Composición florística de los bosques de Polylepis Yauyinazo y Chaqsii-Chaqsii, Reserva Paisajística Nor Yauyos-Cochas, Lima

Los bosques de Polylepis forman parte de la vegetación natural de los Andes entre los 3500 y 5000 msnm, con una distribución comúnmente restringida a laderas rocosas y quebradas. Al encontrarse en los altos Andes estos bosques forman áreas diferentes a las que comúnmente se observan, facilitándose la formación de variados micro-hábitats en las que se han encontrado una gran diversidad de especies vegetales. Durante los años 2008-2010 se realizaron recolectas de muestras botánicas dentro de los bosques Yauyinazo y Chaqsii-Chaqsii de la Reserva Paisajística Nor Yauyos-Cochas, en dos épocas del año (húmeda y seca). Se da a conocer la composición de la flora vascular y la variación temporal en los bosques en estudio. Se registró, para ambos bosques, un total de 282 especies agrupadas en 173 géneros y 62 familias, donde las Asteraceae y Poaceae fueron las familias más diversas. Con respecto a la forma de crecimiento las plantas herbáceas y arbustivas fueron las más frecuentes con 71.6 % y 17.4 % respectivamente. En el bosque Yauyinazo se registraron 232 especies agrupadas en 157 géneros y 58 familias y en el bosque Chaqsii-Chaqsii 213 especies en 138 géneros y 56 familias. Draba soratensis y Stellaria weddellii se citan como especie confirmada y nuevo registro en el Perú respectivamente, además se identifica una nueva especie para la ciencia Thalictrum peruvianum. Se registraron 41 especies endémicas y 13 especies de flora silvestre amenazada, evidenciándose la importancia de los bosques de Polylepis. Existe una variación en la composición de especies entre la época húmeda y seca, expresada por el índice de Jaccard con un valor de 0.65 en el bosque Yauyinazo y 0.62 en el bosque Chaqsii-Chaqsii, siendo las especies herbáceas las más afectadas por la estacionalidad.Tesi

Thalictrum peruvianum (Ranunculaceae), una especie nueva de Lima, Perú

A new species, Thalictrum peruvianum H. Trinidad & A. Cano (Ranunculaceae), is described from central Peru. It is characterized for having very small and solitary flowers that born opposite to the leaves, and by winged stigma. These characters distinguish this new taxon from other South American species.Se describe e ilustra una nueva especie Thalictrum peruvianum H. Trinidad & A. Cano (Ranunculaceae) del centro de Perú. Está caracterizada por presentar flores solitarias muy pequeñas que nacen opuestas a las hojas y un estigma alado. Estos caracteres diferencian este nuevo taxón del resto de especies sudamericanas

Molecular data reveal hidden diversity in the central Andean species Weberbauera spathulifolia (Thelypodieae: Brassicaceae)

Weberbauera (Brassicaceae, tribe Thelypodieae) comprises 18 species distributed along the central Andes of Argentina, Bolivia, Chile and Peru. Of these species, W. spathulifolia has the largest geographical range in the genus, extending c. 3000 km along the Andean highlands from La Rioja Province in Argentina to Ancash Department in Peru. This species also shows the greatest morphological variation in the genus. However, whether this geographical and morphological variation represents one or more lineages remains unclear. In this study, we analyse W. spathulifolia across its entire distribution range using molecular, morphological and ecological data. Because there is no phylogenetic analysis for the genus, we generated a comprehensive molecular sampling using nuclear (ITS) and plastid (trnL-F and trnH-psbA) sequences for other Weberbauera spp. and representatives of South American Thelypodieae. Results support the presence of two different lineages within W. spathulifolia, one in the northern part of the species range and the other distributed across its southern and central range. In addition to the morphological differences and the allopatric distribution, these lineages also differ in their climatic niches. Therefore, we propose here to retain the northern lineage under W. spathulifolia and to treat the southern-central lineage under W. orophila, comb. nov. Phylogenetic placement of Weberbauera spp. among the South American Thelypodieae is also analysed and discussed. Results of this study contribute to understanding the biodiversity and evolution of the Andean Brassicaceae.Fil: Salariato, Diego Leonel. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Botánica Darwinion. Academia Nacional de Ciencias Exactas, Físicas y Naturales. Instituto de Botánica Darwinion; ArgentinaFil: Trinidad, Huber. Universidad Nacional Mayor de San Marcos; PerúFil: Cano, Asunción. Universidad Nacional Mayor de San Marcos; PerúFil: Zuloaga, Fernando Omar. Consejo Nacional de Investigaciones Científicas y Técnicas. Instituto de Botánica Darwinion. Academia Nacional de Ciencias Exactas, Físicas y Naturales. Instituto de Botánica Darwinion; ArgentinaFil: Al Shehbaz, Ihsan. Missouri Botanical Garden; Estados Unido

