High-Resolution Millimeter Imaging of Submillimeter Galaxies

By L. Tacconi, R. Neri, S. Chapman, R. Genzel, I. Smail, R. Ivison, F. Bertoldi, A. Blain, P. Cox, T. Greve and 1 more. 2005

409 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/e3d09c62ae891a39ad866941fe4a402dda206a51

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In Astronomy and Astrophysics

1. P. Hopkins
2. L. Hernquist
3. R. Dav'e
4. R. Somerville
5. D. M. Alexander
6. A. Dekel
7. D. Narayanan
8. Thomas J. Cox

In Nuclear and High Energy Physics

1. P. Hopkins
2. L. Hernquist
3. D. M. Alexander
4. R. Ivison
5. I. Smail
6. C. Carilli
7. E. Quataert
8. S. Chapman

Citations in the corpus

• FAST MOLECULAR OUTFLOWS IN LUMINOUS GALAXY MERGERS: EVIDENCE FOR QUASAR FEEDBACK FROM HERSCHEL (2013, methodology): “%) previously derived in z ∼ 2 – 3.4 sub-mm galaxies (Tacconi et al. 2006).”
• GRAVITATIONAL LENS MODELS BASED ON SUBMILLIMETER ARRAY IMAGING OF HERSCHEL-SELECTED STRONGLY LENSED SUB-MILLIMETER GALAXIES AT z > 1.5 (2013, background): “…based primarily on radio observations (Chapman et al. 2004; Muxlow et al. 2005; Biggs & Ivison 2008; Casey et al. 2009), but also includes a handful of with mm size measurements (Tacconi et al. 2006, 2010; Daddi et al. 2010) and the assumption that the radio and far-IR sizes are correlated.”
• The LABOCA survey of the Extended Chandra Deep Field-South: clustering of submillimetre galaxies (2011, background): “…to the potential nonisotropic orientation of the QSO hosts on the sky and the lack of high-resolution velocity fields necessary to solve for this (Coppin et al. 2008), as well as the general difficulties in modelling CO kinematics (e.g. Tacconi et al. 2006; Bothwell et al. 2010; Engel et al. 2010).”
• A MASSIVE MOLECULAR GAS RESERVOIR IN THE z = 5.3 SUBMILLIMETER GALAXY AzTEC-3 (2010, result): “This is comparable to the values found for z&2 SMGs (typically 2×109M⊙ kpc −2; Tacconi et al. 2006, 2008), and about half of the peak gas density of the z=6.42 quasar J1148+5251 (3.5×109M⊙ kpc −2; Riechers et al. 2009).”
• EXTRAGALACTIC MILLIMETER-WAVE SOURCES IN SOUTH POLE TELESCOPE SURVEY DATA: SOURCE COUNTS, CATALOG, AND STATISTICS FOR AN 87 SQUARE-DEGREE FIELD (2009, background): “…et al. 2005; Chapman et al. 2005; Kovács et al. 2006; Pope et al. 2006); (2) they are forming stars prodigiously at ∼1000 M yr−1 (Chapman et al. 2005; Tacconi et al. 2006); (3) their abundance appears to peak at z ∼ 2.5 (Pope et al. 2005; Chapman et al. 2005; Aretxaga et al. 2007; Chapin et al.…”
• THE STELLAR MASS CONTENT OF SUBMILLIMETER-SELECTED GALAXIES (2010, methodology): “Moreover, high-resolution millimeter observations by Tacconi et al. (2006, 2008) and Bothwell et al. (2010) suggest that the CO-emitting region (R ∼ 1 − 2kpc) in SMGs is frequently smaller than the overall stellar mass and star formation distribution (Chapman et al. 2004; Biggs & Ivison 2008;…”
• Evidence for a Population of High-Redshift Submillimeter Galaxies from Interferometric Imaging (2007, background): “However, only a fraction of these redshifts have been confirmed via CO (Greve et al. 2005; Tacconi et al. 2006) or mid–infrared (Lutz et al. 2005; Menéndez-Delmestre et al. 2007; Valiante et al. 2007) spectroscopy.”
• A Herschel view of the far-infrared properties of submillimetre galaxies (2012, background): “This considration is perhaps questionable because in high-redshift starforming galaxies, the diameter of the region forming stars span a wide range of values from 1 to 10 kpc (Chapman et al. 2004; Muxlow et al. 2005; Tacconi et al. 2006, 2008; Biggs & Ivison 2008; Casey et al. 2009; Iono et al. 2009”
