The host galaxies of 106 rapidly evolving transients discovered by the Dark Energy Survey

Wiseman, P.; Pursiainen, M.; Childress, M.; Swann, E.; Smith, M.; Galbany, L.; Lidman, C.; Davis, T. M.; Gutiérrez, C. P.; Möller, A.; Thomas, B. P.; Frohmaier, C.; Foley, R. J.; Hinton, S. R.; Kelsey, L.; Kessler, R.; Lewis, G. F.; Sako, M.; Scolnic, D.; Sullivan, M.; Vincenzi, M.; Abbott, T. C.; Aguena, M.; Allam, S.; Annis, J.; Bertin, E.; Bhargava, S.; Brooks, D.; Burke, D. L.; Carnero Rosell, A.; Carollo, D.; Carrasco Kind, M.; Carretero, J.; Costanzi, M.; da Costa, L. N.; Diehl, H. T.; Doel, P.; Everett, S.; Fosalba, P.; Frieman, J.; García-Bellido, J.; Gaztanaga, E.; Glazebrook, K.; Gruen, D.; Gruendl, R. A.; Gschwend, J.; Gutierrez, G.; Hollowood, D. L.; Honscheid, K.; James, D. J.; Kuehn, K.; Kuropatkin, N.; Lima, M.; Maia, M. G.; Marshall, J. L.; Martini, P.; Menanteau, F.; Miquel, R.; Palmese, A.; Paz-Chinchón, F.; Plazas, A. A.; Romer, A. K.; Sanchez, E.; Scarpine, V.; Schubnell, M.; Serrano, S.; Sevilla-Noarbe, I.; Sommer, N. E.; Suchyta, E.; Swanson, M. C.; Tarle, G.; Tucker, B. E.; Tucker, D. L.; Varga, T. N.; Walker, A. R.

doi:10.1093/mnras/staa2474

Title: The host galaxies of 106 rapidly evolving transients discovered by the Dark Energy Survey

Abstract

Rapidly evolving transients (RETs), also termed fast blue optical transients, are a recently discovered group of astrophysical events that display rapid luminosity evolution. RETs typically rise to peak in less than 10 d and fade within 30, a time-scale unlikely to be compatible with the decay of Nickel-56 that drives conventional supernovae (SNe). Their peak luminosity spans a range of -15 < Mg < -22.5, with some events observed at redshifts greater than 1. Their evolution on fast time-scales has hindered high-quality follow-up observations, and thus their origin and explosion/emission mechanism remains unexplained. In this paper, we present the largest sample of RETs to date, comprising 106 objects discovered by the Dark Energy Survey, and perform the most comprehensive analysis of RET host galaxies. Using deep-stacked photometry and emission lines from OzDES spectroscopy, we derive stellar masses and star formation rates (SFRs) for 49 host galaxies, and metallicities ([O/H]) for 37. Here, we find that RETs explode exclusively in star-forming galaxies and are thus likely associated with massive stars. Comparing RET hosts to samples of host galaxies of other explosive transients as well as field galaxies, we find that RETs prefer galaxies with high specific SFRs ($$\langle$$log(sSFR)$$\rangle$$ ~ -9.6), indicating a link to young stellar populations, similar to stripped-envelope SNe. RET hosts appear to show a lack of chemical enrichment, their metallicities akin to long-duration gamma-ray bursts and superluminous SN host galaxies ($$\langle$$12+ log (O/H)$$\rangle$$ ~ 9.4). There are no clear relationships between mass or SFR of the host galaxies and the peak magnitudes or decline rates of the transients themselves.

Authors:

^[1];

^[1]; Swann, E. ^[2]; Smith, M. ^[1];

^[3];

^[4];

^[5]; Gutiérrez, C. P. ^[1]; Möller, A. ^[6]; Thomas, B. P. ^[2]; Frohmaier, C. ^[2]; Foley, R. J. ^[7]; Hinton, S. R. ^[5]; Kelsey, L. ^[1]; Kessler, R. ^[8]; Lewis, G. F. ^[9]; Sako, M. ^[10];

^[11]; Sullivan, M. ^[1] more »