Contribution to Andean flora from Oyón District , Lima, Peru

En este trabajo se presenta el inventario de plantas vasculares de montaña alta (altitudes de 4000 a 4810 m) del noreste del distrito de Oyón, región Lima, Perú. Las colectas se realizaron durante los periodos marzo a mayo de 2014 y de 2015, y setiembre a noviembre de 2014. Se encontraron 47 familias, 112 géneros y 181 especies, de las cuales 94 no estaban registradas para la región Lima. Se presenta la lista de todas las especies encontradas con referencia a los colectores, número de colecta y altitud de colecta. Se argumenta la necesidad de multiplicar los inventarios botánicos locales que permitirían conocer mejor la diversidad de la flora, la distribución de las especies, y los endemismos en la vegetación altoandina.In this paper, the inventory of vascular plants of high mountains (altitudes of 4000-4810 m) from northeast Oyon district, Lima, Peru is presented. Specimens were collected during March to May 2014 and 2015 and September to November 2015. 47 families, 112 genera and 181 species are reported, of which 94 were the first record for Lima region. For each species are given collector names, collect number and elevation. New local botanical inventories are needed for better evaluating the diversity, species distribution patterns and endemism in the high Andean vegetation

Flora y vegetación de suelos crioturbados y hábitats asociados en los alrededores del abra Apacheta, Ayacucho - Huancavelica (Perú)

around Abra Apacheta, in Cangallo (Ayacucho) and Huaytara (Huancavelica) Provinces. The aims of this study were: to study vascular floristic composition of High Andes (over 4500 m of altitude) and characterize highland vegetation. There were used conventional techniques for botanical collection and vegetation coverage measurements by intersection-line transects and Point Quadrat modifyed method. There were registered 134 species of vascular plants (Pteridophytes, Gymnospems, Eudicots and Monocots) grouped in 60 genera and 23 families. Eudicots were the dominant group with 74% of the total registered, 82% in genera and 77% in species; followed by Monocots with 13%, 13% and 21% in the previous categories. Monilophytes (ferns) were poorly represented by two families (9%), two genera (3%) and two species (1%); while Gymnosperms only registered one specie (Ephedra rupestris Benth.). By the quantitative analysis three types of plant communities associated to cryoturbated soils were characterized, we also report two types of associated vegetation: grasslands and rocky areas.Se presentan los resultados del estudio de la flora y vegetación de suelos crioturbados y hábitats asociados realizados en la zona del Abra Apacheta, en las provincias de Cangallo (Ayacucho) y Huaytará (Huancavelica). Los objetivos fueron: estudiar la composición de la flora vascular de los altos Andes (por encima de los 4500 m de altitud) y caracterizar la vegetación altoandina. Se aplicaron técnicas convencionales de colecta botánica, así como evaluaciones de la cobertura vegetal mediante transectos. Se registraron 134 especies de plantas vasculares agrupadas en 60 géneros y 23 familias. Las eudicotiledóneas son el grupo dominante con el 74% del total de familias reportadas, 82% en géneros y 77% en especies; seguido por las monocotiledóneas (13% de las familias, 13% de los géneros y 21% de las especies). Los monilófitos (helechos) están representados por dos familias (9%), dos géneros (3%) y dos especies (1%); mientras que para las gimnospermas se registra una sola especie (Ephedra rupestris Benth.). Tres tipos de comunidades en suelos crioturbados fueron caracterizadas y es reportada la presencia de dos tipos de vegetación asociada: pajonales y vegetación de roquedales

