'Vlba' web sites
New vlba site
www.vlba.nrao.edu 2013-03-12
vlba Site National RadioAstronomy Observatory NRAO Home vlba Information For Astronomers Teachers Students Useful Links Very Large Array VLA VLA Expansion Project EVLA Press Releases Image Gallery Frequently Asked Questions EPO newsletters Assistant Director Page VLA Welcome to the Very Long Baseline Array. The vlba is a system of ten radio.telescope antennas,each with a dish 25 meters 82 feet in diameter and weighing 240 tons.
www.vlba.nrao.edu 2013-03-12
vlba Site National RadioAstronomy Observatory NRAO Home vlba Information For Astronomers Teachers Students Useful Links Very Large Array VLA VLA Expansion Project EVLA Press Releases Image Gallery Frequently Asked Questions EPO newsletters Assistant Director Page VLA Welcome to the Very Long Baseline Array. The vlba is a system of ten radio.telescope antennas,each with a dish 25 meters 82 feet in diameter and weighing 240 tons.
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Known problems with e vla and vlba archival data
vlba archival data Known problems with E VLA and vlba archival data This page was last updated on 2015 Jun 19 10 56 MDT to keep track of known problems that affected data taken with the VLA EVLA and or the vlba that appears and is remaining either in the data archive, or in the programs reading the data archive into the data reduction packages. For current problems that are affecting current data, and thus also are not fixed in
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Nrao very long baseline array teachers and students
vlba Teachers and Students Information For Astronomers Teachers Students Useful Links Very Large Array VLA Press Releases Image Gallery Frequently Asked Questions EPO newsletters Assistant Director Page VLA Information for Teachers and Students A variety of programs is available for teachers and students at the Very Large Array or through the National Radio Astronomy Observatory at several of our locations. The majority of our
Welcome. university of iowa astronomy and astrophysics. robert mutel
astro.physics.uiowa.edu 2015-08-13 ⚑r&d
vlba , and the Arecibo Observatory. We are also frequent users of space.based facilities including the Chandra X.ray Observatory, the XMM.Newton X.ray Observatory, and the Hubble Space Telescope. In addition, we have active programs in the development of radio and X.ray instrumentation and are currently involved preparing a rocket flight for soft X.ray spectroscopy. We offer undergraduate B.S., B.A. degrees in astronomy and
astro.physics.uiowa.edu 2015-08-13 ⚑r&d
vlba , and the Arecibo Observatory. We are also frequent users of space.based facilities including the Chandra X.ray Observatory, the XMM.Newton X.ray Observatory, and the Hubble Space Telescope. In addition, we have active programs in the development of radio and X.ray instrumentation and are currently involved preparing a rocket flight for soft X.ray spectroscopy. We offer undergraduate B.S., B.A. degrees in astronomy and
European vlbi network newsletter 17. may 2007
www.ira.inaf.it 2015-08-13 ⚑tech ⚑music
vlba terminals, are becoming obsolete. Plans has been made to face this serious problem. But again, there are difficulties in coordinating the efforts to move faster towards new solutions. New backends have been designed in the recent past based on the huge progresses made by digital technology. EVN has endorsed a project called Digital Base Band Converters. Haystack is developing the so called DBE and NRAO is working, in
www.ira.inaf.it 2015-08-13 ⚑tech ⚑music
vlba terminals, are becoming obsolete. Plans has been made to face this serious problem. But again, there are difficulties in coordinating the efforts to move faster towards new solutions. New backends have been designed in the recent past based on the huge progresses made by digital technology. EVN has endorsed a project called Digital Base Band Converters. Haystack is developing the so called DBE and NRAO is working, in
Vlbi. e.merlin
www.e-merlin.ac.uk 2015-08-13 ⚑music
vlba , the GBT, and or the VLA telescopes in the U.S. Additionally the MERLIN and now e.MERLIN array often observes alongside the rest of the EVN in joint MERLIN and EVN experiments. The combination of these two unique arrays is massively complementary, with the MERLIN e.MERLIN array providing vital short.spacing data increasing the EVN sensitivity to larger scale emission. EVN Proposals EVN proposals should be submitted via the
www.e-merlin.ac.uk 2015-08-13 ⚑music
vlba , the GBT, and or the VLA telescopes in the U.S. Additionally the MERLIN and now e.MERLIN array often observes alongside the rest of the EVN in joint MERLIN and EVN experiments. The combination of these two unique arrays is massively complementary, with the MERLIN e.MERLIN array providing vital short.spacing data increasing the EVN sensitivity to larger scale emission. EVN Proposals EVN proposals should be submitted via the