School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK
Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK
PITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA
The Research School of Astronomy and Astrophysics, Australian National University, ACT 2601, Australia
School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia
Université Clermont Auvergne, CNRS/IN2P3, Laboratoire de Physique de Clermont, F-63000 Clermont-Ferrand, France
Santa Cruz Institute for Particle Physics, Santa Cruz, CA 95064, USA
Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, USA;Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, NSW 2006, Australia
Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, PA 19104, USA
Department of Physics, Duke University Durham, NC 27708, USA
Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile
Departamento de Física Matemática, Instituto de Física, Universidade de São Paulo, CP 66318, São Paulo, SP 05314-970, Brazil;Laboratório Interinstitucional de e-Astronomia – LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA
CNRS, UMR 7095, Institut d’Astrophysique de Paris, F-75014 Paris, France;Sorbonne Universités, UPMC Univ Paris 06, UMR 7095, Institut d’Astrophysique de Paris, F-75014 Paris, France
Department of Physics and Astronomy, Pevensey Building, University of Sussex, Brighton BN1 9QH, UK
Department of Physics & Astronomy, University College London, Gower Street, London WC1E 6BT, UK
Kavli Institute for Particle Astrophysics & Cosmology, PO Box 2450, Stanford University, Stanford, CA 94305, USA;SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Av. Complutense, E-28040, Madrid, Spain
INAF, Astrophysical Observatory of Turin, I-10025 Pino Torinese, Italy
Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 W. Green Street, Urbana, IL 61801, USA;National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA
Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain
INAF – Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy;Institute for Fundamental Physics of the Universe, Via Beirut 2, I-34014 Trieste, Italy
Laboratório Interinstitucional de e-Astronomia – LIneA, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil;Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
Institut d’Estudis Espacials de Catalunya (IEEC), E-08034 Barcelona, Spain;Institute of Space Sciences (ICE, CSIC), Campus UAB, Carrer de Can Magrans, s/n, E-08193 Barcelona, Spain
Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA;Fermi National Accelerator Laboratory, PO Box 500, Batavia, IL 60510, USA
Instituto de Fisica Teorica UAM/CSIC, Universidad Autonoma de Madrid, E-28049 Madrid, Spain
Centre for Astrophysics & Supercomputing, Swinburne University of Technology, Victoria 3122, Australia
Kavli Institute for Particle Astrophysics & Cosmology, PO Box 2450, Stanford University, Stanford, CA 94305, USA;SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA;Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA
Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA;Department of Physics, The Ohio State University, Columbus, OH 43210, USA
Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA
Australian Astronomical Optics, Macquarie University, North Ryde, NSW 2113, Australia;Lowell Observatory, 1400 Mars Hill Road, Flagstaff, AZ 86001, USA
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA;Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA
Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain;Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA;Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544, USA
Department of Physics, University of Michigan, Ann Arbor, MI 48109, USA
Computer Science and Mathematics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
National Center for Supercomputing Applications, 1205 West Clark St., Urbana, IL 61801, USA
Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse, D-85748 Garching, Germany;Universitäts-Sternwarte, Fakultät für Physik, Ludwig-Maximilians Universität München, Scheinerstr 1, D-81679 München, Germany

Publication Date:: Mon Aug 17 00:00:00 EDT 2020

Research Org.:: SLAC National Accelerator Lab., Menlo Park, CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States); Univ. of Michigan, Ann Arbor, MI (United States)

Sponsoring Org.:: USDOE Office of Science (SC), Basic Energy Sciences (BES); USDOE Office of Science (SC), High Energy Physics (HEP); Science and Technology Facilities Council (STFC) (United Kingdom); European Research Council (ERC); European Funds for Regional Development (FEDER); National Science Foundation (NSF); Brazilian Instituto Nacional de Ciencia e Tecnologia (INCT); Ministry of Economic Affairs and Digital Transformation of Spain (MINECO)

Contributing Org.:: DES Collaboration

OSTI Identifier:: 1706144

Alternate Identifier(s):: OSTI ID: 1768044; OSTI ID: 1783771; OSTI ID: 1819569

Report Number(s):: FERMILAB-PUB-20-206-AE; DES-2020-0534; arXiv:2005.08653
Journal ID: ISSN 0035-8711; oai:inspirehep.net:1823375