Intradural spinal neurocysticercosis: Case presentation

Introduction: Neurocysticercosis (NCC) is a common parasitic infection of the central nervous system caused by the larvae of the Taenia solium. Spinal cord involvement is very uncommon. Clinical case: A female patient with a history of NCC presented with chronic and recurrent headache associated with motor and sensory deficit, which develops tonic-clonic convulsion, with spatial disorientation. She also had intracranial hypertension syndrome, meningitis syndrome, and pyramidal sygns suggestive of spinal NCC. Conclusions: Neurocysticercosis usually occurs in developing countries and should be considered as a differential diagnosis of neurological diseases. Early diagnosis and treatment are mandatory, as well as education to the community to primary prevention

The CARMENES search for exoplanets around M dwarfs High-resolution optical and near-infrared spectroscopy of 324 survey stars

The CARMENES radial velocity (RV) survey is observing 324 M dwarfs to search for any orbiting planets. In this paper, we present the survey sample by publishing one CARMENES spectrum for each M dwarf. These spectra cover the wavelength range 520–1710 nm at a resolution of at least R >80 000, and we measure its RV, Hα emission, and projected rotation velocity. We present an atlas of high-resolution M-dwarf spectra and compare the spectra to atmospheric models. To quantify the RV precision that can be achieved in low-mass stars over the CARMENES wavelength range, we analyze our empirical information on the RV precision from more than 6500 observations. We compare our high-resolution M-dwarf spectra to atmospheric models where we determine the spectroscopic RV information content, Q, and signal-to-noise ratio. We find that for all M-type dwarfs, the highest RV precision can be reached in the wavelength range 700–900 nm. Observations at longer wavelengths are equally precise only at the very latest spectral types (M8 and M9). We demonstrate that in this spectroscopic range, the large amount of absorption features compensates for the intrinsic faintness of an M7 star. To reach an RV precision of 1 m s−1 in very low mass M dwarfs at longer wavelengths likely requires the use of a 10 m class telescope. For spectral types M6 and earlier, the combination of a red visual and a near-infrared spectrograph is ideal to search for low-mass planets and to distinguish between planets and stellar variability. At a 4 m class telescope, an instrument like CARMENES has the potential to push the RV precision well below the typical jitter level of 3–4 m s−1

The CARMENES search for exoplanets around M dwarfs High-resolution optical and near-infrared spectroscopy of 324 survey stars

The CARMENES radial velocity (RV) survey is observing 324 M dwarfs to search for any orbiting planets. In this paper, we present the survey sample by publishing one CARMENES spectrum for each M dwarf. These spectra cover the wavelength range 520–1710 nm at a resolution of at least R >80 000, and we measure its RV, Hα emission, and projected rotation velocity. We present an atlas of high-resolution M-dwarf spectra and compare the spectra to atmospheric models. To quantify the RV precision that can be achieved in low-mass stars over the CARMENES wavelength range, we analyze our empirical information on the RV precision from more than 6500 observations. We compare our high-resolution M-dwarf spectra to atmospheric models where we determine the spectroscopic RV information content, Q, and signal-to-noise ratio. We find that for all M-type dwarfs, the highest RV precision can be reached in the wavelength range 700–900 nm. Observations at longer wavelengths are equally precise only at the very latest spectral types (M8 and M9). We demonstrate that in this spectroscopic range, the large amount of absorption features compensates for the intrinsic faintness of an M7 star. To reach an RV precision of 1 m s−1 in very low mass M dwarfs at longer wavelengths likely requires the use of a 10 m class telescope. For spectral types M6 and earlier, the combination of a red visual and a near-infrared spectrograph is ideal to search for low-mass planets and to distinguish between planets and stellar variability. At a 4 m class telescope, an instrument like CARMENES has the potential to push the RV precision well below the typical jitter level of 3–4 m s−1

