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1472465_-Table_1_Array_performance_and_key_science_projects_

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Table 1: Array Performance and Key Science Projects

Array

Date

Beam Size (arcsec)

S{{sub|rms}} (mJy)

Speed (deg{{sup|2}}s{{sup|-1}})

Key Science

ATA-42

Nov, 2005

245 x 118

0.54

0.02

FiGSS: 5 GHz Continuum Survey, Galactic Plane Molecular Spectroscopy , SETI Galactic Center Survey

ATA-98

July, 2006

120 x 80

0.23

0.11

ATHIXS† Trial Surveys, HI Stellar Outflows Survey, SETI Targeted Survey: 100 stars

ATA-206

April, 2007

75 x 65

0.11

0.44

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array, Deep continuum and transient surveys, SETI Targeted Surveys

ATA-350

June, 2008

77 x 66

0.065

1.40

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array Deep continuum and transient surveys, SETI Targeted Surveys

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Table 1: Array performance and key science projects

Array

Status

Beam size (arcsec)

Srms (mJy)

Speed (deg²s−1)

Key science

ATA-42

Dish construction complete; commissioning in progress with 32 input, dual polarization (64 total inputs) correlator.

245 x 118

0.54

0.02

FiGSS: 5 GHz Continuum Survey, Galactic Plane Molecular Spectroscopy, SETI Galactic Center Survey

ATA-98

Awaiting results ATA-42 for funding

120 x 80

0.2

0.11

ATHIXS† Trial Surveys, HI Stellar Outflows Survey, SETI Targeted Survey: 100 stars

ATA-206

TBD

75 x 65

0.11

0.44

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array, Deep continuum and transient surveys, SETI Targeted Surveys

ATA-350

TBD

77 x 66

0.065

1.40

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array Deep continuum and transient surveys, SETI Targeted Surveys

Note. Beam size and continuum sensitivity (Srms are estimated for a 6 minute, 100 MHz continuum snapshot observation at transit of a source at 40° declination at a wavelength of 21 cm. Speed is given for a survey at 21 cm observations with a bandwidth of 100 MHz that reaches 1 mJy rms. †ATHIXS is an all-sky deep HI extragalactic HI survey.


Revision 667604339 at Fri Jun 19 11:14:09 CEST 2015 Diff at Wikipedia Position: 0

UNIQUE_ 2c158d81-96a7-46d4-8f11-1ab7e6c9c1dd d3705870-b206-48b5-8060-2836d598ad82 UNIQUE_ c2eacdb2-93b4-4083-b829-a7011bdbb8ad UNIQUE_ 72c37c27-fd99-4f7a-b80a-15ace161c8bb UNIQUE_ 2001ec97-e441-455d-aee0-b134572d75d5 UNIQUE_ 86aa0d16-41f9-4a49-a30b-82589c59ee9a

Table 1: Array performance and key science projects

Array

Status

Beam size (arcsec)

Srms (mJy)

Speed (deg²s−1)

Key science

ATA-42

Dish construction complete; commissioning in progress with 32 input, dual polarization (64 total inputs) correlator.

245 x 118

0.54

0.02

FiGSS: 5 GHz Continuum Survey, Galactic Plane Molecular Spectroscopy, SETI Galactic Center Survey

ATA-98

Awaiting results ATA-42 for funding

120 x 80

0.2

0.11

ATHIXS† Trial Surveys, HI Stellar Outflows Survey, SETI Targeted Survey: 100 stars

ATA-206

TBD

75 x 65

0.11

0.44

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array, Deep continuum and transient surveys, SETI Targeted Surveys

ATA-350

TBD

77 x 66

0.065

1.40

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array Deep continuum and transient surveys, SETI Targeted Surveys

Note. Beam size and continuum sensitivity (Srms are estimated for a 6-minute, 100 MHz continuum snapshot observation at transit of a source at 40° declination at a wavelength of 21 cm. Speed is given for a survey at 21 cm observations with a bandwidth of 100 MHz that reaches 1 mJy rms. †ATHIXS is an all-sky deep HI extragalactic HI survey.


