adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019ApJ...881...53T (acknowledgments)
We thank Shugo Michikoshi and Hiroshi Kobayashi for fruitful discussion. We also thank the anonymous referee for insightful and constructive comments that helped to improve the manuscript. This work was supported by JSPS KAKENHI grant Nos. JP18J20360, 16H02160, 18H05436, 18H05437, and 19K14764, and in part by the National Astronomical Observatory of Japan (NAOJ) Atacama Large Millimeter/submillimeter Array (ALMA) Scientific Research grant No. 2016-02A (SZT).
Paper: 2018MNRAS.479.1722C (acknowledgments)
ACKNOWLEDGEMENTS SDC and SW acknowledges support from the ERC starting grant No. 679852 ‘RADFEEDBACK’. APW, ADC and PCC gratefully acknowledge the support of a consolidated grant (ST/N000706/1) from the UK Science and Technology Facilities Council. STS acknowledges funding by the Deutsche Forschungsgemeinschaft (DFG) via the Sonderforschungsbereich SFB 956 Conditions and Impact of Star Formation (subproject A4) and the Bonn-Cologne Graduate School. RLS gratefully acknowledges the support of a UK Science and Technology Facilities Council postgraduate studentship. SEJ gratefully acknowledge the support of postgraduate scholarships from the School of Physics Astronomy at Cardiff University and the UK Science and Technology Facilities Council. SW further thanks the DFG for funding through the Collaborative Research Center (SFB956) on the ‘Conditions and impact of star formation’. PCC acknowledges support from the European Community’s Horizon 2020 Programme H2020-COMPET-2015, through the StarFormMapper Project (number 687528). SDC would like to thank Volker Ossenkopf for useful discussions about radiation transfer. The authors would also like to thank the anonymous referee for their helpful comments on the paper. This work was performed using the facilities of the Advanced Research Computing at Cardiff Division, Cardiff University.
Paper: 2016A&A...585A..16C (acknowledgments)
The project was funded by FONDATION MERAC. We acknowledge support from the Programme National de Physique Stellaire (PNPS) of the Institut Nationale de Sciences de l’Univers of CNRS. S.M.A. and S.A.K. acknowledge the SCOPES grant No. IZ73Z0-152485 for financial support.
Paper: 2016ApJ...824..143L (acknowledgments)
We are grateful to the referee for helpful comments. This work was funded by the Natural Science Foundation of China under grant numbers 11133001 and 11333004, and the Strategic Priority Research Program of CAS (under grant number XDB09000000).
Paper: 2016ApJ...831..132G (acknowledgments)
This research was supported under the Australian Research Council funding scheme (FT110100263). GADS warmly thanks Chien Peng for useful discussions. This research has made use of the NASA/IPAC Extragalactic Database (NED). Based on observations made with the NASA/ESA Hubble Space Telescope , obtained through program GO-13050.
Paper: 2018MNRAS.474.1810H (acknowledgments)
Acknowledgements We thank the anonymous referee for his/her careful review and insightful comments. TH is financially supported by the Japan Society for the Promotion of Science (JP15J10520 and JP26800113).
Paper: 2018A&A...609A..91R (acknowledgments)
The authors thank the anonymous referee for useful and constructive comments which improved the paper. We want to thank A. Tielens and J. Slavin for providing the hot gas spectrum shown in Fig. 5 . The research leading to these results has received funding from the European Union Seventh Framework Programme FP7-2011 under grant agreement No. 284405. C.R. and M.G. acknowledge funding by the Austrian Science Fund (FWF): project number P24790. The computational results presented have been achieved using the Vienna Scientific Cluster (VSC). This publication was supported by the Austrian Science Fund (FWF). This research has made use of NASA’s Astrophysics Data System. All figures were made with the free Python module Matplotlib ( Hunter 2007 ). This research made use of Astropy, a community-developed core Python package for Astronomy ( Astropy Collaboration et al. 2013 ).
Paper: 2015ApJ...810...57S (acknowledgments)
This work was supported by the NASA Astrobiology Institute's Virtual Planetary Laboratory Lead Team, funded through the NASA Astrobiology Institute under solicitation NNH12ZDA002C and Cooperative Agreement Number NNA13AA93A. T.R. gratefully acknowledges support from an appointment to the NASA Postdoctoral Program at NASA Ames Research Center, administered by Oak Ridge Affiliated Universities. This work benefited from the use of advanced computational, storage, and networking infrastructure provided by the Hyak supercomputer system at the University of Washington. This research has made use of NASA's Astrophysics Data System. We thank Dave Crisp and Robin Wordsworth for helpful comments and discussion. We are grateful for the comments of an anonymous reviewer, which allowed us to greatly improve this manuscript.
Paper: 2018MNRAS.474.4245W (acknowledgments)
ACKNOWLEDGEMENTS This work has used data from the European Space Agency (ESA) mission Gaia ( https://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC; https://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. We would like to thank Prof. X. D. Li from the Nanjing University for useful discussions. We would like to thank the referee, Dr Benito Marcote, who carefully read the original draft and shared valuable comments and suggestions that greatly improved the quality of this paper. Facilities: VLBA
Paper: 2017ApJ...834..129W (acknowledgments)
Roman R. Rafikov is an IBM Einstein Fellow at the Institute of Advanced Study; his financial support is provided by the NSF via grants AST-1409524, AST-1515763, NASA via grants 14-ATP14-0059, 15-XRP15-2-0139, and The Ambrose Monell Foundation. Jenny E. Greene acknowledges funding from the National Science Foundation under Grant No. AAG: #1310405. We are thankful to Dr. Adam Myers, Dr. Michael Eracleous, and Dr. Zoltan Haiman for useful comments and suggestions.
Paper: 2019ApJ...872...47M (acknowledgments)
We thank Mary Putman, David Schiminovich, Yong Zheng, and our referee for their useful discussions and thoughtful feedback, which have helped us improve various drafts of this manuscript. Many thanks to Lauren Corlies for sharing her C loudy models used in our mock observations. We acknowledge support from NSF grants AST-1312888, AST-1615955, and DGE-1644869 and NASA grant NNX15AB20G, as well as computational resources from NSF XSEDE and Columbia University’s compute cluster. Simulations were run on the Texas Advanced Computing Center Stampede supercomputer and were performed using the publicly available Enzo code ( http://enzo-project.org ) and analyzed with the yt package (Turk et al. 2011 ). Enzo is the product of a collaborative effort of many independent scientists from numerous institutions around the world. Their commitment to open science has helped make this work possible. The Flatiron Institute is supported by the generosity of the Simons Foundation.
Paper: 2019A&A...623A.178D (acknowledgments)
We would like to thank the anonymous referee for their comments and suggestions. The authors also wish to thank Ivan Milić for useful discussions during the analysis of the presented work. Financial support by the Spanish Ministry of Economy and Competitiveness through projects AYA2014-60476-P and AYA2014-60833-P are gratefully acknowledged. CJDB acknowledges Fundación La Caixa for the financial support received in the form of a PhD contract. AAR also acknowledges financial support through the Ramón y Cajal fellowships. This research has made use of NASA’s Astrophysics Data System Bibliographic Services. JdlCR is supported by grants from the Swedish Research Council (2015-03994), the Swedish National Space Board (128/15) and the Swedish Civil Contingencies Agency (MSB). This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (SUNMAG, grant agreement 759548). The Swedish 1-m Solar Telescope is operated on the island of La Palma by the Institute for Solar Physics of Stockholm University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. The Institute for Solar Physics is supported by a grant for research infrastructures of national importance from the Swedish Research Council (registration number 2017-00625). This research has made use of NASA’s Astrophysics Data System Bibliographic Services. We acknowledge the community effort devoted to the development of the following open-source packages that were used in this work: numpy ( http://www.numpy.org/ ), matplotlib ( https://matplotlib.org/ ) This research has made use of SunPy, an open-source and free community-developed solar data analysis package written in Python ( SunPy Community et al. 2015 ). The author thankfully acknowledges the technical expertise and assistance provided by the Spanish Supercomputing Network (Red Española de Supercomputación), as well as the computer resources used: the LaPalma Supercomputer, located at the Instituto de Astrofísica de Canarias.
