Accreting Protoplanets in the LkCa 15 Transition Disk

Exoplanet detections have revolutionized astronomy, offering new insights into solar system architecture and planet demographics. While nearly 1900 exoplanets have now been discovered and confirmed, none are still in the process of formation. Transition discs, protoplanetary disks with inner clearings best explained by the influence of accreting planets, are natural laboratories for the study of planet formation. Some transition discs show evidence for the presence of young planets in the form of disc asymmetries or infrared sources detected within their clearings, as in the case of LkCa 15. Attempts to observe directly signatures of accretion onto protoplanets have hitherto proven unsuccessful. Here we report adaptive optics observations of LkCa 15 that probe within the disc clearing. With accurate source positions over multiple epochs spanning 2009 - 2015, we infer the presence of multiple companions on Keplerian orbits. We directly detect H{\alpha} emission from the innermost companion, LkCa 15 b, evincing hot (~10,000 K) gas falling deep into the potential well of an accreting protoplanet.Comment: 35 pages, 3 figures, 1 table, 9 extended data item

New Spatially Resolved Observations of the T Cha Transition Disk and Constraints on the Previously Claimed Substellar Companion

We present multi-epoch non-redundant masking observations of the T Cha transition disk, taken at the VLT and Magellan in H, Ks, and L' bands. T Cha is one of a small number of transition disks that host companion candidates discovered by high-resolution imaging techniques, with a putative companion at a position angle of 78 degrees, separation of 62 mas, and contrast at L' of 5.1 mag. We find comparable binary parameters in our re-reduction of the initial detection images, and similar parameters in the 2011 L', 2013 NaCo L', and 2013 NaCo Ks data sets. We find a close-in companion signal in the 2012 NaCo L' dataset that cannot be explained by orbital motion, and a non-detection in the 2013 MagAO/Clio2 L' data. However, Monte-carlo simulations show that the best fits to the 2012 NaCo and 2013 MagAO/Clio2 followup data may be consistent with noise. There is also a significant probability of false non-detections in both of these data sets. We discuss physical scenarios that could cause the best fits, and argue that previous companion and scattering explanations are inconsistent with the results of the much larger dataset presented here.Comment: 25 pages, 22 figures, accepted for publication in Ap

The brightest gamma-ray flaring blazar in the sky: AGILE and multi-wavelength observations of 3C 454.3 during November 2010

Since 2005, the blazar 3C 454.3 has shown remarkable flaring activity at all frequencies, and during the last four years it has exhibited more than one gamma-ray flare per year, becoming the most active gamma-ray blazar in the sky. We present for the first time the multi-wavelength AGILE, SWIFT, INTEGRAL, and GASP-WEBT data collected in order to explain the extraordinary gamma-ray flare of 3C 454.3 which occurred in November 2010. On 2010 November 20 (MJD 55520), 3C 454.3 reached a peak flux (E>100 MeV) of F_gamma(p) = (6.8+-1.0)E-5 ph/cm2/s on a time scale of about 12 hours, more than a factor of 6 higher than the flux of the brightest steady gamma-ray source, the Vela pulsar, and more than a factor of 3 brighter than its previous super-flare on 2009 December 2-3. The multi-wavelength data make a thorough study of the present event possible: the comparison with the previous outbursts indicates a close similarity to the one that occurred in 2009. By comparing the broadband emission before, during, and after the gamma-ray flare, we find that the radio, optical and X-ray emission varies within a factor 2-3, whereas the gamma-ray flux by a factor of 10. This remarkable behavior is modeled by an external Compton component driven by a substantial local enhancement of soft seed photons.Comment: Accepted for publication in ApJ Letters. 18 Pages, 4 Figures, 1 Tabl

Validation of a score tool for measurement of histological severity in juvenile dermatomyositis and association with clinical severity of disease.

