A search for the lenses in the Herschel Bright Sources (HerBS) sample

A search for the lenses in the Herschel Bright Sources (HerBS) sample
复制标题

搜索 Herschel Bright Sources (HerBS) 样本中的镜片

DOI：
10.1093/mnras/staa506
复制
发表时间：
2020
期刊：
Monthly Notices of the Royal Astronomical Society
影响因子：
4.8
通讯作者：
Bakx T
Bakx T
中科院分区：
物理与天体物理2区
文献类型：
--
作者：
Bakx T

文献摘要

参考文献

被引文献

相似文献

验证亚毫米星系是引力透镜需要花费大量时间和高分辨率天文台进行观测。在这里，我们的目标是通过与光学（SDSS）和近红外（VIKING）调查的交叉比较，加强赫歇尔亮源（草本）中引力透镜的证据，以寻找前景透镜星系候选者。对最亮的草本源的分辨率观测已经表明，大多数草本源是透镜状的，一个星系演化模型预测，大约76%的草本源是透镜状的，尽管通过SDSS调查，我们只能识别25%的源可能的前景透镜。然而，通过近红外VIKING调查，我们能够识别57%的源可能的前景透镜，我们估计82%的HerBS源在VIKING图像上有透镜，即使我们不能在每种情况下识别透镜。我们发现透镜和赫歇尔源之间的角偏移比预期的要大，如果透镜是由单个星系完成的。我们还发现，透镜状草本源的比例随着500微米通量密度的降低而下降，这是星系演化模型所期望的。最后，我们将统计维京交叉识别应用到整个赫歇尔-阿特拉斯星表中，我们也发现透镜源的数量随着500微米通量密度的降低而减少。
Verifying that sub-mm galaxies are gravitationally lensed requires time-expensive observations with oversubscribed high-resolution observatories. Here, we aim to strengthen the evidence of gravitational lensing within theHerschelBright Sources (HerBS) by cross-comparing their positions to optical (SDSS) and near-infrared (VIKING) surveys, in order to search for the foreground lensing galaxy candidates. Resolved observations of the brightest HerBS sources have already shown that most are lensed, and a galaxy evolution model predicts that ∼76 per cent of the total HerBS sources are lensed, although with the SDSS survey we are only able to identify the likely foreground lenses for 25 per cent of the sources. With the near-infrared VIKING survey, however, we are able to identify the likely foreground lenses for 57 per cent of the sources, and we estimate that 82 per cent of the HerBS sources have lenses on the VIKING images even if we cannot identify the lens in every case. We find that the angular offsets between lens andHerschelsource are larger than that expected if the lensing is done by individual galaxies. We also find that the fraction of HerBS sources that are lensed falls with decreasing 500-micron flux density, which is expected from the galaxy evolution model. Finally, we apply our statistical VIKING cross-identification to the entireHerschel-ATLAS catalogue, where we also find that the number of lensed sources falls with decreasing 500-micron flux density.
The second Herschel–ATLAS Data Release – III. Optical and near-infrared counterparts in the North Galactic Plane field
第二次赫歇尔-阿特拉斯数据发布 – III. 北银河面场中的光学和近红外装置
DOI： 10.1093/mnras/sty151
发表时间： 2017
期刊： Monthly Notices of the Royal Astronomical Society
影响因子： 4.8
作者：
C. Furlanetto;C. Furlanetto;S. Dye;N. Bourne;S. Maddox;S. Maddox;L. Dunne;L. Dunne;S. Eales;E. Valiante;M. Smith;Daniel J. B. Smith;R. Ivison;R. Ivison;E. Ibar
通讯作者： E. Ibar
