20 results on '"J. Pforr"'
Search Results
2. The size and pervasiveness of Ly α-UV spatial offsets in star-forming galaxies at z ∼ 6
- Author
-
Tommaso Treu, Y. Khusanova, Tucker Jones, Nimish P. Hathi, Patricia Bolan, Brian C. Lemaux, K. H. Huang, Carlos Alvarez, Kasper B. Schmidt, Steve Fuller, L. Guaita, Debora Pelliccia, Laura Pentericci, E. Vanzella, O. Le Fèvre, Charlotte Mason, Victoria Strait, B. Ribeiro, Anton M. Koekemoer, R. E. Ryan, Austin Hoag, Marusa Bradac, Pratik J. Gandhi, J. Pforr, Laboratoire d'Astrophysique de Marseille (LAM), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Semi-major axis ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,medicine.disease_cause ,01 natural sciences ,techniques: photometric ,galaxies: high-redshift ,0103 physical sciences ,medicine ,Anisotropy ,Spectroscopy ,010303 astronomy & astrophysics ,Reionization ,Astrophysics::Galaxy Astrophysics ,Physics ,010308 nuclear & particles physics ,gravitational lensing: strong ,Astronomy and Astrophysics ,Astrophysics - Astrophysics of Galaxies ,Redshift ,Galaxy ,Space and Planetary Science ,[SDU]Sciences of the Universe [physics] ,reionization ,Astrophysics::Earth and Planetary Astrophysics ,galaxies: evolution ,Ultraviolet ,techniques: spectroscopic - Abstract
We study the projected spatial offset between the ultraviolet continuum and Ly$\alpha$ emission for 65 lensed and unlensed galaxies in the Epoch of Reionization ($5\leq z\leq7$), the first such study at these redshifts, in order to understand the potential for these offsets to confuse estimates of the Ly$\alpha$ properties of galaxies observed in slit spectroscopy. While we find that ~40% of galaxies in our sample show significant projected spatial offsets ($|\Delta_{Ly\alpha-UV}|$), we find a modest average offset of 0.61$\pm$0.08 kpc. A small fraction of our sample, ~10%, exhibits offsets of 2-4 kpc, sizes that are larger than the effective radii of typical galaxies at these redshifts. An internal comparison and a comparison to studies at lower redshift yielded no significant evidence of evolution of $|\Delta_{Ly\alpha-UV}|$ with redshift. In our own sample, UV-bright galaxies showed offsets a factor of three greater than their fainter counterparts, 0.89$\pm$0.18 vs. 0.27$\pm$0.05 kpc, respectively. We argue that offsets are likely not the result of merging processes, but are rather due to internal anisotropic processes resulting from stellar feedback facilitates Ly$\alpha$ fluorescence and/or backscattering from nearby or outflowing gas. The reduction in the Ly$\alpha$ flux due to offset effects for various observational setups was quantified through mock observations of simple simulations. It was found that the loss of Ly$\alpha$ photons for galaxies with average offsets is not, if corrected for, a limiting factor for all but the narrowest slit widths (, Comment: 21 pages, 7 figures, 2 tables. Updated with the accepted MNRAS version that includes minor changes to the text and two tables
- Published
- 2021
- Full Text
- View/download PDF
3. Optimization of the Winding Arrangement to Increase the Zero-Sequence Inductance of a Synchronous Machine With Multifunctional Converter Drive
- Author
-
T. Hackner, Jan Abraham Ferreira, J. Pforr, and Henk Polinder
- Subjects
Engineering ,business.industry ,Stator ,Ripple ,Electrical engineering ,Industrial and Manufacturing Engineering ,law.invention ,Inductance ,Control and Systems Engineering ,law ,Electromagnetic coil ,Boost converter ,Inverter ,Electrical and Electronic Engineering ,business ,Synchronous motor ,Voltage - Abstract
An automotive electric-power-steering synchronous machine driven from a multifunctional converter has the advantage of increased system voltage. The integration of the boost converter in the inverter and the electrical machine leads to new requirements for the machine design due to dc currents and increased high-frequency ripple currents in the motor windings. In this paper, the ripple currents of a synchronous machine with a multifunctional converter are investigated. Three winding arrangements are analyzed and compared to reduce the ripple currents together with interleaved pulsewidth modulation. This paper contains finite-element simulations of the zero-sequence flux and analyses of the ripple currents with and without low-frequency ac modulation and, hence, when operated at high and low rotational speed. The magnitude of the ripple current depends on the zero-sequence inductance. By rearranging the coils in the stator slots, the zero-sequence inductance is significantly increased. Experimental results are correlating well with theoretical predictions and demonstrate that the phase and star-point ripple currents are almost halved.
