Yanping Chen

ORCID: 0000-0001-8821-0309
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About
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Research Areas
  • Stellar, planetary, and galactic studies
  • Astronomy and Astrophysical Research
  • Galaxies: Formation, Evolution, Phenomena
  • Gamma-ray bursts and supernovae
  • Astronomical Observations and Instrumentation
  • Astrophysics and Star Formation Studies
  • Space exploration and regulation
  • Spectroscopy and Laser Applications
  • Radio Astronomy Observations and Technology
  • Space Science and Extraterrestrial Life
  • Atmospheric Ozone and Climate
  • Ideological and Political Education
  • Astrophysics and Cosmic Phenomena
  • Ionosphere and magnetosphere dynamics
  • Micro and Nano Robotics
  • Adaptive optics and wavefront sensing
  • Pain Mechanisms and Treatments
  • Insect and Pesticide Research
  • AI and Multimedia in Education
  • Bee Products Chemical Analysis
  • Phase Equilibria and Thermodynamics
  • Molecular Communication and Nanonetworks
  • Astrophysical Phenomena and Observations
  • Insect and Arachnid Ecology and Behavior
  • Insect-Plant Interactions and Control

New York University Abu Dhabi
2015-2024

Wuhan Technical College of Communications
2024

Agricultural Research Service
2020-2024

Fujian Provincial Cancer Hospital
2024

Zhejiang University
2024

Hohai University
2023

Shanghai Jiao Tong University
2023

Texas Tech University Health Sciences Center
2022

Texas Tech University
2022

Fujian Academy of Agricultural Sciences
2020

Abdurrouf Katherine Accetta C. Aerts V. Silva Aguirre Romina Ahumada and 95 more Nikhil Ajgaonkar N. Filiz Ak Shadab Alam Carlos Allende Prieto Andrés Almeida F. Anders Scott F. Anderson Brett H. Andrews Borja Anguiano E. Aquino-Ortíz Alfonso Aragón‐Salamanca M. Argudo–Fernández M. Ata M Aubert V. Ávila-Reese Carles Badenes R. H. Barbá Kathleen A. Barger J. K. Barrera-Ballesteros Rachael L. Beaton Timothy C. Beers Francesco Belfiore Chad F. Bender Mariangela Bernardi Matthew A. Bershady Florian Beutler C. Moni Bidin Jonathan C. Bird Dmitry Bizyaev Guillermo A. Blanc Michael R. Blanton Nicholas Fraser Boardman A. Bolton M. Boquien J. Borissova Jo Bovy W. N. Brandt Jordan Brown Joel R. Brownstein M. Brusa Johannes Büchner Kevin Bundy Joseph N. Burchett Martin Bureau Adam J. Burgasser Tuesday K. Cabang Stephanie Campbell Michele Cappellari Joleen K. Carlberg Fábio Wanderley R. Carrera Jennifer Cash Yanping Chen Wei-Huai Chen Brian Cherinka C. Chiappini Peter Doohyun Choi S. Drew Chojnowski Haeun Chung Nicolas Clerc Roger E. Cohen Julia M. Comerford Johan Comparat L. N. da Costa Kevin R. Covey Jeffrey D. Crane I. Cruz-González Connor Culhane Kátia Cunha Y. Sophia Dai G. Damke Jeremy Darling James W. Davidson Roger L. Davies Kyle Dawson Nathan De Lee Aleksandar M. Diamond‐Stanic M. Cano-Díaz H. Domínguez Sánchez John Donor Chris Duckworth T. Dwelly Daniel J. Eisenstein Y. Elsworth Éric Emsellem Mike Eracleous S. Escoffier Xiaohui Fan Emily Farr Shuai Feng José G. Fernández-Trincado Diane Feuillet Andreas Filipp Sean P. Fillingham Peter M. Frinchaboy

This paper documents the seventeenth data release (DR17) from Sloan Digital Sky Surveys; fifth and final fourth phase (SDSS-IV). DR17 contains complete of Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, which reached its goal surveying over 10,000 nearby galaxies. The MaNGA Stellar Library (MaStar) accompanies this data, providing observations almost 30,000 stars through instrument during bright time. also Galactic Evolution Experiment 2 (APOGEE-2) survey publicly...

