NAME HS 1700 Protocluster , the SIMBAD biblio

NAME HS 1700 Protocluster , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST10:46:44


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Title First 3 Authors
2005ApJ...626...44S 14 4 173 Spectroscopic identification of a protocluster at z=2.300: environmental dependence of galaxy properties at high redshift. STEIDEL C.C., ADELBERGER K.L., SHAPLEY A.E., et al.
2007ApJ...668...23P 93 23 Morphologies of galaxies in and around a protocluster at z = 2.300. PETER A.H.G., SHAPLEY A.E., LAW D.R., et al.
2010MNRAS.407..846D 442 T   A     X   F     10 18 33 Excess AGN activity in the
z = 2.30 protocluster in HS 1700+64.
DIGBY-NORTH J.A., NANDRA K., LAIRD E.S., et al.
2011ApJ...736..160S 107           X         2 5 305 Diffuse Lyα emitting halos: a generic property of high-redshift star-forming galaxies. STEIDEL C.C., BOGOSAVLJEVIC M., SHAPLEY A.E., et al.
2011ApJ...740L..31E 231           X C       5 15 38 Filamentary large-scale structure traced by six Lyα blobs at z = 2.3. ERB D.K., BOGOSAVLJEVIC M. and STEIDEL C.C.
2012ApJ...750...67R 22       D               1 17 270 The gaseous environment of high-z galaxies: precision measurements of neutral hydrogen in the circumgalactic medium of z ∼ 2-3 galaxies in the Keck baryonic structure survey. RUDIE G.C., STEIDEL C.C., TRAINOR R.F., et al.
2012ApJ...757L..30R 16       D               1 16 57 The temperature-density relation in the intergalactic medium at redshift $ < z$ > = 2.4. RUDIE G.C., STEIDEL C.C. and PETTINI M.
2013ApJ...765...87L viz 41           X         1 5 23 Concurrent supermassive black hole and galaxy growth: linking environment and nuclear activity in z = 2.23 Hα emitters. LEHMER B.D., LUCY A.B., ALEXANDER D.M., et al.
2013ApJ...769..146R 19       D               1 15 111 The column density distribution and continuum opacity of the intergalactic and circumgalactic medium at redshift $ < z$ > = 2.4. RUDIE G.C., STEIDEL C.C., SHAPLEY A.E., et al.
2013ApJ...774..130K 156           X         4 29 37 The mass-metallicity relation of a z ∼ 2 protocluster with MOSFIRE. KULAS K.R., McLEAN I.S., SHAPLEY A.E., et al.
2013ApJ...776...75F 43           X         1 4 33 Searching for neutral hydrogen halos around z ∼ 2.1 and z ∼ 3.1 Lyα emitting galaxies. FELDMEIER J.J., HAGEN A., CIARDULLO R., et al.
2013ApJ...778..170K 40           X         1 11 27 The formation of the massive galaxies in the SSA22 z = 3.1 protocluster. KUBO M., UCHIMOTO Y.K., YAMADA T., et al.
2013ApJ...779..127C 99       D       C       3 20 226 Ancient light from young cosmic cities: physical and observational signatures of galaxy proto-clusters. CHIANG Y.-K., OVERZIER R. and GEBHARDT K.
2015MNRAS.449L..68C 302 T   A     X C       6 21 8 A blind CO detection of a distant red galaxy in the

HS1700+64 protocluster
.
CHAPMAN S.C., BERTOLDI F., SMAIL I., et al.
2015MNRAS.453..951C 262     A     X C       6 19 5 A millimetre-wave redshift search for the unlensed HyLIRG, HS1700.850.1. CHAPMAN S.C., BERTOLDI F., SMAIL I., et al.
2016MNRAS.460.3861K viz 2970     A D S   X C       73 32 11 Herschel protocluster survey: a search for dusty star-forming galaxies in protoclusters at z = 2-3. KATO Y., MATSUDA Y., SMAIL I., et al.
2016A&ARv..24...14O 170           X C       3 19 176 The realm of the galaxy protoclusters. OVERZIER R.A.
2017ApJ...839..131C 18       D               1 38 90 Mapping the Most Massive Overdensities Through Hydrogen (MAMMOTH). II. Discovery of the extremely massive overdensity BOSS1441 at z = 2.32. CAI Z., FAN X., BIAN F., et al.
2018MNRAS.474.4612L 58       D     X         2 33 9 Characterising and identifying galaxy protoclusters. LOVELL C.C., THOMAS P.A. and WILKINS S.M.
2018MNRAS.473.1977S viz 48           X         1 6 42 MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z = 2.5. SHIMAKAWA R., KODAMA T., HAYASHI M., et al.
2019ApJ...874...54M viz 251           X C       5 14 11 The fraction of active galactic nuclei in the USS 1558-003 Protocluster at z = 2.53. MACUGA M., MARTINI P., MILLER E.D., et al.
2019MNRAS.488.1790L 150     A     X         4 72 7 Two sub-millimetre bright protoclusters bounding the epoch of peak star-formation activity. LACAILLE K.M., CHAPMAN S.C., SMAIL I., et al.
2019ApJ...883..142H 17       D               1 89 67 SILVERRUSH. VIII. Spectroscopic identifications of early large-scale structures with protoclusters over 200 Mpc at z ∼ 6-7: strong associations of dusty star-forming galaxies. HARIKANE Y., OUCHI M., ONO Y., et al.
2019PASJ...71L...2K 50           X         1 3 24 Lyα view around a z = 2.84 hyperluminous QSO at a node of the cosmic web. KIKUTA S., MATSUDA Y., CEN R., et al.
2019ApJ...887..214K 42           X         1 14 ~ Planck far-infrared detection of Hyper Suprime-Cam protoclusters at z ∼ 4: hidden AGN and star formation activity. KUBO M., TOSHIKAWA J., KASHIKAWA N., et al.
2020A&A...642A..37B 175           X C       3 6 31 The DIANOGA simulations of galaxy clusters: characterising star formation in protoclusters. BASSINI L., RASIA E., BORGANI S., et al.
2020A&A...642A.149V 85           X         2 15 13 Chandra reveals a luminous Compton-thick QSO powering a Lyα blob in a z = 4 starbursting protocluster. VITO F., BRANDT W.N., LEHMER B.D., et al.
2021ApJ...919...51M viz 44           X         1 24 7 On the nature of AGN and star formation enhancement in the z = 3.1 SSA22 protocluster: the HST WFC3 IR view. MONSON E.B., LEHMER B.D., DOORE K., et al.
2021A&A...654A.121P 104       D     X         3 67 12 Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z = 2.16 in the Cosmos field. POLLETTA M., SOUCAIL G., DOLE H., et al.
2022ApJ...926...70W 18       D               1 48 14 The Mass-Metallicity Relation at Cosmic Noon in Overdense Environments: First Results from the MAMMOTH-Grism HST Slitless Spectroscopic Survey. WANG X., LI Z., CAI Z., et al.
2022A&A...662A..54T viz 63       D     X         2 17 10 The 700 ks Chandra Spiderweb Field. I. Evidence for widespread nuclear activity in the protocluster. TOZZI P., PENTERICCI L., GILLI R., et al.
2023ApJ...947...75K 93           X         2 4 2 UV and Lyα Halos of Lyα Emitters across Environments at z = 2.84. KIKUTA S., MATSUDA Y., INOUE S., et al.

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