Low-Ionization Emission Regions in Quasars: Gas Properties Probed with Broad O I and Ca II Lines

We have compiled the emission-line fluxes of O I 8446, O I 11287, and the near-IR Ca II triplet (8579) observed in 11 quasars. These lines are considered to emerge from the same gas as do the Fe II lines in the low-ionized portion of the broad emission line region (BELR). The compiled quasars are distributed over wide ranges of redshift (0.06 < z < 1.08) and of luminosity (-29.8 < M_B < -22.1), thus representing a useful sample to investigate the line-emitting gas properties in various quasar environments. The measured line strengths and velocities, as functions of the quasar properties, are analyzed using photoionization model calculations. We found that the flux ratio between Ca II and O I 8446 is hardly dependent on the redshift or luminosity, indicating similar gas density in the emission region from quasar to quasar. On the other hand, a scatter of the O I 11287/8446 ratios appears to imply the diversity of the ionization parameter. These facts invoke a picture of the line-emitting gases in quasars that have similar densities and are located at regions exposed to various ionizing radiation fluxes. The observed O I line widths are found to be remarkably similar over more than 3 orders of magnitude in luminosity, which indicates a kinematically determined location of the emission region and is in clear contrast to the well-studied case of H I lines. We also argue about the dust presence in the emission region since the region is suggested to be located near the dust sublimation point at the outer edge of the BELR.Comment: Accepted for publication in ApJ; minor rewordings mad

Shocks and dust survival in nearby active galaxies: implications for the alignment effect

One of the most popular explanations for the so-called alignment effect in high redshift (z>0.7) radio galaxies is the scattering by dust of the hidden quasar light. As shown by De Young (1998) a problem with the dust scattering model is that the short destruction time-scale for dust grains means that they will not survive the passage of the radio jet. We investigate the survival of dust in the extended ionised gas of nearby active galaxies with jet/gas interactions. We discuss the implications on the alignment effect of high redshift (>0.7) radio galaxies. We conclude that although shocks are likely to destroy dust grains in regions of interaction, dust might survive in enough quantities to scatter light from the active nucleus and produce alignment between scattered light and the radio structures. We propose an observational test to investigate the existence of dust in shocked regions based on the sensitivity of calcium to depletion onto dust grains.Comment: 8 pages, 1 Figure, 3 tables, accepted for publication in MNRA

Background model of NaI(Tl) detectors for the ANAIS Dark Matter Project

A thorough understanding of the background sources is mandatory in any experiment searching for rare events. The ANAIS (Annual Modulation with NaI(Tl) Scintillators) experiment aims at the confirmation of the DAMA/LIBRA signal at the Canfranc Underground Laboratory (LSC). Two NaI(Tl) crystals of 12.5 kg each produced by Alpha Spectra have been taking data since December 2012. The complete background model of these detectors and more precisely in the region of interest will be described. Preliminary background analysis of a new 12.5 kg crystal received at Canfranc in March 2015 will be presented too. Finally, the power of anticoincidence rejection in the region of interest has been analyzed in a 4x 5 12.5 kg detector matrix.Comment: Contributed to the 11th Patras Workshop on Axions, WIMPs and WISPs, Zaragoza, June 22 to 26, 201

Generation of Bright Two-Color Continuous Variable Entanglement

We present the first measurement of squeezed-state entanglement between the twin beams produced in an Optical Parametric Oscillator (OPO) operating above threshold. Besides the usual squeezing in the intensity difference between the twin beams, we have measured squeezing in the sum of phase quadratures. Our scheme enables us to measure such phase anti-correlations between fields of different frequencies. In the present measurements, wavelengths differ by ~1 nm. Entanglement is demonstrated according to the Duan et al. criterion [Phys. Rev. Lett. 84, 2722 (2000)] $\Delta^2\hat{p}_- +\Delta^2\hat{q}_+=1.47(2)<2$. This experiment opens the way for new potential applications such as the transfer of quantum information between different parts of the electromagnetic spectrum.Comment: 4 pages, 3 figures, submitted to Phys. Rev. Let

Seguiment del contingut de nitrats al sòl i en planta en parcel·les comercials de panís al Pla d'Urgell

