Mjy PowerPoint PPT Presentations

Radio traces massive SF, AGN jets. Characterization of uJy population to ... blending leads to some overestimated MIR fluxes, while aperture photometry ...

SPIRE PS imaging 3-10 mJy 5s 1hr (obs. mode dependent, but all three bands) PACS PS imaging 3 mJy 5s 1hr (two bands simultaneously) ...

tends to show depolarization (typically the degree of polarization ... measured to have 325 mJy by Xu et al. (1995), but only 175 mJy is ...

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... Billions of galaxies, HI mass function evolution poorly ... Jy- mJy (up to 1016 M?? of HI) Angular scale 5' T 30', freq res 500 khz. Challenging theory ...

Optical identifications of the S850 2 mJy sources ... Cambridge: Andrew Blain, Malcolm Longair. UCL: Rob Ivison. JACH: Tim Jenness ...

Smax=0.167 Jy/beam, rms=0.03 mJy/beam. VLA, B-Array. VLA, A-Array ... Degree of Radio Polarization and X-ray Emission. Conclusion ...

The study of galaxy formation is emerging as a dominant theme for astronomy in the 21st Century. ... 3 minutes of ALMA observing time gives 1 mJy sensitivity. ...

?T = 23 mK, ~0.3 mJy. Angular scale 5' T 20', freq res 500 khz ... Biggest collecting area in this band. Half in central 1km core, rest in 50 km Y. ...

The JCMT Nearby Galaxies Legacy Survey: Star Forming Molecular Gas in ... Sensitivity set by extragalactic confusion limit (1.3 mJy/beam rms) ...

Intensity and polarization model fitting; Helical B ... Intensity (mJy) 1) 1310.0. 1b) 230.5. 2) 82.8. 3) 113.2. Polarization ... 15 GHZ Intensity map with ...

Space Infrared Telescope Facility. Predicted Spectrum of. Brown Dwarf GL229B. The IRS Short-Lo Sensitivity (5s, 500s) is ~ 0.5 mJy (Spectrum from Marley et al) ...

Main result: star-forming galaxies make up only 1/3 of the sub-mJy radio sources ... We have used a wealth of multi-wavelength information in the radio, optical, and ...

`Piggyback' redshift surveys of radio galaxies at z 0.3 ... Needs new large-area (50-100 deg2) sub-mJy radio survey. ... the local radio-source population is ...

5.0 GHz Area=6 sr Slim 30 mJy N 55000 GB6 (Gregory et al. 1996) ... 0.8 GHz Area=7900 deg2 Slim 6-10 mJ N. 2x105 NVSS (Condon et al. 1993, 1998) ...

Extragalactic Sources: ~ 600.000 sources between 1 mJy and 2 Jy (Dole H. et al astro-ph/0002283) ... resolution. MIPS resolution (H. Dole, (H.Dole, MIPS) MIPS) ...

CIB vs COB vs CMB. Extragalactic Background Light SED now well constrained ... COB ~ CIB ~ 24/23 nW m-2 sr-1. EBL: for 1 visible photon = 115 IR photons. EBL ...

Calibration for Campaign 7: Ch' 1

Present radio observations and maps. Show preliminary analysis. Summarize the results ... PA = 128 1215 303. z = 0.130. VLA image, from FIRST survey. peak ...

problem of weak radio emission. FR II or FR I ? Hans-Rainer Kl ckner. Alejo ... population of obscured radio quit quasars. postulated from hard X-ray background ...

Sensitivity selected on the basis of appropriate PWV for that wavelength. ... Note: these numbers are for a non-heterodyne spectrograph. 5.87E-20. 64.6. 1.5. 91. 3300 ...

Measuring Fluctuations & Counts Mattia Vaccari & Alberto Franceschini & Giulia Rodighiero & Stefano Berta Department of Astronomy - University of Padova

Veronique Buat, Jonathan Davies, Kate Isaak, Walter K Gear, ... R~1000 integrated spectroscopy (Balmer decrement, metallicity...) with CARELEC at the OHP ...

survey of EGRET-like blazar candidates. ... background EGRET photons. J0906 ... EGRET upper limit only lies in the overlap between two 3EG sources. So...

... Class I: 70 3000 Ratio of Spitzer IRAC to submm emission F3.6/F850 0.003 A form of thermal ...

Data Analysis Mode: Preliminary results available for incoherent addition ... P0: Barycentric period of the pulsar (s) S400: Mean flux density at ...

Low Hanging Fruit in The New Radio Sky or Radio Surveys and Transients with the Allen Telescope Arra

Our VLBA survey, now half complete, is not biased with flat-spectrum targets. ... NOAO is operated by AURA, Inc., under a cooperative agreement with the NSF. ...