Grant/Contract Number:: AC02-07CH11359; AC02-76SF00515; AC02-05CH11231; ST/R000506/1; ST/P006760/1; AST-1536171; AST-1138766; SEV-2016-0588; SEV-2016-0597; MDM-2015-0509; FPA2015-68048; ESP2015-66861; AYA2015-71825; 291329; 240672; 306478; 465376/2014-2; SC0019193

Resource Type:: Accepted Manuscript

Journal Name:: Monthly Notices of the Royal Astronomical Society

Additional Journal Information:: Journal Volume: 498; Journal Issue: 2; Journal ID: ISSN 0035-8711

Publisher:: Royal Astronomical Society

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; transients: supernovae; galaxies: star formation; galaxies: abundances; galaxies: photometry

Citation Formats


                    Wiseman, P., Pursiainen, M., Childress, M., Swann, E., Smith, M., Galbany, L., Lidman, C., Davis, T. M., Gutiérrez, C. P., Möller, A., Thomas, B. P., Frohmaier, C., Foley, R. J., Hinton, S. R., Kelsey, L., Kessler, R., Lewis, G. F., Sako, M., Scolnic, D., Sullivan, M., Vincenzi, M., Abbott, T. C., Aguena, M., Allam, S., Annis, J., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carollo, D., Carrasco Kind, M., Carretero, J., Costanzi, M., da Costa, L. N., Diehl, H. T., Doel, P., Everett, S., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Glazebrook, K., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M. G., Marshall, J. L., Martini, P., Menanteau, F., Miquel, R., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Sommer, N. E., Suchyta, E., Swanson, M. C., Tarle, G., Tucker, B. E., Tucker, D. L., Varga, T. N., and Walker, A. R. The host galaxies of 106 rapidly evolving transients discovered by the Dark Energy Survey.  United States: N. p., 2020. 
Web.  doi:10.1093/mnras/staa2474.

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                    Wiseman, P., Pursiainen, M., Childress, M., Swann, E., Smith, M., Galbany, L., Lidman, C., Davis, T. M., Gutiérrez, C. P., Möller, A., Thomas, B. P., Frohmaier, C., Foley, R. J., Hinton, S. R., Kelsey, L., Kessler, R., Lewis, G. F., Sako, M., Scolnic, D., Sullivan, M., Vincenzi, M., Abbott, T. C., Aguena, M., Allam, S., Annis, J., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carollo, D., Carrasco Kind, M., Carretero, J., Costanzi, M., da Costa, L. N., Diehl, H. T., Doel, P., Everett, S., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Glazebrook, K., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M. G., Marshall, J. L., Martini, P., Menanteau, F., Miquel, R., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Sommer, N. E., Suchyta, E., Swanson, M. C., Tarle, G., Tucker, B. E., Tucker, D. L., Varga, T. N., & Walker, A. R. The host galaxies of 106 rapidly evolving transients discovered by the Dark Energy Survey.  United States.  https://doi.org/10.1093/mnras/staa2474

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                    Wiseman, P., Pursiainen, M., Childress, M., Swann, E., Smith, M., Galbany, L., Lidman, C., Davis, T. M., Gutiérrez, C. P., Möller, A., Thomas, B. P., Frohmaier, C., Foley, R. J., Hinton, S. R., Kelsey, L., Kessler, R., Lewis, G. F., Sako, M., Scolnic, D., Sullivan, M., Vincenzi, M., Abbott, T. C., Aguena, M., Allam, S., Annis, J., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carollo, D., Carrasco Kind, M., Carretero, J., Costanzi, M., da Costa, L. N., Diehl, H. T., Doel, P., Everett, S., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Glazebrook, K., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M. G., Marshall, J. L., Martini, P., Menanteau, F., Miquel, R., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Sommer, N. E., Suchyta, E., Swanson, M. C., Tarle, G., Tucker, B. E., Tucker, D. L., Varga, T. N., and Walker, A. R. Mon .  
"The host galaxies of 106 rapidly evolving transients discovered by the Dark Energy Survey".  United States.  https://doi.org/10.1093/mnras/staa2474.  https://www.osti.gov/servlets/purl/1706144.