- Published
- 2012
- Full Text
- View/download PDF
4. Evolution of clustering length, large-scale bias, and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey (VUDS)
- Author
-
A. Durkalec, O. Le Fèvre, A. Pollo, S. de la Torre, P. Cassata, B. Garilli, V. Le Brun, B. C. Lemaux, D. Maccagni, L. Pentericci, L. A. M. Tasca, R. Thomas, E. Vanzella, G. Zamorani, E. Zucca, R. Amorín, S. Bardelli, L. P. Cassarà, M. Castellano, A. Cimatti, O. Cucciati, A. Fontana, M. Giavalisco, A. Grazian, N. P. Hathi, O. Ilbert, S. Paltani, B. Ribeiro, D. Schaerer, M. Scodeggio, V. Sommariva, M. Talia, L. Tresse, D. Vergani, P. Capak, S. Charlot, T. Contini, J. G. Cuby, J. Dunlop, S. Fotopoulou, A. Koekemoer, C. López-Sanjuan, Y. Mellier, J. Pforr, M. Salvato, N. Scoville, Y. Taniguchi, P. W. Wang, Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), AUTRES, INAF - Osservatorio Astronomico di Roma (OAR), Istituto Nazionale di Astrofisica (INAF), Oncology Institute of Southern Switzerland, INAF - Osservatorio Astronomico di Bologna (OABO), University of Bologna, Department of Astronomy [Amherst], University of Massachusetts [Amherst] (UMass Amherst), University of Massachusetts System (UMASS)-University of Massachusetts System (UMASS), ISDC Data Centre for Astrophysics, University of Geneva [Switzerland], INAF- Milano, INAF - Osservatorio Astrofisico di Arcetri (OAA), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), SUPA, Institute for Astronomy, University of Edinburgh, Aristotle University of Thessaloniki, Space Telescope Science Institute (STSci), Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institute of cosmology and gravitation, University of Portsmouth, Max-Planck-Institut für Extraterrestrische Physik (MPE), California Institute of Technology (CALTECH), ANR-11-IDEX-0001,Amidex,INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE(2011), European Project: 268107,EC:FP7:ERC,ERC-2010-AdG_20100224,EARLY(2011), Durkalec, A., Le Fevre, O., Pollo, A., De La Torre, S., Cassata, P., Garilli, B., Le Brun, V., Lemaux, B.C., Maccagni, D., Pentericci, L., Tasca, L.A.M., Thomas, R., Vanzella, E., Zamorani, G., Zucca, E., Amorin, R., Bardelli, S., Cassara, L.P., Castellano, M., Cimatti, A., Cucciati, O., Fontana, A., Giavalisco, M., Grazian, A., Hathi, N.P., Ilbert, O., Paltani, S., Ribeiro, B., Schaerer, D., Scodeggio, M., Sommariva, V., Talia, M., Tresse, L., Vergani, D., Capak, P., Charlot, S., Contini, T., Cuby, J.G., Dunlop, J., Fotopoulou, S., Koekemoer, A., Lopez-Sanjuan, C., Mellier, Y., Pforr, J., Salvato, M., Scoville, N., Taniguchi, Y., Wang, P.W., Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), University of Bologna/Università di Bologna, Université de Genève = University of Geneva (UNIGE), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), and Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Large-scale structure of Universe ,statistical [methods] ,Population ,Dark matter ,Cosmology: observations ,Galaxies: evolution ,Methods: statistical ,Astronomy and Astrophysics ,Space and Planetary Science ,Astrophysics ,Correlation function (astronomy) ,01 natural sciences ,Cosmology: observation ,0103 physical sciences ,Cluster analysis ,education ,010303 astronomy & astrophysics ,evolution [galaxies] ,Physics ,education.field_of_study ,010308 nuclear & particles physics ,Astronomy and Astrophysic ,observations [cosmology] ,Redshift ,Galaxy ,Amplitude ,large-scale structure of Universe ,Halo ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We investigate the evolution of galaxy clustering for galaxies in the redshift range 2.0, Comment: 19 pages, 10 figures, submitted to A&A
- Published
- 2015
- Full Text
- View/download PDF
