Discovery of a possibly old galaxy at z=6.027z=6.027, multiply imaged by the massive cluster Abell 383

We report the discovery of a unique $z=6.027$ galaxy, multiply imaged by the cluster Abell 383 and detected in new Hubble Space Telescope ACS and WFC3 imaging, as well as in Warm Spitzer observations. This galaxy was selected as a pair of i-dropouts; its suspected high redshift was confirmed by the measurement of a strong Lyman-alpha line in both images using Keck/DEIMOS. Combining Hubble and Spitzer photometry after correcting for contamination by line emission (estimated to be a small effect), we identify a strong Balmer break of 1.5 magnitudes. Taking into account the magnification factor of 11.4+/-1.9 (2.65+/-0.17 mag) for the brightest image, the unlensed AB magnitude for the source is 27.2+/-0.05 in the H band, corresponding to a 0.4 L* galaxy, and 25.7+/-0.08 at 3.6 um. The UV slope is consistent with beta~2.0, and from the rest-frame UV continuum we measure a current star formation rate of 2.4+/-1.1 Msol/yr. The unlensed half-light radius is measured to be 300 pc, from which we deduce a star-forming surface density of ~10 Msol/yr/kpc2. The Lyman-alpha emission is found to be extended over ~3" along the slit, corresponding to ~5 kpc in the source plane. This can be explained by the presence of a much larger envelope of neutral hydrogen around the star-forming region. Finally, fitting the spectral energy distribution using 7 photometric data points with simple SED models, we derive the following properties: very little reddening, an inferred stellar mass of M*=6e9 Msol, and an inferred age of ~800 Myrs (corresponding to a redshift of formation of ~18). The star-formation rate of this object was likely much stronger in the past than at the time of observation, suggesting that we may be missing a fraction of galaxies at z~6 which have already faded in rest-frame UV wavelengths.Comment: 6 pages, 3 figures, MNRAS in press, replaced with accepted version including minor comment

Introduction to the special issue: ‘Negation and Clitics in French: Interaction and Variation'

This introduction presents very briefly some of the main issues currently discussed around negation particles and clitics in contemporary French and taken up by the six contributions it assembles, namely language change (grammaticalisation of clitics into agreement markers, completion of the Jespersen Cycle) vs. stable variation, and external (sociolinguistic) or internal (phonotactic, prosodic, or syntactic) factors triggering variation in both cases; the hypothesis of a potential diglossia in French opposing two grammars with considerable syntactic differences. Five out of six contributions focus on modern standard and non-standard varieties of French, with a formal theoretical background, while one shows a more philological-descriptive approach and is dedicated to Old French manuscript

Einfluss überwinternder Wasservögel auf Chara-Arten und Dreissena polymorpha am westlichen Bodensee / [Bearb. Stefan Werner]. Hrsg. von der LfU, Landesanstalt für Umweltschutz Baden-Württemberg

Eine fachübergreifende Zusammenarbeit von Fachleuten aus den Bereichen Makrophyten, Makrozoobenthos und Ornithologie hat am Bodensee zum ersten Mal das Beziehungsgefüge zwischen limnischen Nahrungsressourcen der Flachwasserzone und deren Hauptprädatoren, den Wasservögeln, aufgezeigt und die hohe Dynamik in diesem Ökosystem beleuchtet. Hierfür wurden bei dieser Untersuchung Stellen am Bodensee ausgewählt, die geeignet waren, um den Einfluss der Wasservögel auf Makrophyten beziehungsweise auf Dreikantmuscheln (Dreissena polymorpha PALLAS) zu untersuchen. Wasservögel wurden in halbmo-natlichem Abstand zwischen September und März quantifiziert und deren Aktivität abge-schätzt. Diese Erfassung wurde tags und nachts mit einem Infrarotgerät oder einem Restlichtverstärker durchgeführt. Die Beprobung von Makrophyten erfolgte über das gesamte Winterhalbjahr in 3 Tiefenstufen (-1, -1,5 und -2 m) bezogen auf die Mittelwasserlinie (MW, Pegel Konstanz = 361 cm) und wurde am Bodensee zum ersten Mal durchge-führt. Die Characeen-Vegetation im flacheren Litoralbereich des Zeller Sees war bis Dezember schon stark von Wasservögeln genutzt worden, während die tieferen Zonen erst nach der Vereisungsperiode im Februar und März abgeweidet wurden. Ferner zeigte die zum Ende des Winters noch vorhandene Biomasse in Fraßschutzkäfigen, dass der Seneszenzpro-zess am Biomasseverlust offensichtlich nur einen geringen Anteil hat. Bis in -2 m Wasser-tiefe wurde die vorhandene Characeen-Biomasse von den Wasservögeln fast vollständig als Nahrungsressource genutzt. In Iznang verknappten die Ressourcen in -1 m Tiefe frü-her als in Gundholzen. Die Vögel wichen aber nicht nach Gundholzen aus, wo noch genügend Nahrung in dieser Tiefenstufe vorhanden war, sondern sie erschlossen zunächst am selben Ort die tieferen Bereiche. Dies belegt eine Bevorzugung bestimmter Nahrungsgründe. Während der Untersuchungen im Dezem-ber 2001 wurden hier 10.000 Kolbenenten festgestellt, die wesentlich zur Reduktion der dortigen Chara-Bestände beitrugen. Aber im Gegensatz zu den Kolbenenten, die im Februar zahlenmäßig gering vertreten waren, schöpften die Blässhühner die aufgrund des gefallenen Wasserstandes leicht erreichbaren Chara-Rasen noch weiter ab. Die limnologischen Untersuchungen der Dreikantmuscheln erfolgten in vier Tiefenstufen (-1, -3, -7 und -11 m) unter dem Mittleren Niedrigwasserstand (MNW, Pegel Konstanz = 264 cm). Die Probennahmen fanden an allen Stellen vor (September), während (Januar) und nach der Prädation (März) durch Wasservögel statt

