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Mul$-‐wavelength ancillary data for HI Deep Fields Ma$ Jarvis University of Oxford & University of the Western Cape 17/03/2015 PHISCC 2015 -‐ Rutgers We need reasonably large fields & mul$-‐λ 3° at z=1 Typical HerMES ASTRODEEP field fields Δz=0.1 at z=1 17/03/2015 PHISCC 2015 -‐ Rutgers 17/03/2015 PHISCC 2015 -‐ Rutgers VIDEO/CFHT/DES/SERVS/SWIRE/HerMES/SCUBA2/MIGHTEE LSST/SKA Elais-S1 XMM-LSS ECDFS Filter Time (per Time (full 5σ AB 5σ UKIDSS Seei Moon source) survey) Vega -DXS ng Z 17.5 hours 456 hours 25.7 25.2 - 0.8 D Y 6.7 hours 175 hours 24.6 24.0 - 0.8 G J 8.0 hours 209 hours 24.5 23.7 22.3 0.8 G H 8.0 hours 221 hours 24.0 22.7 22 0.8 B K 6.7 hours 180 hours 23.5 21.7 20.8 0.8 B s 17/03/2015 PHISCC 2015 -‐ Rutgers The VISTA Deep Extragalac$c Observa$ons (VIDEO) Survey 0.12 sq.deg i.e. ~1/100th of the total area of VIDEO 17/03/2015 PHISCC 2015 -‐ Rutgers “Typical” mul$-‐wavelength coverage over southern deep fields •  Heterogeneous X-‐ray data from Chandra/XMM (eROSITA soon) •  GALEX: FUV + NUV to AB ~24 (~6arcsec resolu$on) •  VST-‐VOICE + DES + HSC + LSST: ugriz to mAB ~26-‐27 (<1arcsec resolu$on) •  UltaVISTA/VIDEO: (Z)YJHKs mAB = 25.7, 25.6, 24.5, 24.0, 23.5 (<0.9arcsec resolu$on) •  SERVS/DeepDrill: Spitzer 3.6 & 4.5um to 2uJy (~2arcsec resolu$on) •  SWIRE IRAC 5.8 & 8.0um to ~30uJy (~3-‐4arcsec resolu$on) •  MIPS 24/70/160um to 0.3,20.100mJy (~10,25,50 arcsec resolu$on) •  Herschel-‐HerMES 110,160,250,350,500um to 31.5,60.2,12.7,10.5,15.2mJy (7,10,18,25,35arcsec resolu$on) •  JVLA/MeerKAT “con$nuum” imaging 1-‐4GHz (~1-‐8arcsec resolu$on) SED fits using the energy-‐balance models of da Cunha et al. 2008 From Smith et al. 2012 17/03/2015 PHISCC 2015 -‐ Rutgers The VISTA Deep Extragalac$c Observa$ons (VIDEO) Survey Combina$on of CFHT+VIDEO we produce for z-‐ PDFs for every source (Jarvis et al 2013). (zspec-‐zphot)/(1+zspec) = 0.014 0.65% catastrophic outliers 3-‐D Density field measurements (Burton, MJ, et al. 2013) 17/03/2015 PHISCC 2015 -‐ Rutgers Spectroscopy!!! •  Exis$ng heterogeneous spectroscopy from various follow-‐up studies of X-‐ray, Spitzer etc etc. Not ideal for deep HI surveys •  Dedicated surveys over ~1sq.deg – e.g. zCOSMOS and VVDS/VUDS. Incomplete and not really targeted at HI counterparts. •  Mainly magnitude limited but some$me colour selec$on for high-‐z So -‐ nowhere near enough!!! 17/03/2015 PHISCC 2015 -‐ Rutgers WEAVE-‐ WHT (2017) (also DESI and 4MOST) 17/03/2015 PHISCC 2015 -‐ Rutgers MOONS – VLT (2018) 17/03/2015 PHISCC 2015 -‐ Rutgers

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Mull-‐wavelength ancillary data for. HI Deep Fields. University of Oxford &. University of the Western Cape. Ma Jarvis. 17/03/2015. PHISCC 2015 -‐ Rutgers

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Mull-‐wavelength ancillary data for. HI Deep Fields. University of Oxford &. University of the Western Cape. Ma Jarvis. 17/03/2015. PHISCC 2015 -‐ Rutgers

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