Hādhā kitāb nashwat al-shumūl fī al-safar ilá Islāmbūl riḥlat ʻallāmat ʻaṣrihi wa-fahhāmat Miṣr, khātimat al-mufassirīn al-marḥūm Abū al-Thanāʼ Shihāb al-Dīn al-sayyid Maḥmūd afandī al-shahīr bi-Alūsīźādah.

Mode of access: Internet.

Okupacja Warszawy : zbiór dokumentów i głosów prasy dotyczących sprawy polskiej w związku z zajęciem Warszawy przez wojska niemieckie, sierpień 1915 r.

Errata slip inserted.

Hāẕā Kitāb-i Khvājah Ḥāfiẓ-i Shīrāzī, [1280, i.e. 1863 or 1864].

Richly elegant copy of the Dīvān of the masterful poet Ḥāfiẓ (Khvājah Shams al-Dīn Muḥammad Shīrāzī, d.1390?).

Iʻānat al-ṭālibīn lil-ʻallāmah al-fāḍil al-ṣāliḥ al-kāmil al-sayyid Abī Bakr al-mashhūr bi-al-Sayyid al-Bakrī ibn al-ʻārif billāh Muḥammad Shaṭā al-Dimyāṭī nazīl Makkah al-musharrafah zādahā Allāh sharafan wa-rifʻah ʻalá ḥall alfāẓ Fatḥ al-muʻīn lil-ʻallāmah Zayn al-Dīn al-Malībārī [microform]. Wuḍiʻa bi-al-hāmish Fatḥ al-muʻīn al-madhkūr. Maʻa taqrīrāt sharīfah wa-ziyādāt munīfah / lil-Bakrī.

Microfilm.

The 2df SDSS LRG and QSO survey: evolution of the luminosity function of luminous red galaxies to z=0.6

We present new measurements of the luminosity function (LF) of luminous red galaxies (LRGs) from the Sloan Digital Sky Survey (SDSS) and the 2dF SDSS LRG and Quasar (2SLAQ) survey. We have carefully quantified, and corrected for, uncertainties in the K and evolutionary corrections, differences in the colour selection methods, and the effects of photometric errors, thus ensuring we are studying the same galaxy population in both surveys. Using a limited subset of 6326 SDSS LRGs (with 0.17 < z < 0.24) and 1725 2SLAQ LRGs (with 0.5 < z < 0.6), for which the matching colour selection is most reliable, we find no evidence for any additional evolution in the LRG LF, over this redshift range, beyond that expected from a simple passive evolution model. This lack of additional evolution is quantified using the comoving luminosity density of SDSS and 2SLAQ LRGs, brighter than M-0.2r - 5 log h(0.7) = - 22.5, which are 2.51 +/- 0.03 x 10(-7) L circle dot Mpc(-3) and 2.44 +/- 0.15 x 10(-7) L circle dot Mpc(-3), respectively (< 10 per cent uncertainty). We compare our LFs to the COMBO-17 data and find excellent agreement over the same redshift range. Together, these surveys show no evidence for additional evolution (beyond passive) in the LF of LRGs brighter than M-0.2r - 5 log h(0.7) = - 21 ( or brighter than similar to L-*).. We test our SDSS and 2SLAQ LFs against a simple 'dry merger' model for the evolution of massive red galaxies and find that at least half of the LRGs at z similar or equal to 0.2 must already have been well assembled (with more than half their stellar mass) by z similar or equal to 0.6. This limit is barely consistent with recent results from semi-analytical models of galaxy evolution.

