4 Comparison of the ALMA and Herschel - ESO

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calibration files and to a pipeline for quick looks as well as a package for complete data reduction. Ideally the pipeline products would be publication quality images. ESO: There is a need to carry out finding surveys for extragalactic/galactic sources using single dishes such as APEX with the LABOCA bolometer camera system. For the time when both instruments are available, an efficient approach would involve a process where ESO reacts quickly to the need for follow-ups to Herschel data. For ALMA it would be useful to allocate observing time as soon as possible to measure variable sources, newly discovered sources, peculiar objects or in general to perform follow-ups of selected fields both in line and continuum that are as complete as possible. Both Organisations: The most pressing need is to coordinate large surveys that are planned in Herschel guaranteed time. There should be a series of dedicated conferences/workshops once the guaranteed time plans for Herschel are complete. These workshops should continue during the lifetime of Herschel. There may be difficulties in arranging for any coordination that involves large blocks of ALMA observing time, since the policies and organisation of ALMA Time Allocation Committees are in the discussion phase. 50
Abbreviations ACA — ALMA Compact Array AGB — asymptotic giant branch AGN — active galactic nucleus ALMA — Atacama Large Millimeter Array APEX — Atacama Pathfinder Experiment ASTRO-F — now named AKARI, a Japanese infrared satellite CDFS — Chandra Deep Field South CIRB — cosmic infrared background COB — cosmic optical background DRSP — Design Reference Science Plan ELT — Extremely large Telescope ESA — European Space Agency ESO — European Southern Observatory FIR — far infrared FP6 — Framework Program 6 (of the EC) FWHP — Full Width to Half Power GLIMPSE — the Galactic Legacy Infrared mid-plane Survey Extraordinaire GMC — Giant Molecular Cloud GOODS — Great Observatories Deep Survey HDF-S — Hubble Deep Field South HIFI — Heterodyne Instrument for the Far Infrared HST — Hubble Space Telescope IF — intermediate frequency IRAM — Institut de Radio Astronomie Millimétrique ISM — interstellar medium ISOCAM — Infrared Space Observatory (near infrared) Camera JCMT — James Clerk Maxwell Telescope LABOCA — Large Bolometer Camera LMT — Large Millimeter Telescope LSB — lower sideband MAMBO — Max Planck Millimeter Bolometer MIPS — Multiband Imaging Photometer for SIRTF (now Spitzer) MIR — mid infrared ODIN — International Astronomy and Aeronomy Satellite PACS — Photodetector Array Camera & Spectrometer pwv — precipitable water vapor rms — root mean square SCUBA — Submillimeter Common User Bolometer Array SED — Spectral Energy Distribution SEST — Swedish Submillimeter Telescope SIS — Superconductor Insulator Superconductor (a low noise microwave mixer) SNR — supernova remnant 51
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Report by the ESA-ESO Working Group
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Contents 1 Executive Summary ......
Page 9 and 10: 1 Executive Summary The Herschel Sa
Page 11 and 12: 2 Introduction The Herschel satelli
Page 13 and 14: 3 Descriptions of Herschel and ALMA
Page 15 and 16: Table 1: ALMA Antenna Arrays and Co
Page 17 and 18: 3.2 Herschel Herschel is a cornerst
Page 19: Table 6: Some Characteristics of th
Page 22 and 23: Figure 6: A three-dimensional plot
Page 24 and 25: Figure 8: A plot of the Herschel HI
Page 27 and 28: 5 Common Calibration of ALMA and He
Page 29 and 30: 6 Specific Examples of Synergies Be
Page 31 and 32: 6.3 High Redshift Objects During th
Page 33 and 34: eview) have also revealed a new cla
Page 35 and 36: In addition to emission lines from
Page 37 and 38: y interactions. Consider the nearby
Page 39 and 40: Figure 12: Data for IC10. The integ
Page 41 and 42: matter interacts with the powerful
Page 43 and 44: In DRSP contribution 2.1.2, Kinetic
Page 45 and 46: The Orion KL region is one of the n
Page 47 and 48: degrees. The GLIMPSE survey is bein
Page 49 and 50: An example is DRSP contribution 3.3
Page 51 and 52: Figure 18: A schematic of the analy
Page 53: 7 Summary The PACS and SPIRE bolome
Page 56 and 57: The full ALMA will be in operation
Page 60 and 61: SWAS — Submillimeter Wave Astrono
Page 62 and 63: Falgarone, E., Hily-Blant, P., Pine
Page 64: Wilson, C. D., 2005 in Proc. of The
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