| human | Q5 |
| P8880 | AstroGen ID | 29332 |
| P227 | GND ID | 140932615 |
| P9467 | IAU member ID | 16970 |
| P2930 | INSPIRE-HEP author ID | R.Skelton.1 |
| P213 | ISNI | 0000000077607506 |
| P496 | ORCID iD | 0000-0001-7393-3336 |
| P214 | VIAF ID | 107899423 |
| P10832 | WorldCat Entities ID | E39PCjvPtyBMFw3hfbv77yK9Tb |
| P27 | country of citizenship | Germany | Q183 |
| P69 | educated at | Heidelberg University | Q151510 |
| P734 | family name | Skelton | Q28152955 |
| Skelton | Q28152955 | ||
| Skelton | Q28152955 | ||
| P735 | given name | Rosalind | Q20165788 |
| Rosalind | Q20165788 | ||
| P463 | member of | International Astronomical Union | Q6867 |
| P106 | occupation | astronomer | Q11063 |
| physicist | Q169470 | ||
| researcher | Q1650915 | ||
| P21 | sex or gender | female | Q6581072 |
| P937 | work location | Heidelberg | Q2966 |
| Q59723515 | 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses |
| Q59938949 | 3D-HST grism spectroscopy of a gravitationally lensed, low-metallicity starburst galaxy at z = 1.847 |
| Q58492573 | 3D-HST+CANDELS: the evolution of the galaxy size-mass distribution since z = 3 |
| Q59938952 | 3D-HST: a wide-field grism spectroscopic survey with the Hubble Space Telescope |
| Q58908452 | A CANDELS-3D-HST synergy: resolved star formation patterns at 0.7 < z < 1.5 |
| Q34435399 | A massive galaxy in its core formation phase three billion years after the Big Bang |
| Q56060696 | A remarkably luminous galaxy at z=11.1 measured with Hubble Space Telescope grism spectroscopy |
| Q59781260 | A tensegrity approach to the optimal reinforcement of masonry domes and vaults through fiber-reinforced composite materials |
| Q59723443 | Ages of massive galaxies at 0.5 > z > 2.0 from 3D-HST rest-frame optical spectroscopy |
| Q58908410 | Bulge growth and quenching since z = 2.5 in CANDELS/3D-HST |
| Q63375732 | CLEAR. I. Ages and Metallicities of Quiescent Galaxies at 1.0 < z < 1.8 Derived from Deep Hubble Space Telescope Grism Data |
| Q59781233 | Composite solar façades and wind generators with tensegrity architecture |
| Q58908458 | Confirmation of small dynamical and stellar masses for extreme emission line galaxies at z ~ 2 |
| Q59723509 | Constraining the low-mass slope of the star formation sequence at 0.5 < z < 2.5 |
| Q114823350 | Decoding the star forming properties of gas-rich galaxy pairs |
| Q59723519 | Dense cores in galaxies out to z = 2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fields |
| Q59927048 | Direct measurements of dust attenuation in z ~ 1.5 star-forming galaxies from 3D-HST: implications for dust geometry and star formation rates |
| Q59781271 | Experimental investigation of the softening–stiffening response of tensegrity prisms under compressive loading |
| Q69206211 | Exploring the chemical link between local ellipticals and their high-redshift progenitors |
| Q112108661 | Extending the evolution of the stellar mass–size relation at z ≤ 2 to low stellar mass galaxies from HFF and CANDELS |
| Q59938954 | First results from the 3D-HST survey: the striking diversity of massive galaxies at z > 1 |
| Q59723460 | Forming compact massive galaxies |
| Q59723318 | Galaxy Mergers up to Z < 2.5. I. The Star Formation Properties of Merging Galaxies at Separations of 3–15 kpc |
| Q59723465 | Galaxy structure as a driver of the star formation sequence slope and scatter |
| Q59806847 | Geometry of star-forming galaxies from SDSS, 3D-HST, and CANDELS |
| Q59723349 | HFF-DeepSpace Photometric Catalogs of the 12 Hubble Frontier Fields, Clusters, and Parallels: Photometry, Photometric Redshifts, and Stellar Masses |
| Q58923160 | HSTHα grism spectroscopy of ROLES: a flatter low-mass slope for thez ∼ 1 SSFR–mass relation |
| Q63375642 | High-redshift Massive Quiescent Galaxies Are as Flat as Star-forming Galaxies: The Flattening of Galaxies and the Correlation with Structural Properties in CANDELS/3D-HST |
