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COSMOS Magellan Spectroscopy

COSMOS Magellan Spectroscopy. Chris Impey and Jonathan Trump Steward Observatory Martin Elvis (CfA), John Huchra (CfA), Pat McCarthy (Carnegie). Magellan IMACS. Inamori Magellan Areal Camera and Spectrograph Multi-object spectrograph 30’ diameter field. Our configuration:

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COSMOS Magellan Spectroscopy

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  1. COSMOS Magellan Spectroscopy Chris Impey and Jonathan Trump Steward Observatory Martin Elvis (CfA), John Huchra (CfA), Pat McCarthy (Carnegie)

  2. Magellan IMACS • Inamori Magellan Areal Camera and Spectrograph • Multi-object spectrograph • 30’ diameter field Our configuration: • 5400-9200 Å spectra • 1” × 11” nod & shuffle slits • Resolution: 10 Å

  3. Tiling Strategy Top: XMM coverage (RA is reverse from at right). Edge effects necessitate overlap Right: Single-pass IMACS strategy, ~5 hours each field

  4. 30’ Slit Maps Field 11, with 221 targets Mask / Sky Plane Detector Plane

  5. Targeting Strategy and Yields Six types of targets with i’<24: • x-ray selected AGN (XMM), priority 1 • radio selected AGN (VLA), priority 2 • BZK, priority 3 • Optically selected z~3-5 AGNs (Peter), priority MH • B, V, and i dropouts (Mauro), priority 3/3/MH • z>1.5 phot-z selected galaxies (Bahram), priority 5 • Yields (average of center fields): • 60% xagn (54/89) • 37% ragn (28/76) • 14% bzk (2/14) • 100% oagn (15/15) • 10% bdrop (55/574), 6% vdrop (7/126), and 100% idrop (2/2) • 4% highz (57/1468)

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