Transcript ALFALFA***H
ALFALFA 2012 Hα 8 14 • Hα ISO Spitzer CO HCN AKARI WISE Herschel Hα Spitzer 8 Spitzer24 PAH Hα Hα Ha Zhu et al. 2008 dwarfs HI HI HI SFR/M HI HI FAST Arecibo Legacy Fast ALFA survey (ALFALFA) • • • • Extragalatic spectral line survey The largest single-aperture telescope (305m) Arecibo L-band Feed Array (ALFA) http://egg.astro.cornell.edu/alfalfa 7 pixel radio camera ALFALFA survey • • • • • To cover 7000 sq deg of high galactic latitude sky 1345-1435 MHz (-2000 to +17,500 km/s for HI line) 5 km/s resolution 2-pass drift mode (total int. time per beam ~ 40 s) ~2.3 mJy rms (per spectral pixel) – MHI~105 M in LG, ~107 M at Virgo • 4400 hrs of telescope time, 5+ years • Started Feb’05, 97% complete (779 runs) as of May’12 – ALFALFA 40% catalog: 15000+ detections covering a cosmologically significant volume at z~0 (Haynes+ 2011) Survey strategy • • • • • ALFA beam size: 3.3’x3.8’ “Almost” fixed azimuth drift mode First pass beams spaced by 14.6’ 2nd pass offset from the 1st to give 1.05’ sampling Highly efficient: 99% “open shutter” time Galactic plane fall sky spring sky fall sky • ALFALFA HI Arecibo SDSS HI 7000 20000 0.06 40% α40 (Martin et al. 2010) • Spitzer IRAC3.6 CfA α40 Spitzer 2600 4.5 4588 3.6/4.5 ALFALFA Zhu et al. 2008 1 RA Dec RA DEC RA DEC 22h to 3h 24d to 32d 2 7h30m to 16h30m 4d to 16d 3 7h30m to 16h30m 24d to 28d • Hα Hα Hα • 2.16 2.4 Hα BFOSC YFOSC 0.07 500-1000 1000 2000 ALFALFA Hα 3-5 NGC 5394/5 Arecibo Spitzer WISE Hα SDSS Spitzer WISE 1) 2) 3) 4) 5) ; ; ; FAST FAST ALFALFA KKR17 KKR17 • • • • • • • RA 15h11m10.2s DEC +11d01m56s z=0.0277, 8283km/s M(HI) = 109.64 Msun 2012/06/15~17 seeing~2" 1h KKR17 KKR17 • • • • 2 SDSS 5 18.21 17.35 17.01 17.45 17.01 B -17.73 µ(B) = 24.18 magsec-2 KKR17 (1) KKR17 (2) KKR17 • KKR17 [NII] 1 • S(Ha)/S(Hb) = 2.58 < 2.87 SCUSS fall sky • ALFALFA spring sky +SCUSS ALFALFA fall sky