The Experts below are selected from a list of 135 Experts worldwide ranked by ideXlab platform
Jennifer G Winters - One of the best experts on this subject based on the ideXlab platform.
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the solar neighborhood xxiii ccd photometric distance estimates of scr targets 77 m dwarf systems within 25 pc
The Astronomical Journal, 2011Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.
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THE SOLAR NEIGHBORHOOD. XXIII. CCD PHOTOMETRIC DISTANCE ESTIMATES OF SCR TARGETS—77 M DWARF SYSTEMS WITHIN 25 pc
The Astronomical Journal, 2010Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, Wei-chun Jao, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.
N C Hambly - One of the best experts on this subject based on the ideXlab platform.
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the solar neighborhood xxiii ccd photometric distance estimates of scr targets 77 m dwarf systems within 25 pc
The Astronomical Journal, 2011Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.
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THE SOLAR NEIGHBORHOOD. XXIII. CCD PHOTOMETRIC DISTANCE ESTIMATES OF SCR TARGETS—77 M DWARF SYSTEMS WITHIN 25 pc
The Astronomical Journal, 2010Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, Wei-chun Jao, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.
Todd J Henry - One of the best experts on this subject based on the ideXlab platform.
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the solar neighborhood xxiii ccd photometric distance estimates of scr targets 77 m dwarf systems within 25 pc
The Astronomical Journal, 2011Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.
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THE SOLAR NEIGHBORHOOD. XXIII. CCD PHOTOMETRIC DISTANCE ESTIMATES OF SCR TARGETS—77 M DWARF SYSTEMS WITHIN 25 pc
The Astronomical Journal, 2010Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, Wei-chun Jao, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.
Charlie T Finch - One of the best experts on this subject based on the ideXlab platform.
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the solar neighborhood xxiii ccd photometric distance estimates of scr targets 77 m dwarf systems within 25 pc
The Astronomical Journal, 2011Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.
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THE SOLAR NEIGHBORHOOD. XXIII. CCD PHOTOMETRIC DISTANCE ESTIMATES OF SCR TARGETS—77 M DWARF SYSTEMS WITHIN 25 pc
The Astronomical Journal, 2010Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, Wei-chun Jao, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.
J P Subasavage - One of the best experts on this subject based on the ideXlab platform.
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the solar neighborhood xxiii ccd photometric distance estimates of scr targets 77 m dwarf systems within 25 pc
The Astronomical Journal, 2011Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.
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THE SOLAR NEIGHBORHOOD. XXIII. CCD PHOTOMETRIC DISTANCE ESTIMATES OF SCR TARGETS—77 M DWARF SYSTEMS WITHIN 25 pc
The Astronomical Journal, 2010Co-Authors: Jennifer G Winters, Todd J Henry, J P Subasavage, Charlie T Finch, Wei-chun Jao, N C HamblyAbstract:We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with μ 0. �� 18 yr −1 , 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using Photographic Plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have π trig 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.