scholarly journals Clinicopathologic and Dermoscopic Features of Acquired Perforating Dermatosis: A Case Report

2019 ◽  
Vol 53 (4) ◽  
Author(s):  
Jay-V James G. Barit ◽  
Felix Paolo J. Lizarondo ◽  
Eileen Liesl A. Cubillan

Acquired perforating dermatosis represents one of the perforating skin disorders showing transepidermal elimination of dermal contents. Dermoscopy showing concentric zones of a central keratotic plug, white-gray structureless area and peripheral brown pigmentation may aid in diagnosis and in sample selection for biopsy.

Lupus ◽  
2020 ◽  
pp. 096120332096570
Author(s):  
Juliana P Ocanha-Xavier ◽  
Camila O Cola-Senra ◽  
Jose Candido C Xavier-Junior

Reticular erythematous mucinosis (REM) was first described 50 years ago, but only around 100 case reports in English have been published. Its relation with other inflammatory skin disorders is still being debated. We report a case of REM, including the clinical and histopathological findings. Also, a systematic review of 94 English-language reported cases is provided. The described criteria for clinical and histopathological diagnosis are highlighted in order to REM can be confidently diagnosed.


Author(s):  
Yohei Koizumi ◽  
Masayuki Kuzuhara ◽  
Masashi Omiya ◽  
Teruyuki Hirano ◽  
John Wisniewski ◽  
...  

Abstract We present the optical spectra of 338 nearby M dwarfs, and compute their spectral types, effective temperatures (Teff), and radii. Our spectra were obtained using several optical spectrometers with spectral resolutions that range from 1200 to 10000. As many as 97% of the observed M-type dwarfs have a spectral type of M3–M6, with a typical error of 0.4 subtype, among which the spectral types M4–M5 are the most common. We infer the Teff of our sample by fitting our spectra with theoretical spectra from the PHOENIX model. Our inferred Teff is calibrated with the optical spectra of M dwarfs whose Teff have been well determined with the calibrations that are supported by previous interferometric observations. Our fitting procedures utilize the VO absorption band (7320–7570 Å) and the optical region (5000–8000 Å), yielding typical errors of 128 K (VO band) and 85 K (optical region). We also determine the radii of our sample from their spectral energy distributions. We find most of our sample stars have radii of <0.6 R⊙, with the average error being 3%. Our catalog enables efficient sample selection for exoplanet surveys around nearby M-type dwarfs.


1997 ◽  
Vol 49 (4) ◽  
pp. 567-585 ◽  
Author(s):  
Yulong Cui ◽  
Kenneth L. Verosub ◽  
Andrew P. Roberts ◽  
Mary Kovacheva

Author(s):  
Mauro Bibancos ◽  
Rodrigo Markus Vaz ◽  
Paulo Ferreira Mega ◽  
Edson Borges Jr. ◽  
Mariana Ribeiro ◽  
...  

Radiocarbon ◽  
2019 ◽  
Vol 61 (4) ◽  
pp. 1009-1027 ◽  
Author(s):  
Zoë A Thomas ◽  
Chris S M Turney ◽  
Alan Hogg ◽  
Alan N Williams ◽  
Chris J Fogwill

ABSTRACTPrecise radiocarbon (14C) dating of sedimentary sequences is important for developing robust chronologies of environmental change, but sampling of suitable components can be challenging in highly dynamic landscapes. Here we investigate radiocarbon determinations of different peat size fractions from six peat sites, representing a range of geomorphological contexts on the South Atlantic subantarctic islands of the Falklands and South Georgia. To investigate the most suitable fraction for dating, 112 measurements were obtained from three components within selected horizons: a fine fraction <0.2 mm, a coarse fraction >0.2 mm, and bulk material. We find site selection is critical, with locations surrounded by high-ground and/or relatively slowly accumulating sites more susceptible to the translocation of older carbon. Importantly, in locations with reduced potential for redeposition of material, our results show that there is no significant or systematic difference between ages derived from bulk material, fine or coarse (plant macrofossil) material, providing confidence in the resulting age model. Crucially, in areas comprising complex terrain with extreme relief, we recommend dating macrofossils or bulk carbon rather than a fine fraction, or employing comprehensive dating of multiple sedimentary fractions to determine the most reliable fraction(s) for developing a robust chronological framework.


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