| 摘要 | 第4-6页 |
| Abstract | 第6-7页 |
| 1 Introduction | 第14-22页 |
| 1.1 Dust emission in the COSMOS field | 第15-17页 |
| 1.2 Dusty star forming galaxies at z>4 | 第17-20页 |
| 1.3 Massive galaxy cluster at high redshift | 第20-22页 |
| 2 "Super-deblended" Far-IR to (sub)mm photometry in the full COSMOS field | 第22-50页 |
| 2.1 Initial catalogs and multi-wavelength data sets | 第22-24页 |
| 2.1.1 Initial catalogs and spectroscopic redshifts | 第22-23页 |
| 2.1.2 Mid-infrared and radio images | 第23页 |
| 2.1.3 Far-infrared and (sub-)millimeter images | 第23-24页 |
| 2.2 Setting up the prior catalogs | 第24-36页 |
| 2.2.1 K_s(+radio) priors for 24 μm and radio images | 第26-28页 |
| 2.2.2 Photometry at MIPS 24 μm on K_s selected priors | 第28-29页 |
| 2.2.3 Photometry at VLA 1.4 and 3 GHz on K_s-selected priors | 第29-33页 |
| 2.2.4 The effective depth of our 24 μm+radio prior catalog | 第33页 |
| 2.2.5 Completing the prior catalog with stellar mass-selected galaxies | 第33-36页 |
| 2.3 "Super-deblended" photometry in the FIR/(sub)mm images | 第36-50页 |
| 2.3.1 SED fitting algorithm | 第39-41页 |
| 2.3.2 Differences in deblending work from L18 | 第41-43页 |
| 2.3.3 SED fitting algorithm and parameters | 第43页 |
| 2.3.4 Faint sources subtraction in COSMOS | 第43-45页 |
| 2.3.5 Flux bias and uncertainties calibration via improved Monte Carlosimulation | 第45-48页 |
| 2.3.6 Selecting additional sources in the residual images | 第48-50页 |
| 3 The COSMOS "Super-deblended" photometry catalog | 第50-64页 |
| 3.1 General properties of the "Super-deblended" photometry catalog | 第50-55页 |
| 3.2 Comparison to catalogs from the literature | 第55-64页 |
| 3.2.1 PEP catalogs | 第56-57页 |
| 3.2.2 SPIRE XID~+ catalogs | 第57-58页 |
| 3.2.3 SCUBA2 catalogs | 第58-59页 |
| 3.2.4 Comparison to ALMA archival photometry | 第59-64页 |
| 4 Exploring high redshift galaxies using "super-deblended" photometry and mmlines | 第64-84页 |
| 4.1 High redshift dusty star forming galaxies candidates | 第64-77页 |
| 4.1.1 Candidates selection at z>4 | 第67-68页 |
| 4.1.2 Redshift-dust temperature degeneracy | 第68-70页 |
| 4.1.3 An interesting case of possible lensing | 第70页 |
| 4.1.4 AGN components at z>4 | 第70-73页 |
| 4.1.5 Counterparts for candidates found in residual images | 第73页 |
| 4.1.6 General sample and final considerations on redshift estimates | 第73-77页 |
| 4.2 Redshift confirmation via ALMA/NOEMA line scans | 第77-84页 |
| 5 Radio selection of high redshift galaxy cluster | 第84-98页 |
| 5.1 Radio continuum emission from galaxies in a z=2.5 cluster | 第86-88页 |
| 5.2 Radio selection of the z=2.5 W16 cluster | 第88-90页 |
| 5.3 Two candidates of galaxy clusters at z～3 | 第90-92页 |
| 5.4 Discussion | 第92-98页 |
| 6 Summary | 第98-100页 |
| References | 第100-106页 |
| AppendixA MIPS 24μm calibration factor | 第106-108页 |
| AppendixB "Super-deblending" Images Products and Simulation Correction Analyses | 第108-124页 |
| B.1 Photometry Image Products | 第108-112页 |
| B.2 Simulation Correction Analyses | 第112-124页 |
| AppendixC High redshift candidates | 第124-134页 |
| Shuowen JlN—Curriculum Vitae | 第134-136页 |
| 致谢 | 第136-138页 |