The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden’s Star

Context.Teegarden’s Star is the brightest and one of the nearest ultra-cool dwarfs in the solar neighbourhood. For its late spectral type (M7.0 V),the star shows relatively little activity and is a prime target for near-infrared radial velocity surveys such as CARMENES.Aims.As part of the CARMENES search for exoplanets around M dwarfs, we obtained more than 200 radial-velocity measurements of Teegarden’sStar and analysed them for planetary signals.Methods.We find periodic variability in the radial velocities of Teegarden’s Star. We also studied photometric measurements to rule out stellarbrightness variations mimicking planetary signals.Results.We find evidence for two planet candidates, each with 1.1M⊕minimum mass, orbiting at periods of 4.91 and 11.4 d, respectively. Noevidence for planetary transits could be found in archival and follow-up photometry. Small photometric variability is suggestive of slow rotationand old age.Conclusions.The two planets are among the lowest-mass planets discovered so far, and they are the first Earth-mass planets around an ultra-cooldwarf for which the masses have been determined using radial velocities.We thank the referee Rodrigo Díaz for a careful review andhelpful comments. M.Z. acknowledges support from the Deutsche Forschungs-gemeinschaft under DFG RE 1664/12-1 and Research Unit FOR2544 “BluePlanets around Red Stars”, project no. RE 1664/14-1. CARMENES isan instrument for the Centro Astronómico Hispano-Alemán de Calar Alto(CAHA, Almería, Spain). CARMENES is funded by the German Max-Planck-Gesellschaft (MPG), the Spanish Consejo Superior de InvestigacionesCientíficas (CSIC), the European Union through FEDER/ERF FICTS-2011-02 funds, and the members of the CARMENES Consortium (Max-Planck-Institut für Astronomie, Instituto de Astrofísica de Andalucía, LandessternwarteKönigstuhl, Institut de Ciències de l’Espai, Institut für Astrophysik Göttingen,Universidad Complutense de Madrid, Thüringer Landessternwarte Tautenburg,Instituto de Astrofísica de Canarias, Hamburger Sternwarte, Centro de Astro-biología and Centro Astronómico Hispano-Alemán), with additional contribu-tions by the Spanish Ministry of Economy, the German Science Foundationthrough the Major Research Instrumentation Programme and DFG ResearchUnit FOR2544 “Blue Planets around Red Stars”, the Klaus Tschira Stiftung, thestates of Baden-Württemberg and Niedersachsen, and by the Junta de Andalucía.Based on data from the CARMENES data archive at CAB (INTA-CSIC). Thisarticle is based on observations made with the MuSCAT2 instrument, devel-oped by ABC, at Telescopio Carlos Sánchez operated on the island of Tener-ife by the IAC in the Spanish Observatorio del Teide. Data were partly col-lected with the 150-cm and 90-cm telescopes at the Sierra Nevada Observa-tory (SNO) operated by the Instituto de Astrofísica de Andalucía (IAA-CSIC).Data were partly obtained with the MONET/South telescope of the MOnitoringNEtwork of Telescopes, funded by the Alfried Krupp von Bohlen und HalbachFoundation, Essen, and operated by the Georg-August-Universität Göttingen,the McDonald Observatory of the University of Texas at Austin, and the SouthAfrican Astronomical Observatory. We acknowledge financial support from theSpanish Agencia Estatal de Investigación of the Ministerio de Ciencia, Inno-vación y Universidades and the European FEDER/ERF funds through projectsAYA2015-69350-C3-2-P, AYA2016-79425-C3-1/2/3-P, AYA2018-84089, BES-2017-080769, BES-2017-082610, ESP2015-65712-C5-5-R, ESP2016-80435-C2-1/2-R, ESP2017-87143-R, ESP2017-87676-2-2, ESP2017-87676-C5-1/2/5-R, FPU15/01476, RYC-2012-09913, the Centre of Excellence ”Severo Ochoa”and ”María de Maeztu” awards to the Instituto de Astrofísica de Canarias (SEV-2015-0548), Instituto de Astrofísica de Andalucía (SEV-2017-0709), and Cen-tro de Astrobiología (MDM-2017-0737), the Generalitat de Catalunya throughCERCA programme”, the Deutsches Zentrum für Luft- und Raumfahrt throughgrants 50OW0204 and 50OO1501, the European Research Council through grant694513, the Italian Ministero dell’instruzione, dell’università de della ricerca andUniversità degli Studi di Roma Tor Vergata through FFABR 2017 and “Mis-sion: Sustainability 2016”, the UK Science and Technology Facilities Council through grant ST/P000592/1, the Israel Science Foundation through grant848/16, the Chilean CONICYT-FONDECYT through grant 3180405, the Mexi-can CONACYT through grant CVU 448248, the JSPS KAKENHI through grantsJP18H01265 and 18H05439, and the JST PRESTO through grant JPMJPR1775