Paper: 2016MNRAS.461.4517D (acknowledgments)
This work is based on observations made with the NASA/ESA Hubble Space Telescope , and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA). Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.
Paper: 2018ApJ...858...90G (acknowledgments)
This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00634.S and ADS/JAO.ALMA#2011.0.00004.SV. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work is partially based on observations carried out with the IRAM IRAM 30 m telescope. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain). The work of M.G. and A.K.L. is partially supported by the National Science Foundation under grant nos. 1615105, 1615109, and 1653300. E.S. acknowledges financial support to the DAGAL network from the People Programme (Marie Curie Actions) of the European Union’s Seventh Framework Programme FP7/2007–2013/under REA grant agreement no. PITN-GA-2011-289313. A.H. acknowledges support from the Centre National d’Etudes Spatiales (CNES). A.U. acknowledges support from Spanish MINECO grants ESP2015-68964 and AYA2016-79006. E.R. is supported by a Discovery Grant from NSERC Canada. F.B. acknowledges funding from the European Unions Horizon 2020 research and innovation programme (grant agreement no. 726384—EMPIRE) This paper made use of the NASA Astrophysics Data Abstract service, AstroPy, the IDL Astronomy User’s Library, CASA, and the NASA Extragalactic Database. M.G. and A.K.L. gratefully acknowledge helpful discussions with Todd Thompson and the OSU galaxy and ISM discussion groups. Diane Cormier is supported by the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement no. 702622. M.J.J.-D. and F.B. acknowledge support from DFG grant BI 1546/1-1. E.O. is supported by grant AST-7173949 from the National Science Foundation.
Paper: 2015MNRAS.452.1045F (acknowledgments)
We thank L. Cortese and L. Spitler for useful discussions. DAF thanks the ARC for financial support via DP130100388. This work was supported by NSF grant AST-1211995. Finally, we thank the referee for a prompt report and several useful suggestions to improve the paper.
Paper: 2020MNRAS.492.3904A (acknowledgments)
ACKNOWLEDGEMENTS Parts of this research were conducted by the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav), through project number CE170100004. EJH acknowledges support from a Australian Research Council DECRA Fellowship (DE170100891). AdUP and CCT acknowledge support from Ramón y Cajal fellowships RyC-2012-09975 and RyC-2012-09984 and the Spanish Ministry of Economy and Competitiveness through project AYA2017-89384-P. DAK acknowledges support from the Spanish research project AYA2017-89384-P. MB acknowledges funding as ‘personal tecnico de apoyo’ under fellowship number PTA2016-13192-I. MC is supported by the David and Ellen Lee Postdoctoral Fellowship at the California Institute of Technology. SA is supported by the CNES Postdoctoral Fellowship at Laboratoire AstroParticule et Cosmologie. SA, AC, CL, and RM acknowledge the financial support of the UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02). SA and NL acknowledge the financial support of the Programme National Hautes Energies (PNHE). DT acknowledges the financial support of the Chinese Academy of Sciences (CAS) PIFI post-doctoral fellowship program (program C). UBAI acknowledges support from the Ministry of Innovative Development through projects FA-Atech-2018-392 and VA-FA-F-2-010. IRiS has been carried out thanks to the support of the OCEVU Labex (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02) funded by the ‘Investissements d’Avenir’ French government program. IRiS and T120 thank all the Observatoire de Haute-Provence staff for the permanent support. SB, NK, RN, and MV acknowledge the Shota Rustaveli National Science Foundation (SRNSF grant No 218070). TAROT has been built with the support of the Institut National des Sciences de l’Univers, CNRS,France. TAROT is funded by the CNES and thanks the help of the technical staff of the Observatoire de Haute Provence, OSU-Pytheas.