Evolution of OH reactivity in NO-free volatile organic compound photooxidation investigated by the fully explicit GECKO-A model

OH reactivity (OHR) is an important control on the oxidative capacity in the atmosphere but remains poorly constrained in many environments, such as remote, rural, and urban atmospheres, as well as laboratory experiment setups under low-NO conditions. For an improved understanding of OHR, its evolution during oxidation of volatile organic compounds (VOCs) is a major aspect requiring better quantification. We use the fully explicit Generator of Explicit Chemistry and Kinetics of Organics in the Atmosphere (GECKO-A) model to study the OHR evolution in the NO-free photooxidation of several VOCs, including decane (an alkane), m-xylene (an aromatic), and isoprene (an alkene). Oxidation progressively produces more saturated and functionalized species. Total organic OHR (including precursor and products, OHRVOC) first increases for decane (as functionalization increases OH rate coefficients) and m-xylene (as much more reactive oxygenated alkenes are formed). For isoprene, C=C&nbsp;bond consumption leads to a rapid drop in OHRVOC before significant production of the first main saturated multifunctional product, i.e., isoprene epoxydiol. The saturated multifunctional species in the oxidation of different precursors have similar average OHRVOC per C&nbsp;atom. The latter oxidation follows a similar course for different precursors, involving fragmentation of multifunctional species to eventual oxidation of C1 and C2 fragments to CO2, leading to a similar evolution of OHRVOC per C&nbsp;atom. An upper limit of the total OH consumption during complete oxidation to CO2 is roughly three per C&nbsp;atom. We also explore the trends in radical recycling ratios. We show that differences in the evolution of OHRVOC between the atmosphere and an environmental chamber, and between the atmosphere and an oxidation flow reactor (OFR), can be substantial, with the former being even larger, but these differences are often smaller than between precursors. The Teflon wall losses of oxygenated VOCs in chambers result in large deviations of OHRVOC from atmospheric conditions, especially for the oxidation of larger precursors, where multifunctional species may suffer substantial wall losses, resulting in significant underestimation of OHRVOC. For OFR, the deviations of OHRVOC evolution from the atmospheric case are mainly due to significant OHR contribution from RO2 and lack of efficient organic photolysis. The former can be avoided by lowering the UV lamp setting in OFR, while the latter is shown to be very difficult to avoid. However, the former may significantly offset the slowdown in fragmentation of multifunctional species due to lack of efficient organic photolysis. &nbsp;</p

Chemical characterization of secondary organic aerosol at a rural site in the southeastern US: insights from simultaneous high-resolution time-of-flight aerosol mass spectrometer (HR-ToF-AMS) and FIGAERO chemical ionization mass spectrometer (CIMS) measurements

The formation and evolution of secondary organic aerosol (SOA) were investigated at Yorkville, GA, in late summer (mid-August to mid-October 2016). The organic aerosol (OA) composition was measured using two online mass spectrometry instruments, the high-resolution time-of-flight aerosol mass spectrometer (AMS) and the Filter Inlet for Gases and AEROsols coupled to a high-resolution time-of-flight iodide-adduct chemical ionization mass spectrometer (FIGAERO-CIMS). Through analysis of speciated organics data from FIGAERO-CIMS and factorization analysis of data obtained from both instruments, we observed notable SOA formation from isoprene and monoterpenes during both day and night. Specifically, in addition to isoprene epoxydiol (IEPOX) uptake, we identified isoprene SOA formation from non-IEPOX pathways and isoprene organic nitrate formation via photooxidation in the presence of NO_x and nitrate radical oxidation. Monoterpenes were found to be the most important SOA precursors at night. We observed significant contributions from highly oxidized acid-like compounds to the aged OA factor from FIGAERO-CIMS. Taken together, our results showed that FIGAERO-CIMS measurements are highly complementary to the extensively used AMS factorization analysis, and together they provide more comprehensive insights into OA sources and composition

