Biases in Virial Black Hole Masses: An SDSS Perspective

We compile black hole (BH) masses for $\sim 60,000$ quasars in the redshift range $0.1 \lesssim z \lesssim 4.5$ included in the Fifth Data Release of the Sloan Digital Sky Survey (SDSS), using virial BH mass estimators based on the \hbeta, \MgII, and \CIV emission lines. We find that: (1) within our sample, the widths of the three lines follow log-normal distributions, with means and dispersions that do not depend strongly on luminosity or redshift;(2) the \MgII- and \hbeta-estimated BH masses are consistent with one another; and (3) the \CIV BH mass estimator may be more severely affected by a disk wind component than the \MgII and \hbeta estimators, giving a positive bias in mass correlated with the \CIV-\MgII blueshift. Most SDSS quasars have virial BH masses in the range $10^8-10^9 M_\odot$. There is a clear upper mass limit of $\sim 10^{10} M_\odot$ for active BHs at $z \gtrsim 2$, decreasing at lower redshifts. Making the reasonable assumptions that the underlying BH mass distribution decreases with mass and that the Eddington ratio distribution at fixed BH mass has non-zero width, we show that the measured virial BH mass distribution and Eddington ratio distribution are subject to Malmquist bias. A radio quasar subsample (with $1.5\lesssim z\lesssim 2.3$) has mean virial BH mass larger by $\sim 0.12$ dex than the whole sample. A broad absorption line (BAL) quasar subsample (with $1.7\lesssim z\lesssim 2.2$) has identical virial mass distribution as the nonBAL sample, with no mean offset. (Abridged)Comment: Updated virial mass measurements; improved presentation of the MC simulation; added new discussion sections; conclusions unchanged. The full table1 is available at http://www.astro.princeton.edu/~yshen/BH_mass/datafile1.txt.tar.g

A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity

(Abridged) We develop a model for the cosmological role of mergers in the evolution of starbursts, quasars, and spheroidal galaxies. Combining halo mass functions (MFs) with empirical halo occupation models, we calculate where major galaxy-galaxy mergers occur and what kinds of galaxies merge, at all redshifts. We compare with observed merger MFs, clustering, fractions, and small-scale environments, and show that this yields robust estimates in good agreement with observations. Making the simple ansatz that major, gas-rich mergers cause quasar activity, we demonstrate that this naturally reproduces the observed rise and fall of the quasar luminosity density from z=0-6, as well as quasar LFs, fractions, host galaxy colors, and clustering as a function of redshift and luminosity. The observed excess of quasar clustering on small scales is a natural prediction of the model, as mergers preferentially occur in regions with excess small-scale galaxy overdensities. We show that quasar environments at all observed redshifts correspond closely to the empirically determined small group scale, where mergers of gas-rich galaxies are most efficient. We contrast with a secular model in which quasar activity is driven by bars/disk instabilities, and show that while these modes probably dominate at Seyfert luminosities, the constraints from clustering (large and small-scale), pseudobulge populations, disk MFs, luminosity density evolution, and host galaxy colors argue that they must be a small contributor to the z>1 quasar luminosity density.Comment: 34 pages, 27 figures, submitted to ApJ. Fixed appearance of Figure

Observational Limits on Type 1 AGN Accretion Rate in COSMOS

We present black hole masses and accretion rates for 182 Type 1 AGN in COSMOS. We estimate masses using the scaling relations for the broad Hb, MgII, and CIV emission lines in the redshift ranges 0.16<z<0.88, 1<z<2.4, and 2.7<z<4.9. We estimate the accretion rate using an Eddington ratio L_I/L_Edd estimated from optical and X-ray data. We find that very few Type 1 AGN accrete below L_I/L_Edd ~ 0.01, despite simulations of synthetic spectra which show that the survey is sensitive to such Type 1 AGN. At lower accretion rates the BLR may become obscured, diluted or nonexistent. We find evidence that Type 1 AGN at higher accretion rates have higher optical luminosities, as more of their emission comes from the cool (optical) accretion disk with respect to shorter wavelengths. We measure a larger range in accretion rate than previous works, suggesting that COSMOS is more efficient at finding low accretion rate Type 1 AGN. However the measured range in accretion rate is still comparable to the intrinsic scatter from the scaling relations, suggesting that Type 1 AGN accrete at a narrow range of Eddington ratio, with L_I/L_Edd ~ 0.1.Comment: Accepted for pulication in ApJ. 7 pages, 5 figures, table 1 available on reques

Fibroza chistică: protocol clinic naţional PCN-93

USMF „Nicolae Testemiţanu”, IMSP Institutul de Ftiziopneumologie „Chiril Draganiuc”, Centrul Naţional de Sănătate a Reproducerii şi Genetică Medicală, IMSP Institutul Mamei şi Copilului Clinica „Em. Coţaga”, IMSP Institutul Mamei şi Copilului, Asociaţia Naţională Învingem Fibroză Chistică din RMProtocolul naţional a fost elaborat de grupul de lucru al Ministerului Sănătăţii al Republicii Moldova (MS RM), constituit din specialiştii Departamentul Pediatrie a Universităţii de Stat de Medicina şi Farmacie „Nicolae Testemiţanu”, Catedrei Chirurgie, Anesteziologie şi Reanimare Pediatrică USMF „Nicolae Testemiţanu”, Centrului de Sănătate a Reproducerii şi Genetică Medicală, Institutul de Ftiziopneumologie „Chiril Draganiuc”. Protocolul de faţă a fost elaborat în conformitate cu ghidurile internaţionale actuale privind FC şi va servi drept bază pentru elaborarea protocoalelor instituţionale. La recomandarea MS RM pentru monitorizarea protocoalelor instituţionale pot fi folosite formulare suplimentare, care nu sunt incluse în protocolul clinic naţional

