Skip to main content
Home

Navigation Menu

  • Back
  • About
    • Back
    • About

      Contact Us

      Business Address
      5241 Broad Branch Rd. NW

      Washington , DC 20015
      United States place Map
      Call Us (202) 387-640
    • Who We Are
      • Back
      • Leadership
      • Our Blueprint For Discovery
      • Board & Advisory Committee
      • Financial Stewardship
      • Awards & Accolades
      • History
    • Connect with Us
      • Back
      • Outreach & Education
      • Newsletter
      • Yearbook
    • Working at Carnegie
      • Back
      • Applications Open: Postdoctoral Fellowships

    Contact Us

    Business Address
    5241 Broad Branch Rd. NW

    Washington , DC 20015
    United States place Map
    Call Us (202) 387-6400
  • Research
    • Back
    • Research Areas & Topics
    • Research Areas & Topics
      • Back
      • Research Areas
      • From genomes to ecosystems and from planets to the cosmos, Carnegie Science is an incubator for cutting-edge, interdisciplinary research.
      • Astronomy & Astrophysics
        • Back
        • Astronomy & Astrophysics
        • Astrophysical Theory
        • Cosmology
        • Distant Galaxies
        • Milky Way & Stellar Evolution
        • Planet Formation & Evolution
        • Solar System & Exoplanets
        • Telescope Instrumentation
        • Transient & Compact Objects
      • Earth Science
        • Back
        • Earth Science
        • Experimental Petrology
        • Geochemistry
        • Geophysics & Geodynamics
        • Mineralogy & Mineral Physics
      • Ecology
        • Back
        • Ecology
        • Atmospheric Science & Energy
        • Adaptation to Climate Change
        • Water Quality & Scarcity
      • Genetics & Developmental Biology
        • Back
        • Genetics & Developmental Biology
        • Adaptation to Climate Change
        • Developmental Biology & Human Health
        • Genomics
        • Model Organism Development
        • Nested Ecosystems
        • Symbiosis
      • Matter at Extreme States
        • Back
        • Matter at Extreme States
        • Extreme Environments
        • Extreme Materials
        • Mineralogy & Mineral Physics
      • Planetary Science
        • Back
        • Planetary Science
        • Astrobiology
        • Cosmochemistry
        • Mineralogy & Mineral Physics
        • Planet Formation & Evolution
        • Solar System & Exoplanets
      • Plant Science
        • Back
        • Plant Science
        • Adaptation to Climate Change
        • Nested Ecosystems
        • Photosynthesis
        • Symbiosis
    • Divisions
      • Back
      • Divisions
      • Biosphere Sciences & Engineering
        • Back
        • Biosphere Sciences & Engineering
        • About

          Contact Us

          Business Address
          5241 Broad Branch Rd. NW

          Washington , DC 20015
          United States place Map
          Call Us (202) 387-640
        • Research
        • Culture
      • Earth & Planets Laboratory
        • Back
        • Earth & Planets Laboratory
        • About

          Contact Us

          Business Address
          5241 Broad Branch Rd. NW

          Washington , DC 20015
          United States place Map
          Call Us (202) 387-640
        • Research
        • Culture
        • Campus
      • Observatories
        • Back
        • Observatories
        • About

          Contact Us

          Business Address
          5241 Broad Branch Rd. NW

          Washington , DC 20015
          United States place Map
          Call Us (202) 387-640
        • Research
        • Culture
        • Campus
    • Instrumentation
      • Back
      • Instrumentation
      • Our Telescopes
        • Back
        • Our Telescopes
        • Magellan Telescopes
        • Swope Telescope
        • du Pont Telescope
      • Observatories Machine Shop
      • EPL Research Facilities
      • EPL Machine Shop
      • Mass Spectrometry Facility
      • Advanced Imaging Facility
  • People
    • Back
    • People
      Observatory Staff

      Featured Staff Member

      Staff Member

      Staff Member

      Professional Title

      Learn More
      Observatory Staff

      Search For

    • Search All People
      • Back
      • Staff Scientists
      • Leadership
      • Biosphere Science & Engineering People
      • Earth & Planets Laboratory People
      • Observatories People
    Observatory Staff
    Dr. Gwen Rudie
    Staff Scientist, Director of the Carnegie Astrophysics Summer Student Internship (CASSI)