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@article{osti_1706144,

  title        = {The host galaxies of 106 rapidly evolving transients discovered by the Dark Energy Survey},

  author       = {Wiseman, P. and Pursiainen, M. and Childress, M. and Swann, E. and Smith, M. and Galbany, L. and Lidman, C. and Davis, T. M. and Gutiérrez, C. P. and Möller, A. and Thomas, B. P. and Frohmaier, C. and Foley, R. J. and Hinton, S. R. and Kelsey, L. and Kessler, R. and Lewis, G. F. and Sako, M. and Scolnic, D. and Sullivan, M. and Vincenzi, M. and Abbott, T. C. and Aguena, M. and Allam, S. and Annis, J. and Bertin, E. and Bhargava, S. and Brooks, D. and Burke, D. L. and Carnero Rosell, A. and Carollo, D. and Carrasco Kind, M. and Carretero, J. and Costanzi, M. and da Costa, L. N. and Diehl, H. T. and Doel, P. and Everett, S. and Fosalba, P. and Frieman, J. and García-Bellido, J. and Gaztanaga, E. and Glazebrook, K. and Gruen, D. and Gruendl, R. A. and Gschwend, J. and Gutierrez, G. and Hollowood, D. L. and Honscheid, K. and James, D. J. and Kuehn, K. and Kuropatkin, N. and Lima, M. and Maia, M. G. and Marshall, J. L. and Martini, P. and Menanteau, F. and Miquel, R. and Palmese, A. and Paz-Chinchón, F. and Plazas, A. A. and Romer, A. K. and Sanchez, E. and Scarpine, V. and Schubnell, M. and Serrano, S. and Sevilla-Noarbe, I. and Sommer, N. E. and Suchyta, E. and Swanson, M. C. and Tarle, G. and Tucker, B. E. and Tucker, D. L. and Varga, T. N. and Walker, A. R.},

  abstractNote = {Rapidly evolving transients (RETs), also termed fast blue optical transients, are a recently discovered group of astrophysical events that display rapid luminosity evolution. RETs typically rise to peak in less than 10 d and fade within 30, a time-scale unlikely to be compatible with the decay of Nickel-56 that drives conventional supernovae (SNe). Their peak luminosity spans a range of -15 < Mg < -22.5, with some events observed at redshifts greater than 1. Their evolution on fast time-scales has hindered high-quality follow-up observations, and thus their origin and explosion/emission mechanism remains unexplained. In this paper, we present the largest sample of RETs to date, comprising 106 objects discovered by the Dark Energy Survey, and perform the most comprehensive analysis of RET host galaxies. Using deep-stacked photometry and emission lines from OzDES spectroscopy, we derive stellar masses and star formation rates (SFRs) for 49 host galaxies, and metallicities ([O/H]) for 37. Here, we find that RETs explode exclusively in star-forming galaxies and are thus likely associated with massive stars. Comparing RET hosts to samples of host galaxies of other explosive transients as well as field galaxies, we find that RETs prefer galaxies with high specific SFRs ($\langle$log(sSFR)$\rangle$ ~ -9.6), indicating a link to young stellar populations, similar to stripped-envelope SNe. RET hosts appear to show a lack of chemical enrichment, their metallicities akin to long-duration gamma-ray bursts and superluminous SN host galaxies ($\langle$12+ log (O/H)$\rangle$ ~ 9.4). There are no clear relationships between mass or SFR of the host galaxies and the peak magnitudes or decline rates of the transients themselves.},

  doi          = {10.1093/mnras/staa2474},

  journal      = {Monthly Notices of the Royal Astronomical Society},

  number       = 2,

  volume       = 498,

  place        = {United States},

  year         = {Mon Aug 17 00:00:00 EDT 2020},

  month        = {Mon Aug 17 00:00:00 EDT 2020}

}

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Supernova host galaxies in the dark energy survey: I. Deep coadds, photometry, and stellar masses

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The 5-yr Dark Energy Survey Supernova Programme (DES-SN) is one of the largest and deepest transient surveys to date in terms of volume and number of supernovae. Identifying and characterizing the host galaxies of transients plays a key role in their classification, the study of their formation mechanisms, and the cosmological analyses. In this work, to derive accurate host galaxy properties, we create depth-optimized coadds using single-epoch DES-SN images that are selected based on sky and atmospheric conditions. For each of the five DES-SN seasons, a separate coadd is made from the other four seasons such that each SN hasmore »« less
Cited by 21
https://doi.org/10.1093/mnras/staa1302
The mystery of photometric twins DES17X1boj and DES16E2bjy

