clean up class-hierarchy mess. simplify ScienceFrame.make() New Situation. class ColdPixelMap ... Could make absolute error map and do proper propagation of ...
twilight flatfielding and gain correction reduces the chip-to-chip zeropoint ... there is no colour term between the UFTI and WFCAM filter systems as measured ...
Title: FMOS mechanical review Author: Ian Lewis Last modified by: Ian Lewis Created Date: 1/31/2002 12:48:53 AM Document presentation format: On-screen Show
Title: PowerPoint-Pr sentation Last modified by: Harald Kuntschner Document presentation format: Custom Company: Micaela Stumpf Other titles: Times New Roman HG ...
Title: PowerPoint Presentation - CCD online presentation Author: Jean Surdej Keywords: CCD Characterisation Last modified by: Stefan Hippler Created Date
... 8 Feb 2005 Too much!!! ~0.5mag brighter d) background and PSF subtraction SN2002cm working image reference subtraction The steps to follow are: ...
... and astrometry ... Limb Astrometry. rotational constraints through limb harmonics. secular ... 1600 days of MDI astrometry (l=6) Appourchaux et al. (2000) ...
An open question in using the subarray readout mode is whether special ... Nudge. Install PIL, FPA. Install Baffle Covers. AT. AT. AT. FPA & Wavefront Sensing Tests ...
Optional to obtain spatially-resolved spectra Spatial resolution along slit/aperture ... Errors in radial velocity since image moves in slit Errors in photometry ...
To find positions of faint I-band objects for quasar candidate selection. ... Create sky and variance images from a boxcar of clipped flattened image. Subtract sky. ...
Parallel Imager for Southern Cosmology Observations ... Parallel implementation, Condor on Linux boxes. Robust and self-tracking. Honed on crowded fields ...
A spectrograph dedicated for SN physics ... Spectrograph: implementation. Under the global shielding. 15 ... The spectrograph : A key instrument for the SNAP mission ...
eclipse libraray in C (ESO, N. Devillard) wrapped with SWIG. fits images and headers as built-in data types ... Persistent Sourcelists (see KGB) Astro-wise Pipelines ...
Photography was invented in 1840s, but use in astronomy only started to become ... in 1970s, full fledge effect in 1980s, spreading to amateur astronomy in 1990s. ...
on OGSE BBs. 1 x 1010 V/W. 1/f knee ~0.125 Hz. Noise density 5 V/Hz1/2. NEP ... Dark current measurements of unstressed detector arrays carried out at MPIA ...
Essential to have a good working instrument. Essential to take all of the relevant calibration data ... Correct data reduction procedures for the data. Check ...
... of morphology, magnitude, color and location ... DEC target 10s magnitudes. ... Limiting Magnitude. L* cluster galaxies at redshift 4000A break ...
Instrument Computer (original system won't work with the camera. ... As evenly illuminated as possible: note vignetting (spots are dust on lenses) Lab Testing ...
The Stellar Populations, Mass-to-Light Ratios and Dark Matter in Spiral Galaxies Roelof S. de Jong Steward Observatory Eric Bell Rob Kennicutt Rob Swaters
Tested separately to find transmittance and responsivity. Simulated with TIMED-SEE solar ... Relevant spectral range is tested, with special attention to range borders ...
NEON Archive School 2006 Introduction to Spectroscopic Techniques (low dispersion) M. Dennefeld (IAP-Paris) Outline Basic optics of gratings and spectrographs ...
... removing magazine, using insertor to inset and remove a manually loaded slitmask ... Needs slitmask magazine, more automated acquisition procedure to be ...
the Lyman-alpha Radiometer onboard PROBA-2. I. From Model to Configuration. II. BESSY Campaigns ... (150 nm, 300 nm), Aluminium, Lyman-alpha (N, XN, VN, and ...
IDL will search for an appropriately named file and automatically compile and run the procedure. ... IDL will compile all procedures in file until it hits the ...
http://www.ast.cam.ac.uk/vdfs/docs/photom.pdf. 10/13/09. Simon Hodgkin CASU. Overview. Conversion from WFCAM counts to Vega magnitudes at airmass unity in the MKO ...
Diffraction limited performance and focusing of high ... How is it possible to observe angstrom wavelength radiation from a nm surface roughness target? ...
Monolithic pixels. Proposal submitted to DESY PRC ... Monolithic:part of the CMOS is used as detector element. Will it work ? dec 2001. els koffeman ...
Galaxy and SN spectrum at the same time. Development in ... Cold test in a cryostat used currently for Herschel in LAM. Warm tests in a dedicated clean room ...
CEA DSM Dapnia SAp. Flux calibration. of the Photometer. Koryo ... DSM/DAPNIA/Sap ... CEA DSM Dapnia SAp. 2. Stable signal for a better photometry. How ...
... packets, merge image data, separate by science channel and filter wheel position ... AIA/HMI Science Team Meeting ... Response of AIA 194 channel shown in red. ...
Image Deconvolution Applied to CCD astronomical images with astrometric purposes Maria Teresa Merino Espasa Universidad de Barcelona (Spain) Summary Introduction to ...
Determines number of photons per ADU (Astronomical data unit)? Readout rate ... Easier to design astronomical instruments. Only standard 3.3V needed. Timing non ...
A large amount (milliliters) of soluble protein is needed ... Size of amyloid crystals (40 m long, 1 m diameter) solved on microfocus beam line in Grenoble. ...
Michelson Doppler Imager (MDI)? Primary Science Objectives. Radial Stratification ... Determine the strength of the toroidal magnetic fields at the base of the ...