A molecular line scan in the Hubble Deep field north

R. Decarli, F. Walter, C. Carilli, D. Riechers, P. Cox, R. Neri, M. Aravena, E. Bell, F. Bertoldi, D. Colombo, E. Da Cunha, E. Daddi, M. Dickinson, D. Downes, R. Ellis, L. Lentati, R. Maiolino, K. M. Menten, H. W. Rix, M. SargentDaniel P Stark, B. Weiner, A. Weiss

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Abstract

We present a molecular line scan in the Hubble Deep Field North (HDF-N) that covers the entire 3 mm window (79-115 GHz) using the IRAM Plateau de Bure Interferometer. Our CO redshift coverage spans z ≲ 0.45, 1 ≲ z ≲ 1.9 and all z ≳ 2. We reach a CO detection limit that is deep enough to detect essentially all z > 1 CO lines reported in the literature so far. We have developed and applied different line-searching algorithms, resulting in the discovery of 17 line candidates. We estimate that the rate of false positive line detections is 2/17. We identify optical/NIR counterparts from the deep ancillary database of the HDF-N for seven of these candidates and investigate their available spectral energy distributions. Two secure CO detections in our scan are identified with star-forming galaxies at z = 1.784 and at z = 2.047. These galaxies have colors consistent with the "BzK" color selection and they show relatively bright CO emission compared with galaxies of similar dust continuum luminosity. We also detect two spectral lines in the submillimeter galaxy HDF 850.1 at z = 5.183. We consider an additional nine line candidates as high quality. Our observations also provide a deep 3 mm continuum map (1σ noise level = 8.6 μJy beam-1). Via a stacking approach, we find that optical/MIR bright galaxies contribute only to <50% of the star formation rate density at 1 < z < 3, unless high dust temperatures are invoked. The present study represents a first, fundamental step toward an unbiased census of molecular gas in "normal" galaxies at high-z, a crucial goal of extragalactic astronomy in the ALMA era.

Original languageEnglish (US)
Article number78
JournalAstrophysical Journal
Volume782
Issue number2
DOIs
StatePublished - Feb 20 2014

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galaxies
dust
astronomy
interferometer
stacking
census
plateau
continuums
color
molecular gases
star formation rate
spectral energy distribution
gas
line spectra
energy
detection
plateaus
interferometers
temperature
luminosity

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Decarli, R., Walter, F., Carilli, C., Riechers, D., Cox, P., Neri, R., ... Weiss, A. (2014). A molecular line scan in the Hubble Deep field north. Astrophysical Journal, 782(2), [78]. https://doi.org/10.1088/0004-637X/782/2/78

A molecular line scan in the Hubble Deep field north. / Decarli, R.; Walter, F.; Carilli, C.; Riechers, D.; Cox, P.; Neri, R.; Aravena, M.; Bell, E.; Bertoldi, F.; Colombo, D.; Da Cunha, E.; Daddi, E.; Dickinson, M.; Downes, D.; Ellis, R.; Lentati, L.; Maiolino, R.; Menten, K. M.; Rix, H. W.; Sargent, M.; Stark, Daniel P; Weiner, B.; Weiss, A.

In: Astrophysical Journal, Vol. 782, No. 2, 78, 20.02.2014.

Research output: Contribution to journalArticle

Decarli, R, Walter, F, Carilli, C, Riechers, D, Cox, P, Neri, R, Aravena, M, Bell, E, Bertoldi, F, Colombo, D, Da Cunha, E, Daddi, E, Dickinson, M, Downes, D, Ellis, R, Lentati, L, Maiolino, R, Menten, KM, Rix, HW, Sargent, M, Stark, DP, Weiner, B & Weiss, A 2014, 'A molecular line scan in the Hubble Deep field north', Astrophysical Journal, vol. 782, no. 2, 78. https://doi.org/10.1088/0004-637X/782/2/78
Decarli R, Walter F, Carilli C, Riechers D, Cox P, Neri R et al. A molecular line scan in the Hubble Deep field north. Astrophysical Journal. 2014 Feb 20;782(2). 78. https://doi.org/10.1088/0004-637X/782/2/78
Decarli, R. ; Walter, F. ; Carilli, C. ; Riechers, D. ; Cox, P. ; Neri, R. ; Aravena, M. ; Bell, E. ; Bertoldi, F. ; Colombo, D. ; Da Cunha, E. ; Daddi, E. ; Dickinson, M. ; Downes, D. ; Ellis, R. ; Lentati, L. ; Maiolino, R. ; Menten, K. M. ; Rix, H. W. ; Sargent, M. ; Stark, Daniel P ; Weiner, B. ; Weiss, A. / A molecular line scan in the Hubble Deep field north. In: Astrophysical Journal. 2014 ; Vol. 782, No. 2.
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