scholarly journals Critical Analysis of Tess Transit Photometric Data: Improved Physical Properties for Five Exoplanets

2021 ◽  
Vol 162 (5) ◽  
pp. 221
Author(s):  
Suman Saha ◽  
Sujan Sengupta
2015 ◽  
Vol 48 (4) ◽  
pp. 1290-1298 ◽  
Author(s):  
Massimo Nespolo

A critical analysis of some basic notions often overlooked in crystallographic education is presented to correct some common oversights occurring both in the literature and in textbooks. The crystal forms (face forms), defined in terms of their geometric eigensymmetry, are 47 in number, not 48 as often found in the literature. The split of the dihedron into dome and sphenoid calls for the consideration of the physical properties of the faces building a form; in that case, however, the same criterion should be used for all forms. By taking the handedness of the faces as representative of the physical properties of the faces, the occurrence of 130 crystallographic face forms (97 affine face forms and 33 enantiomorphic pairs) is demonstrated. Next, the correct use of non-coprime Miller indices when a centred unit cell is adopted is shown, and the inconsistent multiplication of Miller indices in the Bravais–Friedel–Donnay–Harker law is pointed out. A geometric derivation of the reflection conditions is reviewed. Finally, the inconsistent presentation of metric restrictions imposed by the structural symmetry is pointed out and corrected.


2015 ◽  
Vol 666 ◽  
pp. 1-16 ◽  
Author(s):  
Anna Laura Pisello ◽  
Federica Rosso

In this chapter a critical analysis about natural materials to enhance energy performance and thermal comfort in indoor and outdoor spaces is dealt with. In particular, thermal insulation and passive cooling application in buildings are analyzed. The physical properties permitting to achieve these benefits are presented, as well as the method and the international standards to measure them. Benefits deriving from these materials’ employment as insulation layers or buildings envelope in general of, or in the case of urban paving, are described and then the single materials are illustrated.Experimental and numerical data, as reported in the bibliography, support the dissertation with examples from the most recent research contributions.


2008 ◽  
Vol 491 (3) ◽  
pp. 713-730 ◽  
Author(s):  
C. J. Walcher ◽  
F. Lamareille ◽  
D. Vergani ◽  
S. Arnouts ◽  
V. Buat ◽  
...  

2020 ◽  
Author(s):  
Josef Hanus ◽  
Ondrej Pejcha ◽  
Ben Shappee

<p>The All-Sky Automated Survey for Supernovae (ASAS-SN) currently<br />operates 24 small-aperture telescopes distributed around the globe to<br />automatically survey the entire visible sky every night down to about<br />g~18 mag. Between 2013 and 2018, the survey used a V filter with<br />limiting magnitude V~17. Although primarily hunting for supernovae and<br />other transients, asteroids are common intruders in the ASAS-SN's<br />images. Here we present efforts to analyze the sparsely sampled V-band<br />photometry extracted from the ASAS-SN images for >10,000 asteroids<br />that get brighter than V~17 mag. The data span years 2013-2018 and<br />sample up to 7 consequent apparitions for each asteroid. We provide<span class="im"><br />details about the photometry extraction and calibration, photometry<br />accuracy, and various statistics such as the typical number of data<br />points per asteroid as a function of the brightness. Finally, we<br /></span> analyze the photometric data with the lightcurve inversion method and<br />derive rotation periods, spin axis directions, and shapes for a sample<span class="im"><br />of studied asteroids. We discuss the typical amount of data sufficient<br />for a successful shape model determination. We compare derived<br />physical properties with those available in the literature to<br /></span> illustrate the reliability of the ASAS-SN photometry.</p>


2021 ◽  
Vol 503 (2) ◽  
pp. 1599-1614
Author(s):  
Michael Poon ◽  
J J Zanazzi ◽  
Wei Zhu

ABSTRACT KH 15D is a system that consists of a young, eccentric binary, and a circumbinary disc that obscures the binary as the disc precesses. We develop a self-consistent model that provides a reasonable fit to the photometric variability that was observed in the KH 15D system over the past 60 yr. Our model suggests that the circumbinary disc has an inner edge rin ≲ 1 au, an outer edge rout ∼ a few au, and that the disc is misaligned relative to the stellar binary by ∼5–16°, with the inner edge more inclined than the outer edge. The difference between the inclinations (warp) and longitude of ascending nodes (twist) at the inner and outer edges of the disc are of order ∼10 and ∼15°, respectively. We also provide constraints on other properties of the disc, such as the precession period and surface density profile. Our work demonstrates the power of photometric data in constraining the physical properties of planet-forming circumbinary discs.


2019 ◽  
Vol 15 (S341) ◽  
pp. 129-133
Author(s):  
M. Boquien ◽  
D. Burgarella ◽  
Y. Roehlly ◽  
V. Buat ◽  
L. Ciesla ◽  
...  

AbstractPanchromatic modeling is one of the most powerful tools at our disposal to measure reliably the physical properties of galaxies across cosmic times. We present here an entirely new implementation in python of one such tool: CIGALE. Developed along three main design principles: simplicity, modularity, and efficiency, it has proven to be a versatile code that in addition to estimating the physical properties of galaxies (or regions within galaxies), can generate arbitrary sets of theoretical models or be used as a library to build other tools. Among its defining features, it is a truly panchromatic code ranging from the far-ultraviolet to the radio that takes into account numerous physical components (including active nuclei or synchrotron emission), that can fit non-photometric data, handle upper limits, determine photometric redshifts, and even build mock catalogs.


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