Paper: 2019MNRAS.482...30S (acknowledgments)
ACKNOWLEDGEMENTS Support for this work was provided by NASA through Einstein Postdoctoral Fellowship grant number PF4-150127 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-03060. TI thanks the Undergraduate Summer Research Program (USRP) at the department of Astrophysical Sciences, Princeton University, for support. JS thanks the Niels Bohr Institute for its hospitality while part of this work was completed, and the Kavli Foundation and the DNRF for supporting the 2017 Kavli Summer Program.
Paper: 2015MNRAS.447.3115J (acknowledgments)
NuGrid acknowledges significant support from NSF grants PHY 02-16783 and PHY 09-22648 (Joint Institute for Nuclear Astrophysics, JINA). RH and CG acknowledge the support from Eurocore project Eurogenesis and ERC Starting Grant No. 306901. RH acknowledges support from the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan. MP acknowledges the support from the Ambizione grant of the SNSF and the SNF grant (Switzerland). AH acknowledges the support by NSF through grant AST-1109394, by US DOE grants FC02-09ER41618 (SciDAC), DE-FG02-87ER40328 and by an ARC Future Fellowship (FT120100363).
Paper: 2019MNRAS.483...70C (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for their thorough and careful reading of this paper and many constructive suggestions. We acknowledge Nicolas Peretto for help with CO data at the locations of some of our sources. HC, HLG, and PC acknowledge support from the European Research Council (ERC) in the form of Consolidator Grant cosmicdust (ERC-2014-CoG-647939). MJB and IDL acknowledge support from the ERC in the form of Advanced Grant SNDUST (ERC-2015-AdG-694520). MM acknowledges support from an STFC Ernest Rutherford fellowship (ST/L003597/1). Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.
Paper: 2019MNRAS.482.2107D (acknowledgments)
ACKNOWLEDGEMENTS This work was supported in part by NASA (National Aeronautics and Space Administration) Astrophysics Theory Program grant NNX14AB37G and NSF (National Science Foundation) grant AST-1411879. UD is immensely grateful to Ben Brown for allocating time on the LCD machines, where all the calculations using dedalus were performed. UD specially thanks Phil Armitage, Bhupendra Mishra, and Vladimir Zhdankin for general discussions. The authors thank the anonymous referee for their constructive comments.
Paper: 2017MNRAS.471.4265E (acknowledgments)
Acknowledgements This project has been supported by Australian Research Council via the Discover Early Career Research Award (DE150100301). Auchettl kindly thanks La Trobe University for funding via a PhD scholarship. Theoretical work (Project AY7) was undertaken with the assistance of resources and services from the NCI, which is supported by the Australian Government. We finally thank the reviewers for their thoughtful comments and suggestions for future work.
Paper: 2015A&A...583A..68M (acknowledgments)
We thank Uwe Lammers, who contributed to the idea and progress of this study, and its funding under ESA Contract No. 4000108677/13/NL/CB. We are grateful to Ulrich Bastian, Alex Bombrun, Anthony Brown, Sergei Klioner, Uwe Lammers, Paul McMillan, Mercedes Ramos-Lerate, and the referee, Floor van Leeuwen, for their helpful feedback to our manuscript. This work was supported by the Gaia Data Processing and Analysis Consortium (DPAC) and uses the AGIS/AGISLab and GaiaTools software packages; special thanks to their maintainers and developers. We gratefully acknowledge financial support from the Swedish National Space Board and the Royal Physiographic Society in Lund.