The Las Campanas/Anglo-Australian Telescope Rich Cluster Survey - III. Spectroscopic studies of X-ray bright galaxy clusters at z similar to 0.1

We present the analysis of the spectroscopic and photometric catalogues of 11 X-ray luminous clusters at 0.07 < z < 0.16 from the Las Campanas/Anglo-Australian Telescope Rich Cluster Survey. Our spectroscopic data set consists of over 1600 galaxy cluster members, of which two-thirds are outside r(200). These spectra allow us to assign cluster membership using a detailed mass model and expand on our previous work on the cluster colour-magnitude relation ( CMR) where membership was inferred statistically. We confirm that the modal colours of galaxies on the CMR become progressively bluer with increasing radius d( B - R)/dr(p) = - 0.011 +/- 0.003 and with decreasing local galaxy density d( B - R)/dlog ( Sigma)= - 0.062 +/- 0.009. Interpreted as an age effect, we hypothesize that these trends in galaxy colour should be reflected in mean H delta equivalent width. We confirm that passive galaxies in the cluster increase in Hd line strength as dH delta/dr(p) = 0.35 +/- 0.06. Therefore, those galaxies in the cluster outskirts may have younger luminosity-weighted stellar populations; up to 3 Gyr younger than those in the cluster centre assuming d( B - R)/dt = 0.03 mag per Gyr. A variation of star formation rate, as measured by [ O II]lambda 3727 angstrom, with increasing local density of the environment is discernible and is shown to be in broad agreement with previous studies from the 2dF Galaxy Redshift Survey and the Sloan Digital Sky Survey. We divide our spectra into a variety of types based upon the MORPHs classification scheme. We find that clusters at z similar to 0.1 are less active than their higher-redshift analogues: about 60 per cent of the cluster galaxy population is non-star forming, with a further 20 per cent in the post-starburst class and 20 per cent in the currently active class, demonstrating that evolution is visible within the past 2 - 3 Gyr. We also investigate unusual populations of blue and very red non-star forming galaxies and we suggest that the former are likely to be the progenitors of galaxies which will lie on the CMR, while the colours of the latter possibly reflect dust reddening. We show that the cluster galaxies at large radii consist of both backsplash ones and those that are infalling to the cluster for the first time. We make a comparison to the field population at z similar to 0.1 and examine the broad differences between the two populations. Individually, the clusters show significant variation in their galaxy populations which we suggest reflects their recent infall histories.

DEA-R:ratio-based comparative efficiency model, its mathematical relation to DEA and its use in applications

We propose a new mathematical model for efficiency analysis, which combines DEA methodology with an old idea-Ratio Analysis. Our model, called DEA-R, treats all possible ratios "output/input" as outputs within the standard DEA model. Although DEA and DEA-R generate different summary measures for efficiency, the two measures are comparable. Our mathematical and empirical comparisons establish the validity of DEA-R model in its own right. The key advantage of DEA-R over DEA is that it allows effective integration of the model with experts' opinions via flexible restrictive conditions on individual "output/input" pairs. © 2007 Springer Science+Business Media, LLC.

Estimate of the (R)USLE rainfall erosivity factor from monthly precipitation data in mainland Spain

The need for continuous recording rain gauges makes it difficult to determine the rainfall erosivity factor (R-factor) of the (R)USLE model in areas without good temporal data coverage. In mainland Spain, the Nature Conservation Institute (ICONA) determined the R-factor at few selected pluviographs, so simple estimates of the R-factor are definitely of great interest. The objectives of this study were: (1) to identify a readily available estimate of the R-factor for mainland Spain; (2) to discuss the applicability of a single (global) estimate based on analysis of regional results; (3) to evaluate the effect of record length on estimate precision and accuracy; and (4) to validate an available regression model developed by ICONA. Four estimators based on monthly precipitation were computed at 74 rainfall stations throughout mainland Spain. The regression analysis conducted at a global level clearly showed that modified Fournier index (MFI) ranked first among all assessed indexes. Applicability of this preliminary global model across mainland Spain was evaluated by analyzing regression results obtained at a regional level. It was found that three contiguous regions of eastern Spain (Catalonia, Valencian Community and Murcia) could have a different rainfall erosivity pattern, so a new regression analysis was conducted by dividing mainland Spain into two areas: Eastern Spain and plateau-lowland area. A comparative analysis concluded that the bi-areal regression model based on MFI for a 10-year record length provided a simple, precise and accurate estimate of the R-factor in mainland Spain. Finally, validation of the regression model proposed by ICONA showed that R-ICONA index overpredicted the R-factor by approximately 19%.

