Ctio PowerPoint PPT Presentations

E6 standard star field observed on same night yielded bizarre values for system ... Broadly 'OK' (bright stars are bright, faint stars are faint) Slope 1 ...

CCD Mosaics at CTIO and SOAR. Ricardo E. Schmidt, CTIO / NOAO SDW2005, Taormina. Abstract: Mosaics based on 2K x 4K CCDs are briefly reviewed.

Red/blue fiber-fed spectrograph. Software. Filter Mount. 12 ... Combination of IRAf tools (for spectrograph calibrations) and code written by G. Jacoby. ...

17-Nov-2003. R. Schmidt, NOAO / CTIO. 1. CCD imaging at CTIO . Detectors and controllers in use ... Leach controllers on SOI. 17-Nov-2003. R. Schmidt, NOAO ...

A DHE SW emulator for the PC has been written by. Nick Buchholz (partial implementation? ... DHE sequencer configuration/download. Provides PAN error monitoring ...

Concentrating on approved and fielded coating materials ... White elastomeric coating present that has not cured, and topcoat is cracking severely ...

CTIO Dark Energy Camera: Scientific Data Management

Take out of T.O. 1-1-8. Improved test to identify dense particulates in media ... Increase in allowable amount for Type II media ...

Fabry-Perot interferometers: Rutgers (CTIO), TAURUS-2 (AAT) ... Lorentzian profile: f(n) = Fo (g/4p2) / ((n - no)2 (g/4p)2) ...

Ricardo E. Schmidt, CTIO / NOAO SDW2005, Taormina. Two 4m class telescopes: 4m Blanco, wide field capability, 30 years old 4.1m SOAR, high image quality,

CTIO 4m with Mosaic imager: 150 half nights over 5 yrs. 3 lunations, ... CTIO 4m, MOSAIC ... Mosaic image WCS registration with IRAF msccmatch, to UCAC2 ...

?dm(r) = ?1h(r) ?2h(r) All physics can be decomposed ... http://www.ctio.noao.edu/~chrism/current/research/C4/dr3. The SDSS-C4 Galaxy Cluster Catalogue ...

... (ESO, OHP, CTIO, VLA) and spaceborne (XMM-Newton, Chandra, INTEGRAL) facilities ... XMM-Newton and INTEGRAL studies of the X-ray and soft gamma-ray emission from ...

The last piece of the processor is a control unit to convert ... ruction Speci. fications for the Simple. Comput. er - Part 1. Instr. u. ctio. n. O. pc. ode ...

166'x166' CTIO CIRIM image (K-band, 30s exposure) Observations Made. Keck II NIRSPEC spectrograph. First high S/N ratio K-band (IR) spectrum of a BH XT system. ...

... deg2, observed for 9 months each every 4 days in 6 bands, 10000 SNe out to z ... altitude of 2200m at Cerro Tololo Inter-American Observatory (CTIO) , Chile (Lat. ...

DECam will greatly expand and extend wide field imaging capability at CTIO ... will provide in-line updates (via 'donut') possibly allowing us to close the ...

525 nights covering. 5000 sq-deg in g,r,i,z and Y band filters. 9 sq-deg ... National Laboratory NOAO/CTIO, CSIC/Institut d'Estudis Espacials de Catalunya ...

1st Chandra observation : 5.7324 days after the burst ... Dark burst ? Two possible candidates with R 23 at t = 1.04 days # CTIO TNG. 4m 3.58m ...

An Optical Emission Line Survey of Large PN. Greg Madsen (U. Sydney) ... V = -50 km/s (PN) V = 0 km/s (ISM) 51 ... Fabry-Perot spectrograph, now at CTIO ...

Using Spitzer and complementary high-resolution ground-based data, we have ... extended in high-resolution HST, CTIO 4m Mosaic & ISPI images. ...

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The Perfect Accessory for Your Furry Friend

Brazilian Tunable Filter Imager (BTFI) Preliminary Design ... Natural guide-star (NGS) operations: Sep'09. Laser guide-star (LGS) operations: ~Sep'10 (tbc) ...

Filo Chordata Cerca de 45 mil esp cies. Caracter sticas exclusivas: Notocorda. Fendas faringianas. Sistema nervoso dorsal Cauda terminal Filogenia dos Cordados ...

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From UCAC to URAT Norbert Zacharias U.S. Naval Observatory Astrometry Department Cataloging Division nz@usno.navy.mil

Materials and Manufacturing Directorate. Air Force Research Laboratory. 1 April 2004 ... Provide prompt and dependable coating technologies and solutions to our ...

FAST spectrograph. 3700 7500 . Recent upgrade to optics. Three or four spectra per night, ... Capability of Spectrograph. SN with R = 19.8 mag. Recent Examples ...

Bright Stars, Dark Energy Robert P. Kirshner HarvardSmithsonian Center for Astrophysics

Title: PowerPoint Presentation Author: Massimo Robberto Last modified by: Massimo Robberto Created Date: 12/6/2004 3:23:54 PM Document presentation format

Current in-house catalog contains 1619 sequences, of which 776 in the north and ... of current catalog sequences. Number of stars/sequence in current catalog ...

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Lyman Break Galaxies in Large Quasar Groups at z~1 G Williger (Louisville/JHU), R Clowes (Central Lancashire), L Campusano (U de Chile), L Haberzettl & J Lauroesch ...

FUN Coordination in Chaos (An Brief History on) How a Planet was Discovered Subo Dong The Ohio State University Microlensing Follow-Up Network

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Calibration Screen Development

Design uses as many of the existing fabrication prints as possible ... can probe to high redshift - need ancillary redshift measurement from DES ...

A Survey of Local Group Galaxies Currently Forming Stars

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Institut d'Estudis Espacials de Catalunya (IEEC/ICE), Institut de Fisica d'Altes ... Will contain 62 2kx4k Image CCDs: 520 megapixels ...

Multi-apparition Photometric study of Vesta family (asteroids ... Events observed, but still unable to acquire complete coverage of the 2 occultation events. ...

Turbulence and Seeing measurements at Dome C

Structure glued to CCD surface must extend to edges of active area ... Flexure Blades. Pins. Circuit Board. M2 -into Moly frame. M3 -mounts to Coldplate. 9/30/09 ...

The Dark Energy Survey

Updates to Rapid Cure Technologies for Field Repair. Mr. Corey Bliss. AFRL/MLSSO ... (6-20.7.2) Skin panels less than 9 square feet, fasteners, rivet heads, screw ...

95% of the Universe is in Dark Energy and Dark matter for which we have no understanding ... Cluster of Galaxies: Largest gravitationally bound objects ...

... textbooks in Spanish, possibly as joint effort among Spanish-speaking countries ... Solar System scale model along the country and/or in public parks ...

Development of the Modern Large Telescope

How do variable stars come to exist in intergalactic space? ... Those classified as outbursts could be supernovae or cataclysmic variables.

Are there disks around BDs? How do they compare to cTTS disks? ... NIR not adequate cold BD photosphere! SED. ISOCAM 6.7&14.3 m excess detected for ~ 10 young BD ...

ATLAS CCD DE EST NDARES OB DE CLASIFICACI N ESPECTRAL. OBSERVADAS CON REOSC ... Est ndares de TE observadas en el azul-rojo con el fin de ampliar los criterios ...

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We have requested suggestions for membership from members of ... Gemini Aspen instruments need $7M/year (US share) LSST Design & Development (already funded) ...

The Dark Energy Survey Camera: DECam