Cardiff University | Prifysgol Caerdydd ORCA
Online Research @ Cardiff 
WelshClear Cookie - decide language by browser settings

Redshift determination and co line excitation modeling for the multiply lensed galaxy hlsw-01

Scott, K. S., Lupu, R. E., Aguirre, J. E., Auld, Robbie Richard, Aussel, H., Baker, A. J., Beelen, A., Bock, J., Bradford, C. M., Brisbin, D., Burgarella, D., Carpenter, J. M., Chanial, P., Chapman, S. C., Clements, D. L., Conley, A., Cooray, A., Cox, P., Dowell, C. D., Eales, Stephen Anthony, Farrah, D., Franceschini, A., Frayer, D. T., Gavazzi, R., Glenn, J., Griffin, Matthew Jospeh, Harris, A. I., Ibar, E., Ivison, R. J., Kamenetzky, J., Kim, S., Krips, M., Maloney, P. R., Matsuhara, H., Mortier, A. M. J., Murphy, E. J., Naylor, B. J., Neri, R., Nguyen, H. T., Oliver, S. J., Omont, A., Page, M. J., Papageorgiou, Andreas, Pearson, C. P., Pérez-Fournon, I., Pohlen, Michael, Rawlings, J. I., Raymond, Gwenifer, Riechers, D., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Scott, D., Seymour, N., Smith, A. J., Symeonidis, M., Tugwell, K. E., Vaccari, M., Vieira, J. D., Vigroux, L., Wang, L., Wright, G. and Zmuidzinas, J. 2011. Redshift determination and co line excitation modeling for the multiply lensed galaxy hlsw-01. Astrophysical Journal 733 (1) , 29. 10.1088/0004-637X/733/1/29

Full text not available from this repository.

Abstract

We report on the redshift measurement and CO line excitation of HERMES J105751.1+573027 (HLSW-01), a strongly lensed submillimeter galaxy discovered in Herschel/SPIRE observations as part of the Herschel Multi-tiered Extragalactic Survey (HerMES). HLSW-01 is an ultra-luminous galaxy with an intrinsic far-infrared luminosity of L FIR = 1.4 × 1013 L , and is lensed by a massive group of galaxies into at least four images with a total magnification of μ = 10.9 ± 0.7. With the 100 GHz instantaneous bandwidth of the Z-Spec instrument on the Caltech Submillimeter Observatory, we robustly identify a redshift of z = 2.958 ± 0.007 for this source, using the simultaneous detection of four CO emission lines (J = 7 → 6, J = 8 → 7, J = 9 → 8, and J = 10 → 9). Combining the measured line fluxes for these high-J transitions with the J = 1 → 0, J = 3 → 2, and J = 5 → 4 line fluxes measured with the Green Bank Telescope, the Combined Array for Research in Millimeter Astronomy, and the Plateau de Bure Interferometer, respectively, we model the physical properties of the molecular gas in this galaxy. We find that the full CO spectral line energy distribution is described well by warm, moderate-density gas with T kin = 86-235 K and cm–3. However, it is possible that the highest-J transitions are tracing a small fraction of very dense gas in molecular cloud cores, and two-component models that include a warm/dense molecular gas phase with T kin ~ 200 K, cm–3 are also consistent with these data. Higher signal-to-noise measurements of the J up ≥ 7 transitions with high spectral resolution, combined with high spatial resolution CO maps, are needed to improve our understanding of the gas excitation, morphology, and dynamics of this interesting high-redshift galaxy.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Uncontrolled Keywords: Galaxies: high-redshift ; Galaxies: individual (HERMES J105751.1+573027); Galaxies: starburst ; Submillimeter: galaxies
Publisher: American Astronomical Society
ISSN: 0004-637X
Last Modified: 04 Jun 2017 02:16
URI: http://orca.cf.ac.uk/id/eprint/11035

Citation Data

Cited 28 times in Google Scholar. View in Google Scholar

Cited 36 times in Scopus. View in Scopus. Powered By Scopus® Data

Cited 28 times in Web of Science. View in Web of Science.

Actions (repository staff only)

Edit Item Edit Item