5. Stellar masses of SDSS-III/BOSS galaxies at z \xa0 0.5 and constraints to galaxy formation models
- Author
-
C. Maraston, J. Pforr, B. M. Henriques, D. Thomas, D. Wake, J. R. Brownstein, D. Capozzi, J. Tinker, K. Bundy, R. A. Skibba, A. Beifiori, R. C. Nichol, E. Edmondson, D. P. Schneider, Y. Chen, K. L. Masters, O. Steele, A. S. Bolton, D. G. York, B. A. Weaver, T. Higgs, D. Bizyaev, H. Brewington, E. Malanushenko, V. Malanushenko, S. Snedden, D. Oravetz, K. Pan, A. Shelden, and A. Simmons
- Published
- 2013
6. Ultra Steep Spectrum Radio Sources in the Lockman Hole: SERVS Identifications and Redshift Distribution at the Faintest Radio Fluxes
- Author
-
L. Bizzocchi, J. Afonso, E. Ibar, M. Grossi, C. Simpson, S. Chapman, M. J. Jarvis, H. Rottgering, R. P. Norris, J. Dunlop, R. J. Ivison, H. Messias, J. Pforr, M. Vaccari, N. Seymour, P. Best, E. Gonz, D. Farrah, J.-S. Huang, M. Lacy, C. Marastron, L. Marchetti, J.-C. Mauduit, S. Oliver, D. Rigopoulou, S. A. Stanford, J. Surace, and G. Zeimann
- Published
- 2011
- Full Text
- View/download PDF
7. Host galaxy subtraction of TeV candidate BL Lacertae objects
- Author
-
Leo O. Takalo, Stefano Ciprini, J. Pforr, Kari Nilsson, Andrei Berdyugin, M. Pasanen, and Elina Lindfors
- Subjects
Physics ,Aperture ,Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,Subtraction ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics ,Function (mathematics) ,Radius ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Galaxy ,Space and Planetary Science ,Calibration ,Physics::Accelerator Physics ,Astrophysics::Earth and Planetary Astrophysics ,Sources of error ,Host (network) ,Astrophysics::Galaxy Astrophysics - Abstract
We have derived R-band host galaxy fluxes of 20 TeV candidate BL Lacertae objects as a function of aperture radius and FWHM. The results are given as correction tables, that list the fluxes (in mJy) of all ``contaminating'' sources (host galaxy + significant nearby objects) as a function of aperture radius and FWHM. We found that the derived fluxes depend strongly on aperture radius, but the FWHM has only a minor effect (a few percent). We also discuss the implications of our findings to optical monitoring programs and potential sources of error in our derived fluxes. During this work we have also constructed new calibration star sequences for 9 objects and present the finding charts and calibrated magnitudes., Accepted for publication in A&A, 24 pages, 6 figures, 3 minor typos corrected
- Published
- 2007
8. Zero-Voltage Switched Multi-Phase Converter utilizing nonlinear and coupled Inductors
- Author
-
J. Pforr and M. Stadler
- Subjects
Engineering ,business.industry ,Ćuk converter ,Electrical engineering ,Hardware_PERFORMANCEANDRELIABILITY ,Converters ,Inductor ,Computer Science::Other ,Power (physics) ,Electric power system ,Hardware_GENERAL ,Electromagnetic coil ,Hardware_INTEGRATEDCIRCUITS ,Electronic engineering ,Waveform ,Commutation ,business - Abstract
A novel zero voltage switched multi-phase converter for the 42V/14V automotive electrical power system has been built and tested. The efficiency of the converter was a main target and switching losses have been reduced using non-linear inductors to achieve zero voltage switching. In comparison to resonant converters with non-linear inductors, the load current is not flowing through the non-linear inductors, reducing their size, cost and power losses. The non-linear inductors act similar to auxiliary resonant commutated poles but without additional switching devices and shape the current waveforms only during commutation. The paper outlines the converter analysis, design and measurements. Experimental results obtained are in good correlation to theoretical predictions.
