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title: The VLT Survey Telescope ATLAS
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date: Fri Feb 20 09:49:45 CET 2015
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keywords: atlas survey
author: http://lodlaundromat.org/.well-known/genid/2fec4d1f6768938d89199b6977624a27#30
note: cite arxiv:1502.05432Comment: 13 pages, 23 figures, submitted to MNRAS
type: Misc

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note: cite arxiv:1502.05681Comment: 14 Pages. 6 Figures. 2nd revised version. To appear in ApJ. Please contact npirzkal@stsci.edu for comments on this paper
keywords: candidate high-z
year: 2015
abstract: We report on our first set of spectroscopic Hubble Space Telescope observations of the z~11 candidate galaxy strongly lensed by the MACSJ0647.7+7015 galaxy cluster. The three lensed images are faint and we show that these early slitless grism observations are of sufficient depth to investigate whether this high-redshift candidate, identified by its strong photometric break at ~1.5 micron, could possibly be an emission line galaxy at a much lower redshift. While such an interloper would imply the existence of a rather peculiar object, we show here that such strong emission lines would clearly have been detected. Comparing realistic, two-dimensional simulations to these new observations we would expect the necessary emission lines to be detected at >5 sigma while we see no evidence for such lines in the dispersed data of any of the three lensed images. We therefore exclude that this object could be a low redshift emission line interloper, which significantly increases the likelihood of this candidate being a bona fide z~11 galaxy.
date: Fri Feb 20 09:50:08 CET 2015
title: Not In Our Backyard: Spectroscopic Support for the CLASH z=11 Candidate MACS0647-JD
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note: cite arxiv:1502.05681Comment: 14 Pages. 6 Figures. 2nd revised version. To appear in ApJ. Please contact npirzkal@stsci.edu for comments on this paper
keywords: candidate high-z
year: 2015
abstract: We report on our first set of spectroscopic Hubble Space Telescope observations of the z~11 candidate galaxy strongly lensed by the MACSJ0647.7+7015 galaxy cluster. The three lensed images are faint and we show that these early slitless grism observations are of sufficient depth to investigate whether this high-redshift candidate, identified by its strong photometric break at ~1.5 micron, could possibly be an emission line galaxy at a much lower redshift. While such an interloper would imply the existence of a rather peculiar object, we show here that such strong emission lines would clearly have been detected. Comparing realistic, two-dimensional simulations to these new observations we would expect the necessary emission lines to be detected at >5 sigma while we see no evidence for such lines in the dispersed data of any of the three lensed images. We therefore exclude that this object could be a low redshift emission line interloper, which significantly increases the likelihood of this candidate being a bona fide z~11 galaxy.
date: Fri Feb 20 09:50:08 CET 2015
title: Not In Our Backyard: Spectroscopic Support for the CLASH z=11 Candidate MACS0647-JD
type: Misc
author: http://lodlaundromat.org/.well-known/genid/2fec4d1f6768938d89199b6977624a27#14

http://arxiv.org/abs/1502.05432
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title: The VLT Survey Telescope ATLAS
year: 2015
date: Fri Feb 20 09:49:45 CET 2015
abstract: The VLT Survey Telescope (VST) ATLAS is an optical ugriz survey aiming to cover ~4700deg^2 of the Southern sky to similar depths as the Sloan Digital Sky Survey (SDSS). From reduced images and object catalogues provided by the Cambridge Astronomical Surveys Unit we first find that the median seeing ranges from 0.8 arcsec FWHM in i to 1.0 arcsec in u, significantly better than the 1.2-1.5 arcsec seeing for SDSS. The 5 sigma magnitude limit for stellar sources is r_AB=22.7 and in all bands these limits are at least as faint as SDSS. SDSS and ATLAS are more equivalent for galaxy photometry except in the z band where ATLAS has significantly higher throughput. We have improved the original ESO magnitude zeropoints by comparing m<16 star magnitudes with APASS in gri, also extrapolating into u and z, resulting in zeropoints accurate to ~+-0.02 mag. We finally compare star and galaxy number counts in a 250deg^2 area with SDSS and other count data and find good agreement. ATLAS data products can be retrieved from the ESO Science Archive, while support for survey science analyses is provided by the OmegaCAM Science Archive (OSA), operated by the Wide-Field Astronomy Unit in Edinburgh.
keywords: atlas survey
author: http://lodlaundromat.org/.well-known/genid/2fec4d1f6768938d89199b6977624a27#30
note: cite arxiv:1502.05432Comment: 13 pages, 23 figures, submitted to MNRAS
type: Misc