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Technical capabilities. e.merlin
vlba Calibrator Survey 0.5 0.2 1 Day.to.day repeatability using surveyed or in.beam sources, and assuming full imaging run. Amplitude calibration 2 1 10 Targets for day.to.day repeatability Notes 1 The Lovell telescope may be included in e.MERLIN at 1.5 and 5 GHz L, C. Its inclusion increases the sensitivity by a factor of between 2 and 3 and reduces the field of view to approximately 20 freq 1.4GHz arcmin, depending on the
Hawaii astronomy archive at hawaii astronomy
www.hawaiiastronomy.com 2012-03-08 ⚑r&d ⚑blog ⚑travel
vlba .25 meters Published by Hawaii Astronomy on June 24, 2008 in Mauna Kea Observatories and Radio. 0 Comments The vlba in consisted of ten radio.telescope antennas, each is a dish with 25 meters in diameter and weighing 240 tons. Located in Mauna Kea, Hawaii, this observatory spans 5,000 miles to St. Croix in the U.S., providing astronomers with the sharpest view of any telescopes in Earth or in space. This site was built in
www.hawaiiastronomy.com 2012-03-08 ⚑r&d ⚑blog ⚑travel
vlba .25 meters Published by Hawaii Astronomy on June 24, 2008 in Mauna Kea Observatories and Radio. 0 Comments The vlba in consisted of ten radio.telescope antennas, each is a dish with 25 meters in diameter and weighing 240 tons. Located in Mauna Kea, Hawaii, this observatory spans 5,000 miles to St. Croix in the U.S., providing astronomers with the sharpest view of any telescopes in Earth or in space. This site was built in
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Hawaii astronomy
vlba .25 meters Published by Hawaii Astronomy on June 24, 2008 in Mauna Kea Observatories and Radio. 0 Comments The vlba in consisted of ten radio.telescope antennas, each is a dish with 25 meters in diameter and weighing 240 tons. Located in Mauna Kea, Hawaii, this observatory spans 5,000 miles to St. Croix in the U.S., providing astronomers with the sharpest view of any telescopes in Earth or in space. This site was built in
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About astronomy at hawaii astronomy
vlba .25 meters Submillimeter Array SMA. 8 6meters James Clerk Maxwell Telescope JCMT.15 meters Caltech Submillimeter Observatory CSO.10.4 meters Gemini Northern Telescope 8.1 meters Subaru Telescope 8.2 Meters W. M. Keck Observatory Keck I and Keck II.10 meters United Kingdom Infrared Telescope UKIRT.3.8 meters Canada.France.Hawaii Telescope CFHT.3.6 meters NASA Infrared Telescope Facility IRTF University of Hawaii UH.2.2
Http://www.rigel.org.uk
www.rigel.org.uk 2015-05-10
vlba , and I m leading a project to investigate a strange class of objects which are compact and have ultra.steep radio spectra we currently do not know what they are. I m also very involved with e.MERLIN, having helped with the commissioning efforts, and now as a collaborator on several of the Legacy programmes, as PI of several regular observing projects, writing and maintaining the data reduction pipeline, scheduling, and acting
www.rigel.org.uk 2015-05-10
vlba , and I m leading a project to investigate a strange class of objects which are compact and have ultra.steep radio spectra we currently do not know what they are. I m also very involved with e.MERLIN, having helped with the commissioning efforts, and now as a collaborator on several of the Legacy programmes, as PI of several regular observing projects, writing and maintaining the data reduction pipeline, scheduling, and acting
Publications. sciplore
www.sciplore.org 2012-11-28 ⚑r&d
vlba Systemlandschaften der Zukunft, chapter E ntwicklung neuer V erfahren zur B estimmung von D okumentenaehnlichkeiten mittels R eferenz. und Z itationsanalyse, pages 163.173. 3. Workshop des Centers for Very Large Business Applications C vlba . Shaker Verlag, Magdeburg, oct 2009. Available at http sciplore.org pub Bibtex INBOOK Gipp09b, chapter E ntwicklung neuer V erfahren zur B estimmung von D okumentenaehnlichkeiten mittels R
www.sciplore.org 2012-11-28 ⚑r&d
vlba Systemlandschaften der Zukunft, chapter E ntwicklung neuer V erfahren zur B estimmung von D okumentenaehnlichkeiten mittels R eferenz. und Z itationsanalyse, pages 163.173. 3. Workshop des Centers for Very Large Business Applications C vlba . Shaker Verlag, Magdeburg, oct 2009. Available at http sciplore.org pub Bibtex INBOOK Gipp09b, chapter E ntwicklung neuer V erfahren zur B estimmung von D okumentenaehnlichkeiten mittels R
Juan cabanela cirriculum vitae
astronomy.mnstate.edu 2013-03-18 ⚑r&d ⚑blog
vlba , ASP Conference Series, Vol. 340, eds. Jonathan D. Romney and Mark J. Reid, 89. Mining Astronomical Databases , Humphreys, R.M., Cabanela, J.E. and Kriessler, J. 2001, in Data Mining for Scientific and Engineering Applications ed. Kamath, C., Kegelmeyer, P., Kumar, V., and Namburu, R. Kluwer Academic Press. The New Luyten Proper Motion Survey, Humphreys, R.M., Cornuelle, C.S., Larsen, J.A., Aldering, G., and Cabanela, J.E.
