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1. Unveiling the hidden Universe with JWST: the contribution of dust-obscured galaxies to the stellar mass function at z ~ 3 – 8

2. The NOEMA observations of GN-z11: constraining the neutral interstellar medium and dust formation in the heart of cosmic reionization at z = 10.6

3. The JWST FRESCO survey: legacy NIRCam/grism spectroscopy and imaging in the two GOODS fields

5. Unveiling the nature of infrared bright, optically dark galaxies with early JWST data

7. The prevalence of galaxy overdensities around UV-luminous Lyman 𝛼 emitters in the Epoch of Reionization

11. New Determinations of the UV Luminosity Functions from z ∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency

12. The Evolutionary Status of Clusters of Galaxies at Z ∼ 1

14. The HST Medium Deep Susrvey: Galaxy Morphology at High Redshift

15. The nature of faint galaxies from the medium deep survey and other deep HST images

16. An Advanced Camera for the Hubble Space Telescope

18. The Medium-Deep Survey Using the Hubble Space Telescope

19. An HR Diagram for the LMC From the Medium Deep Survey

25. HDUV: The Hubble Deep UV Legacy Survey

27. The HDUV Survey: Six Lyman Continuum Emitter Candidates atz∼ 2 Revealed byHSTUV Imaging

31. THE BRIGHT END OF THEz∼ 9 ANDz∼ 10 UV LUMINOSITY FUNCTIONS USING ALL FIVE CANDELS FIELDS

32. z≳ 7 GALAXIES WITH REDSPITZER/IRAC [3.6]–[4.5] COLORS IN THE FULL CANDELS DATA SET: THE BRIGHTEST-KNOWN GALAXIES ATz∼ 7–9 AND A PROBABLE SPECTROSCOPIC CONFIRMATION ATz= 7.48

34. A REMARKABLY LUMINOUS GALAXY ATZ= 11.1 MEASURED WITHHUBBLE SPACE TELESCOPEGRISM SPECTROSCOPY

35. ULTRADEEP IRAC IMAGING OVER THE HUDF AND GOODS-SOUTH: SURVEY DESIGN AND IMAGING DATA RELEASE

41. UV LUMINOSITY FUNCTIONS AT REDSHIFTSz∼ 4 TOz∼ 10: 10,000 GALAXIES FROMHSTLEGACY FIELDS

46. THE MOST LUMINOUSz∼ 9-10 GALAXY CANDIDATES YET FOUND: THE LUMINOSITY FUNCTION, COSMIC STAR-FORMATION RATE, AND THE FIRST MASS DENSITY ESTIMATE AT 500 Myr

47. THE SPECTRAL ENERGY DISTRIBUTIONS OF z ∼ 8 GALAXIES FROM THE IRAC ULTRA DEEP FIELDS: EMISSION LINES, STELLAR MASSES, AND SPECIFIC STAR FORMATION RATES AT 650 MYR

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