A quasar-galaxy mixing diagram: quasar spectral energy distribution shapes in the optical to near-infrared

We define a quasar-galaxy mixing diagram using the slopes of their spectral energy distributions (SEDs) from 1 \u3bcm to 3000 \uc5 and from 1 to 3 \u3bcm in the rest frame. The mixing diagram can easily distinguish among quasar-dominated, galaxy-dominated and reddening-dominated SED shapes. By studying the position of the 413 XMM-selected type 1 AGN in the wide-field `Cosmic Evolution Survey' in the mixing diagram, we find that a combination of the Elvis et al. mean quasar SED with various contributions from galaxy emission and some dust reddening is remarkably effective in describing the SED shape from 0.3 to 3 \u3bcm for large ranges of redshift, luminosity, black hole mass and Eddington ratio of type 1 AGN. In particular, the location in the mixing diagram of the highest luminosity AGN is very close (within 1\u3c3) to that of the Elvis et al. SED template. The mixing diagram can also be used to estimate the host galaxy fraction and reddening in quasar. We also show examples of some outliers which might be AGN in different evolutionary stages compared to the majority of AGN in the quasar-host galaxy co-evolution cycle

Impact of opioid-free analgesia on pain severity and patient satisfaction after discharge from surgery: multispecialty, prospective cohort study in 25 countries

Background: Balancing opioid stewardship and the need for adequate analgesia following discharge after surgery is challenging. This study aimed to compare the outcomes for patients discharged with opioid versus opioid-free analgesia after common surgical procedures.Methods: This international, multicentre, prospective cohort study collected data from patients undergoing common acute and elective general surgical, urological, gynaecological, and orthopaedic procedures. The primary outcomes were patient-reported time in severe pain measured on a numerical analogue scale from 0 to 100% and patient-reported satisfaction with pain relief during the first week following discharge. Data were collected by in-hospital chart review and patient telephone interview 1 week after discharge.Results: The study recruited 4273 patients from 144 centres in 25 countries; 1311 patients (30.7%) were prescribed opioid analgesia at discharge. Patients reported being in severe pain for 10 (i.q.r. 1-30)% of the first week after discharge and rated satisfaction with analgesia as 90 (i.q.r. 80-100) of 100. After adjustment for confounders, opioid analgesia on discharge was independently associated with increased pain severity (risk ratio 1.52, 95% c.i. 1.31 to 1.76; P &lt; 0.001) and re-presentation to healthcare providers owing to side-effects of medication (OR 2.38, 95% c.i. 1.36 to 4.17; P = 0.004), but not with satisfaction with analgesia (beta coefficient 0.92, 95% c.i. -1.52 to 3.36; P = 0.468) compared with opioid-free analgesia. Although opioid prescribing varied greatly between high-income and low- and middle-income countries, patient-reported outcomes did not.Conclusion: Opioid analgesia prescription on surgical discharge is associated with a higher risk of re-presentation owing to side-effects of medication and increased patient-reported pain, but not with changes in patient-reported satisfaction. Opioid-free discharge analgesia should be adopted routinely

Francophony in the Moldova Republic

Before 1812, the current Republic of Moldova, then a territory of the Rumanian region called Moldova, chose France as a cultural model and outlet. After this date, the territory became part of the Russian Empire under the name of Basarabia and thus entered a completely different cultural space at the border of civilizations. Nowadays, is the discourse related to culture and identity doubled or divided? Some Moldavans opt for a Rumanian identity and others a Moldovan one in a context with many multicultural aspects. A representative of the headquarters of an international organization asked a Moldavian colleague under which nationality he should be put down on a list of employees. “Moldavian” was chosen for citizens of the Republique of Moldova only for the Rumanian representative to object that this nationality did not in fact exist. What would have been your answer to this question had you been the Moldovan representative?Avant 1812, l'actuelle République de Moldavie, partie intégrante de la région roumaine appelée Moldavie, avait comme modèle et débouché culturel la France. Après cette date, rattachée à l'Empire Russe, elle a dû rentrer, sous le nom de Bessarabie dans un tout autre giron culturel, à la frontière des civilisations. Aujourd'hui, le discours relatif à la culture et à l'identité est-il double ou dédoublé ? Certains Moldaves plaident pour leur identité roumaine, d'autres pour leur identité moldave et ceci sur un fond à nombreuses touches multiculturelles. Un représentant du quartier général d'une organisation internationale a demandé à un collaborateur moldave son avis quant à la nationalité qu'il faudrait indiquer sur la liste des employés. Puisqu'au moment où, pour les ressortissants de la République de Moldavie, il a été écrit «moldave», le représentant roumain a objecté que cette nationalité n'existe pas. Si vous étiez le représentant moldave, que répondriez-vous

LA TERMINOLOGIE DES POLITIQUES LINGUISTIQUES: UNE APPROCHE INTERCULTURELLE

Durant les deux dernières décenniesla Républiquede Moldova a élaboré des politiques linguistiques, ainsi que d’autres politiques, en déclarant son adhésion aux standards des traités internationaux et aux valeurs de la démocratie. Néanmoins, l’utilisation des notions et terminologies «fabriquées» localement, ou inspirées des documents internationaux ne s’est pas traduit en actions effectives pour confirmer les aspirations de l’Etat moldave pour la démocratie et, plus récemment pour le rapprochement de l’UE.The Terminology of language policy: an intercultural approach During the last two decadesMoldovahas developed language policies in the same way that other policies, declaring its adherence to the standards of international treaties and values of democracy. Nevertheless, the use of notions and terminologies "made" locally, or inspired by international documents has not really been transposed into effective actions to confer, the aspirations of theMoldovanStatefor democracy, and most recently for rapprochement with the European Union. </p