other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
SpARCS J104922+564032 , the SIMBAD biblio (30 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.05.04CEST05:19:50 |
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 |
---|---|---|---|---|---|---|---|---|---|
2015ApJ...809..173W | 1693 | A | S X C | 41 | 11 | 30 | An extreme starburst in the core of a rich galaxy cluster at z = 1.7. | WEBB T., NOBLE A., DEGROOT A., et al. | |
2015ApJ...814...96W | 164 | X | 4 | 5 | 59 | The star formation history of BCGs to z = 1.8 from the SpARCS/SWIRE survey: evidence for significant in situ star formation at high redshift. | WEBB T.M.A., MUZZIN A., NOBLE A., et al. | ||
2016A&A...593A...2A | 265 | A | X C | 6 | 174 | 14 | Size growth of red-sequence early-type galaxies in clusters in the last 10 Gyr. | ANDREON S., DONG H. and RAICHOOR A. | |
2017ApJ...843..126D | 423 | D | X C | 10 | 6 | 7 | Galaxy merger candidates in high-redshift cluster environments. | DELAHAYE A.G., WEBB T.M.A., NANTAIS J., et al. | |
2017ApJ...844L..17W | 316 | K A | X | 8 | 2 | 15 | Detection of a substantial molecular gas reservoir in a brightest cluster galaxy at z = 1.7. | WEBB T.M.A., LOWENTHAL J., YUN M., et al. | |
2018MNRAS.479.3563F | 346 | D | X C F | 7 | 42 | 8 | The rate of Type-Ia supernovae in galaxy clusters and the delay-time distribution out to redshift 1.75. | FRIEDMANN M. and MAOZ D. | |
2019MNRAS.487.1210T | 1488 | K A | X C F | 34 | 3 | ~ | Multiwavelength radio observations of a brightest cluster galaxy at z = 1.71: detection of a modest active galactic nucleus and evidence for extended star formation. | TRUDEAU A., WEBB T., HLAVACEK-LARRONDO J., et al. | |
2020MNRAS.491.3751D | 485 | D | S X C | 10 | 42 | 38 | The growth of brightest cluster galaxies and intracluster light over the past 10 billion years. | DEMAIO T., GONZALEZ A.H., ZABLUDOFF A., et al. | |
2020A&A...635L..10C | 324 | K A | X | 8 | 7 | ~ | Environmental processing in cluster core galaxies at z = 1.7. | CASTIGNANI G., COMBES F. and SALOME P. | |
2020A&A...635A..32C | 443 | D | X C | 10 | 127 | ~ | Molecular gas in distant brightest cluster galaxies. | CASTIGNANI G., COMBES F., SALOME P., et al. | |
2020ApJ...893...10F | 1813 | T A | X C | 41 | 12 | ~ |
Constraining the mass of the emerging galaxy cluster SpARCS1049+56 at z = 1.71 with infrared weak lensing. |
FINNER K., JEE M.J., WEBB T., et al. | |
2020ApJ...898L..50H | 1859 | A | S X C | 42 | 3 | 10 | Evidence of runaway gas cooling in the absence of supermassive black hole feedback at the epoch of cluster formation. | HLAVACEK-LARRONDO J., RHEA C.L., WEBB T., et al. | |
2020A&A...640A..65C | 85 | X | 2 | 35 | 17 | Molecular gas in CLASH brightest cluster galaxies at z ∼ 0.2 - 0.9. | CASTIGNANI G., PANDEY-POMMIER M., HAMER S.L., et al. | ||
2020A&A...641L...6D | 43 | X | 1 | 19 | ~ | Discovery of molecular gas fueling galaxy growth in a protocluster at z = 1.7. | D'AMATO Q., GILLI R., PRANDONI I., et al. | ||