- Published
- 2007
- Full Text
- View/download PDF
9. Feed-forward control of non-linear inductors providing soft-switching of DC-DC-converters
- Author
-
J. Pforr and M. Stadler
- Subjects
Operating point ,Nonlinear system ,Engineering ,Control theory ,business.industry ,Boost converter ,Electronic engineering ,Feed forward ,Digital control ,Converters ,Network topology ,Inductor ,business - Abstract
A novel auxiliary circuit with a current controlled non-linear inductor has been developed to achieve soft-switching for different converter topologies. This paper outlines the operation principle of the auxiliary circuit and gives details about the control of the non-linear inductor. A model has been developed that allows the calculation of the control current dependent on the operating point of the converter. This model has been implemented into a digital controller. A prototype converter has been built and tested to verify theoretical predictions. Measurements have shown that the efficiency of the prototype converter is greatly improved by the auxiliary circuit. Experimental results are in good correlation with theoretical prediction.
- Published
- 2007
- Full Text
- View/download PDF
10. A non-sense mutation in the corneodesmosin gene in a Mexican family with hypotrichosis simplex of the scalp
- Author
-
N.O. Dávalos, J. Pforr, R. Kruse, Luis E. Figuera, R.C. Betz, Ingrid P. Dávalos, A. García‐Vargas, Verónica Judith Picos-Cárdenas, Markus M. Nöthen, and D. García‐Cruz
- Subjects
Male ,Adolescent ,Nonsense mutation ,Dermatology ,Biology ,Corneodesmosin ,Exon ,medicine ,Humans ,Child ,Gene ,Mexico ,Glycoproteins ,Genetics ,integumentary system ,Base Sequence ,Chromosome ,Alopecia ,Middle Aged ,medicine.disease ,Pedigree ,medicine.anatomical_structure ,Codon, Nonsense ,Scalp ,Mutation (genetic algorithm) ,Hypotrichosis ,Intercellular Signaling Peptides and Proteins ,Chromosomes, Human, Pair 6 ,Female - Abstract
Summary Background Hypotrichosis simplex of the scalp (HSS; MIM 146520) is a rare autosomal dominant form of non-syndromic alopecia that affects men and women equally. Up to now, only a small number of families with HSS have been reported. The affected individuals experience a diffuse progressing hair loss from childhood to adulthood that is confined to the scalp. Recently, HSS has been mapped to the short arm of chromosome 6 (6p21.3), allowing mutations in the corneodesmosin gene (CDSN) to be identified as the cause of the disorder. To date, two stop mutations have been found in three unrelated families with HSS of different ethnic origin. Objectives To describe the first HSS-family with Latin American (Mexican) background comprising 6 generations and to identify a mutation in the CDSN gene. Patients/Methods The patients were examined by a clinician and blood samples were taken. After DNA extraction, sequencing analysis of the CDSN gene and restriction enzyme analysis with PsuI were performed. Results By direct sequencing of the two exons of the CDSN gene, a nonsense mutation was identified in the index patient in exon 2, resulting in a premature stop codon (Y239X). The mutation cosegregates perfectly in the family with the disease and was not found in 300 control chromosomes using a restriction enzyme analysis with PsuI. Conclusions A nonsense mutation was identified in the first family with HSS of Latin American ethnical background. Our data provide molecular genetic evidence for a 3rd stop mutation in exon 2 of the CDSN gene being responsible for HSS. All to date known nonsense mutations responsible 3 for HSS are clustered in a region of 40 amino acids which is in accordance with a dominant negative effect conferred by aggregates of truncated CDSN proteins.
- Published
- 2005
11. A novel power factor corrected single ended resonant converter with three phase supply
- Author
-
J. Pforr and L. Hobson
- Subjects
Power supply rejection ratio ,Engineering ,Switched-mode power supply ,Buck converter ,business.industry ,AC adapter ,Electrical engineering ,Electronic engineering ,Power semiconductor device ,Power factor ,AC power ,business ,Switched-mode power supply applications - Abstract
A three-phase rectifier stage, enabling a whole class of switched mode and resonant switched mode power converters to automatically draw sinusoidal input currents from a three-phase supply, is introduced. The proposed technique offers advantages including very simple power circuits, simple control and protection, and very-high-quality input currents. The power factor correction method is described, and the analysis, design, and performance obtained from a buck-type single-ended resonant converter with three-phase supply based on this principle are outlined. Results for a 2.5 kW/40 kHz prototype converter, utilizing a single high-speed GTO as the active switching device and operating directly offline from a 415 V three-phase mains supply, are presented to verify theoretical predictions. The measured input current waveforms drawn from the three-phase supply are sinusoidal with approximately unity power factor. >