    Featured Staff Member

    Gwen Rudie

    Dr. Gwen Rudie

    Staff Scientist, Director of the Carnegie Astrophysics Summer Student Internship (CASSI)

    Learn More
    Observatory Staff
    Dr. Gwen Rudie
    Staff Scientist, Director of the Carnegie Astrophysics Summer Student Internship (CASSI)

    Gwen Rudie specializes in observational studies of distant galaxies and the diffuse gas which surrounds them—the circumgalactic medium.

    Search For

    Search All Staff
  • Events
    • Back
    • Events
    • Search All Events
      • Back
      • Public Events
      • Biosphere Science & Engineering Events
      • Earth & Planets Laboratory Events
      • Observatories Events

    Upcoming Events

    Events

    Events

    Solar telescopes at the Carnegie Science Observatories annual Open House
    Public Program

    City of Astronomy Week 2025

    Carnegie Astronomers

    November 16

    12:00pm PST

    Caleb Sharf NLS - A Giant Leap
    Public Program

    The Giant Leap

    Dr. Caleb Scharf

    November 6

    6:30pm EST

    Two people look at each other
    Public Program

    Face Value: How the Brain Shapes Human Connection

    Nancy Kanwisher

    October 29

    6:30pm EDT

  • News
    • Back
    • News
    • Search All News
      • Back
      • Biosphere Science & Engineering News
      • Earth & Planets Laboratory News
      • Observatories News
      • Carnegie Science News
    News

    Recent News

    News

    News and updates from across Carnegie Science.
    Read all News
    This 500-million-year-old trilobite from Utah has an organic-rich carapace that preserves a record of the original biomolecules. Credit: Robert Hazen.
    Breaking News
    November 17, 2025

    Chemical evidence of ancient life detected in 3.3-billion-year-old rocks

    Joe Berry and Lorenzo Rosa
    Breaking News
    November 14, 2025

    Two Carnegie Scientists Named 2025 Highly Cited Researchers

    NLS - Caleb Scharf - Full Auditorium
    Breaking News
    November 10, 2025

    Five ways Caleb Scharf’s "The Giant Leap" might rewire how you think about life

  • Donate
    • Back
    • Donate
      - ,

    • Make a Donation
      • Back
      • Support Scientific Research
      • The Impact of Your Gift
      • Carnegie Champions
      • Planned Giving
    Jo Ann Eder

    I feel passionately about the power of nonprofits to bolster healthy communities.

    - Jo Ann Eder , Astronomer and Alumna

    Header Text

    Postdoctoral alumna Jo Ann Eder is committed to making the world a better place by supporting organizations, like Carnegie, that create and foster STEM learning opportunities for all. 