2020MNRAS.499.3061N | 170 | X | 4 | 5 | ~ | The H α star formation main sequence in cluster and field galaxies at z ∼ 1.6. | NANTAIS J., WILSON G., MUZZIN A., et al. | ||
2021MNRAS.502.5882F | 17 | D | 2 | 67 | 16 | The delay time distribution of Type-Ia supernovae in galaxy clusters: the impact of extended star-formation histories. | FREUNDLICH J. and MAOZ D. | ||
2021ApJ...909L..29D | 87 | X | 2 | 36 | 5 | A CO Survey of SpARCS star-forming brightest cluster galaxies: evidence for uniformity in BCG molecular gas processing across cosmic time. | DUNNE D.A., WEBB T.M.A., NOBLE A., et al. | ||
2021A&A...648A..11O | 409 | D | S X C | 8 | 17 | 13 | Diffuse radio emission from galaxy clusters in the LOFAR Two-metre Sky Survey Deep Fields. | OSINGA E., VAN WEEREN R.J., BOXELAAR J.M., et al. | |
2021ApJ...912...87H | 17 | D | 1 | 70 | 7 | The HST See Change program. I. Survey design, pipeline, and supernova discoveries. | HAYDEN B., RUBIN D., BOONE K., et al. | ||
2021A&A...649A..42C | 17 | D | 1 | 141 | 14 | Physical properties of brightest cluster galaxies up to redshift 1.80 based on HST data. | CHU A., DURRET F. and MARQUEZ I. | ||
2022ApJ...930...25B | 1103 | T A | S X C | 22 | 3 | 3 |
An Assessment of the In Situ Growth of the Intracluster Light in the High-redshift Galaxy Cluster SpARCS1049+56. |
BARFETY C., VALIN F.-A., WEBB T.M.A., et al. | |
2022A&A...665A..48M | 45 | X | 1 | 12 | ~ | The strongest cool core in REXCESS: Missing X-ray cavities in RXC J2014.8-2430. | MROCZKOWSKI T., DONAHUE M., VAN MARREWIJK J., et al. | ||
2022ApJ...940...24L | 18 | D | 1 | 30 | 2 | A GMOS/IFU Study of Jellyfish Galaxies in Massive Clusters. | LEE J.H., LEE M.G., MUN J.Y., et al. | ||
2022A&A...667A..52C | 134 | X | 3 | 18 | 2 | Star-forming and gas-rich brightest cluster galaxies at z ∼ 0.4 in the Kilo-Degree Survey. | CASTIGNANI G., RADOVICH M., COMBES F., et al. | ||
2022A&A...668A..18Z | 45 | X | 1 | 14 | 4 | Extending empirical constraints on the SZ-mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at z ≳ 1. | ZOHREN H., SCHRABBACK T., BOCQUET S., et al. | ||
2023Natur.613...37J | 112 | D | X | 3 | 10 | 3 | Intracluster light is already abundant at redshift beyond unity. | JOO H. and JEE M.J. | |
2023ApJ...947...44C | 280 | X | 6 | 5 | ~ | SPT-CL J2215-3537: A Massive Starburst at the Center of the Most Distant Relaxed Galaxy Cluster. | CALZADILLA M.S., BLEEM L.E., McDONALD M., et al. | ||
2023A&A...672A.139C | 47 | X | 1 | 22 | ~ | Star-forming brightest cluster galaxies at z ∼ 0.4 in KiDS Further studies of cold gas and stellar properties. | CASTIGNANI G., RADOVICH M., COMBES F., et al. | ||
2023ApJ...954...56O | 93 | X | 2 | 76 | ~ | X-Ray Cavity Dynamics and Their Role in the Gas Precipitation in Planck Sunyaev-Zeldovich (SZ) Selected Clusters. | OLIVARES V., SU Y., FORMAN W., et al. | ||
2023A&A...677A...3C | 47 | X | 1 | 12 | ~ | A z = 1.85 galaxy group in CEERS: Evolved, dustless, massive intra-halo light and a brightest group galaxy in the making. | COOGAN R.T., DADDI E., LE BAIL A., et al. |