- Published
- 2003
- Full Text
- View/download PDF
12. Beam-based alignment of SRF cavities in an electron injector linac.
- Author
-
F Hug, M Arnold, T Bahlo, J Pforr, and N Pietralla
- Published
- 2018
- Full Text
- View/download PDF
13. A Subarcsecond Near-infrared View of Massive Galaxies at z > 1 with Gemini Multi-conjugate Adaptive Optics.
- Author
-
M. Lacy, K. Nyland, M. Mao, P. Jagannathan, J. Pforr, S. E. Ridgway, J. Afonso, D. Farrah, P. Guarnieri, E. Gonzales-Solares, M. J. Jarvis, C. Maraston, D. M. Nielsen, A. O. Petric, A. Sajina, J. A. Surace, and M. Vaccari
- Subjects
SUPERGIANT stars ,ADAPTIVE optics ,ASTRONOMICAL observations ,STAR formation ,ACTIVE galactic nuclei - Abstract
We present images taken using the Gemini South Adaptive Optics Imager (GSAOI) with the Gemini Multi-conjugate Adaptive Optics System (GeMS) in three 2 arcmin
2 fields in the Spitzer Extragalactic Representative Volume Survey. These GeMS/GSAOI observations are among the first ≈0.″1 resolution data in the near-infrared spanning extragalactic fields exceeding 1.′5 in size. We use these data to estimate galaxy sizes, obtaining results similar to those from studies with the Hubble Space Telescope, though we find a higher fraction of compact star-forming galaxies at z > 2. To disentangle the star-forming galaxies from active galactic nuclei (AGNs), we use multiwavelength data from surveys in the optical and infrared, including far-infrared data from Herschel, as well as new radio continuum data from the Australia Telescope Compact Array and Very Large Array. We identify ultraluminous infrared galaxies (ULIRGs) at z ∼ 1–3, which consist of a combination of pure starburst galaxies and AGN/starburst composites. The ULIRGs show signs of recent merger activity, such as highly disturbed morphologies and include a rare candidate triple-AGN. We find that AGNs tend to reside in hosts with smaller scale sizes than purely star-forming galaxies of similar infrared luminosity. Our observations demonstrate the potential for MCAO to complement the deeper galaxy surveys to be made with the James Webb Space Telescope. [ABSTRACT FROM AUTHOR]- Published
- 2018
- Full Text
- View/download PDF
14. THE HOST GALAXIES OF MICRO-JANSKY RADIO SOURCES.
- Author
-
K. M. Luchsinger, M. Lacy, K. M. Jones, J. C. Mauduit, J. Pforr, J. A. Surace, M. Vaccari, D. Farrah, E. Gonzales-Solares, M. J. Jarvis, C. Maraston, L. Marchetti, S. Oliver, J. Afonso, D. Cappozi, and A. Sajina
- Published
- 2015
- Full Text
- View/download PDF
15. Optical single-shot readout of spin qubits in silicon.
- Author
-
Gritsch A, Ulanowski A, Pforr J, and Reiserer A
- Abstract
Small registers of spin qubits in silicon can exhibit hour-long coherence times and exceeded error-correction thresholds. However, their connection to larger quantum processors is an outstanding challenge. To this end, spin qubits with optical interfaces offer key advantages: they can minimize the heat load and give access to modular quantum computing architectures that eliminate cross-talk and offer a large connectivity. Here, we implement such an efficient spin-photon interface based on erbium dopants in a nanophotonic resonator. We demonstrate optical single-shot readout of a spin in silicon whose coherence exceeds the Purcell-enhanced optical lifetime, paving the way for entangling remote spins via photon interference. As erbium dopants can emit coherent photons in the minimal-loss band of optical fibers, and tens of such qubits can be spectrally multiplexed in each resonator, the demonstrated hardware platform offers unique promise for distributed quantum information processing based on scalable, integrated silicon devices., Competing Interests: Competing interests: The authors declare no competing interests., (© 2024. The Author(s).)