Revision 707634864 at Tue Mar 01 00:22:56 CET 2016 Diff at Wikipedia Position: 0

UNIQUE_ 2c158d81-96a7-46d4-8f11-1ab7e6c9c1dd UNIQUE_ d3705870-b206-48b5-8060-2836d598ad82 UNIQUE_ c2eacdb2-93b4-4083-b829-a7011bdbb8ad UNIQUE_ 72c37c27-fd99-4f7a-b80a-15ace161c8bb UNIQUE_ 2001ec97-e441-455d-aee0-b134572d75d5 UNIQUE_ 86aa0d16-41f9-4a49-a30b-82589c59ee9a

Table 1: Array performance and key science projects

Array

Status

Beam size (arcsec)

Srms (mJy)

Speed (deg²s−1)

Key science

ATA-42

Dish construction complete; commissioning in progress with 32 input, dual polarization (64 total inputs) correlator

245 x 118

0.54

0.02

FiGSS: 5 GHz Continuum Survey, Galactic Plane Molecular Spectroscopy, SETI Galactic Center Survey

ATA-98

Awaiting results ATA-42 for funding

120 x 80

0.2

0.11

ATHIXS† Trial Surveys, HI Stellar Outflows Survey, SETI Targeted Survey: 100 stars

ATA-206

TBD{{what?|date=February 2016}}

75 x 65

0.11

0.44

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array, Deep continuum and transient surveys, SETI Targeted Surveys

ATA-350

TBD

77 x 66

0.065

1.40

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array Deep continuum and transient surveys, SETI Targeted Surveys

Note: Beam size and continuum sensitivity (Srms are estimated for a 6-minute, 100 MHz continuum snapshot observation at transit of a source at 40° declination at a wavelength of 21 cm. Speed is given for a survey at 21 cm observations with a bandwidth of 100 MHz that reaches 1 mJy rms. †ATHIXS is an all-sky deep HI extragalactic HI survey.

Revision 707930334 at Wed Mar 02 18:03:28 CET 2016 Diff at Wikipedia Position: 0

UNIQUE_ 2c158d81-96a7-46d4-8f11-1ab7e6c9c1dd d3705870-b206-48b5-8060-2836d598ad82 UNIQUE_ c2eacdb2-93b4-4083-b829-a7011bdbb8ad UNIQUE_ 72c37c27-fd99-4f7a-b80a-15ace161c8bb UNIQUE_ 2001ec97-e441-455d-aee0-b134572d75d5 UNIQUE_ 86aa0d16-41f9-4a49-a30b-82589c59ee9a

Table 1: Array performance and key science projects

Array

Status

Beam size (arcsec)

Srms (mJy)

Speed (deg²s−1)

Key science

ATA-42

Dish construction complete; commissioning in progress with 32 input, dual polarization (64 total inputs) correlator

245 x 118

0.54

0.02

FiGSS: 5 GHz Continuum Survey, Galactic Plane Molecular Spectroscopy, SETI Galactic Center Survey

ATA-98

Awaiting results ATA-42 for funding

120 x 80

0.2

0.11

ATHIXS† Trial Surveys, HI Stellar Outflows Survey, SETI Targeted Survey: 100 stars

ATA-206

Development phase not completed

75 x 65

0.11

0.44

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array, Deep continuum and transient surveys, SETI Targeted Surveys

ATA-350

Development phase not completed

77 x 66

0.065

1.40

ATHIXS, Map The Magnetized Galactic ISM, Pulsar Timing Array Deep continuum and transient surveys, SETI Targeted Surveys

Note: Beam size and continuum sensitivity (Srms are estimated for a 6-minute, 100 MHz continuum snapshot observation at transit of a source at 40° declination at a wavelength of 21 cm. Speed is given for a survey at 21 cm observations with a bandwidth of 100 MHz that reaches 1 mJy rms. †ATHIXS is an all-sky deep HI extragalactic HI survey.