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Shoubaneh Hemmati

Identifiers

  • name variant Shoubaneh Hemmati 0.60 · backfill

Papers (37)

  1. Diffusion-based Galaxy Simulations for the Roman High Latitude Survey astro-ph.CO · 2026 · author #5
  2. Large Scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4 astro-ph.GA · 2023 · author #6
  3. The Universe SPHEREx Will See: Empirically Based Galaxy Simulations and Redshift Predictions astro-ph.CO · 2023 · author #8
  4. The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques astro-ph.GA · 2022 · author #34
  5. COSMOS-Web: An Overview of the JWST Cosmic Origins Survey astro-ph.GA · 2022 · author #40
  6. Deblending Galaxies with Generative Adversarial Networks astro-ph.CO · 2022 · author #1
  7. A Machine Learning Approach to Predict Missing Flux Densities in Multi-band Galaxy Surveys astro-ph.GA · 2022 · author #4
  8. Categorizing models using Self-Organizing Maps: an application to modified gravity theories probed by cosmic shear astro-ph.CO · 2021 · author #2
  9. Selection of massive evolved galaxies at $3 \leq z \leq 4.5$ in the CANDELS fields astro-ph.GA · 2020 · author #4
  10. Cosmology with the Wide-Field Infrared Survey Telescope -- Multi-Probe Strategies astro-ph.CO · 2020 · author #8
  11. Cosmology with the Wide-Field Infrared Survey Telescope -- Synergies with the Rubin Observatory Legacy Survey of Space and Time astro-ph.CO · 2020 · author #13
  12. Spectroscopic Confirmation of a Coma Cluster Progenitor at z ~ 2.2 astro-ph.GA · 2020 · author #10
  13. Bridging between the integrated and resolved main sequence of star formation astro-ph.GA · 2020 · author #1
  14. The CANDELS/SHARDS multi-wavelength catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission line fluxes and Star Formation Rates astro-ph.GA · 2019 · author #33
  15. Horizon-AGN virtual observatory -- 2: Template-free estimates of galaxy properties from colours astro-ph.GA · 2019 · author #6
  16. Bringing manifold learning and dimensionality reduction to SED fitters astro-ph.GA · 2019 · author #1
  17. The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s astro-ph.IM · 2019 · author #37
  18. Photometric Redshift Calibration Requirements for WFIRST Weak Lensing Cosmology: Predictions from CANDELS astro-ph.GA · 2018 · author #1
  19. WFIRST Science Investigation Team "Cosmology with the High Latitude Survey" Annual Report 2017 astro-ph.CO · 2018 · author #10
  20. SPLASH-SXDF Multi-wavelength Photometric Catalog astro-ph.GA · 2017 · author #13
  21. Scientific Synergy Between LSST and Euclid astro-ph.IM · 2017 · author #15
  22. Type Ia Supernova Distances at z > 1.5 from the Hubble Space Telescope Multi-Cycle Treasury Programs: The Early Expansion Rate astro-ph.CO · 2017 · author #22
  23. The clustering of H$\beta$+[OIII] and [OII] emitters since $z \sim 5$: dependencies with line luminosity and stellar mass astro-ph.GA · 2017 · author #9
  24. CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS Extended Groth Strip astro-ph.GA · 2017 · author #7
  25. Cosmic Web of Galaxies in the COSMOS Field: Public Catalog and Different Quenching for Centrals and Satellites astro-ph.GA · 2016 · author #7
  26. The Local [CII] 158 um Emission Line Luminosity Function astro-ph.GA · 2016 · author #1
  27. The Nature of H$\beta+$[O{\sc iii}] and [O{\sc ii}] emitters to $z \sim 5$ with HiZELS: stellar mass functions and the evolution of EWs astro-ph.GA · 2016 · author #7
  28. A Correlation Between Ly{\alpha} Spectral Line Profile and Rest-Frame UV Morphology astro-ph.GA · 2015 · author #2
  29. Spectroscopic Study of Star-forming Galaxies in Filaments and the Field at $z\sim$0.5: Evidence for Environmental Dependence of Electron Density astro-ph.GA · 2015 · author #4
  30. Nebular and Stellar Dust Extinction Across the Disk of Emission-Line Galaxies on Small (KPC) Scales astro-ph.GA · 2015 · author #1
  31. Two Type Ia Supernovae at Redshift ~2 : Improved Classification and Redshift Determination with Medium-band Infrared Imaging astro-ph.CO · 2015 · author #5
  32. Beyond Spheroids and Discs: Classifications of CANDELS Galaxy Structure at 1.4 < z < 2 via Principal Component Analysis astro-ph.GA · 2015 · author #10
  33. Evidence for PopIII-like stellar populations in the most luminous Lyman-$\alpha$ emitters at the epoch of re-ionisation: spectroscopic confirmation astro-ph.GA · 2015 · author #8
  34. Evolution of the H$\beta$+[OIII] and [OII] luminosity functions and the [OII] star-formation history of the Universe up to $z$ ~ 5 from HiZELS astro-ph.GA · 2015 · author #7
  35. Kpc-scale Properties of Emission-line Galaxies astro-ph.GA · 2014 · author #1
  36. A Study of Massive and Evolved Galaxies at High Redshift astro-ph.GA · 2014 · author #3
  37. Ly{\alpha} Emission from High Redshift Sources in COSMOS astro-ph.CO · 2012 · author #7

Mentions

  • 2312.10222 #6 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2312.04636 #8 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2110.13171 #2 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2211.07865 #40 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2212.01915 #34 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2208.14781 #4 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2211.04488 #1 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2004.05271 #8 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2004.04702 #13 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2005.12507 #4 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2002.01011 #1 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 2002.06207 #10 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1905.13233 #6 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1905.10379 #1 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1908.00569 #33 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1808.10458 #1 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1902.05569 #37 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1705.01101 #9 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1711.05280 #13 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1804.03628 #10 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1710.00844 #22 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1710.08489 #15 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1703.05768 #7 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1611.05451 #7 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1611.03092 #1 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1604.02456 #7 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1508.03100 #5 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1504.01751 #10 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1510.08446 #2 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1510.05009 #4 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1510.02506 #1 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1504.01734 #8 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1503.00004 #7 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1409.4791 #1 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1408.3684 #3 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1208.6031 #7 · arxiv_oai · confidence 0.70 Shoubaneh Hemmati
  • 1510.08446 #2 · backfill · confidence 0.70 Shoubaneh Hemmati
  • 1510.05009 #4 · backfill · confidence 0.70 Shoubaneh Hemmati
  • 1510.02506 #1 · backfill · confidence 0.70 Shoubaneh Hemmati
  • 1508.03100 #5 · backfill · confidence 0.70 Shoubaneh Hemmati
  • 1504.01751 #10 · backfill · confidence 0.70 Shoubaneh Hemmati
  • 1504.01734 #8 · backfill · confidence 0.70 Shoubaneh Hemmati
  • 1503.00004 #7 · backfill · confidence 0.70 Shoubaneh Hemmati
  • 1409.4791 #1 · backfill · confidence 0.70 Shoubaneh Hemmati
  • 1408.3684 #3 · backfill · confidence 0.70 Shoubaneh Hemmati
  • 1208.6031 #7 · backfill · confidence 0.70 Shoubaneh Hemmati

Frequent Coauthors