A. Site Development for Large Telescope Support Facilities

1966 ◽  
Vol 27 ◽  
pp. 193-200

I call then first for comments about site development for large telescopes. Byron Hill has been for a long time the superintendent of the Palomar Mountain Station of the Mt Wilson and Palomar Observatories, and I think he is peculiarly fitted to tell us about the construction of the initial mountain facilities, and transport, support shop, and so on.

1966 ◽  
Vol 27 ◽  
pp. 193-210
Author(s):  
A. E. Whitford

I call then first for comments about site development for large telescopes. Byron Hill has been for a long time the superintendent of the Palomar Mountain Station of the Mt Wilson and Palomar Observatories, and I think he is peculiarly fitted to tell us about the construction of the initial mountain facilities, and transport, support shop, and so on.


The strategy of heart tissue engineering is simple enough: first remove all the cells from a organ then take the protein scaffold left behind and repopulate it with stem cells immunologically matched to the patient in need. While various suc- cessful methods for decellularization have been developed, and the feasibility of using decellularized whole hearts and extracellular matrix to support cells has been demonstrated, the reality of creating whole hearts for transplantation and of clinical application of decellularized extracellular matrix-based scaffolds will require much more research. For example, further investigations into how lineage-restricted progenitors repopulate the decellularized heart and differentiate in a site-specific manner into different populations of the native heart would be essential. The scaffold heart does not have to be human. Pig hearts carries all the essential components of the extracellular matrix. Through trial and error, scaling up the concentration, timing and pressure of the detergents, researchers have refined the decellularization process on hundreds of hearts and other organs, but this is only the first step. Further, the framework must be populated with human cells. Most researchers in the field use a mixture of two or more cell types, such as endothelial precursor cells to line blood vessels and muscle progenitors to seed the walls of the chambers. The final challenge is one of the hardest: vasculariza- tion, placing a engineered heart into a living animal, integration with the recipient tissue, and keeping it beating for a long time. Much remains to be done before a bioartificial heart is available for transplantation in humans.


1963 ◽  
Vol 19 ◽  
pp. 126-131
Author(s):  
C. R. Lynds

The concern has been expressed many times by Dr. Bowen and others that a significant portion of the seeing deterioration may occur in levels of the atmosphere very near the ground, within a few tenths of meters of the ground. When I refer to the quality of seeing I am refering to the image size one observes in a telescope of very large aperture and I will assume that this is equivalent to image motion as observed in telescopes of very small aperture. I will not attempt a further justification for this concern; however this is the basis for the studies we are just beginning at Kitt Peak, where we will attempt to quantitatively show whether or not there is need for concern about the very low levels of the atmosphere. So we begin with the thesis that much of the poor seeing observed at a site, the enlargement of photographic or visual images as observed through a large telescope, is due to refractive inhomogeneities in the lower levels of the atmosphere, within less than 100 m above the telescope. We presume that these inhomogeneities are of local origin and that their distribution and motion is determined primarily by site topography, wind direction and velocity. The few experiments we have made thus far at Kitt Peak have been designed to ascertain quantitatively the importance of these factors. Our approach has been to make observations of the large-aperture seeing with simultaneous observations of the thermal structure of the air accessible to us immediately above the telescope.


2013 ◽  
Vol 59 (No. 1) ◽  
pp. 1-7 ◽  
Author(s):  
S. Chauchard ◽  
F. Guibal ◽  
C. Carcaillet

Traditional land use has shaped the Mediterranean region for a long time and has resulted in present-day complex landscapes. The land abandonment dating from the 19<sup>th</sup> century at a site located in the southwestern Alps (France) makes it possible to analyse how present-day forest stands inherit from past land uses. Tree composition and tree age structure were analysed in three stands resulting from different former land uses, i.e. ancient coppice, formerly grazed area and formerly tilled area. The ancient coppice contains the densest tree cover and is dominated by Fagus sylvatica, whereas the formerly ploughed and&nbsp; grazed areas are less dense, both dominated by Pinus sylvestris. Forest stand in the ancient coppice is older than in the formerly grazed area, and forest stand is the youngest in the formerly ploughed area. These stand differences are largely explained by former land use and the abandonment process. Albeit strong changes result from the land abandonment, these landscapes inherit aspects of their land use during the 19<sup>th</sup>century at least and the dynamics does not match the expected pattern of soil fertility. &nbsp;


1984 ◽  
Vol 79 ◽  
pp. 845-849
Author(s):  
Syuso Isobe

AbstractA brief background and a description are given of the plan to build a large telescope of 5m to 7.5m class as the Japanese National Large Telescope.