OBJECTIVES: To study muscle biopsy tissue from patients with juvenile dermatomyositis (JDM) in order to test the reliability of a score tool designed to quantify the severity of histological abnormalities when applied to biceps humeri in addition to quadriceps femoris. Additionally, to evaluate whether elements of the tool correlate with clinical measures of disease severity. METHODS: 55 patients with JDM with muscle biopsy tissue and clinical data available were included. Biopsy samples (33 quadriceps, 22 biceps) were prepared and stained using standardised protocols. A Latin square design was used by the International Juvenile Dermatomyositis Biopsy Consensus Group to score cases using our previously published score tool. Reliability was assessed by intraclass correlation coefficient (ICC) and scorer agreement (α) by assessing variation in scorers' ratings. Scores from the most reliable tool items correlated with clinical measures of disease activity at the time of biopsy. RESULTS: Inter- and intraobserver agreement was good or high for many tool items, including overall assessment of severity using a Visual Analogue Scale. The tool functioned equally well on biceps and quadriceps samples. A modified tool using the most reliable score items showed good correlation with measures of disease activity. CONCLUSIONS: The JDM biopsy score tool has high inter- and intraobserver agreement and can be used on both biceps and quadriceps muscle tissue. Importantly, the modified tool correlates well with clinical measures of disease activity. We propose that standardised assessment of muscle biopsy tissue should be considered in diagnostic investigation and clinical trials in JDM

Imaging protoplanets: observing transition disks with non-redundant masking

Transition disks, protoplanetary disks with inner clearings, are promising objects in which to directly image forming planets. The high contrast imaging technique of non-redundant masking is well posed to detect planetary mass companions at several to tens of AU in nearby transition disks. We present non-redundant masking observations of the T Cha and LkCa 15 transition disks, both of which host posited sub-stellar mass companions. However, due to a loss of information intrinsic to the technique, observations of extended sources (e.g. scattered light from disks) can be misinterpreted as moving companions. We discuss tests to distinguish between these two scenarios, with applications to the T Cha and LkCa 15 observations. We argue that a static, forward-scattering disk can explain the T Cha data, while LkCa 15 is best explained by multiple orbiting companions.Comment: SPIE conference proceedin

Circumstellar discs: What will be next?

This prospective chapter gives our view on the evolution of the study of circumstellar discs within the next 20 years from both observational and theoretical sides. We first present the expected improvements in our knowledge of protoplanetary discs as for their masses, sizes, chemistry, the presence of planets as well as the evolutionary processes shaping these discs. We then explore the older debris disc stage and explain what will be learnt concerning their birth, the intrinsic links between these discs and planets, the hot dust and the gas detected around main sequence stars as well as discs around white dwarfs.Comment: invited review; comments welcome (32 pages

Mutations in PNPLA6 are linked to photoreceptor degeneration and various forms of childhood blindness

