91̽»¨

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding 91̽»¨
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
91̽»¨
Black Hole

Lensing of space time around a black hole. At 91̽»¨ we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Jamie Leech

Senior Researcher

Sub department

  • Astrophysics

Research groups

  • The Square Kilometre Array (SKA)
  • Experimental radio cosmology
  • C-BASS
jamie.leech@physics.ox.ac.uk
Telephone: 01865 (2)73299
Denys Wilkinson Building, room 764
  • About
  • Publications

Astronomical receiver modelling using scattering matrices

Monthly Notices of the Royal Astronomical Society 91̽»¨ University Press (OUP) 446:2 (2015) 1252-1267

Authors:

OG King, ME Jones, C Copley, RJ Davis, JP Leahy, J Leech, SJC Muchovej, TJ Pearson, AC Taylor

Instrumentation for single-dish observations with The Greenland Telescope

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 9153 (2014) 91531v-91531v-11

Authors:

Paul K Grimes, K Asada, R Blundell, R Burgos, H-H Chang, MT Chen, D Goldie, C Groppi, CC Han, PTP Ho, YD Huang, M Inoue, D Kubo, P Koch, J Leech, E de Lera Acedo, P Martin-Cocher, H Nishioka, M Nakamura, S Matsushita, SN Paine, N Patel, P Raffin, W Snow, TK Sridharan, R Srinivasan, CN Thomas, E Tong, M-J Wang, C Wheeler, S Withington, G Yassin, L-Z Zeng

WARM MOLECULAR GAS IN LUMINOUS INFRARED GALAXIES**Based on Herschel observations. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

The Astrophysical Journal Letters American Astronomical Society 787:2 (2014) l23

Authors:

N Lu, Y Zhao, CK Xu, Y Gao, L Armus, JM Mazzarella, KG Isaak, AO Petric, V Charmandaris, T Díaz-Santos, AS Evans, J Howell, P Appleton, H Inami, K Iwasawa, J Leech, S Lord, DB Sanders, B Schulz, J Surace, PP van der Werf

The C-Band All-Sky Survey (C-BASS): design and implementation of the northern receiver

\mnras 438 (2014) 2426-2439

Authors:

OG King, ME Jones, EJ Blackhurst, C Copley, RJ Davis, C Dickinson, CM Holler, MO Irfan, JJ John, JP Leahy, J Leech, SJC Muchovej, TJ Pearson, MA Stevenson, AC Taylor

The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey - IX. 12CO J = 3→2 observations of NGC 2976 and NGC 3351

Monthly Notices of the Royal Astronomical Society 436:1 (2013) 921-933

Authors:

BK Tan, J Leech, D Rigopoulou, BE Warren, CD Wilson, D Attewell, M Azimlu, GJ Bendo, HM Butner, E Brinks, P Chanial, DL Clements, V Heesen, F Israel, JH Knapen, HE Matthews, AMJ Mortier, S Mühle, JR Sánchez-Gallego, RPJ Tilanus, A Usero, P Van der Werf, M Zhu

Abstract:

We present 12CO J = 3→2 maps of NGC 2976 and NGC 3351 obtained with the James Clerk Maxwell Telescope (JCMT), both early targets of the JCMT Nearby Galaxy Legacy Survey (NGLS). We combine the present observations with 12CO J = 1→0 data and find that the computed 12CO J = 3→2 to 12CO J = 1→0 line ratio (R31) agrees with values measured in other NGLS field galaxies. We compute the MH2 value and find that it is robust against the value of R31 used. Using HI data from The HI Nearby Galaxy Survey, we find a tight correlation between the surface density of H2 and star formation rate density for NGC 3351 when 12CO J = 3→2 data are used. Finally, we compare the 12CO J = 3→2 intensity with the polycyclic aromatic hydrocarbon (PAH) 8 μm surface brightness and find a good correlation in the high surface brightness regions. We extend this study to include all 25 Spitzer Infrared Nearby Galaxies Survey galaxies within the NGLS sample and find a tight correlation at large spatial scales. We suggest that both PAH 8 μm and 12CO J = 3→2 are likely to originate in regions of active star formation. © 2013 The Authors Published by 91̽»¨ University Press on behalf of the Royal Astronomical Society.

Pagination

  • First page First
  • Previous page Prev
  • Page 1
  • Page 2
  • Current page 3
  • Page 4
  • Page 5
  • Page 6
  • Page 7
  • Page 8
  • Page 9
  • …
  • Next page Next
  • Last page Last

Footer 91̽»¨

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

91̽»¨,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

© 91̽»¨ - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics