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The formation of planetary systems with SPICA
DOI: 10.1017/pasa.2021.31 Bibcode: 2021PASA...38...55K

Waters, L. B. F. M.; Kamp, I.; Wolf, S. +37 more

In this era of spatially resolved observations of planet-forming disks with Atacama Large Millimeter Array (ALMA) and large ground-based telescopes such as the Very Large Telescope (VLT), Keck, and Subaru, we still lack statistically relevant information on the quantity and composition of the material that is building the planets, such as the tota…

2021 Publications of the Astronomical Society of Australia
Herschel 13
Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the cosmic noon with a SPICA-like mission
DOI: 10.1017/pasa.2021.13 Bibcode: 2021PASA...38...21S

Bisigello, Laura; Kohno, Kotaro; Alonso-Herrero, Almudena +31 more

We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to demonstrate how deep spectrophotometric surveys covering large cosmological volumes over extended fields (1–$15\, \rm{deg^2}$) with a mid-IR imaging spectrometer (17–$36\, \rm{\rm{\upmu m}}$) in conjunction with deep$70\, \rm{\rm{\upmu m}}$photometr…

2021 Publications of the Astronomical Society of Australia
Herschel 8
The nature and likely redshift of GLEAM J0917-0012
DOI: 10.1017/pasa.2021.35 Bibcode: 2021PASA...38...49D

Lehnert, Matthew D.; Stern, Daniel; De Breuck, Carlos +10 more

We previously reported a putative detection of a radio galaxy at $z=10.15$ , selected from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey. The redshift of this source, GLEAM J0917-0012, was based on three weakly detected molecular emission lines observed with the Atacama Large Millimetre Array (ALMA). In order to c…

2021 Publications of the Astronomical Society of Australia
Herschel 7
The role of SPICA-like missions and the Origins Space Telescope in the quest for heavily obscured AGN and synergies with Athena
DOI: 10.1017/pasa.2021.26 Bibcode: 2021PASA...38...33B

Pozzi, F.; Rodighiero, G.; Feltre, A. +21 more

In the black hole (BH)-galaxy co-evolution framework, most of the star formation (SF) and the BH accretion are expected to take place in highly obscured conditions. The large amount of gas and dust absorbs most of the UV-to-soft-X radiation and re-emits it at longer wavelengths, mostly in the IR. Thus, obscured active galactic nuclei (AGN) are ver…

2021 Publications of the Astronomical Society of Australia
Herschel 7
Simulating infrared spectro-photometric surveys with a SPRITZ
DOI: 10.1017/pasa.2021.57 Bibcode: 2021PASA...38...64B

Pozzi, F.; Rodighiero, G.; Schaerer, D. +19 more

Mid- and far-infrared (IR) photometric and spectroscopic observations are fundamental to a full understanding of the dust-obscured Universe and the evolution of both star formation and black hole accretion in galaxies. In this work, using the specifications of the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) as a baseline, we in…

2021 Publications of the Astronomical Society of Australia
Herschel 3