Signal-to-Noise Ratios for Possible Stellar Occultations by Pluto

A. S. Bosh; J. L. Elliott; Sarah E. Kruse; R. L. Baron; E. W. Dunham; L. M. French

doi:10.1016/0019-1035(86)90090-4

Signal-to-Noise Ratios for Possible Stellar Occultations by Pluto

A. S. Bosh, J. L. Elliott, Sarah E. Kruse, R. L. Baron, E. W. Dunham, L. M. French

Research output: Contribution to journal › Article › peer-review

Abstract

Signal-to-noise ratios and magnitudes in the Johnson BVR system are presented for mine stars that might be occulted by Pluto during the period 1985–1990. From these calculations of the signal-to-noise ratio that could be achieved with a 1-m telescope, we find that each star (if occulted) is sufficiently bright to give useful information about a possible atmosphere of Pluto.

Original language	American English
Journal	Icarus
Volume	66
DOIs	https://doi.org/10.1016/0019-1035(86)90090-4
State	Published - Jun 1 1986
Externally published	Yes

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https://doi.org/10.1016/0019-1035(86)90090-4

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@article{1746309face747f1804444edb1dd5b5e,

title = "Signal-to-Noise Ratios for Possible Stellar Occultations by Pluto",

abstract = " Signal-to-noise ratios and magnitudes in the Johnson BVR system are presented for mine stars that might be occulted by Pluto during the period 1985–1990. From these calculations of the signal-to-noise ratio that could be achieved with a 1-m telescope, we find that each star (if occulted) is sufficiently bright to give useful information about a possible atmosphere of Pluto.",

author = "Bosh, \{A. S.\} and Elliott, \{J. L.\} and Kruse, \{Sarah E.\} and Baron, \{R. L.\} and Dunham, \{E. W.\} and French, \{L. M.\}",

year = "1986",

month = jun,

day = "1",

doi = "10.1016/0019-1035(86)90090-4",

language = "American English",

volume = "66",

journal = "Icarus",

}

TY - JOUR

T1 - Signal-to-Noise Ratios for Possible Stellar Occultations by Pluto

AU - Bosh, A. S.

AU - Elliott, J. L.

AU - Kruse, Sarah E.

AU - Baron, R. L.

AU - Dunham, E. W.

AU - French, L. M.

PY - 1986/6/1

Y1 - 1986/6/1

N2 - Signal-to-noise ratios and magnitudes in the Johnson BVR system are presented for mine stars that might be occulted by Pluto during the period 1985–1990. From these calculations of the signal-to-noise ratio that could be achieved with a 1-m telescope, we find that each star (if occulted) is sufficiently bright to give useful information about a possible atmosphere of Pluto.

AB - Signal-to-noise ratios and magnitudes in the Johnson BVR system are presented for mine stars that might be occulted by Pluto during the period 1985–1990. From these calculations of the signal-to-noise ratio that could be achieved with a 1-m telescope, we find that each star (if occulted) is sufficiently bright to give useful information about a possible atmosphere of Pluto.

UR - https://digitalcommons.usf.edu/geo_facpub/948

UR - https://doi.org/10.1016/0019-1035(86)90090-4

U2 - 10.1016/0019-1035(86)90090-4

DO - 10.1016/0019-1035(86)90090-4

M3 - Article

VL - 66

JO - Icarus

JF - Icarus

ER -

Signal-to-Noise Ratios for Possible Stellar Occultations by Pluto

Abstract

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