quasars may have become active only recently because the galaxies in low-density environments evolve later to the phase where quasar activity can be triggered. In Paper III we extended the analysis of Paper II to other types of AGN besides quasars. We found that different types of AGN have different large-scale environments. Radio galaxies are more concentrated in superclusters, while quasars and Seyfert galaxies prefer low-density environments. Different environments indicate that AGN have different roles in galaxy evolution. Our results suggest that activity of galaxies may depend on their environment on the large scale. Our results in Paper III raised questions of the cause of the environment-dependency in the evolution of galaxies. Because high-density large-scale environments contain richer groups and clusters than the underdense environments, our results could reflect smaller-scale effects. In Paper IV we addressed this problem by studying the group and supercluster scale environments of galaxies together. We compared the galaxy populations in groups of different richnesses in different large-scale environments. We found that the large-scale environment affects the galaxies independently of the group richness. Galaxies in low-density environments on the large scale are more likely to be star-forming than those in superclusters even if they are in groups with the same richness. Based on these studies, the conclusion of this dissertation is that the large-scale environment affects the evolution of galaxies. This may be caused by different “speed” of galaxy evolution in low and high-density environments: galaxies in dense environments reach certain phases of evolution earlier than galaxies in underdense environments. As a result, the low-density regions at low redshifts are populated by galaxies in earlier phases of evolution than galaxies in high-density regions.

Loistehon säätö ja kompensointi

Kantaverkkoyhtiö Fingrid Oy on tarkastellut kantaverkosta otettua tai tuotettua loistehoa alueittain Fingridin määrittelemällä maantieteellisellä tavalla. Alue koostuu liittymispisteistä, jotka ovat yksittäisten verkkoyhtiöiden liittymispisteitä. Yhden alueen sisällä voi siis olla monia eri verkkoyhtiöiden liittymispisteitä. Vuodesta 2016 alkaen loistehon tarkastelu vaihtuu aluetarkastelusta liittymispistetarkasteluun. Liittymispistetarkasteluun siirtymisen myötä tulee verkkoyhtiöiden investoida erinäisiin kompensointiratkaisuihin, jotta yksittäisten liittymispisteiden loistehot pysyvät Fingridin asettaman loistehon tarkasteluikkunan sisällä. Työssä perehdytään erinäisiin kompensointiratkaisuihin ja niiden kytkentöihin sekä kytkentöjen vaikutuksiin olemassa olevaan sähköverkkoon. Lisäksi työssä käsitellään tuulivoimaloiden hyödyntämistä loistehon säädössä. Esimerkkitapauksessa tarkastellaan erästä Caruna Oy:n verkkoa ja pohditaan teknistä ja mahdollisimman taloudellista kompensointiratkaisua kyseiseen verkkoon. Työn lopputulos on, että maakaapeloinnin määrän kasvaessa loistehon kompensoinnin tarve kasvaa. Näin ollen Fingrid Oy:ltä tarvitaan selkeitä linjauksia moneen ongelmakohtaan, kuten tuotanto-kulutuspisteen loistehon tarkasteluun. Lisäksi Energiavirastolta tarvitaan kannusteita loistehon kompensointiin, sillä verkkoyhtiöiden liiketoiminta perustuu regulaatiomalliin ja kompensointilaitteiston yksikköhinnasto on hyvin suppea.

Evaluation of Location Intelligence exploitation in capital-intensive business

As technology has developed it has increased the number of data produced and collected from business environment. Over 80% of that data includes some sort of reference to geographical location. Individuals have used that information by utilizing Google Maps or different GPS devices, however such information has remained unexploited in business. This thesis will study the use and utilization of geographically referenced data in capital-intensive business by first providing theoretical insight into how data and data-driven management enables and enhances the business and how especially geographically referenced data adds value to the company and then examining empirical case evidence how geographical information can truly be exploited in capital-intensive business and what are the value adding elements of geographical information to the business. The study contains semi-structured interviews that are used to scan attitudes and beliefs of an organization towards the geographic information and to discover fields of applications for the use of geographic information system within the case company. Additionally geographical data is tested in order to illustrate how the data could be used in practice. Finally the outcome of the thesis provides understanding from which elements the added value of geographical information in business is consisted of and how such data can be utilized in the case company and in capital-intensive business.