Journal Article Pursiainen, M. ; Gutiérrez, C. P. ; Wiseman, P. ; ... - Monthly Notices of the Royal Astronomical Society

In this paper, we present an analysis of DES17X1boj and DES16E2bjy, two peculiar transients discovered by the Dark Energy Survey (DES). They exhibit nearly identical double-peaked light curves that reach very different maximum luminosities (more »« less
Cited by 4
https://doi.org/10.1093/mnras/staa995
μ⋆ masses: weak-lensing calibration of the Dark Energy Survey Year 1 redMaPPer clusters using stellar masses

Journal Article Pereira, M. E. S. ; Palmese, A. ; Varga, T. N. ; ... - Monthly Notices of the Royal Astronomical Society

We present the weak-lensing mass calibration of the stellar-mass-based μ_{more » $$\star$$} mass proxy for redMaPPer galaxy clusters in the Dark Energy Survey Year 1. For the first time, we are able to perform a calibration of μ_$$\star$$ at high redshifts, z > 0.33. In a blinded analysis, we use ~6000 clusters split into 12 subsets spanning the ranges 0.1 ≤ z < 0.65 and μ$$\star$$ up to $${\sim} 5.5 \times 10^{13} \, \mathrm{M}_{\odot }$$, and infer the average masses of these subsets through modelling of their stacked weak-lensing signal. In our model, we account for the following sources of systematic uncertainty: shear measurement and photometric redshift errors, miscentring, cluster-member contamination of the source sample, deviations from the Navarro–Frenk–White halo profile, halo triaxiality, and projection effects. We use the inferred masses to estimate the joint mass–μ_$$\star$$–z scaling relation given by $$\langle M_{200c} | \mu _{\star },z \rangle = M_0 (\mu _{\star }/5.16\times 10^{12} \, \mathrm{M_{\odot }})^{F_{\mu _{\star }}} ((1+z)/1.35)^{G_z}$$. We find $$M_0= (1.14 \pm 0.07) \times 10^{14} \, \mathrm{M_{\odot }}$$ with $$F_{\mu _{\star }}= 0.76 \pm 0.06$$ and Gz = -1.14 ± 0.37. We discuss the use of μ_$$\star$$ as a complementary mass proxy to the well-studied richness λ for: (i) exploring the regimes of low z, λ < 20 and high λ, z ~1; and (ii) testing systematics such as projection effects for applications in cluster cosmology.« less
https://doi.org/10.1093/mnras/staa2687
First cosmology results using type Ia supernovae from the Dark Energy Survey: the effect of host galaxy properties on supernova luminosity

Journal Article Smith, M. ; Sullivan, M. ; Wiseman, P. ; ... - Monthly Notices of the Royal Astronomical Society

We present improved photometric measurements for the host galaxies of 206 spectroscopically confirmed type Ia supernovae discovered by the Dark Energy Survey Supernova Program (DES-SN) and used in the first DES-SN cosmological analysis. For the DES-SN sample, when considering a 5D (z, x1, c, α, β) bias correction, we find evidence of a Hubble residual ‘mass step’, where SNe Ia in high-mass galaxies (>1010M⊙) are intrinsically more luminous (after correction) than their low-mass counterparts bymore »« less
Cited by 44
https://doi.org/10.1093/mnras/staa946
Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z ∼ 1

Journal Article Gupta, N. ; Pannella, M. ; Mohr, J. J. ; ... - Monthly Notices of the Royal Astronomical Society

Here, we study the properties of the Sydney University Molonglo Sky Survey (SUMSS) 843 MHz radio active galactic nuclei (AGNs) population in galaxy clusters from two large catalogues created using the Dark Energy Survey (DES): ~11,800 optically selected RM-Y3 and ~1000 X-ray selected MARD-Y3 clusters. We show that cluster radio loud AGNs are highly concentrated around cluster centres tomore »« less
Cited by 6
https://doi.org/10.1093/mnras/staa832

Similar Records

Title: The host galaxies of 106 rapidly evolving transients discovered by the Dark Energy Survey

