THE SECOND-GENERATION z (REDSHIFT) AND EARLY UNIVERSE SPECTROMETER. I. FIRST-LIGHT OBSERVATION OF A HIGHLY LENSED LOCAL-ULIRG ANALOG AT HIGH- z

• Published in: The Astrophysical journal 2014-01, Vol.780 (2), p.1-8
• Main Authors: FERKINHOFF, CARL, Brisbin, Drew, Parshley, Stephen, Nikola, Thomas, Stacey, Gordon J, Schoenwald, Justin, Higdon, James L, Higdon, Sarah J U, Verma, Aprajita, Riechers, Dominik
• Format: Article
• Language: English
• Subjects: Arrays; ASTROPHYSICS; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; BOLOMETERS; DENSITY; DETECTION; DISSOCIATION; EMISSION; FAR ULTRAVIOLET RADIATION; Focal plane; GALAXIES; Gratings (spectra); GRAVITATIONAL LENSES; HERA STORAGE RING; LUMINOSITY; MULTIPARTICLE SPECTROMETERS; PARTICLE IDENTIFICATION; PERTURBED ANGULAR CORRELATION; RED SHIFT; Spectrometers; SPECTROSCOPY; TELESCOPES; UNIVERSE; VISIBLE RADIATION
• ISSN: 0004-637X; 1538-4357
• DOI: 10.1088/0004-637X/780/2/142

We recently commissioned our new spectrometer, the second-generation z(Redshift) and Early Universe Spectrometer (ZEUS-2) on the Atacama Pathfinder Experiment telescope. ZEUS-2 is a submillimeter grating spectrometer optimized for detecting the faint and broad lines from distant galaxies that are redshifted into the telluric windows from 200 to 850 mu m. It uses a focal plane array of transition-edge sensed bolometers, the first use of these arrays for asttophysical spectroscopy. ZEUS-2 promises to be an important tool for studying galaxies in the years to come because of its synergy with Atacama Large Millimeter Array and its capabilities in the short submillimeter windows that are unique in the post-Herschel era. Here, we report on our first detection of the [C sub(II)] 158 mu m line with ZEUS-2. We detect the line at z ~ 1.8 from H-ATLAS J091043.1-000322 with a line flux of (6.44 + or - 0.42) x 10 super(-18) W m super(-2). Combined with its far-IR luminosity and a new Herschel-PACS detection of the [C sub(II)] 63 mu m line, we model the line emission as coming from a photo-dissociation region with far-ultraviolet radiation field, G ~ 2 x 10 super(4) G sub(0), gas density, n ~ 1 x 10 super(3) cm super(-3) and size between ~ 0.4 and 1 kpc. On the basis of this model, we conclude that H-ATLAS J091043.1-000322 is a high-redshift analog of a local ultra-luminous IR galaxy; i.e., it is likely the site of a compact starburst caused by a major merger. Further identification of these merging systems is important for constraining galaxy formation and evolution models.