NOEMA complementarity with NIKA2

Abstract

IRAM operates two observatories - the 30-meter Telescope on Pico Veleta in Spain and NOEMA, an interferometer of ten 15-meter antennas on Plateau de Bure in France. Both observatories allow to observe at millimeter wavelengths. Here, we aim at discussing the complementary between continuum observations with NOEMA and NIKA2 at the 30m and their role at the cutting edge of research in astronomy. In particular, we will review possible synergies of continuum studies from nearby star forming regions to high redshift galaxies at cosmological distances.

6 pages, 3 figures, to appear in the proceedings of the international conference entitled mm Universe @ NIKA2, Grenoble (France), June 2019, EPJ Web of conferences

References in corpus (8)

• Cosmic Star Formation History
• The SCUBA Legacy Catalogue: Continuum Objects Detected by SCUBA
• The NIKA2 large field-of-view millimeter continuum camera for the 30-m IRAM telescope
• Lambda = 3 mm line survey of nearby active galaxies
• Probing changes of dust properties along a chain of solar-type prestellar and protostellar cores in Taurus with NIKA
• CO, H2O, H2O+ line and dust emission in a z = 3.63 strongly lensed starburst merger at sub-kiloparsec scales
• The Sunyaev-Zel'dovich Effect at Five Arc-seconds: RXJ1347.5-1145 Imaged by ALMA
• A centrally concentrated sub-solar mass starless core in the Taurus L1495 filamentary complex