astronomy.mnstate.edu 2013-03-18 ⚑r&d ⚑blog
vlba , ASP Conference Series, Vol. 340, eds. Jonathan D. Romney and Mark J. Reid, 89. Mining Astronomical Databases , Humphreys, R.M., Cabanela, J.E. and Kriessler, J. 2001, in Data Mining for Scientific and Engineering Applications ed. Kamath, C., Kegelmeyer, P., Kumar, V., and Namburu, R. Kluwer Academic Press. The New Luyten Proper Motion Survey, Humphreys, R.M., Cornuelle, C.S., Larsen, J.A., Aldering, G., and Cabanela, J.E.
Downrange
www.spacecalendar.com 2012-05-22 ⚑finance
vlba , David Thompson. Jun 6.8 NASA Lunar Science Institute 8211; Colorado Center For Lunar Dust and Atmospheric Studies, Boulder CO Dust, Atmosphere and Plasma Moon and Small Bodies. 8217; Jun 6.15 United Nations Office for Outer Space Affairs, Vienna, Austria 8216;55th Committee on the Peaceful Uses of Outer Space Meeting. 8217; Jun 8 8211; Jul 10 American Astronomical Society, NASA, et al, Cross Plains TX Student CanSat
www.spacecalendar.com 2012-05-22 ⚑finance
vlba , David Thompson. Jun 6.8 NASA Lunar Science Institute 8211; Colorado Center For Lunar Dust and Atmospheric Studies, Boulder CO Dust, Atmosphere and Plasma Moon and Small Bodies. 8217; Jun 6.15 United Nations Office for Outer Space Affairs, Vienna, Austria 8216;55th Committee on the Peaceful Uses of Outer Space Meeting. 8217; Jun 8 8211; Jul 10 American Astronomical Society, NASA, et al, Cross Plains TX Student CanSat
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Nrao very long baseline array teachers and students
vlba Teachers and Students Information For Astronomers Teachers Students Useful Links Very Large Array VLA Press Releases Image Gallery Frequently Asked Questions EPO newsletters Assistant Director Page VLA Information for Teachers and Students A variety of programs is available for teachers and students at the Very Large Array or through the National Radio Astronomy Observatory at several of our locations. The majority of our
European vlbi network newsletter 17. may 2007
www.ira.inaf.it 2015-08-13 ⚑tech ⚑music
vlba terminals, are becoming obsolete. Plans has been made to face this serious problem. But again, there are difficulties in coordinating the efforts to move faster towards new solutions. New backends have been designed in the recent past based on the huge progresses made by digital technology. EVN has endorsed a project called Digital Base Band Converters. Haystack is developing the so called DBE and NRAO is working, in
www.ira.inaf.it 2015-08-13 ⚑tech ⚑music
vlba terminals, are becoming obsolete. Plans has been made to face this serious problem. But again, there are difficulties in coordinating the efforts to move faster towards new solutions. New backends have been designed in the recent past based on the huge progresses made by digital technology. EVN has endorsed a project called Digital Base Band Converters. Haystack is developing the so called DBE and NRAO is working, in
Vlbi. e.merlin
www.e-merlin.ac.uk 2015-08-13 ⚑music
vlba , the GBT, and or the VLA telescopes in the U.S. Additionally the MERLIN and now e.MERLIN array often observes alongside the rest of the EVN in joint MERLIN and EVN experiments. The combination of these two unique arrays is massively complementary, with the MERLIN e.MERLIN array providing vital short.spacing data increasing the EVN sensitivity to larger scale emission. EVN Proposals EVN proposals should be submitted via the
www.e-merlin.ac.uk 2015-08-13 ⚑music
vlba , the GBT, and or the VLA telescopes in the U.S. Additionally the MERLIN and now e.MERLIN array often observes alongside the rest of the EVN in joint MERLIN and EVN experiments. The combination of these two unique arrays is massively complementary, with the MERLIN e.MERLIN array providing vital short.spacing data increasing the EVN sensitivity to larger scale emission. EVN Proposals EVN proposals should be submitted via the
MORE
ⓘ
Technical capabilities. e.merlin
vlba Calibrator Survey 0.5 0.2 1 Day.to.day repeatability using surveyed or in.beam sources, and assuming full imaging run. Amplitude calibration 2 1 10 Targets for day.to.day repeatability Notes 1 The Lovell telescope may be included in e.MERLIN at 1.5 and 5 GHz L, C. Its inclusion increases the sensitivity by a factor of between 2 and 3 and reduces the field of view to approximately 20 freq 1.4GHz arcmin, depending on the