Radiocontinuum PNe in the Magellanic Clouds

Well-Matched SWIRE MIPS 24/70/160 micron & SDSS Optical Coverage Particularly so at low (0

Title: GBT Status: Current Observing Capabilities Author: dbalser Last modified by: dbalser Created Date: 11/8/2002 1:29:46 AM Document presentation format

Project Scientist LMT. Instituto Nacional de Astrofisica, Optica y Electronica ... Basic observational properties of the ISM and galaxies at FIR-mm wavelengths. ...

Title: Diapositiva 1 Author: Franco Mantovani Last modified by: fmantovani Created Date: 2/18/2004 7:48:30 PM Document presentation format: On-screen Show (4:3)

Title: Requirements, constraints and expectations for bolometers prototypes at the 30m telescope Author: Administrator Last modified by: Administrator

What you get (resolution, FOV, sensitivity) Previous low frequency VLBI ... I'm not a low-frequency expert! This is (mainly) not VLBI in the current, ...

Relation to (sub)mm galaxies (Barger, Chapman, Blain, Dannerbauer, ... Temperature redshift degeneracy: measure (1 z)/T_D (Blain 1999) ...

V. Tudose (UvA, AIRA), R. Fender (Soton, UvA), M. Garrett (JIVE), J. Miller-Jones (UvA), Z. Paragi (JIVE), R. Spencer (Jodrell) ... avoids embarrassing situations. ...

Title: PowerPoint Presentation Author: sjc Last modified by: sjc Created Date: 11/6/2002 2:56:15 AM Document presentation format: On-screen Show Company

Reionization: the movie. 8Mpc comoving. Constraint I: Gunn-Peterson Effect. Fan et al 2006 ... Twilight zone': study of first light limited to near-IR to radio l's ...

... Herschel probes the rest-frame bolometric emission from galaxies as they formed most of their stars Wedding Cake Survey GOODS-S 0.04 deg^2 GOODS-N 0.04 ...

The VLA can also tune between 1100 and 1225 MHz, but with limited capability. The EVLA @ L-band. EVLA antennas will tune between 930-2000 MHz. ...

Title: PowerPoint Presentation Last modified by: unknown Created Date: 1/1/1601 12:00:00 AM Document presentation format: (4:3) Other titles

... extra-solar systems (Minier, Lineweaver, Burton, Purcell, Longmore, Norris, 2003) ... Plane (Minier, Burton, Wong, Purcell, Hill, Longmore, Barnes, 2002 2003) ...

Sensitivity as a function of frequency: Colored lines are derived via ... the end WIDAR will provide 64 completely independent subband pairs (independent ...

limb brightening clearly revealed by VSOP ... orientation, limb brightening seem to be in agreement with VLBA at 43 GHz. Marscher et al. 2002 ...

16 micron Imaging in the GOODS fields with the Spitzer IRS. Harry Teplitz ... Pilot Study: GTO 16 mm in GOODS-N ... GOODS South. Data obtained in Feb 05. Some ...

Error recognition is used to determine defects in the data ... is more instructive. Mega-wavelength. Jansky. 16. Example Edit msplot (2) ...

GRB Host Galaxies S. R.Kulkarni, E. J. Berger & Caltech GRB group

Synthesis Imaging in Radio Astronomy, 1998, ASP Conf. Series, Vol 180, eds. ... Radio telescopes are Diffraction Limited. Incident waves ...

High Angular Resolution SMA Imaging of High Redshift Galaxies at 345 GHz ... new population of dust-enshrouded starburst galaxies at high redshift. ...

Tenth Summer Synthesis Imaging Workshop. University of New ... Brighten and deflect. Gomez et al. 2000. 26. Where Most X-rays & ?-rays Are Emitted. clouds ...

The SWIRE Spitzer survey has detected by far the largest set of Sub-Millimeter ... Chapman, Blain, Smail, Ivison 2005. SCUBA(-MAMBO) census of high-z ULIRGs ...

angular distance between radio counterpart and 3EG source ... Survey (4 sub-catalogs) 91m Green Bank. White et al. 1992 ' Binary ' sky exposure ...

Title: No Slide Title Author: andy lawrence Last modified by: James Created Date: 1/27/1997 3:20:31 PM Document presentation format: On-screen Show (4:3)

Title: Pulsar Powerhouse: The Center of the Crab Nebula Author: M Bietenholz Last modified by: michael Created Date: 1/4/1980 12:41:10 AM Document presentation format

Result: A leap of over two orders of magnitude in both spatial resolution and sensitivity ... Resolution increase of up to an order of magnitude ...