B band filters M.Lampton UCB Space Sciences Lab Nov 2003 More charts added Mar 2006, Oct 2006, Apr 2007.

Slides:



Advertisements
Similar presentations
14 Sep 2006NVO Summer School T HE US N ATIONAL V IRTUAL O BSERVATORY Shape of Galaxy Rotation Curves A multiwavelength study using the VO Barbara.
Advertisements

Day-5. Announcements 1 st Quarter Observing Night Next Thursday – Oct. 10 Start time will be 7:30pm Start set-up at ~6:30pm in Atrium.
DESIGN OF 2.2-INCH LED BACKLIGHT UNITS FOR BRIGHTNESS UNIFORMITY AND REDUCTION OF HOT-SPOT EFFECT Jeng-Feng Lin, Chin-Chieh Kang, and Chih-Yang Liu Department.
Photometric Techniques I Preliminary reductions and calibrations Sergio Ortolani Dipartimento di Astronomia Universita’ di Padova,Italy.
Announcements No lab this week’s due to Tuesday’s observing night Homework: Chapter 5 # 1, 2, 5, 6, 8 & 9 Dark Sky Observing Night next week on Wednesday.
CCD Observing VSS Workshop Hampshire Astronomical Group 13 th March 2010 Roger Pickard, Director BAA VSS.
CLASH: Cluster Lensing And Supernova survey with Hubble ACS Parallels WFC3 Parallels 6 arcmin. = 2.2 z=0.5 Footprints of HST Cameras: ACS FOV in.
The Robotic Palomar 60-inch Optical Afterglow Catalog: 2007 János Kelemen, Konkoly Observatory S. Bradley Cenko, CalTech. SRL Derek Fox, Penn State Univ.
Observational techniques meeting #5. Future surveys Narrow (pencil beam): HDF UDF GOODs Cosmos MCT JWST.
Ge/Ay133 What (exo)-planetary science can be done with transits and microlensing?
Noise Reduction in Digital Images Lana Jobes Research Advisor: Dr. Jeff Pelz.
The Nature of Light In Astronomy II. The Earth’s atmosphere absorbs most of EM spectrum, including all UV, X ray, gamma ray and most infrared. We have.
Telescopes in the world Lison Malo Student CRAQ workshop.
1 Filter parameters using stars alone? M.Lampton Space Sciences Lab U.C.Berkeley 8 Sept 2003 Updated 31 Oct 2003 using Bower filter functions, starting.
P. Price (U. of Hawaii) and many others Discovery and identification of the very high redshift afterglow of GRB J. B. Haislip, et al. astro-ph ,
Undergraduate Research Experiences at BGSU Presented by Katie Guldenschuh & Andy Layden BRAVO BG! Orlando Florida February 2005.
The Photometric Calibration of the Dark Energy Survey D. L. Tucker 1, S. S. Allam 1, J. T. Annis 1, R. Armstrong 2, J. P. Bernstein 3, E. Bertin 4, D.
You are an alien from another world. You have alien eyes. What do you notice about your vision? Put on your cosmic visors. Your job is to visit planet.
The KPNO 4m “Mayall” Telescope Arjun Dey (NOAO). National Optical Astronomy Observatory Mission: provide the best ground-based astronomical capabilities.
Your Observing Challenge: White Dwarfs in Open Star Clusters.
Sonia Cianci a,b, Joss Bland-Hawthorn b and John O’Byrne a a University of Sydney, Australia b Anglo-Australian Observatory Designing ultra-narrowband.
NICMOS IntraPixel Sensitivity Chun Xu and Bahram Mobasher Space Telescope Science Institute Abstract We present here the new measurements of the NICMOS.
4. Telescopes Light gathering power and resolution Optical and radio telescopes Limitations of Earth’s atmosphere and satellite missions. Instruments (prism.
JWST calibration requirements Harald Kuntschner. JWST - an overview NIRCam –0.6-5 microns –FoV: 2.16x4.4 arcmin (0.0317” for short band and ” for.
MEMS-based Spectrographs
The LSST Exposure Time Calculator was developed to model the effects of LSST design changes on signal-to-noise ratio and survey depth. The ETC utilizes.
ASTR_4170 Special Topics: Photometry & Filter Systems Day-5.
The B-V colors and photometric variability of Nix and Hydra, Pluto’s two small satellites Max Mutchler (STScI) S. Alan Stern (SwRI) Hal Weaver (JHU/APL)
What can we learn from the luminosity function and color studies? THE SDSS GALAXIES AT REDSHIFT 0.1.
SDSS griz photometry (first experiences at Baja Observatory) T. Hegedüs – A. Szing – J. Vinkó* Baja Astronomical Observatory, * Szeged University KOLOS.
Observing the Solar System with HST Amy Simon NASA’s Goddard Space Flight Center.
First T Dwarf Discoveries from the 2MASS/Lick All-Sky T Dwarf Search M.W. McElwain (University of California Los Angeles), A.J. Burgasser (University of.
Optical Observations of J : An LMXB in Transition Paul A. Mason New Mexico State University Emmanuel Gonzalez University of Texas at El Paso Edward.