• Dusty Star Forming Galaxies at High Redshift (2014, background): “At higher redshifts, the best measurements of DSFG timescales come from 850 µm-selected SMGs with CO measurements (Neri et al., 2003; Greve et al., 2005; Tacconi et al., 2006, 2008; Coppin et al., 2008b; Bothwell et al., 2010; Casey et al., 2011a; Bothwell et al., 2013a).”
• THE FIRST POSITIVE DETECTION OF MOLECULAR GAS IN A GRB HOST GALAXY (2009, background): “Emission-line studies of CO and other molecules, meanwhile, lack sufficient spatial resolution to resolve the gas beyond the local universe (e.g., Tacconi et al. 2006).”
• LSD: Lyman-break galaxies Stellar populations and Dynamics – I. Mass, metallicity and gas at z∼ 3.1 (2009, positive): “The corresponding gas densities range between 300 and 2000 M pc−2, similar to the values derived for LBGs and ULIRGs by Coppin et al. (2007) and Tacconi et al. (2006).”
• COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS (2014, methodology): “…in z>0.5 galaxies were restricted to luminous, gas and dust rich, outliers, such as starbursts and mergers, significantly above the main-sequence line at their respective redshifts (e.g. Greve et al. 2005, Tacconi et al. 2006, 2008, Riechers 2013, Carilli & Walter 2013, Bothwell et al. 2013).”
• High-redshift clumpy discs and bulges in cosmological simulations (2009, methodology): “…estimates for typical high-redshift SFGs, both the indirect estimates based on the Kennicutt–Schmidt relation (Erb et al. 2006; Genzel et al. 2006) and the direct estimates based on CO observations (Daddi et al. 2004; Greve et al. 2005; Tacconi et al. 2006, 2008; Daddi et al. 2008, 2009).”
• PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions (2017, methodology): “19 CO 2-1, 3-2 or 4-3 detections of above main-sequence submillimeter galaxies (SMGs) between z=1.2 and 3.4, obtained with the IRAM PdBI by Greve et al. (2005), Tacconi et al. (2006, 2008) and Bothwell et al. (2013).”
• Cool Gas in High-Redshift Galaxies (2013, methodology): “…(Frayer et al. 1998, Frayer et al. 1999 using OVRO) and extensive campaigns, in particular done at the PdBI (Neri et al. 2003, Greve et al. 2005, Tacconi et al. 2006, 2008, Engel et al. 2010, Bothwell et al. 2010, 2013) have characterized the molecular interstellar medium in exquisite detail.”
• REGULARITY UNDERLYING COMPLEXITY: A REDSHIFT-INDEPENDENT DESCRIPTION OF THE CONTINUOUS VARIATION OF GALAXY-SCALE MOLECULAR GAS PROPERTIES IN THE MASS-STAR FORMATION RATE PLANE (2013, positive): “The episodic and merger-related nature of ULIRGs at low redshift is well-accepted (e.g., Sanders & Mirabel 1996; and references therein) but is harder to prove for SBs in the distant universe (e.g., Tacconi et al. 2006, Daddi et al. 2009, Ivison et al. 2013).”
• Star Formation in the Hosts of High-z QSOs: Evidence from Spitzer PAH Detections (2008, background): “…occurs at luminosities similar to the upper end of the luminosity range spanned by the submm galaxy population, a limit that is often related to the star formation rate in a maximal starburst that is converting much of its gas into stars over just a few dynamical times (e.g. Tacconi et al. 2006).”
• From Rings to Bulges: Evidence for Rapid Secular Galaxy Evolution at z ~ 2 from Integral Field Spectroscopy in the SINS Survey (2008, background): “On the high end, the calibration is by z 0 ultraluminous infrared galaxies (ULIRGs; Kennicutt 1998) and z 1Y3 SMGs (Tacconi et al. 2006, 2008).”
• HerMES: CANDIDATE GRAVITATIONALLY LENSED GALAXIES AND LENSING STATISTICS AT SUBMILLIMETER WAVELENGTHS (2012, background): “The star-formation regions in SMGs are thought to be a few to 10 kpc in extent (e.g. Tacconi et al. 2006; Younger et al. 2008; Hailey-Dunsheath et al. 2010; Ferkinhoff et al. 2011), although some may be as small as ∼ 100 pc (Swinbank et al. 2010).”