Abstract

Citation Formats

The Absolute rate of lgrb Formation journal, June 2016

The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package journal, August 2018

GRB hosts through cosmic time: VLT/X-Shooter emission-line spectroscopy of 96 journal, September 2015

MEASURED METALLICITIES AT THE SITES OF NEARBY BROAD-LINED TYPE Ic SUPERNOVAE AND IMPLICATIONS FOR THE SUPERNOVAE GAMMA-RAY BURST CONNECTION journal, March 2008

The Prism Multi-Object Survey (Primus). i. Survey Overview and Characteristics journal, October 2011

Secondary standard stars for absolute spectrophotometry journal, March 1983

Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds journal, June 1998

The Sloan Digital sky Survey-Ii Supernova Survey: Search Algorithm and Follow-Up Observations journal, December 2007

Superluminous supernovae from the Dark Energy Survey journal, May 2019

Gamma-ray bursts from stellar mass accretion disks around black holes journal, March 1993

The Zwicky Transient Facility: System Overview, Performance, and First Results journal, December 2018

Superluminous supernova progenitors have a half-solar metallicity threshold journal, June 2017

Evolutionary stellar population synthesis with MILES - I. The base models and a new line index system journal, March 2010

Probing Cosmic Star Formation Using Long Gamma‐Ray Bursts: New Constraints from the Spitzer Space Telescope journal, May 2006

SN2018kzr: A Rapidly Declining Transient from the Destruction of a White Dwarf journal, October 2019

An unusual supernova in the error box of the γ-ray burst of 25 April 1998 journal, October 1998

Observations of Gamma-Ray Bursts of Cosmic Origin journal, May 1973

The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole? journal, December 2018

corner.py: Scatterplot matrices in Python journal, June 2016

THE LOCAL HOSTS OF TYPE Ia SUPERNOVAE journal, December 2009

Automated Transient Identification in the dark Energy Survey journal, August 2015

The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra journal, June 2020

Core-Collapse Supernovae and host Galaxy Stellar Populations journal, October 2012

The Cosmic Core-Collapse Supernova rate does not Match the Massive-Star Formation rate journal, August 2011

Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift /BAT6 complete sample of bright LGRBs: III. Stellar masses, star formation rates, and metallicities at z > 1 journal, February 2019

Galaxy And Mass Assembly: the G02 field, Herschel–ATLAS target selection and data release 3 journal, November 2017

The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS Spectroscopic Survey of the Chandra Deep Field-South: Arizona CDFS Environment Survey (ACES) journal, August 2012

Cosmic evolution and metal aversion in superluminous supernova host galaxies journal, September 2017

A fast-evolving luminous transient discovered by K2/Kepler journal, March 2018

OzDES multi-object fibre spectroscopy for the Dark Energy Survey: results and second data release journal, May 2020

Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies journal, September 2006

Stellar Mass-To-Light Ratios from Galaxy Spectra: how Accurate can they be? journal, November 2009

Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift /BAT6 complete sample of bright LGRBs : II. Star formation rates and metallicities at journal, May 2016

Hydrogen-poor Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey journal, January 2018

Wind-reprocessed Transients journal, April 2020

A High-Metallicity host Environment for the Long-Duration grb 020819 journal, February 2010

The relationship between infrared, optical, and ultraviolet extinction journal, October 1989

Selecting superluminous supernovae in faint galaxies from the first year of the Pan-STARRS1 Medium Deep Survey journal, February 2015

Metallicity Calibrations and the Mass‐Metallicity Relation for Star‐forming Galaxies journal, July 2008

ALMA Observations of Molecular Gas in the Host Galaxy of AT2018cow journal, July 2019

The Sloan Digital Sky Survey: Technical Summary journal, September 2000

Long γ‐Ray Bursts and Type Ic Core‐Collapse Supernovae Have Similar Locations in Hosts journal, November 2008

The chemical enrichment of long gamma-ray bursts nurseries up to z = 2 journal, March 2017

UV Star Formation Rates in the Local Universe journal, December 2007

THE EFFECT OF PROGENITOR AGE AND METALLICITY ON LUMINOSITY AND 56 Ni YIELD IN TYPE Ia SUPERNOVAE journal, January 2009

Galactic Stellar and Substellar Initial Mass Function journal, July 2003

Progenitor mass constraints for core-collapse supernovae from correlations with host galaxy star formation★: CC SN environments journal, June 2012