Chile Sky Background at ESO/la Silla in the Visible and Near IR Leonardo Vanzi -Olivier R. Hainaut European Southern Observatory La Silla - Chile.
15 October Observational Astronomy Direct imaging Photometry Kitchin pp ,
Structural Properties of Galaxies in the Local Universe Paul Allen Mount Stromlo Observatory The Australian National University Simon Driver, Alister Graham,
Dark Energy Probes with DES (focus on cosmology) Seokcheon Lee (KIAS) Feb Section : Survey Science III.
The Dust Environment of V838 Mon based on the Light Echo, and Afsar-Bond Star Cluster Vitaly Goranskij Sternberg Astronomical Institute of the Moscow University.
SNAP CCD Development Progress Hakeem Oluseyi January 9, 2003.
The Photometric Calibration of the Dark Energy Survey D. L. Tucker 1, S. S. Allam 1, J. T. Annis 1, R. Armstrong 2, J. P. Bernstein 3, E. Bertin 4, D.
Surveying the Universe with SNAP Tim McKay University of Michigan Department of Physics Seattle AAS Meeting: 1/03 For the SNAP collaboration.
G.Vasileiadis, CTA Meeting 4-5 May-2006 High Altitude UBV Observations E.Giraud, I.Toledo, P.Valvin & G.Vasileiadis LPTA/Montpellier, Un.Cath Chile.
Welcome to the First CLASH Science Team Meeting September 20 – 21, 2010 Granada, Spain.
A Photometric Study of Unstudied Open Clusters Berkeley 49 & 84 in the SDSS Jinhyuk Ryu and Myung Gyoon Lee Department of Physics & Astronomy, Seoul National.
The B-V colors and photometric variability of Nix and Hydra, Pluto’s two small satellites Max Mutchler (STScI) S. Alan Stern (SwRI) Hal Weaver (JHU/APL)
Photometric calibration in Astro-WISE For the Astro-WISE consortium: Gijs Verdoes Kleijn OmegaCEN/Kapteyn Groningen University (and Philippe Heraudeau,
From Pan-STARRS to PTF Wing-Huen Ip Institutes of Astronomy and Space Sciences National Central University Nov. 25, 2011 Sun-Moon Lake, Taiwan.
SNAP Calibration Program Steps to Spectrophotometric Calibration The SNAP (Supernova / Acceleration Probe) mission’s primary science.
1 WIYN One Degree Imager. 2 Filter Changer 3 Demonstration Filters  Sloan g’ r’ and i’ delivered from Infinite Optics  Johnson U on order from Barr.
TIPS - Oct 13, 2005 M. Sirianni Temperature change for ACS CCDs: initial study on scientific performance M. Sirianni, T. Wheeler, C.Cox, M. Mutchler, A.
1 A French participation to SNAP A.EALET. 2Outline Scientific interest Supernova in the world The French expertise in SN Historical participation The.
Announcements After lecture, adjourn to the observatory to start set-up for Dark Sky Observing night Forecast for Thursday doesn’t look good (60% chance.
1 Small Telescopes and the Photometric Calibration of the Sloan Digital Sky Survey (SDSS) Douglas Tucker.
SDSS-II Photometric Calibration:
Astronomy 1010 Planetary Astronomy Fall_2015 Day-23.
A Broad Band Imager for the European Solar Telescope Matteo Munari & Salvo Scuderi INAF – Osservatorio Astrofisico di Catania Massimo Cecconi INAF – FGG.
2/6/2016 DCH-1 JWST/MIRI Space Telescope Science Institute The Infrared Sky: Background Considerations for JWST Dean C. Hines & Christine Chen MIRI Instrument.
1 Target Selection Workshop Report Nick Mostek Dec 6, 2010 BigBOSS Science Telecon.
Galactic Astronomy 銀河物理学特論 I Lecture 3-2: Evolution of Luminosity Functions of Galaxies Seminar: Lily et al. 1995, ApJ, 455, 108 Lecture: 2011/12/12.
The SNAP Instrument Suite Session Chris Bebek (for Mike Lampton) Lawrence Berkeley National Laboratory 9 January 2003.
Astronomy 1020 Stellar Astronomy Spring_2016 Day-3.
Scientific DetectorWorkshop, 2005 Taormina Characterization of 1.7um cutoff detectors for SNAP Roger Smith Caltech.
LSST CCD Chip Calibration Tiarra Stout. LSST Large Synoptic Survey Telescope Camera – 1.6 m by 3 m. 3.2 billion pixels kg (~6173 lbs) 10 square.
Rachel Anderson Laura Parker William Harris Department of Physics & Astronomy, McMaster University Hamilton, Ontario, L8S-4M1, Canada Searching for Galaxy.
Validation of HLA Source Lists Feb. 4, 2008 Brad Whitmore 1.Overview 2.Plots 3.Summary.
Probing the mass accretion process in the neighbourhood of SN1987A
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.
GROND an optical/NIR 7-channel imager:
Figure 1 from European Southern Observatory Very Large Telescope Optical Spectroscopy of BL Lacertae Objects. III. An Extension of the Sample (Image 1.
Infrared Instrumentation for Small Telescopes
Presentation transcript:

B band filters M.Lampton UCB Space Sciences Lab Nov 2003 More charts added Mar 2006, Oct 2006, Apr 2007

Lampton B-band filters2 M.S.Bessell “UBVRI Passbands” PASP Figure 8 B90: Bessell 1990: GaAs + 2GG385+1BG12+1BG18 B18t: Cousins 1973: S13 + 3GG13 BB: Bessell 1976, 1979: S13 + 2GG BG12+1BG18 BGR: Graham 1982: GaAs + 3GG13

Lampton B-band filters3 Stanishev et al astro-ph/ (2007)

Lampton B-band filters4

Lampton B-band filters5

Lampton B-band filters6 KPNO glass filters for use with CCDs: B: 1mm BG12 + 2mm BG39 + 1mm GG385

Lampton B-band filters7 KPNO “B” band interference

Lampton B-band filters8 The RGO Glass Broad Band Filters (UBVRIZ)

Lampton B-band filters9 MDM Observatory's 8K CCD array project: FILTERS FOR THE 8K CCD ARRAY

Lampton B-band filters10 ESO La Silla standard filter sets: Blue, red

Lampton B-band filters Gemini

Lampton B-band filters Santa Barbara Instrument Group

Lampton B-band filters Santa Barbara Instrument Group

Lampton B-band filters14 Single-band filter and sets; over 100 models UV-VIS_NIR

Lampton B-band filters Andover Corporation

Lampton B-band filters Andover Corporation

Lampton B-band filters17 HST WFC3 F438W (dotted)

Lampton B-band filters18 SDSS filters Fukugita et al 1996 AJ blue side cutoff due to glass dye; reasonably rapid cutoff red side cutoff due to multi layer interference film overall good efficiency overall little ripple

Lampton B-band filters19 Megacam CFHT

Lampton B-band filters20 Cenko et al “Palomar 60 inch” astro-ph/ pdf

Lampton B-band filters21 Asiago Database on filter Photometry Systems (ADPS) Moro, D., & Munari, U., 2000, A&AS, 147, 361 (Paper I) More than 100 photometric systems compared Several hundred UBV ugriz etc systems GIF plots Text listings Hot links to most of the original work ADPS 2003: Fiorucci & Munari A&A 401 pp , Paper II –Parameters for all filters: various mean wavelengths, widths at 50% and 10%, asymmetries; synthetic photometry

Lampton B-band filters22 Conclusions There are a variety of B band filter profiles One has a large asymmetry towards the red Most are nearly symmetrical Best choice for SNAP needs to be explored In our longest NIR passband, a redward extension is a serious contributor to our dark current owing to thermal tails of warm objects within our telescope We should explore symmetrical passbands