chilesconpol.com

CHILES Continuum Polarization

An ultra-deep radio survey in COSMOS. CHILES Con Pol is a full-polarization continuum radio survey at 1.4 GHz covering 0.2 square degrees of the COSMOS. Field The survey is being performed with the Karl G. Jansky. Very Large Array (VLA). Deep drilling on a single pointing in B configuration for a total of 1000 hours. The field center is located at (J2000) R.A. 10:01:24.0 Decl. 2:21:00.0, corresponding to Galactic coordinates Long. 236.8 Lat. 42.4. Tab above for more details. We invite the astronomical co...

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CHILES Continuum Polarization | chilesconpol.com Reviews

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An ultra-deep radio survey in COSMOS. CHILES Con Pol is a full-polarization continuum radio survey at 1.4 GHz covering 0.2 square degrees of the COSMOS. Field The survey is being performed with the Karl G. Jansky. Very Large Array (VLA). Deep drilling on a single pointing in B configuration for a total of 1000 hours. The field center is located at (J2000) R.A. 10:01:24.0 Decl. 2:21:00.0, corresponding to Galactic coordinates Long. 236.8 Lat. 42.4. Tab above for more details. We invite the astronomical co...

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CHILES Continuum Polarization | chilesconpol.com Reviews

https://chilesconpol.com

An ultra-deep radio survey in COSMOS. CHILES Con Pol is a full-polarization continuum radio survey at 1.4 GHz covering 0.2 square degrees of the COSMOS. Field The survey is being performed with the Karl G. Jansky. Very Large Array (VLA). Deep drilling on a single pointing in B configuration for a total of 1000 hours. The field center is located at (J2000) R.A. 10:01:24.0 Decl. 2:21:00.0, corresponding to Galactic coordinates Long. 236.8 Lat. 42.4. Tab above for more details. We invite the astronomical co...

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chilesconpol.com

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CHILES Continuum Polarization

http://www.chilesconpol.com/acknowledgements.html

An ultra-deep radio survey in COSMOS. The National Radio Astronomy Observatory (NRAO). Is a facility of the National Science Foundation (NSF). Operated under cooperative agreement by Associated Universities, Inc. Work at Columbia University. Is supported in part by the National Science Foundation (NSF). Through AST Grant No. 1413102. Work at Michigan State University. Is supported in part by the National Science Foundation (NSF). Through AST Grant No. 1412980. Work at UMass Amherst. The John Fell Fund.

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CHILES Continuum Polarization

http://www.chilesconpol.com/publications.html

An ultra-deep radio survey in COSMOS. 2015 CHILES Con Pol Collaboration Design: TEMPLATED.

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CHILES Continuum Polarization

http://www.chilesconpol.com/data.html

An ultra-deep radio survey in COSMOS. We will publish Data Release 1 in 2018. This will be based on the first 180 hours of observational data in total intensity only. DR1 will contain images and a multi-wavelength cross-matched source catalog, and will be presented alongside key scientific findings from our team. We will publish Data Release 2 in 2021. This final data release will present results from the complete 1000 hours of observational data in full polarization.

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CHILES Continuum Polarization

http://www.chilesconpol.com/news.html

An ultra-deep radio survey in COSMOS. Observations for the 2016 B-configuration are now complete. This brings our total observing time to 610 hours. Only 2 more B-configurations to go! Observations for the 2016 B-configuration have commenced. Today marks the public release of a new CASA task called invgain. This task will invert the gain solutions in a caltable. Invgain is needed to enable direction-dependent calibration for peeling outlier sources in our field of view.

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CHILES Continuum Polarization

http://www.chilesconpol.com/index.html

An ultra-deep radio survey in COSMOS. CHILES Con Pol is a full-polarization continuum radio survey at 1.4 GHz covering 0.2 square degrees of the COSMOS. Field The survey is being performed with the Karl G. Jansky. Very Large Array (VLA). Deep drilling on a single pointing in B configuration for a total of 1000 hours. The field center is located at (J2000) R.A. 10:01:24.0 Decl. 2:21:00.0, corresponding to Galactic coordinates Long. 236.8 Lat. 42.4. Tab above for more details. We invite the astronomical co...

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https://4pisky.org/projects

Exploring the transient universe. The AMI Large Array Rapid Response Mode. Target of opportunity follow-up of transients with radio facilities is for the most part a manual affair, and as a result radio follow-up observations are not normally obtained until hours or even days after an initial discovery in another waveband. ALARRM is a uniquely long-running fully automated radio response programme, jointly operated between the 4PiSky group and the MRAO. To robotically trigger on. The ALARRM programme also...

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CHILES Continuum Polarization

An ultra-deep radio survey in COSMOS. CHILES Con Pol is a full-polarization continuum radio survey at 1.4 GHz covering 0.2 square degrees of the COSMOS. Field The survey is being performed with the Karl G. Jansky. Very Large Array (VLA). Deep drilling on a single pointing in B configuration for a total of 1000 hours. The field center is located at (J2000) R.A. 10:01:24.0 Decl. 2:21:00.0, corresponding to Galactic coordinates Long. 236.8 Lat. 42.4. Tab above for more details. We invite the astronomical co...

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