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| HRG14 J123635.50+621350.1 , the SIMBAD biblio (18 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST08:04:31 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 2009ApJ...704..117K | 31 | 2 | Lyman break galaxies at z ∼ 5: rest-frame UV spectra. III. | KAJINO H., OHTA K., IWATA I., et al. | |||||
|
2011PASJ...63S.379K |
15 | D | 2 | 10045 | 46 | MOIRCS Deep Survey. IX. Deep near-infrared imaging data and source catalog. | KAJISAWA M., ICHIKAWA T., TANAKA I., et al. | ||
|
2014ApJS..214...24S |
15 | D | 1 | 97940 | 733 | 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses. | SKELTON R.E., WHITAKER K.E., MOMCHEVA I.G., et al. | ||
|
2015ApJ...803...34B |
16 | D | 2 | 10313 | 1045 | UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields. | BOUWENS R.J., ILLINGWORTH G.D., OESCH P.A., et al. | ||
|
2015ApJ...814...95F |
16 | D | 1 | 176 | 40 | An increasing stellar baryon fraction in bright galaxies at high redshift. | FINKELSTEIN S.L., SONG M., BEHROOZI P., et al. | ||
|
2015ApJ...815...57U |
16 | D | 1 | 306 | 7 | A correlation between Lyα spectral line profile and rest-frame UV morphology. | U V., HEMMATI S., DARVISH B., et al. | ||
|
2016ApJS..224...15X |
16 | D | 1 | 1499 | 121 | The 2 Ms Chandra Deep Field-North survey and the 250 Ks Extended Chandra Deep Field-South survey: improved point-source catalogs. | XUE Y.Q., LUO B., BRANDT W.N., et al. | ||
| 2017ApJ...846L..30S | 2845 | A | S X C | 70 | 3 | 11 | The MOSDEF survey: first measurement of nebular oxygen abundance at z > 4. | SHAPLEY A.E., SANDERS R.L., REDDY N.A., et al. | |
|
2018ApJS..237...12O |
16 | D | 1 | 25243 | 42 | HDUV: the Hubble Deep UV Legacy Survey. | OESCH P.A., MONTES M., REDDY N., et al. | ||
|
2018MNRAS.478.3740A |
16 | D | 1 | 1561 | 2 | A simultaneous search for high-z LAEs and LBGs in the SHARDS survey. | ARRABAL HARO P., RODRIGUEZ ESPINOSA J.M., MUNOZ-TUNON C., et al. | ||
| 2018ApJ...869...92R | 80 | X | 1 | 2 | 80 | The MOSDEF survey: significant evolution in the rest-frame optical emission line equivalent widths of star-forming galaxies at z = 1.4-3.8. | REDDY N.A., SHAPLEY A.E., SANDERS R.L., et al. | ||
|
2020MNRAS.495.1807A |
16 | D | 1 | 1551 | ~ | Differences and similarities of stellar populations in LAEs and LBGs at z ∼ 3.4-6.8. | ARRABAL HARO P., RODRIGUEZ ESPINOSA J.M., MUNOZ-TUNON C., et al. | ||
| 2021MNRAS.508.1686W | 170 | X C | 3 | 5 | 17 | Assessing the sources of reionization: a spectroscopic case study of a 30x lensed galaxy at z ∼ 5 with Lyα, C IV, Mg II, and [Ne III]. | WITSTOK J., SMIT R., MAIOLINO R., et al. | ||
|
2021ApJS..257...68S |
17 | D | 2 | 9083 | 17 | The Spitzer/IRAC Legacy over the GOODS fields: full-depth 3.6, 4.5, 5.8, and 8.0 µm mosaics and photometry for >9000 galaxies at z ∼ 3.5-10 from the GOODS Reionization Era wide-Area Treasury from Spitzer (GREATS). | STEFANON M., LABBE I., OESCH P.A., et al. | ||
| 2025ApJ...989..209S | 3247 | A | X C | 69 | 4 | ~ | The AURORA Survey: The Nebular Attenuation Curve of a Galaxy at z = 4.41 from Ultraviolet to Near-infrared Wavelengths. | SANDERS R.L., SHAPLEY A.E., TOPPING M.W., et al. | |
| 2025ApJ...994..170K | 93 | C | 1 | 6 | ~ | The AURORA Survey: Tracing Galactic Outflows at z ≳ 2.5 with JWST/NIRSpec Near-ultraviolet Absorption Lines. | KEHOE E., SHAPLEY A.E., SANDERS R.L., et al. | ||
| 2026ApJ...996...37P | 300 | X | 6 | 6 | ~ | The AURORA Survey: Ionizing Photon Production Efficiency with Minimal Nebular Dust Attenuation Systematics. | PAHL A.J., SHAPLEY A., REDDY N.A., et al. | ||
| 2026ApJ...999...15R | 300 | X C | 5 | 14 | ~ | The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z = 1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-unity Dust Covering Fractions. | REDDY N.A., SHAPLEY A.E., SANDERS R.L., et al. |