Gerald E. Kron

University of Stuttgart

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Katherine C. Gordon

United States Naval Academy

A. V. Hewitt

Total (France)

H. D. Ables

United States Naval Observatory

Uwe Rau

Forschungszentrum Jülich

J.H. Werner

University of Stuttgart

I. I. Papiashvili

United States Naval Observatory

S. C. B. Gascoigne

Australian National University

Merle F. Walker

University of California, Santa Cruz

Gabriele Nelles

Stuttgart University of Applied Sciences

Jim B. Breckinridge

California Institute of Technology

Cooperative Institutions

Kitt Peak National Observatory

Max Planck Society

Association of Universities For Research In Astronomy

U.S. National Science Foundation

California Institute of Technology

United States Naval Observatory

University of Stuttgart

Purple Mountain Observatory

University of California, Berkeley

Max Planck Institute for Polymer Research

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An interesting asymmetry in the distribution of reddening material in the Galaxy.

PASP (1973)

Gerald E. Kron H. H. Guetter

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Bulletin Number 513 - The new electric drive for the 36-inch refractor.

Lick Observatory Bulletins (1943)

Gerald E. Kron

Refracting telescope

10.5479/ads/bib/1943licob.19.155k

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Integrated photometry and light distribution of 21 Southern-Hemisphere galactic globular clusters

Publications of the Astronomical Society of the Pacific (1986)

Gerald E. Kron Keith C. Gordon

Total magnitudes and brightness distributions were determined by computer analysis of multiaperture observations of 21 galactic globular clusters made in 1960-1961 at the Mount Stromlo Observatory. The results were compared with the Kron and Mayall (1960) data. In addition, total magnitudes of seven NGC clusters determined by several other investigators using multiaperture observations were compared in order to estimate the accuracy obtainable in these determinations. Comparison of the present (B-V) results on the 21 clusters with the (V-I) measures of the Kron and Mayall PVI system showed no significant differences in colors measured through different apertures on the same night, although night-to-night differences were considerable.

10.1086/131791

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Progress in the Development of the Lick-Stromlo Electronic Camera

Advances in electronics and electron physics (1966)

Gerald E. Kron I. I. Papiashvili

Photocathode

Professional video camera

Nuclear emulsion

10.1016/s0065-2539(08)61641-8

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New techniques in photometry.

Robotics and Applications (1980)

Gerald E. Kron

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"Distortions" in the Light-Variation of the Spectroscopic Binary HD 22124

Publications of the Astronomical Society of the Pacific (1955)

Ivan L. Thomsen Helmut A. Abt Gerald E. Kron

Variation (astronomy)

10.1086/126857

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The Practical Use of Photocells at Maximum Performance

Publications of the Astronomical Society of the Pacific (1948)

Gerald E. Kron

Search Bar to Enter New Query quick field: Author First Author Abstract Year Fulltext Select a field or operator abstract abstract only acknowledgements affiliation arXiv category author count author bibcode bibliographic group bib abbrev, e.g. ApJ body of article data archive collection citation count doctype doi entdate first author fulltext identifier inst keyword object orcid page property publication full name date published title volume year citations() pos() references() reviews() similar() topn() trending() useful() single wildcard: ? wildcard: * exact match: = All Search Terms Your search returned 0 results Your search returned 0 results

Photoresistor

10.1086/126055

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The Coefficient of Limb Darkening for YZ (21) Cassiopeiae in Red Light.

The Astrophysical Journal (1942)

Gerald E. Kron

view Abstract Citations (21) References Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Coefficient of Limb Darkening for YZ (21) Cassiopeiae in Red Light. Kron, Gerald E. Abstract The eclipsing variable YZ Cassiopeiae has been observed with a red-sensitive caesium-cell photo- electric photometer, resulting in a light-curve having the necessary degree of precision for the calculation of darkening coefficients. Descriptions of the methods used for observing and for analysis are given. The color class of the secondary component was determined as F5, in agreement with earlier work. The darkening coefficient of the A3 component is 0.33, that of the F5 component is 0.5 at a mean wave length of X6700. INTRODUCTIO Publication: The Astrophysical Journal Pub Date: September 1942 DOI: 10.1086/144445 Bibcode: 1942ApJ....96..173K full text sources ADS |

Limb darkening

Radial velocity

10.1086/144445

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