1998 ◽  
Vol 11 (2) ◽  
pp. 689-691
Author(s):  
Kazimierz StȩpieŃ

Let me first remind you of the subject of the present Joint Discussion. It is about spectroscopy with large telescopes. As I have never done any spectroscopic research of my own and I have never observed with a very large telescope, I am certainly the right person to summarize the most recent results in this area.


2016 ◽  
Author(s):  
David M McCandlish ◽  
Premal Shah ◽  
Joshua B Plotkin

Recent studies of protein evolution contend that the longer an amino acid substitution is present at a site, the less likely it is to revert to the amino acid previously occupying that site. Here we study this phenomenon of decreasing reversion rates rigorously, and in a much more general context. We show that, under weak mutation and for arbitrary fitness landscapes, reversion rates decrease with time for any site that is involved in at least one epistatic interaction. Specifically, we prove that, at stationarity, the hazard function of the distribution of waiting times until reversion is strictly decreasing for any such site. Thus, in the presence of epistasis, the longer a particular character has been absent from a site, the less likely the site will revert to its prior state. We also explore several examples of this general result, which share a common pattern whereby the probability of having reverted increases rapidly at short times to some substantial value before becoming almost flat after a few substitutions at other sites. This pattern indicates a characteristic tendency for reversion to occur either almost immediately after the initial substitution or only after a very long time.


Author(s):  
Nick Worden

Most people are familiar with crowdfunding sites such as Kickstarter and GoFundMe—sites that allow users to part with their money in exchange for products or donate their capital to organizations they believe in. However, these sites have one trait in common: they do not offer contributors equity or a promise for future profits. For a long time, selling equity meant complying with the costly requirements of federal securities laws, which was cost-prohibitive for many small businesses; it was illegal for businesses to offer equity over a site in the way businesses on Kickstarter offered products. The Jumpstart Our Business Startups (JOBS) Act changed that. Small businesses, initially precluded from raising capital through the promise of equity, could do so now. However, the passage of the JOBS Act came with a number of requirements for businesses trying to sell equity via crowdfunding. In particular, these businesses could not offer their equity through just any Internet site. They had to do so through a registered intermediary—a gatekeeper to the equity crowdfunding scene. These intermediaries came in two types: broker-dealers (a familiar party in securities law) and a new statutorily created entity called a “funding portal.” Funding portals have many requirements imposed on them, but unlike broker-dealers, they are not required to be licensed to act as an intermediary. The absence of a licensing requirement for funding portals is problematic. The first litigated case involving a funding portal, Department of Enforcement v. DreamFunded Marketplace, LLC, presented that the lack of a licensing requirement threatens the twin purposes of the JOBS Act: capital formation and investor protection.


1963 ◽  
Vol 19 ◽  
pp. 253-256 ◽  
Author(s):  
A. R. Hogg

In 1957 the Joint Observatory of Yale and Columbia Universities commenced a series of site surveys in Australia under the direction of Dr. I. Epstein. While astronomers at Mount Stromlo Observatory were greatly interested in this activity, it was not until 1958 that Mount Stromlo actively commenced site testing. Tests were initiated in the first instance with a desire to find a not-too-distant location suitable for a field station where observing conditions would be better than those at Mount Stromlo, and later with the idea of finding a site anywhere in Australia which would satisfy the needs of a large telescope.


1984 ◽  
Vol 79 ◽  
pp. 675-678
Author(s):  
J. Lequeux

Interstellar matter is certainly one of the fields where a very large telescope (VLT) will prove to be most fruitful. This includes (somewhat paradoxically, but this will be explained later) the study of extended emissions. I will now examine in turn the different domains of interest for a VLT.I. Neutral diffuse matterOptical and near IR observations will mainly contribute to this domain through high-resolution spectroscopy of interstellar absorption lines in the spectra of stars. These lines are resonant lines of atoms (NaI, KI, etc.) or ions (CaII, TiII, etc.) as well as of some molecules (CH+, CH, CN, CS+, C2 in the near IR). Clearly this kind of study is always photon - limited; a VLT will collect more photons than present telescopes, thus increase the possibilities considerably.


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