Chemical characterization of secondary organic aerosol at a rural site in the southeastern US: insights from simultaneous high-resolution time-of-flight aerosol mass spectrometer (HR-ToF-AMS) and FIGAERO chemical ionization mass spectrometer (CIMS) measurements

The formation and evolution of secondary organic aerosol (SOA) were investigated at Yorkville, GA, in late summer (mid-August to mid-October 2016). The organic aerosol (OA) composition was measured using two online mass spectrometry instruments, the high-resolution time-of-flight aerosol mass spectrometer (AMS) and the Filter Inlet for Gases and AEROsols coupled to a high-resolution time-of-flight iodide-adduct chemical ionization mass spectrometer (FIGAERO-CIMS). Through analysis of speciated organics data from FIGAERO-CIMS and factorization analysis of data obtained from both instruments, we observed notable SOA formation from isoprene and monoterpenes during both day and night. Specifically, in addition to isoprene epoxydiol (IEPOX) uptake, we identified isoprene SOA formation from non-IEPOX pathways and isoprene organic nitrate formation via photooxidation in the presence of NO_x and nitrate radical oxidation. Monoterpenes were found to be the most important SOA precursors at night. We observed significant contributions from highly oxidized acid-like compounds to the aged OA factor from FIGAERO-CIMS. Taken together, our results showed that FIGAERO-CIMS measurements are highly complementary to the extensively used AMS factorization analysis, and together they provide more comprehensive insights into OA sources and composition

The BepiColombo Laser Altimeter (BELA) during Near-Earth Commissioning Phase (NECP)

The ESA/JAXA joint mission BepiColombo to Mercury was launched successfully on October 20, 2018 (UTC) from Kourou, French Guiana. Currently BepiColombo is on its nominal 7-years cruise to the innermost planet. BepiColombo consists of two spacecraft, the Mercury Planetary Orbiter (MPO) and the Mercury Magnetospheric Orbiter (MMO), both targeted for different orbits around Mercury after arrival in December 2025. The BepiColombo Laser Altimeter (BELA) is one of ten payloads on the MPO. After launch the spacecraft and the instruments entered the Near-Earth Commissioning Phase (NECP), including a first switch-on of BELA on November24, 2018. Here we report on the status of the instrument based on the analysis of NECP data and on data from a second switch-on, planned for June 2019

Gravitationally Lensed Galaxies at 2<z<3.5: Direct Abundance Measurements of Lya Emitters

Strong gravitational lensing magnifies the flux from distant galaxies, allowing us to detect emission lines that would otherwise fall below the detection threshold for medium-resolution spectroscopy. Here we present the detection of temperature-sensitive oxygen emission lines from three galaxies at 2<z<3.5, which enables us to directly determine the oxygen abundances and thereby double the number of galaxies at z>2 for which this has been possible. The three galaxies have ~10% solar oxygen abundances in agreement with strong emission line diagnostics. Carbon and nitrogen ratios relative to oxygen are sub-solar as expected for young metal-poor galaxies. Two of the galaxies are Lya emitters with rest-frame equivalent widths of 20 A and 40 A, respectively, and their high magnification factors allow us for the first time to gain insight into the physical characteristics of high-redshift Lya emitters. Using constraints from the physical properties of the galaxies, we accurately reproduce their line profiles with radiative transfer models. The models show a relatively small outflow in agreement with the observed small velocity offsets between nebular emission and interstellar absorption lines.Comment: 10 pages, Accepted for publication in MNRA

The Low Mass End of the Fundamental Relation for Gravitationally Lensed Star Forming Galaxies at 1<z<6

We present VLT/X-shooter spectra of 13 galaxies in the redshift range 1< z < 6, which are strongly lensed by massive galaxy clusters. Spectroscopic redshifts are measured for nine galaxies, while three sources have redshifts determined from continuum breaks in their spectra. The stellar masses of the galaxies span four orders of magnitude between 10^7 and 10^11 M_sun and have luminosities at 1500 A rest-frame between 0.004 and 9 L^* after correcting for the magnification. This allows us to probe a variety of galaxy types from young, low-mass starburst galaxies to massive evolved galaxies. The lensed galaxies with stellar masses less than 10^10 M_sun have a large scatter compared to the fundamental relation between stellar mass, star formation rates and oxygen abundances. We provide a modified fit to the fundamental relation for low-mass, low-metallicity galaxies with a weaker dependence of the metallicity on either the star formation rate or stellar mass compared to low-redshift, high-mass and high-metallicity SDSS galaxies.Comment: 21 pages, Accepted for publication in MNRA