10.3847/1538-4365/ac4414 article EN cc-by The Astrophysical Journal Supplement Series 2022-03-16
Bela Abolfathi David S. Aguado Gabriela Aguilar Carlos Allende Prieto Andrés Almeida and 95 more Tonima Tasnim Ananna F. Anders Scott F. Anderson Brett H. Andrews Borja Anguiano Alfonso Aragón‐Salamanca M. Argudo–Fernández E. Armengaud M. Ata É. Aubourg V. Ávila-Reese Carles Badenes S. Bailey Christophe Balland Kathleen A. Barger J. K. Barrera-Ballesteros Curtis Bartosz Fabienne A. Bastien Dominic Bates Falk Baumgarten Julian Bautista Rachael L. Beaton Timothy C. Beers Francesco Belfiore Chad F. Bender Mariangela Bernardi Matthew A. Bershady Florian Beutler Jonathan C. Bird Dmitry Bizyaev Guillermo A. Blanc Michael R. Blanton Michael Blomqvist A. Bolton M. Boquien J. Borissova Jo Bovy Christian Andres Bradna Diaz William Nielsen Brandt J. Brinkmann Joel R. Brownstein Kevin Bundy Adam J. Burgasser E. Burtin Nicolás G. Busca Caleb I. Cañas M. Cano-Díaz Michele Cappellari R. Carrera Andrew R. Casey Bernardo Cervantes Sodi Yanping Chen Brian Cherinka C. Chiappini Peter Doohyun Choi Drew Chojnowski Chia-Hsun Chuang Haeun Chung Nicolas Clerc Roger E. Cohen Julia M. Comerford Johan Comparat Janaina Correa do Nascimento L. N. da Costa Marie-Claude Cousinou Kevin R. Covey Jeffrey D. Crane I. Cruz-González Kátia Cunha Gabriele S Ilha G. Damke Jeremy Darling James W. Davidson Kyle Dawson Miguel Icaza-Lizaola Axel de la Macorra Sylvain de la Torre Nathan De Lee Victoria de Sainte Agathe Alice Deconto Machado F. Dell’Agli Timothée Delubac Aleksandar M. Diamond‐Stanic John Donor Juan José Downes Niv Drory Hélion du Mas des Bourboux Christopher Duckworth T. Dwelly Jamie Dyer Garrett Ebelke Arthur Eigenbrot Daniel J. Eisenstein Y. Elsworth Éric Emsellem

The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) has been in operation since 2014 July. This paper describes second data release from this phase, and 14th SDSS overall (making Data Release Fourteen or DR14). makes taken by SDSS-IV its first two years (2014–2016 July) public. Like all previous releases, DR14 is cumulative, including most recent reductions calibrations phase began operations 2000. New public extended Baryon Oscillation Spectroscopic Survey; Apache Point...

10.3847/1538-4365/aa9e8a article EN cc-by The Astrophysical Journal Supplement Series 2018-04-19
Franco D. Albareti Carlos Allende Prieto Andrés Almeida F. Anders Scott F. Anderson and 95 more Brett H. Andrews Alfonso Aragón‐Salamanca M. Argudo–Fernández E. Armengaud É. Aubourg V. Ávila-Reese Carles Badenes S. Bailey B. Barbuy Kathleen A. Barger J. K. Barrera-Ballesteros Curtis Bartosz Sarbani Basu Dominic Bates G. Battaglia Falk Baumgarten Julien Baur Julian Bautista Timothy C. Beers Francesco Belfiore Matthew A. Bershady S. Bertrán de Lis Jonathan C. Bird Dmitry Bizyaev Guillermo A. Blanc Michael R. Blanton Michael Blomqvist A. Bolton J. Borissova Jo Bovy William Nielsen Brandt J. Brinkmann Joel R. Brownstein Kevin Bundy E. Burtin Nicolás G. Busca H. Camacho M. Cano-Díaz Michele Cappellari R. Carrera Yanping Chen Brian Cherinka Edmond Cheung C. Chiappini Drew Chojnowski Chia-Hsun Chuang Haeun Chung Rafael Fernando Cirolini Nicolas Clerc Roger E. Cohen Julia M. Comerford Johan Comparat Janaina Correa do Nascimento Marie-Claude Cousinou Kevin R. Covey Jeffrey D. Crane Rupert A. C. Croft Kátia Cunha Jeremy Darling James W. Davidson Kyle Dawson L. N. da Costa Gabriele S Ilha Alice Deconto Machado Timothée Delubac Nathan De Lee Axel de la Macorra Sylvain de la Torre Aleksandar M. Diamond‐Stanic John Donor Juan José Downes Niv Drory Cheng Du Hélion du Mas des Bourboux T. Dwelly Garrett Ebelke Arthur Eigenbrot Daniel J. Eisenstein Y. Elsworth Éric Emsellem Michael Eracleous S. Escoffier Michael L. Evans J. Falcón‐Barroso Xiaohui Fan Ginevra Favole Emma Fernández-Alvar José G. Fernández-Trincado Diane Feuillet Scott W. Fleming Andreu Font-Ribera Gordon Freischlad Peter M. Frinchaboy Hai Fu Yang Gao

