Author(s):  
D. Scott Birney ◽  
Guillermo Gonzalez ◽  
David Oesper

2021 ◽  
Vol 11 (6) ◽  
pp. 2671
Author(s):  
Gerhard Ulbricht ◽  
Mario De De Lucia ◽  
Eoin Baldwin

In recent years Microwave Kinetic Inductance Detectors (MKIDs) have emerged as one of the most promising novel low temperature detector technologies. Their unrivaled scalability makes them very attractive for many modern applications and scientific instruments. In this paper we intend to give an overview of how and where MKIDs are currently being used or are suggested to be used in the future. MKID based projects are ongoing or proposed for observational astronomy, particle physics, material science and THz imaging, and the goal of this review is to provide an easily usable and thorough list of possible starting points for more in-depth literature research on the many areas profiting from kinetic inductance detectors.


Author(s):  
M. K. Tsvetkov ◽  
K. Y. Stavrev ◽  
K. P. Tsvetkova ◽  
E. H. Semkov ◽  
A. S. Mutafov ◽  
...  

1996 ◽  
Vol 169 ◽  
pp. 533-549
Author(s):  
Charles J. Lada

We now stand at the threshold of the 21st century having witnessed perhaps the greatest era of astronomical discovery in the history of mankind. During the twentieth century the subject of astronomy was revolutionized and completely transformed by technology and physics. Advances in technology that produced radio astronomy, infrared astronomy, UV, X and γ ray astronomy, large telescopes on the ground, in balloons, aircraft and space coupled with advances in nuclear, atomic and high energy physics forever changed the way in which the universe is viewed. Indeed, it is altogether likely that future historians of science will consider the twentieth century as the Golden Age of observational astronomy. As a measure of how far we have come in the last 100 years, recall that at the turn of this century the nature of spiral nebulae and of the Milky Way itself as an island universe were not yet revealed. The expansion of the universe and the microwave background were not yet discovered and exotic objects such as quasars, pulsars, gamma-ray bursters and black holes were not even envisioned by the most imaginative authors of science fiction. The interstellar medium, with its giant molecular clouds, magnetic fields and obscuring dust was unknown. Not even the nature of stars, these most fundamental objects of the astronomical universe, was understood.


2001 ◽  
Vol 24 (3) ◽  
pp. 110-116
Author(s):  
Christopher J. Corbally

AbstractTwo seemingly incongruous components have come together about every two years: the serene terraces of the Pope’s summer residence at Castel Gandolfo, and the noisy exuberance of 25 beginning-level graduate students. Add in a small faculty of first-rate professors and a resourceful local support team, and one has the ingredients for the month-long Vatican Observatory Summer Schools. The eighth School takes place in the summer of 2001, and its goals are the same as when the series started in 1986: to encourage and motivate a mix of young people from industrialized and developing countries who are at critical moments of their research careers, and to make a small, but significant contribution to the progress of developing countries by exposing some of their most talented young citizens to people involved in high quality research in astrophysics. This account outlines the nature of the Schools, their follow-up, and something of how the spirit of sharing of personal and institutional resources is achieved.


2019 ◽  
Vol 57 (1) ◽  
pp. 79-112 ◽  
Author(s):  
Susanna L. Widicus Weaver

The recent advancements in far-infrared (far-IR) astronomy brought about by the Herschel, SOFIA, and ALMA observatories have led to technological advancements in millimeterwave and submillimeterwave laboratory spectroscopy that is used to support molecular observations. This review gives an overview of rotational spectroscopy and its relationship with observational astronomy, as well as an overview of laboratory spectroscopic techniques focusing on both historical approaches and new advancements. Additional topics discussed include production and detection techniques for unstable molecular species of astrochemical interest, data analysis approaches that address spectral complexity and line confusion, and the current state of and limitations to spectral line databases. Potential areas for new developments in this field are also reviewed. To advance the field, the following challenges must be addressed: ▪ Data acquisition speed, spectral sensitivity, and analysis approaches for complex mixtures and broadband spectra are the greatest limitations—and hold the greatest promise for advancement—in this field of research. ▪ Full science return from far-IR observatories cannot be realized until laboratory spectroscopy catches up with the data rate for observations. ▪ New techniques building on those used in the microwave and IR regimes are required to fill the terahertz gap.


1972 ◽  
Vol 2 (2) ◽  
pp. 70-71
Author(s):  
J. R. Prescott

Observational astronomy extends, in terms of energy in the electromagnetic spectrum, from below 10-8eV to above 108eV. Studies of cosmic rays extend this range to the neighbourhood of 1019eV (about a Joule) and the aspects of high energy astrophysics discussed in the present paper are those concerned with cosmic rays of energy upwards of about 1015eV.


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