LSQ13fn: A type II-Plateau supernova with a possibly low metallicity progenitor that breaks the standardised candle relation∗

We present optical imaging and spectroscopy of supernova (SN) LSQ13fn, a type II supernova with several hitherto-unseen properties. Although it initially showed strong symmetric spectral emission features attributable to He ii, N iii, and C iii, reminiscent of some interacting SNe, it transitioned into an object that would fall more naturally under a type II-Plateau (IIP) classification. However, its spectral evolution revealed several unusual properties: metal lines appeared later than expected, were weak, and some species were conspicuous by their absence. Furthermore, the line velocities were found to be lower than expected given the plateau brightness, breaking the SN IIP standardised candle method for distance estimates. We found that, in combination with a short phase of early-time ejecta-circumstellar material interaction, metal-poor ejecta, and a large progenitor radius could reasonably account for the observed behaviour. Comparisons with synthetic model spectra of SNe IIP of a given progenitor mass would imply a progenitor star metallicity as low as 0.1 Z_⊙. LSQ13fn highlights the diversity of SNe II and the many competing physical effects that come into play towards the final stages of massive star evolution immediately preceding core-collapse.

Comparison between CDC and WHO BMI z-score and their relation with metabolic risk markers in Northern Portuguese obese adolescents

Growth-curves are an important tool for evaluating the anthropometric development in pediatrics. The different growth-curves available are based in different populations, what leads to different cut-offs. Pediatric obesity tracks into adulthood and is associated with increased cardiovascular risk. The accurate assessment of a child nutritional status using growth-curves can indicate individuals that are either obese or in risk of becoming obese, allowing an early intervention. Moreover, the association between the data obtained from growth-curves with specific metabolic risk factors further highlights the importance of these charts. This study aimed to evaluate the associations between body mass index z-score (BMIzsc), determined using the growth-curves from the Centre for Disease Control and Prevention (CDC) and from the World Health Organization (WHO), with cardiovascular risk factors, represented here by metabolic syndrome (MS) and insulin resistance (IR) related parameters. The study involved 246 obese adolescents (10-18 years, 122 females). MS was defined according to the International Diabetes Federation. IR was considered for HOMA-IR greater than 2.5.

Wstępne uwagi o powszechnym głosowaniu korespondencyjnym w wyborach prezydenckich w 2015 r. (wybrane zagadnienia)

Instytucja mężów zaufania, często określana mianem „niemych obserwatorów wyborów”, traktowana jest z dużym dystansem i budzi wśród przedstawicieli doktryny prawa konstytucyjnego, jak również świata polityki, wiele wątpliwości. Zadaniem mężów zaufania jest reprezentowanie podczas wyborów interesu kandydata, bądź listy kandydatów, przed komisją wyborczą i czuwanie nad prawidłowym przebiegiem czynności wyborczych, w tym przede wszystkim zliczaniem głosów i ustalaniem wyników wyborów. Ma zatem istotne znaczenie dla zapewnienia rzetelności i uczciwości procedur wyborczych, jak również poszanowania podstawowych zasad prawa wyborczego, w szczególności zasady powszechności i wolności wyborów oraz tajności głosowania. Niestety w Kodeksie wyborczym uregulowana jest stosunkowo fragmentarycznie, zaś jej dookreślenie znajduje się w wytycznych Państwowej Komisji Wyborczej. Przed wyborami pojawiają się również różne (opracowywane najczęściej przez partie polityczne) instrukcje, określane także mianem vademecum, czy poradniki dla mężów zaufania, których treść może budzić wątpliwości. Wywołuje to potrzebę debaty przedstawicieli doktryny i polityków nad funkcjami i konstrukcją prawną instytucji mężów zaufania w polskim prawie wyborczym, jak i stosownymi jego zmianami.

