Brian McLeod Smithsonian Astrophysical Observatory

Slides:



Advertisements
Similar presentations
The Mercury Imaging X-ray Spectrometer (MIXS): Lessons learned for the ATHENA Wide Field Imager (WFI) GW Fraser, A Martindale and C Thomas Space Research.
Advertisements

990901EIS_Opt.1 The Instrument: Optical Design Dr. John T. Mariska Data Coordination Scientist Naval Research Laboratory
Megacam Imaging of the Extended Groth Strip M. Ashby, B. McLeod, J.-S. Huang, P. Barmby, G. Fazio, C. Papovich, S. Willner.
1 PreCam and Global Calibrations Douglas L. Tucker & Sahar Allam DES-Calib/PreCam Telecon 28 October 2011.
XRT X-ray Observations of Solar Magnetic Reconnection Sites
MMT Megacam Brian McLeod Smithsonian Astrophysical Observatory.
Some Chandra Basics. Chandra X-Ray Observatory.
The Research School of Astronomy and Astrophysics of the Australian National University at Mt Stromlo Observatory is developing a wide-field Cassegrain.
Solar-B XRT XRT-1 The Science and Capability of the Solar-B / X-Ray Telescope Solar-B XRT Presenter: Ed DeLuca Smithsonian Astrophysical Observatory.
HI at moderate redshifts Philip Lah Science with MIRA workshop Research School of Astronomy & Astrophysics Mount Stromlo Observatory.
SDW20051 Vincent Lapeyrère LESIA – Observatoire de Paris Calibration of flight model CCDs for CoRoT mission.
SDW 2005, TaorminaReiss et al., We Must be MAD1 We Must be MAD Pushing FIERA to its Limits Roland Reiss, Andrea Balestra, Claudio Cumani, Christoph Geimer,
Observational Astrophysics II: May-June, Observational Astrophysics II (L2)
The Evolution of Stars and Gas in Galaxies: PhD Midterm Philip Lah A journey with noise and astrometry.
Flares and Eruptive Events Observed with the XRT on Hinode Kathy Reeves Harvard-Smithsonian Center for Astrophysics.
Adding TDI mode to PRISM Li Zeng Advisor: Brian Taylor Jan.25, 2008.
Observational Astrophysics II: May-June, Observational Astrophysics II (L2) Getting our NIRF What do want to do? 1.Image a selected.
Dynamical modeling of the DI dust ejecta cloud Tanyu Bonev (Institute of Astronomy and National Astronomical Observatory, Bulgaria) and the ESO DI observing.
June X-Ray Spectroscopy with Microcalorimeters1 X-Ray Spectrometry with Microcalorimeters.
Photon Transfer Method 1. Using two identical flat field exposures it is possible to measure the read noise of a CCD with the Photon Transfer method. Two.
3rd Integral Bart Work Shop Chocerady - November 1-3, Patrizia Ferrero GRB Too observations in Loiano Patrizia Ferrero (IASF-BO, OACT & Universita’
New 42” Camera Status November 20, 2009 Ted Dunham, Peter Collins, Tom Bida, Georgi Mandushev, and Saeid Zoonemat Kermani.
Application of Gravitational Lensing Models to the Brightest Strongly Lensed Lyman Break Galaxy – the 8 o’clock arc E. Buckley-Geer 1, S. Allam 1,2, H.
E. BertinAstro-WISE workshop 11/ TERAPIX: SCAMP E.Bertin (IAP & Obs. de Paris/LERMA)
Telescope Guiding with a HyViSI H2RG Used in Guide Mode Lance Simms Detectors for Astronomy /2/09.
DCDS for roundtable Paul Jorden 10 Oct 2013 Scientific Detector Workshop, Florence e2vMatthew Bastable and others RAL Matthew Clapp and others.
PACS Hitchhiker’s Guide to Herschel Archive Workshop – Pasadena 6 th - 10 th Oct 2014 The SPIRE Photometer and its Observing Modes Bernhard Schulz (NHSC/IPAC)
Hubble Space Telescope Coronagraphs John Krist JPL.
Aldo Dell'Oro INAF- Observatory of Turin Detailed analysis of the signal from asteroids by GAIA and their size estimation Besançon November 6-7, 2003.
AST3-1 photometry from Dome A Bin Ma, Peng Wei, Yi Hu, Zhaohui Shang NAOC AST3
Shapelets analysis of weak lensing surveys Joel Bergé (CEA Saclay) with Richard Massey (Caltech) Alexandre Refregier (CEA Saclay) Joel Bergé (CEA Saclay)
The Active Optics System S. Thomas and the AO team.
