SSC Home Page

FLS: Extragalactic Component Requirements


SPITZER HOME || SPITZER SCIENCE || INSTRUMENTS || SCIENCE USER SUPPORT || SEARCH

+ - General Information
- Spitzer News
- Research Categories
- Science Schedules
- Advisory Groups
- Observing Rules
- Legacy Program
- First-Look Survey
+ - Observatory & Instruments
- Overview
- PCS
- IRAC
- IRS
- MIPS
- AOTs
+ - Science User Support
- Proposal Kit
- Documents
- Tools
+ - Approved Programs
- Observing Schedules
+ - Data Archives / Analysis
- Science Archive Access
- Post-BCD Tools
+ - Data Analysis Funding
- Information
+ - FAQ
- Search site
The extragalactic component of the FLS was designed to meet these requirements:
  • A 5 square degree imaging survey with IRAC and MIPS to a shallow depth of about one minute per pixel on the sky.

    • A total of 4 square degrees within the Spitzer Continuous Viewing Zone (CVZ), in an area where IR cirrus is low: 17h10m+61d, where I(100um) = 1-2 MJy/sr

    • A separate 1 square degree region whose location will depend on the sky visibility at the end of In-Orbit Checkout (IOC):
      1. in near-CVZ area of low cirrus at 16h20m+54d30m, where I(100um) = 0.4 MJy/sr, or
      2. within the CVZ, if area in (a) is not accessible at the conclusion of IOC.

    • MIPS Shallow Survey: 5 passes at fast speed, incorporating three bands
      • Total T(int) = 75 sec per point (24 and 70 um), 15 sec (160 um)
      • Depth reached is 1.3 mJy at 24 um; confusion-limited at 160 um
      • Scan rate = 1 sq.deg. per 3 hours, plus 30% overheads
      • Following estimates for a 5 square degree, 20-hour survey

        wavelength
        (µm)
        Flux Limit
        (mJy, 5-sigma)
        Gain over
        Past
        Source
        Counts
        241.3~ 100~ 400
        704.5~ 50~ 1500
        16027.0~ 8*~ 2500
        * ISO covered a few square degrees

    • IRAC Shallow Survey: 4 bands simultaneously
      • Total T(int) = 5x12 sec per point
      • Requires ~ 5 hours per sq.deg., including overheads
      • Following estimates for a 5 square degree, 20-hour survey

        wavelength
        (µm)
        Flux Limit
        (mJy, 5-sigma)
        Gain over
        Past
        Source
        Counts
        mean z for L* elliptical
        3.6/4.50.04>> 1stars + ?~ 1
        5.80.04~ 1*stars + ?~ 0.4
        8.00.06~ 1*~ 1500~ 0.3
        * ISO covered a few square arcminutes

  • Within the above area, a MIPS/IRAC verification survey of 0.25 square degree or less, with ten times the integration time.

    • Should fit within ~30% of time dedicated to shallow survey

  • Incorporation of ancillary data recommended, primarily for identification purposes.

    • Deep R-band or I-band survey, to R(5-sigma) ~ 25.5 mag
    • Near-infrared K-band survey to K ~ 18 mag
    • Radio survey at 1.4 GHz to 5-sigma sensitivity of ~ 90 micro-Janskys

  • Conservative experimental design, emphasizing reliability at the expense of sensitivity.


SPITZER HOME || SPITZER SCIENCE || INSTRUMENTS || SCIENCE USER SUPPORT || SEARCH

help@spitzer.caltech.edu
http://ssc.spitzer.caltech.edu/fls/extragal/req.html
This file was last modified on Mon Oct 23 16:07:24 2006.

California Institute of Technology Jet Propulsion Laboratory NASA