Abstract The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) began observations in 2014 July. It pursues three core programs: Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2), Mapping Nearby Galaxies at APO (MaNGA), and Extended Baryon Oscillation Spectroscopic (eBOSS). As well as its program, eBOSS contains two major subprograms: Time Domain (TDSS) SPectroscopic IDentification ERosita Sources (SPIDERS). This paper describes first data release from SDSS-IV,...

10.3847/1538-4365/aa8992 article EN The Astrophysical Journal Supplement Series 2017-12-01
David S. Aguado Romina Ahumada Andrés Almeida Scott F. Anderson Brett H. Andrews and 95 more Borja Anguiano E. Aquino-Ortíz Alfonso Aragón‐Salamanca M. Argudo–Fernández M Aubert V. Ávila-Reese Carles Badenes Sandro B Rembold Kathleen A. Barger J. K. Barrera-Ballesteros Dominic Bates Julian Bautista Rachael L. Beaton Timothy C. Beers Francesco Belfiore Mariangela Bernardi Matthew A. Bershady Florian Beutler Jonathan C. Bird Dmitry Bizyaev Guillermo A. Blanc Michael R. Blanton Michael Blomqvist A. Bolton M. Boquien J. Borissova Jo Bovy William Nielsen Brandt J. Brinkmann Joel R. Brownstein Kevin Bundy Adam J. Burgasser Nell Byler M. Cano-Díaz Michele Cappellari R. Carrera Bernardo Cervantes Sodi Yanping Chen Brian Cherinka Peter Doohyun Choi Haeun Chung Damien Coffey Julia M. Comerford Johan Comparat Kevin R. Covey Gabriele S Ilha L. N. da Costa Y. Sophia Dai G. Damke Jeremy Darling Roger L. Davies Kyle Dawson Victoria de Sainte Agathe Alice Deconto Machado A. Del Moro Nathan De Lee Aleksandar M. Diamond‐Stanic H. Domínguez Sánchez John Donor Niv Drory Hélion du Mas des Bourboux Chris Duckworth T. Dwelly Garrett Ebelke Éric Emsellem S. Escoffier José G. Fernández-Trincado Diane Feuillet Johanna-Laina Fischer Scott W. Fleming Amelia Fraser-McKelvie Gordon Freischlad Peter M. Frinchaboy Hai Fu L. Galbany Rafael Garcia‐Dias D. A. García–Hernández Luis Alberto Garma Oehmichen M. A. G. Maia Héctor Gil-Marín Kathleen Grabowski Meng Gu Hong Guo Jae‐Won Ha Emily Harrington Sten Hasselquist Christian R. Hayes Fred Hearty Hector Hernández Toledo Harry Hicks David W. Hogg Kelly Holley‐Bockelmann Jon A. Holtzman Bau-Ching Hsieh John Douglas Hunt

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by fourth phase of SDSS (SDSS-IV) across its three operation (July 2014-July 2017). This is third SDSS-IV, and fifteenth from (Data Release Fifteen; DR15). New come MaNGA - 4824 datacubes, as well stellar spectra in Stellar Library (MaStar), set survey-supported analysis products (e.g. gas kinematics, emission line, other maps) Data Analysis Pipeline (DAP), a new visualisation...

10.3847/1538-4365/aaf651 article EN cc-by The Astrophysical Journal Supplement Series 2019-01-31

Rabbit meat could play an important role in health, the rural economy, and sustainable development. has excellent nutritional features, such as high protein content, low-fat a percentage of unsaturated fatty acids, low cholesterol sodium levels. In addition, rabbit production contributes to maintaining economic activities marginal areas. However, consumption is still limited due several factors higher cost commercial food that slowing down rabbits’ breeding. Socio-demographic...