Development of CCDs for the SXI We have developed 2 different types of CCDs for the SXI in parallel.. *Advantage =>They are successfully employed for current.
Preparing the telescope and CCD-camera for observations Andrych K, Tvardovskyi D.
A Thermospheric Lidar for He 1083 nm, Density and Doppler Measurements
Slicing the Universe CCDs for MUSE Roland Reiss a, Sebastian Deiries a, Jean Louis Lizon a, Manfred Meyer a, Javier Reyes a, Roland Bacon b, François Hénault.
System Performance Metrics and Current Performance Status George Angeli.
IPHAS Early Data Release E. A. Gonzalez-Solares IPHAS Consortium AstroGrid National Astronomy Meeting, 2007.
Physics 114: Lecture 13 Error Analysis, Part III Dale E. Gary NJIT Physics Department.
MMIRS Status A.Szentgyorgyi/SAO 30 April Imaging 7 x 7 arcmin FOV 0.2 arcsec pixels Y,J,H & K wavelength coverage Spectroscopy Multislit (4’ x 7’)
Telescope Desiderata. Various Goals Imagery / surveys - discovery, census – Consider scales, POSS vs HST, etc Astrometry / motions / distances Photometry.
1 Harvard-Smithsonian Center for Astrophysics Magellan SAC 9/04 MMIRS Status Report Brian McLeod.
Flares and Eruptive Events Observed with the XRT on Hinode Kathy Reeves Harvard-Smithsonian Center for Astrophysics.
THE CCD RIDDLE REVISTED: SIGNAL VERSUS TIME – LINEAR SIGNAL VERSUS VARIANCE – NON-LINEAR Mark Downing, Peter Sinclaire. European Southern Observatory ESO.
Photometry and Astrometry: Bright Point Sources May 16, 2006 Cullen Blake.
LFC Troubleshooting Report G. Rahmer The problem CCD#2 reported as failing intermittently in August '08 Bad images become more common in.
Gaia SSWG Workshop May Focal Plane Detection D. Hestroffer (IMCCE) & F. Arenou (GEPI) Paris Observatory On-board detection procedure but not localisation.
The First Release of AST3 point source catalog from Dome A, Antarctica in 2012 MA Bin, WEI Peng, SHANG Zhaohui, LIU Qiang, HU Yi (NAOC) 973 课题二
The PFA focal plane camera
Tracing the coronal emission in AGN with VLT/NACO
Y. Q. Xue et al ApJS doi: / /195/1/10 Information:
Table 1. Details of the HST WFPC2 imaging and WHT ISIS spectroscopy presented in this paper. The F656N filter has central wavelength λ6560 Å and a FWHM.
Chandra Science Highlight
Institute of Cosmos Sciences - University of Barcelona
Figure 3 from Spectral Line Survey toward the Young Massive Protostar NGC 2264 CMM3 in the 4 mm, 3 mm, and 0.8 mm Bands (Image 1 of 12) Yoshimasa Watanabe.
A one-dimensional look at the recent HETG data
Astronomy 920 Commissioning of the Prime Focus Imaging Spectrograph
Pan-STARRS Gigapixel Camera
Observational Astronomy Astrometry
Pushing FIERA to its Limits Reiss et al., We Must be MAD
WFCAM Photometric Calibration
EPIC Calibration & Operations Meeting
Pan-STARRS Gigapixel Camera
UCAC U.S. Naval Observatory CCD Astrograph Catalog T.J. Rafferty
Pan-STARRS Gigapixel Camera
FMOS astrometry plan Masayuki Akiyama.
Long-term trends in EPIC pn energy response
Chandra Science Highlight
The Image The pixels in the image The mask The resulting image 255 X
Chandra Science Highlight
Presentation transcript:

Brian McLeod Smithsonian Astrophysical Observatory MMT Megacam Brian McLeod Smithsonian Astrophysical Observatory

Basic Parameters 36 2048x4608 13.5micron pixels (e2v ccd42-90) 0.08”/pixel, currently binned by 2 to 0.16” 200kps through 72 amplifiers 2 additional ccd42-90s for guiding/focus SAO-built controller by John Geary

Megacam as seen at SDW2002

CCD SIMULATOR TEST BOX SCOPE CONNECTIONS

300mmx300mm Sloan-r filter by Sagem

Megacam Performance Gain: 3-4 e-/ADU Read noise: 4-5e- at 200kHz CCD Temps: -115C to -130C depending on focal plane location Some large scale flat fielding errors

Image Quality FWHM (ARCSEC) PIXEL POSITION

Astrometry Error relative to 2Mass catalog: 0.16” Dec Err (”) RA Err

NGC6791 r-band 120s J. Hartman et al. astro-ph/ 0504487