- Published
- 2025
- Full Text
- View/download PDF
16. A large duplication in LIPH underlies autosomal recessive hypotrichosis simplex in four Middle Eastern families.
- Author
-
Nahum S, Pasternack SM, Pforr J, Indelman M, Wollnik B, Bergman R, Nöthen MM, König A, Khamaysi Z, Betz RC, and Sprecher E
- Subjects
- Child, Chromosome Disorders enzymology, Chromosome Disorders pathology, Chromosome Disorders physiopathology, Chromosomes, Human, Pair 3, DNA Mutational Analysis, Exons genetics, Genes, Recessive, Genetic Predisposition to Disease, Hair abnormalities, Hair growth & development, Hair pathology, Hair Follicle growth & development, Hair Follicle pathology, Humans, Hypotrichosis enzymology, Hypotrichosis pathology, Hypotrichosis physiopathology, Israel, Lipase metabolism, Microsatellite Repeats genetics, Pedigree, Polymorphism, Genetic, Turkey, Arabs, Chromosome Disorders genetics, Gene Duplication, Hair Follicle metabolism, Hypotrichosis genetics, Lipase genetics
- Abstract
Autosomal recessive hypotrichosis simplex (ARHS) manifests with paucity of hair appearing during early childhood. We assessed four affected families. We initially genotyped three of these families for a panel of microsatellite markers spanning all ARHS-associated loci and obtained data suggesting linkage to 3q27, encompassing LIPH, which had previously been shown to be associated with ARHS. Accordingly, a homozygous duplication mutation in exon 2 of this gene (c.280_369dup; p.Gly94_Lys123dup) was found to segregate with the disease in all the families. Through the identification of the first duplication mutation in the human LIPH gene, we provide further evidence supporting a role for the phospholipase signalling pathway in hair growth and differentiation.
- Published
- 2009
- Full Text
- View/download PDF
17. Loss-of-function mutations in the filaggrin gene and alopecia areata: strong risk factor for a severe course of disease in patients comorbid for atopic disease.
- Author
-
Betz RC, Pforr J, Flaquer A, Redler S, Hanneken S, Eigelshoven S, Kortüm AK, Tüting T, Lambert J, De Weert J, Hillmer AM, Schmael C, Wienker TF, Kruse R, Lutz G, Blaumeiser B, and Nöthen MM
- Subjects
- Adolescent, Adult, Aged, Aged, 80 and over, Alopecia Areata pathology, Case-Control Studies, Child, Child, Preschool, Comorbidity, Dermatitis, Atopic pathology, Disease Progression, Female, Filaggrin Proteins, Humans, Male, Middle Aged, Risk Factors, Severity of Illness Index, Alopecia Areata genetics, Dermatitis, Atopic genetics, Intermediate Filament Proteins genetics, Mutation genetics
- Abstract
Alopecia areata (AA) is a common dermatological disease, which affects nearly 2% of the general population. Association of AA with atopic disease has been repeatedly reported. Loss-of-function mutations in the filaggrin gene (FLG) may be considered as promising candidates in AA, as they have been observed to be a strong risk factor in atopic dermatitis. The FLG mutations R501X and 2282del4 were genotyped in a large sample of AA patients (n=449) and controls (n=473). Although no significant association was observed in the patient sample overall, FLG mutations were significantly associated with the presence of atopic dermatitis among AA patients. Furthermore, the presence of FLG mutations had a strong impact on the clinical course of AA in comorbid patients. For example, 19 of the 22 mutation carriers among AA patients with atopic dermatitis showed a severe form of the disease (P=0.003; odds ratio (OR)=5.47 (95% confidence interval (CI): 1.59-18.76)). In conclusion, our data suggest that when AA occurs in conjunction with FLG-associated atopic disorder, the clinical presentation of AA may be more severe.
- Published
- 2007
- Full Text
- View/download PDF
18. Identification of mutations in the human hairless gene in two new families with congenital atrichia.
- Author
-
Betz RC, Indelman M, Pforr J, Schreiner F, Bauer R, Bergman R, Lentze MJ, Nöthen MM, Cichon S, and Sprecher E
- Subjects
- Alopecia ethnology, DNA genetics, DNA Mutational Analysis, Exons genetics, Female, Humans, Infant, Iran, Jews genetics, Male, Pedigree, Saudi Arabia, Alopecia genetics, Mutation genetics, Transcription Factors genetics
- Abstract
Congenital atrichia (AUC) is a form of isolated alopecia with an autosomal recessive mode of inheritance. Patients are born with normal hair but this is shed almost completely during the first weeks or months of life and never regrows. In many families the development of papular lesions is noted as an additional phenotypic feature, which defines a related phenotype designated as atrichia with papular lesions (APL). Using positional cloning strategies and the molecular findings in hairless recessive (hr/hr) mice, an animal model for AUC, mutations in the human hairless gene (HR) have been identified as a cause of AUC and APL. To date, more than 20 different mutations of the HR gene have been reported in AUC and APL including different mutation types scattered over the entire HR gene length. In this report, we describe two families of Saudi Arabian and Jewish Iranian origin comprising a number of individuals with clinical features suggestive of AUC. We therefore hypothesized that affected members may carry mutations in the HR gene. After sequencing the complete coding region of the HR gene in the Saudi Arabian family, we identified a homozygous insertion of a G (c.2661dupG; p.Thr888DfsX38) in exon 12, resulting in a premature stop codon. In a Jewish Iranian patient, we identified a homozygous splice site mutation c.1557-1G > T in intron 4. The latter mutation has been previously reported in a compound heterozygous state. In the present report, we describe the second exonic insertion mutation in the human HR gene and the first mutation in exon 12. Our study emphasizes the importance of sequencing the complete coding sequence and exon/intron junctions in the molecular diagnostics of AUC and APL.