10.3390/su15032008 article EN Sustainability 2023-01-20

We measure equivalent widths (EW) - focussing on two unique features (NaI and TiO2) of low-mass stars (<0.3M\odot) for luminous red galaxy spectra from the Sloan Digital Sky Survey (SDSS) X-Shooter Lens (XLENS) in order to study end initial mass function (IMF). compare these EWs those derived simple stellar population models computed with different IMFs, ages, [{\alpha}/Fe], elemental abundances. find that are able simultaneously reproduce observed NaD {\lambda}5895 Na I {\lambda}8190...

10.1088/2041-8205/753/2/l32 article EN The Astrophysical Journal Letters 2012-06-21

Abstract Background The ectoparasitic mite Varroa destructor has emerged as the primary pest of domestic honey bees ( Apis mellifera ). Here we present an initial survey V. genome carried out to advance our understanding biology and identify new avenues for control. This sequence provides immediate resources molecular population-genetic analyses - interactions defines challenges ahead a comprehensive project. Results size was estimated by flow cytometry be 565 Mbp, larger than most sequenced...

10.1186/1471-2164-11-602 article EN cc-by BMC Genomics 2010-10-25

The SDSS-IV Mapping Nearby Galaxies at APO (MaNGA) program has been operating from 2014-2020, and now observed a sample of 9,269 galaxies in the low redshift universe (z ~ 0.05) with integral-field spectroscopy. With rest-optical (\lambda\lambda 0.36 - 1.0 um) spectral resolution R 2000 instrumental line-spread function (LSF) typically 1sigma width about 70 km/s, which poses challenge for study 20-30 km/s velocity dispersion ionized gas present-day disk galaxies. In this contribution, we...

10.3847/1538-3881/abcaa2 article EN The Astronomical Journal 2021-01-06

We present the second data release (DR2) of X-shooter Spectral Library (XSL), which contains all spectra obtained over six semesters that program. This supersedes our first from Chen et al. (2014, A&amp;A, 565, A117), with a larger number (813 observations 666 stars) and more extended wavelength coverage as near-infrared arm spectrograph are now included. The DR2 then consist three segments were observed simultaneously and, if combined, cover range between ∼300 nm ∼2.45 μ m at spectral...

10.1051/0004-6361/201936825 article EN Astronomy and Astrophysics 2020-01-10

We present the first release of XSL, X-Shooter Spectral Library. This contains 237 stars spanning wavelengths 3000--10200 Å observed at a resolving power $R \equiv λ/ Δλ\sim 10000$. The spectra were obtained ESO's 8-m Very Large Telescope (VLT). sample O -- M, long-period variable (LPV), C and S stars. are flux-calibrated telluric-corrected. describe new technique for telluric correction. wavelength coverage, spectral resolution type this library make it well suited to stellar population...

10.1051/0004-6361/201322505 article EN Astronomy and Astrophysics 2014-04-02

The X-shooter Spectral Library (XSL) is an empirical stellar library at medium spectral resolution covering the wavelength range from 3000 \AA to 24 800 \AA. This aims provide a benchmark for population studies. In this work, we present uniform set of atmospheric parameters, effective temperatures, surface gravities, and iron abundances 754 spectra 616 XSL stars. We used full-spectrum fitting package ULySS with MILES as reference fit ultraviolet-blue (UVB) visible (VIS) spectra. tested...

10.1051/0004-6361/201834273 article EN Astronomy and Astrophysics 2019-07-01

We present the third data release (DR3) of X-shooter Spectral Library (XSL). This moderate-to-high resolution, near-ultraviolet-to-near-infrared ($350-2480$ nm, R $\sim$ 10 000) spectral library is composed 830 stellar spectra 683 stars. DR3 improves upon previous by providing combined de-reddened three segments over full $350-2480$ nm wavelength range. It also includes additional 20 M-dwarf from ESO archive. provide detailed comparisons between this and Gaia EDR3, MILES, NGSL, CaT library,...

10.1051/0004-6361/202142388 article EN Astronomy and Astrophysics 2022-01-26

Inflammatory bowel disease (IBD) is a group of recurrent chronic inflammatory diseases, including Crohn’s (CD) and ulcerative colitis (UC). Although IBD has been extensively studied for decades, its cause pathogenesis remain unclear. Existing research suggests that may be the result an interaction between genetic factors, environmental factors gut microbiome. closely related to non-coding RNAs (ncRNAs). NcRNAs are composed microRNA(miRNA), long RNA(lnc RNA) circular RNA(circ RNA). Compared...

