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1 as molecular biology, particle physics, and astronomy.
2 of the universe is a long-standing quest in astronomy.
3 om communications to radar, broadcasting and astronomy.
4 ay have substantial effects in observational astronomy.
5 ranging from biology to materials science to astronomy.
6 in the interstellar medium with far-infrared astronomy.
7 s, has brought about a revolution in optical astronomy.
8 the Kuiper belt-has opened a new frontier in astronomy.
9 alysis to biomedical diagnostics, vision and astronomy.
13 ser-induced guide star has long been used in astronomy, and more recently in microscopy to compensate
14 it went on to change forever many fields of astronomy, and to capture the public's imagination with
17 , thus represent important targets for radio astronomy because they offer the possibilities of confir
18 a crucial role in the development of stellar astronomy because, as a consequence of the stars having
20 ide variety of applications (particularly in astronomy), but are difficult to integrate into large ar
21 pproaches, commonly used in epidemiology and astronomy, can be applied in the context of genetic sequ
22 of cosmic structure; summarize its impact on astronomy, cosmology, and physics; and look ahead by out
24 nning in the early 1960s, the field of X-ray astronomy has exploded, experiencing a ten-billion-fold
26 s of artificial light at night on scientific astronomy, human health, ecological processes and aesthe
27 arriers of the diffuse interstellar bands in astronomy, indicating their persistence in interstellar
30 is a ubiquitous challenge, crucial in radio astronomy, medical imaging, navigation, and classical an
32 tion by stimulated emission of radiation; in astronomy mega-masers are masers in galaxies that are >/
33 V for single 6-keV photons, and future X-ray astronomy missions anticipate the need for 1,000-pixel a
36 h a capability that links the National Radio Astronomy Observatory's Very Large Array radio interfero
37 e been used widely to correct aberrations in astronomy, offer a solution here but also present new ch
38 Exoplanet detections have revolutionized astronomy, offering new insights into solar system archi
40 was thought until recently to be useless to astronomy, primarily because the opacity of the interste
41 itive phenomena is of critical importance in astronomy, spectroscopy, biology, and remote sensing.
43 ion observations are often possible in radio astronomy, they are usually limited to quite narrow fiel
44 and so deeply embedded into the language of astronomy through the Hubble diagram, the Hubble constan
46 t as well as the chop-nod method in infrared astronomy, to characterize nanomaterials without the inf
48 ng optical devices, originally developed for astronomy, whose optical properties can be changed in re
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