1 / 22

FMOS on COSMOS

FMOS on COSMOS. Tomo GOTO (ifa/Subaru, JSPS fellow). J=20.1 H=19.8. Current status. Open for common use starting 10A. Only IRS1, low resolution mode available (200 fibers). Full 400 fibers, high-resolution will be operational from 11A. Continuum sensitivity. For 1 hour, 4pix,

kyle
Download Presentation

FMOS on COSMOS

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. FMOS on COSMOS Tomo GOTO (ifa/Subaru, JSPS fellow) T.Goto

  2. T.Goto

  3. J=20.1 H=19.8 T.Goto

  4. Current status • Open for common use starting 10A. • Only IRS1, low resolution mode available (200 fibers). • Full 400 fibers, high-resolution will be operational from 11A. T.Goto

  5. Continuum sensitivity For 1 hour, 4pix, S/N=5 at (ABmag) In reality, 1.05-1.7um T.Goto

  6. Line sensitivity For 1 hour, S/N=5 at 1x10-16 erg/cm2/s Corrected for fiber loss T.Goto

  7. Proposal deadline 9/30/10 FMOS instrument team is preparing a proposal. T.Goto

  8. FMOS team SSP proposal draft • Galaxy/AGN , SXDS • Photoz sample 10 nights, • X-ray AGN: 10 nights • Emitter : 5 nights • Cluster: 16 nights • Subaru deep field (photoz+emitter) :8 nights • AKARI NEP (mid-IR source) : 5 nights • Redshift space distortion :50 nights • Pending :10 nights. • Total 140 nights (including weather factor). T.Goto

  9. Why not COSMOS field? • HST morphology is irreplaceable. • Accurate photo-z is essential when continuum sensitivity is not good. • Many one line only detections expected. Need photo-z to use data. • X-ray, Spitzer, Herschel coverages are better than other large field. T.Goto

  10. Public COSMOS data • RA (J2000) = 10:00:28.6, DEC (J2000) = +02:12:21.0 • 588 orbits of HST/ACS, ~2 million objects to IAB < 27; • Photo-z accurate to Δz < 1% (30 bands) • GALEX, CFHTui, • Subaru (Bvgri, z =26.5AB+13 Int. bands, NBs) • UKIRT YHK, KPNO J, • X-ray • XMM • Chandra ~1700 Chandra sources down to 610-16 cgs, >half with spectroscopic redshifts. 1.8 Ms,1sq.deg,@160 ksec,1761 sources (Elvis et al) • IR • Spitzer IRAC/MIPS, 3,4,5,8,24,70,160um. 24um>0.42mJy. • RADIO, VLA • Spectra • ZCOSMOS, 10,000 spectra at z<1 T.Goto Maximum science output from rich data sets (HST,photoz…)

  11. Cosmos data in future • UltraVista Y=26.7, J=26.6,H=26.1, K=25.6 • Herschel PACS/SPIRE (100,160,250,350, 500um) • WFC3 data 0.1sq.deg T.Goto

  12. Excellent Spitzer coverage T.Goto

  13. N sources • X-ray sources XMM:1886, Chandra 1761 • 24um: 17713 • 70um: 1513 • 160um: 499 • VLA: 2901 • Photoz: 1<z<1.6, 39582 galaxies. • => FMOS T.Goto

  14. FMOS 1hr sensitivity T.Goto

  15. My proposal to the FMOS team • 1<z<1.6 with Hβ, [OIII], Hα • Hα flux>3x10-16 erg/s/cm2 (1hr exposure) • 18277 galaxies • 18277/400x2hrs, => 11 nights • could include • 24um sources • X-ray sources • LAE/LBG at high-z T.Goto

  16. My proposal to the FMOS team Science cases at 1<z<1.6 • 100Mpc scale, includes rich cluster to field(5x106 Mpc3) • LF, MF, HαLF, SFRD • Morphology, environment, SFR • AGN/SB • X-ray/radio/IR sources • Obscured sources… • With spec-z and Hαluminosity T.Goto

  17. Response were very interesting….. T.Goto

  18. FMOS teams response: “Tomo, What you are saying is absolutely right.” “COSMOS is the best field to observe.” But…. COSMOS cannot be included in the initial targets because… part of us are cosmos members. “This is a complicated political issue, Tomo” ??? T.Goto

  19. So COSMOS won’t be in initial targets. I failed. According to Japanese tradition, I should do HARAKIRI But not so soon, T.Goto

  20. T.Goto

  21. My life is saved! • FMOS team does not want to PI COSMOS field, but they welcome someone else to do the field. • SSP must open the proposal to entire Japanese community. They will accept proposal for additional field. • “Tomo, COSMOS stands a good chance.” T.Goto

  22. Summary • COSMOS is a good target for FMOS SSP. • It won’t be in the initial list of targets. • But it is likely, to be added to targets at later stage, if we keep pushing. • We can do a lot with 20k NIR spectra. T.Goto

More Related