Hawaii astronomy archive at hawaii astronomy
www.hawaiiastronomy.com 2012-03-08 ⚑r&d ⚑blog ⚑travel
vlba .25 meters Published by Hawaii Astronomy on June 24, 2008 in Mauna Kea Observatories and Radio. 0 Comments The vlba in consisted of ten radio.telescope antennas, each is a dish with 25 meters in diameter and weighing 240 tons. Located in Mauna Kea, Hawaii, this observatory spans 5,000 miles to St. Croix in the U.S., providing astronomers with the sharpest view of any telescopes in Earth or in space. This site was built in
www.hawaiiastronomy.com 2012-03-08 ⚑r&d ⚑blog ⚑travel
vlba .25 meters Published by Hawaii Astronomy on June 24, 2008 in Mauna Kea Observatories and Radio. 0 Comments The vlba in consisted of ten radio.telescope antennas, each is a dish with 25 meters in diameter and weighing 240 tons. Located in Mauna Kea, Hawaii, this observatory spans 5,000 miles to St. Croix in the U.S., providing astronomers with the sharpest view of any telescopes in Earth or in space. This site was built in
MORE
ⓘ
Hawaii astronomy
vlba .25 meters Published by Hawaii Astronomy on June 24, 2008 in Mauna Kea Observatories and Radio. 0 Comments The vlba in consisted of ten radio.telescope antennas, each is a dish with 25 meters in diameter and weighing 240 tons. Located in Mauna Kea, Hawaii, this observatory spans 5,000 miles to St. Croix in the U.S., providing astronomers with the sharpest view of any telescopes in Earth or in space. This site was built in
Juan cabanela cirriculum vitae
astronomy.mnstate.edu 2013-03-18 ⚑r&d ⚑blog
vlba , ASP Conference Series, Vol. 340, eds. Jonathan D. Romney and Mark J. Reid, 89. Mining Astronomical Databases , Humphreys, R.M., Cabanela, J.E. and Kriessler, J. 2001, in Data Mining for Scientific and Engineering Applications ed. Kamath, C., Kegelmeyer, P., Kumar, V., and Namburu, R. Kluwer Academic Press. The New Luyten Proper Motion Survey, Humphreys, R.M., Cornuelle, C.S., Larsen, J.A., Aldering, G., and Cabanela, J.E.
astronomy.mnstate.edu 2013-03-18 ⚑r&d ⚑blog
vlba , ASP Conference Series, Vol. 340, eds. Jonathan D. Romney and Mark J. Reid, 89. Mining Astronomical Databases , Humphreys, R.M., Cabanela, J.E. and Kriessler, J. 2001, in Data Mining for Scientific and Engineering Applications ed. Kamath, C., Kegelmeyer, P., Kumar, V., and Namburu, R. Kluwer Academic Press. The New Luyten Proper Motion Survey, Humphreys, R.M., Cornuelle, C.S., Larsen, J.A., Aldering, G., and Cabanela, J.E.
Hawaii astronomy archive at hawaii astronomy
www.hawaiiastronomy.com 2012-03-08 ⚑r&d ⚑blog ⚑travel
vlba .25 meters Published by Hawaii Astronomy on June 24, 2008 in Mauna Kea Observatories and Radio. 0 Comments The vlba in consisted of ten radio.telescope antennas, each is a dish with 25 meters in diameter and weighing 240 tons. Located in Mauna Kea, Hawaii, this observatory spans 5,000 miles to St. Croix in the U.S., providing astronomers with the sharpest view of any telescopes in Earth or in space. This site was built in
www.hawaiiastronomy.com 2012-03-08 ⚑r&d ⚑blog ⚑travel
vlba .25 meters Published by Hawaii Astronomy on June 24, 2008 in Mauna Kea Observatories and Radio. 0 Comments The vlba in consisted of ten radio.telescope antennas, each is a dish with 25 meters in diameter and weighing 240 tons. Located in Mauna Kea, Hawaii, this observatory spans 5,000 miles to St. Croix in the U.S., providing astronomers with the sharpest view of any telescopes in Earth or in space. This site was built in
MORE
ⓘ
Hawaii astronomy
vlba .25 meters Published by Hawaii Astronomy on June 24, 2008 in Mauna Kea Observatories and Radio. 0 Comments The vlba in consisted of ten radio.telescope antennas, each is a dish with 25 meters in diameter and weighing 240 tons. Located in Mauna Kea, Hawaii, this observatory spans 5,000 miles to St. Croix in the U.S., providing astronomers with the sharpest view of any telescopes in Earth or in space. This site was built in
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