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Träfflista för sökning "WFRF:(Petrus P) "

Search: WFRF:(Petrus P)

  • Result 1-25 of 81
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1.
  • Desgrange, C., et al. (author)
  • In-depth direct imaging and spectroscopic characterization of the young Solar System analog HD 95086
  • 2022
  • In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 664
  • Journal article (peer-reviewed)abstract
    • Context. HD 95086 is a young nearby Solar System analog hosting a giant exoplanet orbiting at 57 au from the star between an inner and outer debris belt. The existence of additional planets has been suggested as the mechanism that maintains the broad cavity between the two belts.Aims. We present a dedicated monitoring of HD 95086 with the VLT/SPHERE instrument to refine the orbital and atmospheric properties of HD 95086 b, and to search for additional planets in this system.Methods. SPHERE observations, spread over ten epochs from 2015 to 2019 and including five new datasets, were used. Combined with archival observations, from VLT/NaCo (2012-2013) and Gemini/GPI (2013-2016), the extended set of astrometric measurements allowed us to refine the orbital properties of HD 95086 b. We also investigated the spectral properties and the presence of a circumplanetary disk around HD 95086 b by using the special fitting tool exploring the diversity of several atmospheric models. In addition, we improved our detection limits in order to search for a putative planet c via the K-Stacker algorithm.Results. We extracted for the first time the JH low-resolution spectrum of HD 95086 b by stacking the six best epochs, and confirm its very red spectral energy distribution. Combined with additional datasets from GPI and NaCo, our analysis indicates that this very red color can be explained by the presence of a circumplanetary disk around planet b, with a range of high-temperature solutions (1400–1600 K) and significant extinction (Av ≳ 10 mag), or by a super-solar metallicity atmosphere with lower temperatures (800–300 K), and small to medium amount of extinction (Av ≲ 10 mag). We do not find any robust candidates for planet c, but give updated constraints on its potential mass and location.
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  • Hinkley, Sasha, et al. (author)
  • The JWST Early Release Science Program for the Direct Imaging and Spectroscopy of Exoplanetary Systems
  • 2022
  • In: Publications of the Astronomical Society of the Pacific. - : IOP Publishing. - 0004-6280 .- 1538-3873. ; 134:1039
  • Journal article (peer-reviewed)abstract
    • The direct characterization of exoplanetary systems with high-contrast imaging is among the highest priorities for the broader exoplanet community. As large space missions will be necessary for detecting and characterizing exo-Earth twins, developing the techniques and technology for direct imaging of exoplanets is a driving focus for the community. For the first time, JWST will directly observe extrasolar planets at mid-infrared wavelengths beyond 5 μm, deliver detailed spectroscopy revealing much more precise chemical abundances and atmospheric conditions, and provide sensitivity to analogs of our solar system ice-giant planets at wide orbital separations, an entirely new class of exoplanet. However, in order to maximize the scientific output over the lifetime of the mission, an exquisite understanding of the instrumental performance of JWST is needed as early in the mission as possible. In this paper, we describe our 55 hr Early Release Science Program that will utilize all four JWST instruments to extend the characterization of planetary-mass companions to ∼15 μm as well as image a circumstellar disk in the mid-infrared with unprecedented sensitivity. Our program will also assess the performance of the observatory in the key modes expected to be commonly used for exoplanet direct imaging and spectroscopy, optimize data calibration and processing, and generate representative data sets that will enable a broad user base to effectively plan for general observing programs in future Cycles.
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  • Pougeoise, E., et al. (author)
  • Experimental study of the lasing modes of 1.3-ÎŒm highly strained InGaAs-GaAs quantum-well oxide-confined VCSELs
  • 2009
  • In: IEEE Photonics Technology Letters. - 1041-1135 .- 1941-0174. ; 21:6, s. 377-379
  • Journal article (peer-reviewed)abstract
    • We present an experimental study of the main modes involved in the emission properties of InGaAs-GaAs quantum-well oxide-confined long wavelength vertical-cavity surface-emitting lasers. Lasing properties are dominated by the so-called "oxide modes" and by aperture modes, respectively, for small and large driving currents. We present complementary investigations of the laser emission including far-field angular distribution and spectroscopic near-field optical microscopy to a better understanding of the nature of the "oxide modes."
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  • Bialesova, L, et al. (author)
  • Epigenetic Regulation of PLIN 1 in Obese Women and its Relation to Lipolysis
  • 2017
  • In: Scientific reports. - : Springer Science and Business Media LLC. - 2045-2322. ; 7:1, s. 10152-
  • Journal article (peer-reviewed)abstract