    Learn more arrow_forward
  • Home

Abstract
Arabidopsis Cytochrome P450 85A2 (AtCYP85A2) was introduced to Arabidopsis thaliana seeds using a seed-specific promoter, pAt5g54000. GUS (beta-Glucuronidase) activity and RT-PCR analysis demonstrated that AtCYP85A2 overexpression only occurred in seeds of a transgenic plant, pAt5g54000-AtCYP85A2::Col-0. A crude enzyme solution prepared pAt5g54000-AtCYP85A2::Col-0 seeds successfully catalyzed the conversion of castasterone (CS) to brassinolide (BL), which was not detected in wild-type seeds. Furthermore, a higher level of CS and BL was detected in pAt5g54000-AtCYP85A2::Col-0 seeds compared to untransformed seeds, thus demonstrating that seed-specific overexpression of AtCYP85A2 efficiently encoded a bi-functional enzyme for brassinosteroids 6-oxidase/brassinolide synthase to generate CS and BL in seeds of pAt5g54000-AtCYP85A2::Col-0. Compared to the wild type, pAt5g54000-AtCYP85A2::Col-0 produced substantially larger seeds with a high concentration of nutrients due to an enhancement in brassinosteroids signaling. Additionally, pAt5g54000-AtCYP85A2::Col-0 exhibited superior seed germination, seedling and rosette plant growth, and flower and silique formation, indicating that seed-specific AtCYP85A2 expression activates overall vegetative and reproductive growth and development in A. thaliana.
View Full Publication open_in_new
Abstract
Brassinosteroid regulates carotenoid content through BZR1-mediated suppression of 4-HYDROXYPHENYLPYRUVATE DIOXYGENASEin Arabidopsis seedlings.
View Full Publication open_in_new
Abstract
The crosstalk mechanism regulating content and signal transduction between brassinosteroids (BRs) and salicylic acid (SA) for plant defense was investigated in Arabidopsis. Compared to the wild type, an increased bacterial resistance was observed in bzr1-1D, a dominant mutant of the BR transcription factor BZR1. In bzr1-1D, SA biosynthetic gene ICS1 expression and endogenous SA content greatly increased upon Pst DC3000 infection, and the direct binding of BZR1 to the ICS1 promoter was confirmed through EMSA and ChIP. In bzr1-1D where NPR1 expression was almost absent, expression of PR genes was increased, and both BZR1 and PR5 expressions increased after SA treatment. EMSA and ChIP verified that BZR1 binds directly to the cis-element present in the PR5 promoter and a pull-down assay showed that TGAs, SA transcription factors upstream of PR genes, interact with BZR1 at the protein level. Crude enzyme assays demonstrated that BR C-6 oxidase activity, a CYP85A1 function, greatly increased during Pst DC3000 infection. In the tga1 tga4 double mutant lacking SA transcription factors TGA1 and TGA4, BR biosynthetic gene CYP85A1 expression was significantly reduced. EMSA and ChIP confirmed that both TGA1 and TGA4 bind to the cis-element present in the CYP85A1 promoter, and castasterone (CS), a bio-active BR, was significantly reduced in tga1 tga4. Taken together, the upregulation of ICS1 expression by BZR1 and CYP85A1 expression by TGA1/4 mutually enhanced endogenous level of BR and SA in Arabidopsis. Furthermore, TGAs and BZR1 interaction at the protein level induces SA-induced immunity through the upregulation of PR5 expression, increasing bacterial resistance in the plant. These results explain the mutual control mechanisms of the synergistic effects BR and SA have on plant defense and confirm BR's effect on plant defense and growth promotion in A. thaliana.
View Full Publication open_in_new
Abstract
This study generated the transgenic Arabidopsis lines pAt5g54000-AtBZR1::Col-0 and pAt5g54000-AtBES1::Col-0, in which Arabidopsis BZR1 and BES1 (AtBZR1 and AtBES1) were seed-specifically expressed with pAt5g54000, a seed-specific promoter. Semi-quantitative RT-PCR and GUS-staining analysis demonstrated that the inserted AtBZR1 and AtBES1 were concentrated in seeds in siliques of transgenic plants. Seed number, length, width, and mass increased in the pAt5g54000-AtBZR1::Col-0 and pAt5g54000-AtBES1::Col-0 mutants compared to untransformed Arabidopsis. The endogenous levels of primary metabolites, such as carbohydrates, proteins, and lipids, in transgenic seeds were also higher than those in wild-type seeds, indicating that both seed size and quality are improved by seed-specific expression of AtBZR1 and AtBES1 in Arabidopsis. In both transgenic Arabidopsis seeds, relative to wild-type seeds, the expression of positive regulatory genes involved in determining seed size, such as SHORT HYPOCOTYL UNDER BLUE1 (AtSHB1), MINISEED3 (AtMINI3), and HAIKU2 (AtIKU2), was increased by up-regulation of AtBZR1 and AtBES1 as well as down-regulation of ABA Deficient 2 (AtABA2) and ABA Insensitive 5 (AtABI5). This result suggests that AtBZR1- and AtBES1-mediated signaling pathways such as AtBZR1/AtBES1 -> AtSHB1 -> AtMINI3 -> AtIKU2 and AtBZR1/AtBES1 -> AtABA2, and/or AtABI5 -> AtSHB1 -> AtMINI3 -> AtIKU2 increase the yield and quality of seeds in transgenic Arabidopsis. Taken together, our findings demonstrated the usefulness and applicability of seed-specific introduction of AtBZR1 and AtBES1 encoding key transcription factors in brassinosteroid signaling to improve seed yield and quality in Arabidopsis.
View Full Publication open_in_new
Abstract
Expression of ABA-deficient 2 (ABA2) gene involved in ABA biosynthesis was downregulated in bes1-D, but upregulated in bes1-KO. Hence, the expression of ABA2 is negatively controlled by the BES1 transcription factor of brassinosteroid signaling in Arabidopsis thaliana. BES1 is directly bound to the E-box sequences in the promoter of ABA2, which reduced the endogenous levels of ABA in the plant. The seeds of aba2-1 and bes1-KO were larger and smaller, respectively, than those of the wild type. In bes1-KO x aba2-1, the reduced seed size in bes1-KO was partly restored to the seed size in aba2-1. Hence, BES1-mediated regulation of seed size is an upstream process for the homeostasis of endogenous ABA to control the seed size. BES1 suppressed the expression of ABA Insensitive 5 (ABI5), a major transcription factor gene in ABA signaling that determines the seed size. It is directly bound to the promoter of ABI5 by BES1-induced downregulation of ABI5. The expression of SHORT HYPOCOTYL UNDER BLUE1, MINISEED3, and HAIKU2 as positively regulatory genes determining the seed size was activated, increasing the seed size in bes1-D. Conclusively, brassinosteroid signaling through BES1 downregulated both the biosynthesis and signaling of ABA, which increased the seed size in Arabidopsis.
View Full Publication open_in_new
Abstract
Dust grains absorb half of the radiation emitted by stars throughout the history of the universe, re-emitting this energy at infrared wavelengths(1-3). Polycyclic aromatic hydrocarbons (PAHs) are large organic molecules that trace millimetre-size dust grains and regulate the cooling of interstellar gas within galaxies(4,5). Observations of PAH features in very distant galaxies have been difficult owing to the limited sensitivity and wavelength coverage of previous infrared telescopes(6,7). Here we present James Webb Space Telescope observations that detect the 3.3 mu m PAH feature in a galaxy observed less than 1.5 billion years after the Big Bang. The high equivalent width of the PAH feature indicates that star formation, rather than black hole accretion, dominates infrared emission throughout the galaxy. The light from PAH molecules, hot dust and large dust grains and stars are spatially distinct from one another, leading to order-of-magnitude variations in PAH equivalent width and ratio of PAH to total infrared luminosity across the galaxy. The spatial variations we observe suggest either a physical offset between PAHs and large dust grains or wide variations in the local ultraviolet radiation field. Our observations demonstrate that differences in emission from PAH molecules and large dust grains are a complex result of localized processes within early galaxies.
View Full Publication open_in_new
Jason Williams