10.3389/fimmu.2024.1406538 article EN cc-by Frontiers in Immunology 2024-06-04

We present the MaNGA FIREFLY Value-Added-Catalogue (VAC) - a catalogue of ~3.7 million spatially resolved stellar population properties across 10,010 nearby galaxies from final data release survey. The full spectral fitting code firefly is employed to derive parameters such as ages, metallicities, and remnant masses, star formation histories, rates dust attenuation. In addition Voronoi-binned measurements, our VAC also provides global properties, central values radial gradients. Two variants...

10.1093/mnras/stac1260 article EN cc-by Monthly Notices of the Royal Astronomical Society 2022-05-04

ABSTRACT Strengthening the synergy between simulations and observations is essential to test galaxy formation evolution theories. To achieve this goal, in first paper of series, we presented a method generate mock SDSS-IV/Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) integral-field spectroscopic from cosmological simulations. In second paper, build iMaNGA catalogue consisting ∼1000 unique galaxies TNG50 simulations, selected mimic SDSS-IV/MaNGA-Primary sample selection. Here,...

10.1093/mnras/stad1337 article EN cc-by Monthly Notices of the Royal Astronomical Society 2023-05-03

ABSTRACT Galaxy formation and evolution simulations are essential tools to probe poorly known astrophysics processes, but particular care is needed compare with galaxy observations, as observed data need be modelled well. We present a method generate mock galaxies from the hydro-dynamical IllustrisTNG which suited integral field spectroscopic observation of SDSS-IV/Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey. First, we include same instrumental effects procedures...

10.1093/mnras/stac1531 article EN cc-by Monthly Notices of the Royal Astronomical Society 2022-06-07

The construction of “double-qualified” teachers is the basic premise for high-quality development higher vocational education, and it also key force colleges to cultivate skilled talents. This paper probes into positioning in colleges, deeply analyzes current situation provides countermeasures teachers.

10.26689/jcer.v8i8.7998 article EN Journal of Contemporary Educational Research 2024-08-16

Royal Jelly (RJ) is a natural substance produced by honeybees, serving not only as nutrition for bee brood and queens but also functional food due to its health-promoting properties. Despite well-known broad-spectrum antibacterial activity, the precise molecular mechanism underlying action has remained elusive. In this study, we investigated impact of RJ on bacteria model MG1655 at half-maximal inhibitory concentration, employing LC-MS/MS analyze proteomic changes. The differentially...

10.1038/s41598-024-70164-5 article EN cc-by-nc-nd Scientific Reports 2024-08-21

Abstract We have constructed an all-sky catalog of optical active galactic nuclei (AGNs) with z &lt; 0.09, based on spectroscopy, from the parent sample galaxies in 2MASS Redshift Survey, a near-complete census nearby universe. Our consists 1929 broad-line AGNs and 6562 narrow-line that satisfy Kauffmann et al. criteria, which 3607 also Kewley criteria. report emission-line widths, fluxes, flux errors, signal-to-noise ratios (S/Ns) all our spectroscopic sample, allowing users to customize...

10.3847/1538-4357/aaffaf article EN The Astrophysical Journal 2019-02-19

Abstract We present the first release of MaNGA Stellar Library (MaStar), which is a large, well-calibrated, high-quality empirical library covering wavelength range 3622–10354 Å at resolving power R ∼ 1800. The spectra were obtained using same instrument as used by Mapping Nearby Galaxies Apache Point Observatory (MaNGA) project, piggybacking on Sloan Digital Sky Survey (SDSS-IV)/Apache Galaxy Evolution Experiment 2-N (APOGEE-2N) observations. Compared to previous libraries, MaStar will have...

10.3847/1538-4357/ab3ebc article EN The Astrophysical Journal 2019-10-01

Aims. The path towards robust near-infrared extensions of stellar population models involves the confrontation between empirical and synthetic spectral libraries across wavelength ranges photospheric emission. Indeed, theory emission enters all synthesis models, even when this is only implicit in association fundamental parameters with library stars. With its near-ultraviolet to coverage, X-shooter Spectral Library (XSL) allows us examine what extent succeed reproducing energy distributions...

10.1051/0004-6361/202039371 article EN cc-by Astronomy and Astrophysics 2021-02-15
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