flint63
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pages: 32-35
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journal: Communications of the ACM
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month: #mar#
abstract: It seems like a paradox but it will soon become reality: The rate at which computers disappear will be matched by the rate at which information technology will increasingly permeate our environment and our lives. This article provides an introduction to the special issue of CACM.
keywords: v1500 acm paper embedded ai device user interaction application zzz.ami zzz.iot
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miki
title: The VLT Survey Telescope ATLAS
year: 2015
date: Fri Feb 20 09:49:45 CET 2015
abstract: The VLT Survey Telescope (VST) ATLAS is an optical ugriz survey aiming to cover ~4700deg^2 of the Southern sky to similar depths as the Sloan Digital Sky Survey (SDSS). From reduced images and object catalogues provided by the Cambridge Astronomical Surveys Unit we first find that the median seeing ranges from 0.8 arcsec FWHM in i to 1.0 arcsec in u, significantly better than the 1.2-1.5 arcsec seeing for SDSS. The 5 sigma magnitude limit for stellar sources is r_AB=22.7 and in all bands these limits are at least as faint as SDSS. SDSS and ATLAS are more equivalent for galaxy photometry except in the z band where ATLAS has significantly higher throughput. We have improved the original ESO magnitude zeropoints by comparing m<16 star magnitudes with APASS in gri, also extrapolating into u and z, resulting in zeropoints accurate to ~+-0.02 mag. We finally compare star and galaxy number counts in a 250deg^2 area with SDSS and other count data and find good agreement. ATLAS data products can be retrieved from the ESO Science Archive, while support for survey science analyses is provided by the OmegaCAM Science Archive (OSA), operated by the Wide-Field Astronomy Unit in Edinburgh.
keywords: atlas survey
author: http://lodlaundromat.org/.well-known/genid/2fec4d1f6768938d89199b6977624a27#30
note: cite arxiv:1502.05432Comment: 13 pages, 23 figures, submitted to MNRAS
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http://arxiv.org/abs/1502.05681
note: cite arxiv:1502.05681Comment: 14 Pages. 6 Figures. 2nd revised version. To appear in ApJ. Please contact npirzkal@stsci.edu for comments on this paper
keywords: candidate high-z
year: 2015
abstract: We report on our first set of spectroscopic Hubble Space Telescope observations of the z~11 candidate galaxy strongly lensed by the MACSJ0647.7+7015 galaxy cluster. The three lensed images are faint and we show that these early slitless grism observations are of sufficient depth to investigate whether this high-redshift candidate, identified by its strong photometric break at ~1.5 micron, could possibly be an emission line galaxy at a much lower redshift. While such an interloper would imply the existence of a rather peculiar object, we show here that such strong emission lines would clearly have been detected. Comparing realistic, two-dimensional simulations to these new observations we would expect the necessary emission lines to be detected at >5 sigma while we see no evidence for such lines in the dispersed data of any of the three lensed images. We therefore exclude that this object could be a low redshift emission line interloper, which significantly increases the likelihood of this candidate being a bona fide z~11 galaxy.
date: Fri Feb 20 09:50:08 CET 2015
title: Not In Our Backyard: Spectroscopic Support for the CLASH z=11 Candidate MACS0647-JD
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