A Mildly Relativistic Outflow from the Energetic, Fast-rising Blue Optical Transient CSS161010 in a Dwarf Galaxy journal, May 2020

The H$\mathsf{\alpha}$ Galaxy Survey: III. Constraints on supernova progenitors from spatial correlations with H$\mathsf{\alpha}$ emission journal, June 2006

The rate of core Collapse Supernovae to Redshift 2.5 from the Candels and Clash Supernova Surveys journal, November 2015

HOST GALAXIES OF TYPE Ia SUPERNOVAE FROM THE NEARBY SUPERNOVA FACTORY journal, May 2013

Diversity of common envelope jets supernovae and the fast transient AT2018cow journal, February 2019

The Universal Relation of Galactic Chemical Evolution: the Origin of the Mass-Metallicity Relation journal, August 2014

Light Curves of Hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory journal, June 2018

A HIGHLY CONSISTENT FRAMEWORK FOR THE EVOLUTION OF THE STAR-FORMING “MAIN SEQUENCE” FROM z ∼ 0-6 journal, September 2014

A very energetic supernova associated with the γ-ray burst of 29 March 2003 journal, June 2003

Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies journal, March 2015

Stellar masses and star formation histories for 10 5 galaxies from the Sloan Digital Sky Survey journal, May 2003

A SPECTROSCOPIC STUDY OF TYPE Ibc SUPERNOVA HOST GALAXIES FROM UNTARGETED SURVEYS journal, October 2012

The Seventh data Release of the Sloan Digital sky Survey journal, May 2009

Luminous Supernovae journal, August 2012

Stellar population synthesis at the resolution of 2003 journal, October 2003

Matplotlib: A 2D Graphics Environment journal, January 2007

Aperture Effects on the Oxygen Abundance Determinations from Califa data journal, July 2016

Studying the environment of AT 2018cow with MUSE journal, May 2020

GAMA: towards a physical understanding of galaxy formation journal, October 2009

The Koala: A Fast Blue Optical Transient with Luminous Radio Emission from a Starburst Dwarf Galaxy at z = 0.27 journal, May 2020

iPTF 16asu: A Luminous, Rapidly Evolving, and High-velocity Supernova journal, December 2017

Aperture corrections for disk galaxy properties derived from the CALIFA survey: Balmer emission lines in spiral galaxies journal, May 2013

The mystery of photometric twins DES17X1boj and DES16E2bjy journal, April 2020

OzDES multifibre spectroscopy for the Dark Energy Survey: 3-yr results and first data release journal, July 2017

Hydrogen-Poor Superluminous Supernovae and Long-Duration Gamma-Ray Bursts have Similar host Galaxies journal, May 2014

Optical Spectra of Supernovae journal, September 1997

Evidence for Late-stage Eruptive Mass Loss in the Progenitor to SN2018gep, a Broad-lined Ic Supernova: Pre-explosion Emission and a Rapidly Rising Luminous Transient journal, December 2019

Classification parameters for the emission-line spectra of extragalactic objects journal, February 1981

Host Galaxies of Type Ic and Broad-lined Type Ic Supernovae from the Palomar Transient Factory: Implications for Jet Production journal, April 2020

Dependence of Type Ia supernova luminosities on their local environment journal, July 2018

The Absolute rate of lgrb Formation
journal, June 2016

The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package
journal, August 2018

GRB hosts through cosmic time: VLT/X-Shooter emission-line spectroscopy of 96
journal, September 2015

MEASURED METALLICITIES AT THE SITES OF NEARBY BROAD-LINED TYPE Ic SUPERNOVAE AND IMPLICATIONS FOR THE SUPERNOVAE GAMMA-RAY BURST CONNECTION
journal, March 2008

The Prism Multi-Object Survey (Primus). i. Survey Overview and Characteristics
journal, October 2011

Secondary standard stars for absolute spectrophotometry
journal, March 1983

Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds
journal, June 1998

The Sloan Digital sky Survey-Ii Supernova Survey: Search Algorithm and Follow-Up Observations
journal, December 2007