Blindness due to retinal degeneration affects millions of people worldwide, but many disease-causing mutations remain unknown. PNPLA6 encodes the patatin-like phospholipase domain containing protein 6, also known as neuropathy target esterase (NTE), which is the target of toxic organophosphates that induce human paralysis due to severe axonopathy of large neurons. Mutations in PNPLA6 also cause human spastic paraplegia characterized by motor neuron degeneration. Here we identify PNPLA6 mutations in childhood blindness in seven families with retinal degeneration, including Leber congenital amaurosis and Oliver McFarlane syndrome. PNPLA6 localizes mostly at the inner segment plasma membrane in photo-receptors and mutations in Drosophila PNPLA6 lead to photoreceptor cell death. We also report that lysophosphatidylcholine and lysophosphatidic acid levels are elevated in mutant Drosophila. These findings show a role for PNPLA6 in photoreceptor survival and identify phospholipid metabolism as a potential therapeutic target for some forms of blindness.Foundation Fighting Blindness CanadaCanadian Institutes of Health ResearchNIHCharles University institutional programmesBIOCEV-Biotechnology and Biomedicine Centre of the Academy of Sciences and Charles University, from the European Regional Development FundMinistry of Health of the Czech RepublicGraduate School of Life Sciences (University of Wuerzburg)Government of Canada through Genome CanadaOntario Genomics InstituteGenome QuebecGenome British ColumbiaMcLaughlin CentreCharles Univ Prague, Inst Inherited Metab Disorders, Fac Med 1, Prague 12000 2, Czech RepublicMcGill Univ, Dept Human Genet, Fac Med, Montreal, PQ H3A 0G1, CanadaGenome Quebec Innovat Ctr, Montreal, PQ H3A 0G1, CanadaClin Res Inst Montreal, Cellular Neurobiol Res Unit, Montreal, PQ H2W 1R7, CanadaMcGill Univ, Montreal, PQ H3A 0G4, CanadaMcGill Univ, Ctr Hlth, Montreal Childrens Hosp, McGill Ocular Genet Lab, Montreal, PQ H3H 1P3, CanadaMcGill Univ, Ctr Hlth, Montreal Childrens Hosp, Dept Paediat Surg, Montreal, PQ H3H 1P3, CanadaMcGill Univ, Ctr Hlth, Montreal Childrens Hosp, Dept Human Genet, Montreal, PQ H3H 1P3, CanadaMcGill Univ, Ctr Hlth, Montreal Childrens Hosp, Dept Ophthalmol, Montreal, PQ H3H 1P3, CanadaUniv Alberta, Royal Alexandra Hosp, Dept Ophthalmol & Visual Sci, Edmonton, AB T5H 3V9, CanadaCharles Univ Prague, Inst Biol & Med Genet, Fac Med 1, Prague 12000 2, Czech RepublicBaylor Coll Med, Dept Mol & Human Genet, Human Genome Sequencing Ctr, Houston, TX 77030 USAUniversidade Federal de São Paulo, Dept Neurol, Div Gen Neurol, BR-04021001 São Paulo, BrazilUniversidade Federal de São Paulo, Dept Neurol, Ataxia Unit, BR-04021001 São Paulo, BrazilNewcastle Univ, Inst Med Genet, Newcastle Upon Tyne NE1 3BZ, Tyne & Wear, EnglandUniversidade Federal de São Paulo, Dept Ophthalmol, BR-04021001 São Paulo, BrazilSo Gen Hosp, Dept Clin Genet, Glasgow G51 4TF, Lanark, ScotlandCardiff Univ, Sch Med, Inst Med Genet, Cardiff CF14 4XN, S Glam, WalesHadassah Hebrew Univ Med Ctr, Dept Ophthalmol, IL-91120 Jerusalem, IsraelOregon Hlth & Sci Univ, Oregon Inst Occupat Hlth Sci, Portland, OR 97239 USAUniv Wurzburg, Lehrstuhl Neurobiol & Genet, D-97074 Wurzburg, GermanyUniv Montreal, Dept Med, Montreal, PQ H3T 1P1, CanadaMcGill Univ, Dept Anat & Cell Biol, Div Expt Med, Montreal, PQ H3A 2B2, CanadaUniversidade Federal de São Paulo, Dept Neurol, Div Gen Neurol, BR-04021001 São Paulo, BrazilUniversidade Federal de São Paulo, Dept Neurol, Ataxia Unit, BR-04021001 São Paulo, BrazilUniversidade Federal de São Paulo, Dept Ophthalmol, BR-04021001 São Paulo, BrazilNIH: EY022356-01NIH: EY018571-05NIH: NS047663-09Charles University institutional programmes: PRVOUK-P24/LF1/3Charles University institutional programmes: UNCE 204011Charles University institutional programmes: SVV2013/266504BIOCEV-Biotechnology and Biomedicine Centre of the Academy of Sciences and Charles University, from the European Regional Development Fund: CZ.1.05/1.1.00/02.0109Ministry of Health of the Czech Republic: NT13116-4/2012Ministry of Health of the Czech Republic: NT14015-3/2013Ontario Genomics Institute: OGI-049Web of Scienc