Colour matters: the effects of lensing on the positional offsets between optical and submillimetre galaxies in Herschel★-ATLAS
颜色很重要：透镜效应对赫歇尔★-ATLAS中光学星系和亚毫米星系之间位置偏移的影响
DOI： --
发表时间： 2014
期刊：
影响因子： --
作者：
N. Bourne;N. Bourne;S. Maddox;S. Maddox;L. Dunne;L. Dunne;S. Dye;S. Eales;C. Hoyos;C. Hoyos;J. González;D. Smith;E. Valiante;G. Zotti;G. Zotti;R. Ivison;K. Rowlands
通讯作者： K. Rowlands
The Herschel-ATLAS Data Release 2. Paper II. Catalogs of Far-infrared and Submillimeter Sources in the Fields at the South and North Galactic Poles
Herschel-ATLAS 数据发布 2。论文 II。
DOI： 10.3847/1538-4365/aab8fc
发表时间： 2017
期刊： The Astrophysical Journal Supplement Series
影响因子： --
作者：
S. Maddox;E. Valiante;P. Cigan;L. Dunne;S. Eales;Matthew W. L. Smith;S. Dye;C. Furlanetto;E. Ibar;G. Zotti;J. S. Millard;N. Bourne;H. Gomez;R. Ivison;D. Scott;I. Valtchanov
通讯作者： I. Valtchanov
CANDIDATE GRAVITATIONALLY LENSED DUSTY STAR-FORMING GALAXIES IN THE HERSCHEL WIDE AREA SURVEYS
DOI： 10.3847/0004-637x/823/1/17
发表时间： 2016-01
期刊： The Astrophysical Journal
影响因子： --
作者：
H. Nayyeri;M. Keele;A. Cooray;D. Riechers;R. Ivison;A. Harris;D. Frayer;A. Baker;S. Chapman;S. Eales;D. Farrah;H. Fu;L. Marchetti;R. Marques-Chaves;P. Mart́ınez-Navajas;S. Oliver;A. Omont;I. Pérez-Fournon;D. Scott;Mattia Vaccari;J. Vieira;M. Viero;L. Wang;J. Wardlow
通讯作者： H. Nayyeri;M. Keele;A. Cooray;D. Riechers;R. Ivison;A. Harris;D. Frayer;A. Baker;S. Chapman;S. Eales;D. Farrah;H. Fu;L. Marchetti;R. Marques-Chaves;P. Mart́ınez-Navajas;S. Oliver;A. Omont;I. Pérez-Fournon;D. Scott;Mattia Vaccari;J. Vieira;M. Viero;L. Wang;J. Wardlow
The third data release of the Kilo-Degree Survey and associated data products
DOI： 10.1051/0004-6361/201730747
发表时间： 2017-03
期刊： Astronomy and Astrophysics
影响因子： 6.5
作者：
J. D. Jong;G. V. Kleijn;T. Erben;H. Hildebrandt;K. Kuijken;G. Sikkema;M. Brescia;Maciej Bilicki;N. Napolitano;V. Amaro;K. Begeman;D. Boxhoorn;H. Buddelmeijer;S. Cavuoti;Fedor I. Getman;A. Grado;E. Helmich;Z. Huang;N. Irisarri;F. L. Barbera;G. Longo;J. McFarland;R. Nakajima;M. Paolillo;E. Puddu;M. Radovich;A. Rifatto;Crescenzo Tortora;E. Valentijn;C. Vellucci;W. Vriend;A. Amon;C. Blake;A. Choi;I. F. Conti;R. Herbonnet;C. Heymans;H. Hoekstra;D. Klaes;J. Merten;L. Miller;P. Schneider;M. Viola
通讯作者： J. D. Jong;G. V. Kleijn;T. Erben;H. Hildebrandt;K. Kuijken;G. Sikkema;M. Brescia;Maciej Bilicki;N. Napolitano;V. Amaro;K. Begeman;D. Boxhoorn;H. Buddelmeijer;S. Cavuoti;Fedor I. Getman;A. Grado;E. Helmich;Z. Huang;N. Irisarri;F. L. Barbera;G. Longo;J. McFarland;R. Nakajima;M. Paolillo;E. Puddu;M. Radovich;A. Rifatto;Crescenzo Tortora;E. Valentijn;C. Vellucci;W. Vriend;A. Amon;C. Blake;A. Choi;I. F. Conti;R. Herbonnet;C. Heymans;H. Hoekstra;D. Klaes;J. Merten;L. Miller;P. Schneider;M. Viola