En aquest treball es presenten els resultats parcials del primer any de seguiment de nitrats al sòl i en planta de parcel·les comercials de panís (Zea mays L.) a la zona regable dels canals d'Urgell. Les parcel·les han estat seleccionades a partir del coneixement dels sòls de la zona i com a principal criteri el de la representativitat espaial. L'excés de nitrogen a la zona, present a les capes freàtiques i a la xarxa de reg i de drenatges, ve donat per l'aplicació en excés de nitrogen als cultius, entre els quals el panís és un dels més importants. A les parcel·les seguides s'han aplicat dosis de nitrogen que van dels 250 als 350 kg N/ha. Els primers resultats mostren com les aplicacions que fan els agricultors són independents de les disponibilitats inicials de nitrogen al sòl. També es mostra com la determinació de nitrats a la base de la tija al final del cicle pot servir per conèixer si les disponibilitats de N han estat excessives. Els rendiments més elevats, 13,5 Mg/ha, han coincidit amb les aplicacions de N més baixes, les disponibilitats de nitrogen també més baixes i amb el contingut de nitrats a la base de la tija més baix (0,4 g NNO3/ kg). Tot això demostra que la racionalització de l'ús del nitrogen és possible.En este trabajo se presentan los resultados parciales del primer año de seguimiento de nitratos en el suelo y en planta de parcelas comerciales de maíz (Zea mays L.) en la zona regable de los canales de Urgell. Las parcelas han sido seleccionadas a partir del conocimiento de los suelos de la zona y como criterio principal el de su representatividad espacial. El exceso de nitrógeno en la zona, presente en las capas freáticas y en la red de riego y de drenajes viene dado por la aplicación en exceso de nitróge-no a los cultivos, dentro de los cuales el maíz es uno de los más importantes. En las parcelas seguidas se han aplicado dosis de nitrógeno que van de los 250 a los 350 kg N/ha. Los primeros resultados muestran como las aplicaciones que hacen los agricultores son independientes de las disponibilidades iniciales de nitrógeno en el suelo. También se muestra como la determinación de nitratos en la base del tallo al final del ciclo puede servir para conocer si las disponibilidades de N han sido excesivas. Los rendimientos más elevados 13,5 Mg/ha han coincidido con las aplicaciones de N más bajas, las disponibilidades de nitrógeno también más bajas y con el contenido de nitratos en la base del tallo más bajo (0,4 g N-NO3/kg). Todo esto demuestra que la racionalización del uso del nitrógeno es posible.This paper presents the partial results of the first year monitoring of soil and plant nitrate contents in commercial maize (Zea mays L.) in the Urgell canal irrigated area. The fields have been selected starting from the knowledge of the soils in the area and their spatial representativeness as main criteria. The excess of nitrogen in the area, present in the groundwater as well as in the irrigation water, is due to overfertilisation of the crops, of which maize is one of the most importants. In the monitored fields the applied nitrogen fertiliser ranges from 250 to 350 kg/ha. The first results show that the farmers’ applications are not related to the initially available soil nitrogen. They also show how the determination of nitrates in the lower part of the stem at the end of the cycle may help to show if the N availability has been excessive. The higher yields, 13.5 Mg/ha are the same with the lower fertilizer applications, with the lower soil N availabilities and with the lower contents of nitrates in the lower part of the stem (0.4 g NNO3/ kg). All of this show there is ample room to rationalize the nitrogen use

A vestige low metallicity gas shell surrounding the radio galaxy 0943-242 at z=2.92

Observations are presented showing the doublet CIV 1550 absorption lines superimposed on the CIV emission in the radio galaxy 0943-242. Within the errors, the redshift of the absorption system that has a column density of N_CIV = 10^{14.5 +- 0.1} cm-2 coincides with that of the deep Ly-alpha absorption trough observed by Rottgering et al. (1995). The gas seen in absorption has a resolved spatial extent of at least 13 kpc (the size of the extended emission line region). We first model the absorption and emission gas as co-spatial components with the same metallicity and degree of excitation. Using the information provided by the emission and absorption line ratios of CIV and Ly-alpha, we find that the observed quantities are incompatible with photoionization or collisional ionization of cloudlets with uniform properties. We therefore reject the possibility that the absorption and emission phases are co-spatial and favour the explanation that the absorption gas has low metallicity and is located further away from the host galaxy (than the emission line gas). The estimated low metallicity for the absorption gas in 0943-242 (Z \~ 1% solar) and its proposed location -outer halo outside the radio cocoon- suggest that its existence preceeds the observed AGN phase and is a vestige of the initial starburst at the onset of formation of the parent galaxy.Comment: 11 pages,5 figures, A&A accepte

Light yield determination in large sodium iodide detectors applied in the search for dark matter

Application of NaI(Tl) detectors in the search for galactic dark matter particles through their elastic scattering off the target nuclei is well motivated because of the long standing DAMA/LIBRA highly significant positive result on annual modulation, still requiring confirmation. For such a goal, it is mandatory to reach very low threshold in energy (at or below the keV level), very low radioactive background (at a few counts/keV/kg/day), and high detection mass (at or above the 100 kg scale). One of the most relevant technical issues is the optimization of the crystal intrinsic scintillation light yield and the efficiency of the light collecting system for large mass crystals. In the frame of the ANAIS (Annual modulation with NaI Scintillators) dark matter search project large NaI(Tl) crystals from different providers coupled to two photomultiplier tubes (PMTs) have been tested at the Canfranc Underground Laboratory. In this paper we present the estimates of the NaI(Tl) scintillation light collected using full-absorption peaks at very low energy from external and internal sources emitting gammas/electrons, and single-photoelectron events populations selected by using very low energy pulses tails. Outstanding scintillation light collection at the level of 15~photoelectrons/keV can be reported for the final design and provider chosen for ANAIS detectors. Taking into account the Quantum Efficiency of the PMT units used, the intrinsic scintillation light yield in these NaI(Tl) crystals is above 40~photoelectrons/keV for energy depositions in the range from 3 up to 25~keV. This very high light output of ANAIS crystals allows triggering below 1~keV, which is very important in order to increase the sensitivity in the direct detection of dark matter