|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| ZFOURGE CDFS 9235 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST14:20:18 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2008ApJ...678..655F | 6 | 7 | 95 | Effects of dust geometry in Lyα galaxies at z = 4.4. | FINKELSTEIN S.L., RHOADS J.E., MALHOTRA S., et al. | ||||
| 2009ApJ...691..465F | 543 | D | S X F | 13 | 16 | 130 | Lyman alpha galaxies: primitive, dusty, or evolved? | FINKELSTEIN S.L., RHOADS J.E., MALHOTRA S., et al. | |
| 2009MNRAS.393.1174F | 165 | D | X F | 4 | 28 | 21 | The expected detection of dust emission from high-redshift Lyman α galaxies. | FINKELSTEIN S.L., MALHOTRA S., RHOADS J.E., et al. | |
| 2011ApJ...735....5F | 1117 | D | X C | 29 | 5 | 31 | Hubble space telescope imaging of Lyα emission at z ~ 4.4. | FINKELSTEIN S.L., COHEN S.H., WINDHORST R.A., et al. | |
| 2013MNRAS.431.3589Z | 15 | D | 1 | 56 | 19 | Lyα luminosity functions at redshift z ∼ 4.5. | ZHENG Z.-Y., FINKELSTEIN S.L., FINKELSTEIN K., 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...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. | ||
|
2016ApJ...830...51S
|
16 | D | 1 | 67525 | 168 | The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. | STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al. |