| Q58492596 | History of galaxy interactions and their impact on star formation over the last 7 gyr from GEMS |
| Q59723504 | How dead are dead galaxies? mid-infrared fluxes of quiescent galaxies at redshift 0.3 < z < 2.5: implications for star formation rates and dust heating |
| Q59938950 | Hα EQUIVALENT WIDTHS FROM THE 3D-HST SURVEY: EVOLUTION WITH REDSHIFT AND DEPENDENCE ON STELLAR MASS |
| Q59938946 | Large-scale star-formation-driven outflows at 1 < z < 2 in the 3D-HST survey |
| Q58492594 | Less than 10 percent of star formation in z ~ 0.6 massive galaxies is triggered by major interactions |
| Q68185724 | Leveraging 3D-HST grism redshifts to quantify photometric redshift performance |
| Q59781272 | Minimum mass design of tensegrity bridges with parametric architecture and multiscale complexity |
| Q69033629 | Modeling the red sequence: hierarchical growth yet slow luminosity evolution |
| Q60023473 | Observations of environmental quenching in groups in the 11 GYR since z = 2.5: different quenching for central and satellite galaxies |
| Q59781263 | On the additive manufacturing, post-tensioning and testing of bi-material tensegrity structures |
| Q59938939 | On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 < z < 2.8 |
| Q59781267 | On the use of tensegrity structures for kinetic solar facades of smart buildings |
| Q59723391 | Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5 |
| Q68949933 | Spatially resolved dust maps from Balmer decrements in galaxies at z ~ 1.4 |
| Q59938953 | Spatially resolved h{alpha} maps and sizes of 57 strongly star-forming galaxies at z ~ 1 from 3D-HST: evidence for rapid inside-out assembly of disk galaxies |
| Q68124589 | Stellar kinematics of z ~ 2 galaxies and the inside-out growth of quiescent galaxies |
| Q56775379 | Structural Control: Past, Present, and Future |
| Q59723433 | The 3D-HST survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for ~ 100,000 galaxies |
| Q59927039 | The MOSFIRE deep evolution field (MOSDEF) survey: rest-frame optical spectroscopy for ~1500 h-selected galaxies at 1.37 <= z <= 3.8 |
| Q59723396 | The Mass, Color, and Structural Evolution of Today’s Massive Galaxies Since z ∼ 5 |
| Q59784063 | The Norma cluster (ACO3627) - II. The near-infrared -band luminosity function |
| Q59723359 | The Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy |
| Q68911275 | The assembly of milky-way-like galaxies since z ~ 2.5 |
| Q69190466 | The close pair fraction of BCGs since z = 0.5: major mergers dominate recent BCG stellar mass growth |
| Q68488061 | The effect of dry mergers on the color-magnitude relation of early-type galaxies |
| Q59723436 | The evolution of the fractions of quiescent and star-forming galaxies as a function of stellar mass since z = 3: increasing importance of massive, dusty star-forming galaxies in the early universe |
| Q68906805 | The merger-driven evolution of massive galaxies |
| Q59852232 | The most luminous z ~ 9-10 galaxy candidates yet found: the luminosity function, cosmic star-formation rate, and the first mass density estimate at 500 myr |
| Q58908397 | The nature of extreme emission line galaxies at z = 1-2: kinematics and metallicities from near-infrared spectroscopy |
| Q59938943 | The radial distribution of star formation in galaxies at z ~ 1 from the 3D-HST survey |
| Q59723427 | The relation between [O III]/H{beta} and specific star formation rate in galaxies at z ~ 2 |
| Q59938942 | The spatial extent and distribution of star formation in 3D-HST mergers at z ∼ 1.5 |
| Q69058957 | The structural evolution of milky-way-like star-forming galaxies since z ~ 1.3 |
| Q59710043 | Where stars form: inside-out growth and coherent star formation from HST H{alpha} maps of 3200 galaxies across the main sequence at 0.7 < z < 1.5 |
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