Paper: 2019MNRAS.487.1040M (acknowledgments)
ACKNOWLEDGEMENTS This study is based on observations made with the SALT under programme 2017-1-MLT-010. BM acknowledges support from the National Research Foundation (NRF) of South Africa and thanks the Institute of Astronomy at KU Leuven for their hospitality. We thank the anonymous referee for a helpful report whose comments helped improve this paper. This paper is based on spectroscopic observations made with the Southern African Large Telescope (SALT) under programme 2017-1-MLT-010 (PI: B. Miszalski). We are grateful to our SALT colleagues for maintaining the telescope facilities and conducting the observations. We thank A.Y. Kniazev for making available his HRS pipeline data products. HVW and RM acknowledge support from the Belgian Science Policy Office under contract BR/143/A2/STARLAB. HVW acknowledges additional support from the Research Council of K.U. Leuven under contract C14/17/082. Polish participation in SALT is funded by grant no. MNiSW DIR/WK/2016/07. This research has been partly founded by the National Science Centre, Poland, through grant OPUS 2017/27/B/ST9/01940 to JM. IRAF is distributed by the National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation.
Paper: 2016ApJ...826...29L (acknowledgments)
We thank Mark Lacy for his advice and useful discussion with regards to the Sajina model, as well as George Helou for suggesting the extended Schmidt law as another point of analysis, and Yong Shi, Michael Brown, and Aditya Togi, whose comments improved the revised version of this paper. This work made use of the remote access computing accounts of the NASA Herschel Science Center, which were very helpful in reducing the Herschel data. L.L. and P.M.O. acknowledges support for this work provided by NASA through an award issued by JPL/Caltech. Support for K.A. is provided by NASA through Hubble Fellowship grant # HST -HF2-51352.001 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. This work is based in part on observations made with Herschel , a European Space Agency Cornerstone Mission with significant participation by NASA. This publication used observations made with the Spitzer Space Telescope , which is operated by the Jet Propulsion Laboratory (JPL)/California Institute of Technology (Caltech) under a contract with NASA. Observations from the Wide-field Infrared Survey Explorer , which is a joint project of the University of California, Los Angeles, and JPL/Caltech, funded by NASA, were also used. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center (IPAC)/Caltech, funded by NASA and the NSF, as well as from the Sloan Digital Sky Survey (Sloan-III), whose funding has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the NSF, and the U.S. DOE Office of Science, and which is managed by the Astrophysical Research Consortium for the Participating Institutions of the Sloan-III Collaboration. Finally, this publication makes use of data from the Galaxy Evolution Explorer , retrieved from the Mikulski Archive for Space Telescopes (MAST), part of the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non- HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. This research has made use of the NASA/IPAC Extragalactic Database (NED) and the Infrared Science Archive (IRSA) which are operated by the JPL/Caltech, under contract with the NASA, and NASA’s Astrophysics Data System (ADS). We also used software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. Facilities: Herschel , Spitzer , WISE , 2MASS , Sloan , GALEX .
Paper: 2018ApJ...867..160H (acknowledgments)
This work was supported by NASA’s Planetary Science Division Internal Scientist Funding Program through the Fundamental Laboratory Research (FLaRe) work package at the NASA Goddard Space Flight Center. Also acknowledged is the NASA Astrobiology Institute through funding to the Goddard Center for Astrobiology under proposal 13-13NAI7-0032. Stephen Brown, Eugene Gerashchenko, and Martin Carts of NASA Goddard’s Radiation Effects Facility are thanked for the operation and maintenance of the Van de Graaff accelerator. Many helpful conversations with Marla Moore and Perry Gerakines are acknowledged.
Paper: 2018ApJ...861..124M (acknowledgments)
The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP/2007–2013)/ERC grant Agreement No. 279954. C.M. would like to thank Antonio J. Cuesta, Bruce A. Bassett, Jarah Evslin, and Hendrik Hildebrandt for their helpful comments, and to acknowledge the support from the joint research training program of CAS and CNRS. We gratefully acknowledge the anonymous reviewers for their commentary that helped improve this paper. Software: CAMB 12 12 http://camb.info/ (Lewis et al. 2000 ; Lewis et al. 2017 ), matplotlib (Hunter 2007 ; Droettboom et al. 2018 ), statsmodels (Seabold et al. 2017 ), NumPy (Walt et al. 2011 ), and SciPy (Jones et al. 2001 ).