Glosa do postanowienia Naczelnego Sądu Administracyjnego z dnia 13 stycznia 2016 r., sygn. akt II GZ 927/15

W glosowanym orzeczeniu Naczelny Sąd Administracyjny stwierdził, że od postanowień wojewódzkich sądów administracyjnych odrzucających skargi z przyczyn formalnych w sprawach wszczętych przed dniem wejścia w życie nowelizacji Prawa o postępowaniu przed sądami administracyjnymi (co miało miejsce 15 sierpnia 2015 r.) przysługuje zażalenie, a nie skarga kasacyjna. Przedmiotowe zagadnienie prawne sprowadza się do właściwej wykładni źle sformułowanych przepisów intertemporalnych. W glosie zaprezentowano istotę środków odwoławczych w postępowaniu sądowoadministracyjnym i scharakteryzowano krótko ostatnią nowelizację Prawa o postępowaniu przed sądami administracyjnymi. Autor prezentuje stanowisko krytyczne w stosunku do tezy postanowienia Naczelnego Sądu Administracyjnego, wskazując, że sąd powinien rozstrzygnąć sprawę co do jej istoty. Pogląd ten został poparty odpowiednią argumentacją z uwzględnieniem konkurencyjnego orzecznictwa Naczelnego Sądu Administracyjnego.

A Z-generáció a jövőről – empirikus vizsgálat eredményei

A Magyar Tudományos Akadémia megbízásából 2007-ben Magyarország 2025 címmel tudományos kutatás keretében szakértői előrejelzésekre és nem szakértői véleményekre építve körvonalaztuk hazánk lehetséges társadalmi-gazdasági jövőalternatíváit (Nováky, szerk. 2010). E kutatás során átfogóan vizsgáltuk azt, hogy miként gondolkodnak a hazai végzős középiskolások és egyetemisták az elkövetkező évekről, különös tekintettel a 2025-ös év Magyarországáról. A kérdőíves megkeresés 1000 fő középiskolásra és 500 fő egyetemistára/főiskolásra terjedt ki (Dörnyei–Nagy, 2010a, b) A 2025-ös évhez közeledve ismét egy kérdőíves lekérdezés segítségével 2015-ben ismét megvizsgáltuk a fiatalok (legfőképpen a középiskolások és a felsőoktatásban tanulók, tehát az Y és a Z generáció) jövőhöz való viszonyát, Magyarország 2025-ben várható jövőjéről alkotott elgondolásait. A 2015-ös kutatás a korábbi szerves folytatása, utánkövetése. A kérdőíves lekérdezés során használt kérdőív a korábbi lekérdezés tapasztalatait felhasználva – apróbb módosításokkal – került lekérdezésre, rövidített formában, de alapjaiban nem volt szándékunk megváltoztatni. E tanulmány két nagy fejezetében az új felmérésről és a változásokról adunk átfogó képet; ez utóbbiban a 2015-ös eredményeinket összehasonlítjuk a 2007-ben végzett felmérés eredményeivel.

1-[(Z)-1-Bromo-2-(butyldichloro-lambda(4)tellanyl)ethenyl]cyclohex-1-ene

The Te(IV) atom in the title compound, [Te(C(4)H(9))(C(8)H(10)Br)Cl(2)] or C(12)H(19)BrCl(2)Te, is in a distorted psi-trigonal-bipyramidal geometry, with the lone pair of electrons projected to occupy a position in the equatorial plane, and with the Cl atoms being mutually trans [172.48 (4)degrees]. Close intramolecular [Te center dot center dot center dot Br = 3.3444 (18) angstrom] and intermolecular [Te center dot center dot center dot Cl = 3.675 (3) angstrom] interactions are observed. The latter lead to centrosymmetric dimers which assemble into layers in the bc plane. The primary connections between layers are of the type C-H center dot center dot center dot Cl.