| CAID: MIPS-290 | Title: Scan Map of Protostellar Region | |
| System: MIPS | Principal: alberto | Deputy: jmuzerolle |
| Objective: | Verify scientific validity of MIPS Scan pipeline products. A possible target is the HH7-11 region which is a bright source of 100Jy at 50um, with some diffuse gas. Could be an ECO. |
| Description: | Acquire normal scan map observations of the HH 7-11 region over a field 1.0 degree square field. MEDIUM scan rate, 60 arcminute square field, 5 arcmin leg offsets, ONE cycle. Can be the same as: Evaluate fully supported AOTs (MIPS Scan) |
| Day: 78.2951388888905 | Suggested Order: R800 | ||
| Must be preceded by these activities (list by CAID): MIPS-326 | |||
| Place in Schedule: After apertrue door open After CTA/instrument cool down and all other instrument testing is complete. For 160um, the backgrd radiance must be less than 5.4E-13 W/cm2/sr (< 6 - 7 K). After Scan AOT functionality testing is complete. Can be concurrent with other AOT/instrument tests. | |||
| Priority: Desired | |||
Conditions | |||
| Maximum telescope temperature: | 6 K | ||
| Minimum telescope temperature: | 5.5 K | ||
| Should activity be repeated if focus changes? | No Repeat if focus changes by 0 mm | ||
| Maximum absolute pointing uncertainty: | 1.4 arcsec (1 sigma radial) | ||
| Maximum precision offset uncertainty: | 0.4 arcsec (1 sigma radial) | ||
| Observatory configuration: | |||
| Go/No Go criteria: | |||
Duration: 180 minutes
| | Real time downlink:
No | | |||
| Data Volume (uncompressed): 290 Mbits | |||
| List Blocks, AORs, SERs, IERs, or unique sequences required (uplink): Standard pipeline system and standard data analysis tools required. MIPS Scan AOT required for uplink. | |||
| List Analysis tools required (downlink): | |||
| Estimate of data turn around: 0 hours | |||
| Description: Fully calibrated MIPS scan map data products in three bands. | |||
| Can proceed in parallel with other activity: No | |||
| Must outcome be confirmed before next activity: No | |||
| Method of Confirmation: Data analysis | |||
| Success criteria: That we can scan map protostellar regions, obtaining calibrated artifact free images. | |||
| Contingency plan: Revisit pipeline and/or AOT design depending on the nature of failure. | |||
Comments | |||
| References: | |||
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Additional Comments:
Required Conditions: CTA and instrument at nominal operating temperature for 160 micron band (mirror at 6 K). Note: This region has very bright IR sources -- this test can investigate how much of an impact there will be in an AOR. | |||
| This activity last updated: 10/8/2002 9:51:06 AM | |||