Jason Williams

Postdoctoral Fellow

Profile Photo

Sarah Sarkisian

Human Resources Specialist

Missing Headshot

Lauren Ploch

Development Officer, Major Gifts

Missing Headshot

Anthony Pahl

Carnegie Fellow

Pagination

  • Previous page chevron_left
  • …
  • Page 162
  • Page 163
  • Page 164
  • Page 165
  • Current page 166
  • Page 167
  • Page 168
  • Page 169
  • Page 170
  • …
  • Next page chevron_right
Subscribe to

Get the latest

Subscribe to our newsletters.

Privacy Policy
Home
  • Instagram instagram
  • Twitter twitter
  • Youtube youtube
  • Facebook facebook

Science

  • Biosphere Sciences & Engineering
  • Earth & Planets Laboratory
  • Observatories
  • Our Research Areas
  • Our Blueprint For Discovery

Legal

  • Financial Statements
  • Conflict of Interest Policy
  • Privacy Policy

Careers

  • Working at Carnegie
  • Scientific and Technical Jobs
  • Administrative & Support Jobs
  • Postdoctoral Program
  • Carnegie Connect (For Employees)

Contact Us

  • Contact Administration
  • Media Contacts

Business Address

5241 Broad Branch Rd. NW

Washington, DC 20015

place Map

© Copyright Carnegie Science 2025