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Items where Author, Editor or other role is "Little, L.T."

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Number of items: 10.

D

Davies, S.R., Little, L.T. (1998) Low noise SIS receiver performance using Pb alloy tunnel junctions. IEE Proceedings - Microwaves Antennas and Propagation, 145 (5). pp. 375-378. ISSN 1350-2417. E-ISSN 1359-706X. (doi:10.1049/ip-map:19982251) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:17682)

Davies, Steven R. and Ellison, Brian N. and Little, L.T. and Matheson, David N. (1995) 800- to 900-GHz SIS receiver for molecular line astronomy. In: Afsar, Mohammed N., ed. Millimeter and Submillimeter Waves II. Proceedings of SPIE . SPIE, pp. 174-177. ISBN 0-8194-1917-6. (doi:10.1117/12.224233) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:19809)

Davies, S.R, Cunningham, C.T., Little, L.T., Matheson, David N. (1992) A 210-280 Ghz Sis Heterodyne Receiver for the Maxwell,James,Clerk Telescope .1. Design and Performance. International Journal of Infrared and Millimeter Waves, 13 (5). pp. 647-658. ISSN 0195-9271. (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:22543)

G

Gibb, A.G., Little, L.T. (1995) HH24-26 - Structure, Dynmics and Chemistry. Astrophysics and Space Science, 224 . pp. 467-468. ISSN 0004-640X. (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:19552)

H

Heaton, B.D., Little, L.T., Yamashita, T., Davies, S.R., Cunningham, C.T., Monteiro, T.S. (1993) The structure of g34.3+0.2 deduced from multitransition molecular line observations of HCO+. Astronomy and Astrophysics, 278 (1). pp. 238-246. ISSN 0004-6361. (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:22135)

L

Little, L.T., Kelly, M.L., Habing, R.J., Millar, T.J. (1995) A study of carbon-monoxide and neutral carbon in the s106 molecular core. Monthly Notices of the Royal Astronomical Society, 277 (1). pp. 307-318. ISSN 0035-8711. (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:19354)

Little, L.T., Gibb, A.G., Heaton, B.D., Ellison, Brian N., Claude, S.M.X. (1994) The CI/CO ratio in the molecular cloud G-34.3+0.2. Monthly Notices of the Royal Astronomical Society, 271 (3). pp. 649-661. ISSN 0035-8711. (doi:10.1093/mnras/271.3.649) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:19862)

Little, L.T., Davies, S.R (1994) A simple multiple beam lo coupler for sis heterodyne arrays. International Journal of Infrared and Millimeter Waves, 15 (6). pp. 935-942. ISSN 0195-9271. (doi:10.1007/bf02096127) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:19861)

Little, L.T. (1994) Interstellar molecular disks around young stars. Quarterly Journal of the Royal Astronomical Society, 35 (1). pp. 11-42. ISSN 0035-8738. (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:19860)

T

Tame, Keith and Price, Mark C. and Little, L.T. (1998) Design and fabrication of a 800-900 GHz Pb-alloy SIS mixing device incorporating an on-substrate tuning element. In: Phillips, Thomas G., ed. Advanced Technology MMW, Radio, and Terahertz Telescopes. Proceedings of SPIE . SPIE, Bellingham, Washington, pp. 63-74. ISBN 0-8194-2804-3. (doi:10.1117/12.317394) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:17186)

This list was generated on Wed Dec 25 19:28:13 2024 GMT.