- Published
- 2007
- Full Text
- View/download PDF
19. Investigation of the p.Ser278Arg polymorphism of the autoimmune regulator (AIRE) gene in alopecia areata.
- Author
-
Pforr J, Blaumeiser B, Becker T, Freudenberg-Hua Y, Hanneken S, Eigelshoven S, Cuyt I, De Weert J, Lambert J, Kruse R, Nöthen MM, and Betz RC
- Subjects
- Alleles, Case-Control Studies, Gene Frequency, Genetic Variation, Humans, Severity of Illness Index, White People genetics, AIRE Protein, Alopecia Areata genetics, Polymorphism, Genetic, Transcription Factors genetics
- Abstract
A recent study has suggested that the g.961C >G (p.Ser278Arg) variant of the autoimmune regulator (AIRE) gene contributes to susceptibility to alopecia areata (AA). We attempted to replicate this finding using a case-control sample of Belgian-German origin (273 patients and 283 controls). Despite adequate power, our study results do not support a significant association of the risk allele in our AA patient sample. This remained the case when we stratified our sample according to severity and family history of disease. Our study results do not support the hypothesis that the g.961C >G (p.Ser278Arg) polymorphism of the AIRE gene is associated with an increased risk for AA.
- Published
- 2006
- Full Text
- View/download PDF
20. A non-sense mutation in the corneodesmosin gene in a Mexican family with hypotrichosis simplex of the scalp.
- Author
-
Dávalos NO, García-Vargas A, Pforr J, Dávalos IP, Picos-Cárdenas VJ, García-Cruz D, Kruse R, Figuera LE, Nöthen MM, and Betz RC
- Subjects
- Adolescent, Base Sequence, Child, Chromosomes, Human, Pair 6 genetics, Female, Humans, Intercellular Signaling Peptides and Proteins, Male, Mexico ethnology, Middle Aged, Pedigree, Alopecia genetics, Codon, Nonsense, Glycoproteins genetics
- Abstract
Background: Hypotrichosis simplex of the scalp (HSS; MIM 146520) is a rare autosomal dominant form of non-syndromic alopecia that affects men and women equally. Up to now, only a small number of families with HSS have been reported. The affected individuals experience a diffuse progressing hair loss from childhood to adulthood that is confined to the scalp. Recently, HSS has been mapped to the short arm of chromosome 6 (6p21.3), allowing mutations in the corneodesmosin gene (CDSN) to be identified as the cause of the disorder. To date, two stop mutations have been found in three unrelated families with HSS of different ethnic origin., Objectives: To describe the first HSS-family with Latin American (Mexican) background comprising 6 generations and to identify a mutation in the CDSN gene., Patients/methods: The patients were examined by a clinician and blood samples were taken. After DNA extraction, sequencing analysis of the CDSN gene and restriction enzyme analysis with PsuI were performed., Results: By direct sequencing of the two exons of the CDSN gene, a nonsense mutation was identified in the index patient in exon 2, resulting in a premature stop codon (Y239X). The mutation co-segregates perfectly in the family with the disease and was not found in 300 control chromosomes using a restriction enzyme analysis with PsuI., Conclusions: A nonsense mutation was identified in the first family with HSS of Latin American ethnical background. Our data provide molecular genetic evidence for a 3rd stop mutation in exon 2 of the CDSN gene being responsible for HSS. All to date known nonsense mutations responsible 3 for HSS are clustered in a region of 40 amino acids which is in accordance with a dominant negative effect conferred by aggregates of truncated CDSN proteins.
- Published
- 2005
- Full Text
- View/download PDF
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.