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An unknown confraternal document of the Třeboň monastery (1416) from the Klosterneuburg archive
No full textThe author publicizes an unpublished confraternal document by the provost and convent of Canons Regular of St. Augustine in Třeboň dated the 3rd February 1416 addressed to St. Dorothy's Monastery in Vienna. The document is kept in an archive of the Klosterneuburg Monastery, where the preserved remains of the St. Dorothy's Monastery's archive are deposited. The document by the Třeboň monastery dated 1416 does not have any special characteristics in comparison with the other confraternal documents written in the Roudnice circle of convents of Canons Regular of St. Augustine; it shows textual similarity to most of the other documents.The author publicizes an unpublished confraternal document by the provost and convent of Canons Regular of St. Augustine in Třeboň dated the 3rd February 1416 addressed to St. Dorothy's Monastery in Vienna. The document is kept in an archive of the Klosterneuburg Monastery, where the preserved remains of the St. Dorothy's Monastery's archive are deposited. The document by the Třeboň monastery dated 1416 does not have any special characteristics in comparison with the other confraternal documents written in the Roudnice circle of convents of Canons Regular of St. Augustine; it shows textual similarity to most of the other documents
1416. Annales Remenses
No full text1416. Annales Remenses. In: Molinier Auguste. Les Sources de l'histoire de France - Des origines aux guerres d'Italie (1494). II. Époque féodale, les Capétiens jusqu'en 1180. Paris : A. Picard et fils, 1902. p. 98
TOI-1416: A system with a super-Earth planet with a 1.07d period
Get PDFTOI 1416 (BD+42 2504, HIP 70705) is a V=10 late G or early K-type dwarf star
with transits detected by TESS. Radial velocities verify the presence of the
transiting planet TOI-1416 b, with a period of 1.07d, a mass of and a radius of , implying a slightly sub-Earth
density of g cm. The RV data also further indicate a tentative
planet c with a period of 27.4 or 29.5 days, whose nature cannot be verified
due to strong suspicions about contamination by a signal related to the Moon's
synodic period of 29.53 days. The near-USP (Ultra Short Period) planet TOI-1416
b is a typical representative of a short-period and hot ( 1570
K) super-Earth like planet. A planet model of an interior of molten magma
containing a significant fraction of dissolved water provides a plausible
explanation for its composition, and its atmosphere could be suitable for
transmission spectroscopy with JWST. The position of TOI-1416 b within the
radius-period distribution corroborates that USPs with periods of less than one
day do not form any special group of planets. Rather, this implies that USPs
belong to a continuous distribution of super-Earth like planets with periods
ranging from the shortest known ones up to ~ 30 days, whose period-radius
distribution is delimitated against larger radii by the Neptune desert and by
the period-radius valley that separates super-Earths from sub-Neptune planets.
In the abundance of small-short periodic planets against period, a plateau
between periods of 0.6 to 1.4 days has however become notable that is
compatible with the low-eccentricity formation channel. For the Neptune desert,
its lower limits required a revision due to the increasing population of short
period planets and new limits are provided. These limits are also given in
terms of the planets' insolation and effective temperatures.Comment: 31 pages, 31 figures, 8 tables, accepted for publication in A&
Demographical characteristics for the participants (N = 1416).
No full textDemographical characteristics for the participants (N = 1416).</p
Going Beyond Counting First Authors in Author Co-citation Analysis
Get PDFThe present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
An unknown confraternal document of the Třeboň monastery (1416) from the Klosterneuburg archive
No full textThe author publicizes an unpublished confraternal document by the provost and convent of Canons Regular of St. Augustine in Třeboň dated the 3rd February 1416 addressed to St. Dorothy\u27s Monastery in Vienna. The document is kept in an archive of the Klosterneuburg Monastery, where the preserved remains of the St. Dorothy\u27s Monastery\u27s archive are deposited. The document by the Třeboň monastery dated 1416 does not have any special characteristics in comparison with the other confraternal documents written in the Roudnice circle of convents of Canons Regular of St. Augustine; it shows textual similarity to most of the other documents
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