|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| ACS-GC 13026669 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:49:01 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2012ApJ...756...72W |
15 | D | 1 | 523 | 6 | A fully identified sample of AEGIS20 microjansky radio sources. | WILLNER S.P., ASHBY M.L.N., BARMBY P., et al. | ||
|
2012ApJS..202....6G |
15 | D | 1 | 2980 | 36 | The Chandra X-ray point-source catalog in the DEEP2 Galaxy Redshift Survey fields. | GOULDING A.D., FORMAN W.R., HICKOX R.C., 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. | ||
|
2016ApJS..225...27M |
16 | D | 1 | 19341 | 548 | The 3D-HST survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for ∼ 100,000 galaxies. | MOMCHEVA I.G., BRAMMER G.B., VAN DOKKUM P.G., et al. | ||
|
2017ApJS..229...32S |
16 | D | 1 | 37883 | 113 | CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS Extended Groth Strip. | STEFANON M., YAN H., MOBASHER B., et al. | ||
|
2020ApJ...888...78S |
16 | D | 1 | 2590 | 25 | A catalog of AGN host galaxies observed with HST/ACS: correlations between star formation and AGN activity. | STEMO A., COMERFORD J.M., BARROWS R.S., et al. | ||
|
2022ApJ...937L..33S |
17 | D | 1 | 956 | 19 | Rest-frame Near-infrared Sizes of Galaxies at Cosmic Noon: Objects in JWST's Mirror Are Smaller than They Appeared. | SUESS K.A., BEZANSON R., NELSON E.J., et al. | ||
| 2025MNRAS.544.4505L | 19 | D | 1 | 92 | ~ | Constraining the AGN tori at cosmic noon using high-resolution JWST imaging and simultaneous SED fitting. | LIYA D.H., ROSARIO D.J. and CHARIDIS M. |