Spacewatch Astrometry and Photometry of Near-Earth Objects

Robert S. McMillan; Jeffrey A. Larsen; Terrence H. Bressi; James V. Scotti; Ronald A. Mastaler; Andrew F. Tubbiolo

doi:10.1017/S1743921315006766

Spacewatch Astrometry and Photometry of Near-Earth Objects

Robert S. McMillan
, Jeffrey A. Larsen
, Terrence H. Bressi
, James V. Scotti
, Ronald A. Mastaler
, Andrew F. Tubbiolo

Lunar and Planetary Lab

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

2 Scopus citations

Abstract

The Spacewatch Project uses four telescopes of apertures 0.9-m, 1.8-m, 2.3-m, and 4-m on Kitt Peak mountain in Arizona for followup astrometry of priority NEOs. Objects as faint as V=23 on the MPC's NEO Confirmation Page, targets of radar, potential impactors, targets of spacecraft observations or visits, and PHAs with future close approaches to Earth receive priority for astrometry.

Original language	English (US)
Pages (from-to)	317-318
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	10
DOIs	https://doi.org/10.1017/S1743921315006766
State	Published - 2016

Keywords

asteroids
astrometry
atlases
minor planets
surveys

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1017/S1743921315006766

Cite this

@article{2f52512e451240d7ab823ea75fcc03fd,

title = "Spacewatch Astrometry and Photometry of Near-Earth Objects",

abstract = "The Spacewatch Project uses four telescopes of apertures 0.9-m, 1.8-m, 2.3-m, and 4-m on Kitt Peak mountain in Arizona for followup astrometry of priority NEOs. Objects as faint as V=23 on the MPC's NEO Confirmation Page, targets of radar, potential impactors, targets of spacecraft observations or visits, and PHAs with future close approaches to Earth receive priority for astrometry.",

keywords = "asteroids, astrometry, atlases, minor planets, surveys",

author = "McMillan, \{Robert S.\} and Larsen, \{Jeffrey A.\} and Bressi, \{Terrence H.\} and Scotti, \{James V.\} and Mastaler, \{Ronald A.\} and Tubbiolo, \{Andrew F.\}",

note = "Publisher Copyright: Copyright {\textcopyright} 2016 International Astronomical Union.",

year = "2016",

doi = "10.1017/S1743921315006766",

language = "English (US)",

volume = "10",

pages = "317--318",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

}

TY - JOUR

T1 - Spacewatch Astrometry and Photometry of Near-Earth Objects

AU - McMillan, Robert S.

AU - Larsen, Jeffrey A.

AU - Bressi, Terrence H.

AU - Scotti, James V.

AU - Mastaler, Ronald A.

AU - Tubbiolo, Andrew F.

PY - 2016

Y1 - 2016

N2 - The Spacewatch Project uses four telescopes of apertures 0.9-m, 1.8-m, 2.3-m, and 4-m on Kitt Peak mountain in Arizona for followup astrometry of priority NEOs. Objects as faint as V=23 on the MPC's NEO Confirmation Page, targets of radar, potential impactors, targets of spacecraft observations or visits, and PHAs with future close approaches to Earth receive priority for astrometry.

AB - The Spacewatch Project uses four telescopes of apertures 0.9-m, 1.8-m, 2.3-m, and 4-m on Kitt Peak mountain in Arizona for followup astrometry of priority NEOs. Objects as faint as V=23 on the MPC's NEO Confirmation Page, targets of radar, potential impactors, targets of spacecraft observations or visits, and PHAs with future close approaches to Earth receive priority for astrometry.

KW - asteroids

KW - astrometry

KW - atlases

KW - minor planets

KW - surveys

UR - https://www.scopus.com/pages/publications/84959544947

UR - https://www.scopus.com/pages/publications/84959544947#tab=citedBy

U2 - 10.1017/S1743921315006766

DO - 10.1017/S1743921315006766

M3 - Article

AN - SCOPUS:84959544947

SN - 1743-9213

VL - 10

SP - 317

EP - 318

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

ER -

Spacewatch Astrometry and Photometry of Near-Earth Objects

Abstract

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this