    • Increased adipocyte lipolysis links obesity to insulin resistance. The lipid droplet coating-protein Perilipin participates in regulation of lipolysis and is implicated in obesity. In the present study we investigate epigenetic regulation of the PLIN1 gene by correlating PLIN1 CpG methylation to gene expression and lipolysis, and functionally evaluating PLIN1 promoter methylation. PLIN1 CpG methylation in adipocytes and gene expression in white adipose tissue (WAT) was quantified in two cohorts by array. Basal lipolysis in WAT explants and adipocytes was quantified by measuring glycerol release. CpG-methylation of the PLIN1 promoter in adipocytes from obese women was higher as compared to never-obese women. PLIN1 promoter methylation was inversely correlated with PLIN1 mRNA expression and the lipolytic activity. Human mesenchymal stem cells (hMSCs) differentiated in vitro into adipocytes and harboring methylated PLIN1 promoter displayed decreased reporter gene activity as compared to hMSCs harboring unmethylated promoter. Treatment of hMSCs differentiated in vitro into adipocytes with a DNA methyltransferase inhibitor increased levels of PLIN1 mRNA and protein. In conclusion, the PLIN1 gene is epigenetically regulated and promoter methylation is inversely correlated with basal lipolysis in women suggesting that epigenetic regulation of PLIN1 is important for increased adipocyte lipolysis in insulin resistance states.
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  • Bonavita, M., et al. (author)
  • New binaries from the SHINE survey
  • 2022
  • In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 663
  • Journal article (peer-reviewed)abstract
    • We present the multiple stellar systems observed within the SpHere INfrared survey for Exoplanet (SHINE). SHINE searched for sub-stellar companions to young stars using high contrast imaging. Although stars with known stellar companions within the SPHERE field of view (< 5.5 arcsec) were removed from the original target list, we detected additional stellar companions to 78 of the 463 SHINE targets observed so far. Twenty-seven per cent of the systems have three or more components. Given the heterogeneity of the sample in terms of observing conditions and strategy, tailored routines were used for data reduction and analysis, some of which were specifically designed for these datasets. We then combined SPHERE data with literature and archival data, TESS light curves, and Gaia parallaxes and proper motions for an accurate characterisation of the systems. Combining all data, we were able to constrain the orbits of 25 systems. We carefully assessed the completeness of our sample for separations between 50–500 mas (corresponding to periods of a few years to a few decades), taking into account the initial selection biases and recovering part of the systems excluded from the original list due to their multiplicity. This allowed us to compare the binary frequency for our sample with previous studies and highlight interesting trends in the mass ratio and period distribution. We also found that, when such an estimate was possible, the values of the masses derived from dynamical arguments were in good agreement with the model predictions. Stellar and orbital spins appear fairly well aligned for the 12 stars that have enough data, which favours a disk fragmentation origin. Our results highlight the importance of combining different techniques when tackling complex problems such as the formation of binaries and show how large samples can be useful for more than one purpose.
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  • Result 1-25 of 81
Type of publication
journal article (45)
doctoral thesis (30)
conference paper (6)
Type of content
peer-reviewed (47)
other academic/artistic (34)
Author/Editor
Petrus, P (24)
Ryden, M (16)
Arner, P (13)
Mejhert, N (8)
Gao, H. (7)
Janson, Markus (7)
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Kvanta, A (7)
Douagi, I (6)
Dahlman, I (6)
Kumar, P. (5)
Andre, H (5)
Aronsson, M (5)
Chauvin, G. (5)
Sassone-Corsi, P (4)
Feldt, M. (4)
Lardner, E (4)
Mesa, D. (4)
Gratton, R. (4)
Langlois, M. (4)
Ménard, F. (4)
Desidera, S. (4)
Schmidt, T. (3)
Meyer, M. (3)
Fernandez-Pello, Ser ... (3)
Bex, Axel (3)
Ljungberg, Börje, Pr ... (3)
Dabestani, Saeed (3)
Marconi, Lorenzo (3)
Volpe, Alessandro (3)
Capitanio, Umberto (3)
Beisland, Christian (3)
Järvinen, Petrus (3)
Stewart, Grant D. (3)
Nisen, Harry (3)
Meijer, Richard P. (3)
Klatte, Tobias (3)
Henning, T. (3)
Backdahl, J (3)
Laurencikiene, J (3)
Nahalkova, Jarmila (3)
Berggren, Jesper (3)
Hammar, Mattias (3)
Falk, A (3)
le Coroller, H (3)
Kulyte, A (3)
Cantalloube, F. (3)
Desgrange, C. (3)
Keppler, M. (3)
Ramos, J. (3)
Bonavita, M. (3)
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University
Uppsala University (34)
Karolinska Institutet (33)
Stockholm University (7)
Lund University (6)
Umeå University (4)
Royal Institute of Technology (3)
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Swedish University of Agricultural Sciences (1)
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Language
English (51)
Latin (30)
Research subject (UKÄ/SCB)
Humanities (25)
Natural sciences (13)
Medical and Health Sciences (5)
Engineering and Technology (2)

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