The CARMENES search for exoplanets around M dwarfs HD147379 b: A nearby Neptune in the temperate zone of an early-M dwarf

We report on the first star discovered to host a planet detected by radial velocity (RV) observations obtained within the CARMENES survey for exoplanets around M dwarfs. HD 147379 (V = 8.9 mag, M = 0.58 ± 0.08 M⊙), a bright M0.0 V star at a distance of 10.7 pc, is found to undergo periodic RV variations with a semi-amplitude of K = 5.1 ± 0.4 m s−1 and a period of P = 86.54 ± 0.06 d. The RV signal is found in our CARMENES data, which were taken between 2016 and 2017, and is supported by HIRES/Keck observations that were obtained since 2000. The RV variations are interpreted as resulting from a planet of minimum mass mP sin i = 25 ± 2 M⊕, 1.5 times the mass of Neptune, with an orbital semi-major axis a = 0.32 au and low eccentricity (e < 0.13). HD 147379 b is orbiting inside the temperate zone around the star, where water could exist in liquid form. The RV time-series and various spectroscopic indicators show additional hints of variations at an approximate period of 21.1 d (and its first harmonic), which we attribute to the rotation period of the star.FEDER/ERF FICTS-2011-02 fundsMajor Research Instrumentation Programme and DFG Research Unit FOR2544 “Blue Planets around Red StarsEuropean Research Council (ERC-279347), Deutsche Forschungsgemeinschaft (RE 1664/12-1, RE 2694/4-1), Bundesministerium für Bildung und Forschung (BMBF-05A14MG3, BMBF-05A17MG3), Spanish Ministry of Economy and Competitiveness (MINECO, grants AYA2015-68012-C2-2-P, AYA2016-79425-C3-1,2,3-P, AYA2015-69350-C3-2-P, AYA2014-54348-C03- 01, AYA2014-56359-P, AYA2014-54348-C3-2-R, AYA2016-79425-C3-3-P and 2013 Ramòn y Cajal program RYC-2013-14875), Fondo Europeo de Desarrollo Regional (FEDER, grant ESP2016-80435-C2-1-R, ESP2015-65712-C5- 5-R), Generalitat de Catalunya/CERCA programme, Spanish Ministerio de Educación, Cultura y Deporte, programa de Formación de Profesorado Universitario (grant FPU15/01476), Deutsches Zentrum für Luft- und Raumfahrt (grants 50OW0204 and 50OO1501), Office of Naval Research Global (award no. N62909-15-1-2011), Mexican CONACyT grant CB-2012-183007