Superluminous supernovae from the Dark Energy Survey
journal, May 2019

Gamma-ray bursts from stellar mass accretion disks around black holes
journal, March 1993

The Zwicky Transient Facility: System Overview, Performance, and First Results
journal, December 2018

Superluminous supernova progenitors have a half-solar metallicity threshold
journal, June 2017

Evolutionary stellar population synthesis with MILES - I. The base models and a new line index system
journal, March 2010

Probing Cosmic Star Formation Using Long Gamma‐Ray Bursts: New Constraints from the Spitzer Space Telescope
journal, May 2006

SN2018kzr: A Rapidly Declining Transient from the Destruction of a White Dwarf
journal, October 2019

An unusual supernova in the error box of the γ-ray burst of 25 April 1998
journal, October 1998

Observations of Gamma-Ray Bursts of Cosmic Origin
journal, May 1973

The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole?
journal, December 2018

corner.py: Scatterplot matrices in Python
journal, June 2016

THE LOCAL HOSTS OF TYPE Ia SUPERNOVAE
journal, December 2009

Automated Transient Identification in the dark Energy Survey
journal, August 2015

The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra
journal, June 2020

Core-Collapse Supernovae and host Galaxy Stellar Populations
journal, October 2012

The Cosmic Core-Collapse Supernova rate does not Match the Massive-Star Formation rate
journal, August 2011

Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift /BAT6 complete sample of bright LGRBs: III. Stellar masses, star formation rates, and metallicities at z > 1
journal, February 2019

Galaxy And Mass Assembly: the G02 field, Herschel–ATLAS target selection and data release 3
journal, November 2017

The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS Spectroscopic Survey of the Chandra Deep Field-South: Arizona CDFS Environment Survey (ACES)
journal, August 2012

Cosmic evolution and metal aversion in superluminous supernova host galaxies
journal, September 2017

A fast-evolving luminous transient discovered by K2/Kepler
journal, March 2018

OzDES multi-object fibre spectroscopy for the Dark Energy Survey: results and second data release
journal, May 2020

Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies
journal, September 2006

Stellar Mass-To-Light Ratios from Galaxy Spectra: how Accurate can they be?
journal, November 2009

Are long gamma-ray bursts biased tracers of star formation? Clues from the host galaxies of the Swift /BAT6 complete sample of bright LGRBs : II. Star formation rates and metallicities at
journal, May 2016

Hydrogen-poor Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey
journal, January 2018

Wind-reprocessed Transients
journal, April 2020

A High-Metallicity host Environment for the Long-Duration grb 020819
journal, February 2010

The relationship between infrared, optical, and ultraviolet extinction
journal, October 1989

Selecting superluminous supernovae in faint galaxies from the first year of the Pan-STARRS1 Medium Deep Survey
journal, February 2015

Metallicity Calibrations and the Mass‐Metallicity Relation for Star‐forming Galaxies
journal, July 2008

ALMA Observations of Molecular Gas in the Host Galaxy of AT2018cow
journal, July 2019

The Sloan Digital Sky Survey: Technical Summary
journal, September 2000

Long γ‐Ray Bursts and Type Ic Core‐Collapse Supernovae Have Similar Locations in Hosts
journal, November 2008

The chemical enrichment of long gamma-ray bursts nurseries up to z = 2
journal, March 2017

UV Star Formation Rates in the Local Universe
journal, December 2007

THE EFFECT OF PROGENITOR AGE AND METALLICITY ON LUMINOSITY AND ⁵⁶ Ni YIELD IN TYPE Ia SUPERNOVAE
journal, January 2009

Galactic Stellar and Substellar Initial Mass Function
journal, July 2003

Progenitor mass constraints for core-collapse supernovae from correlations with host galaxy star formation★: CC SN environments
journal, June 2012

A Mildly Relativistic Outflow from the Energetic, Fast-rising Blue Optical Transient CSS161010 in a Dwarf Galaxy
journal, May 2020

The H$\mathsf{\alpha}$ Galaxy Survey: III. Constraints on supernova progenitors from spatial correlations with H$\mathsf{\alpha}$ emission
journal, June 2006

The rate of core Collapse Supernovae to Redshift 2.5 from the Candels and Clash Supernova Surveys
journal, November 2015

HOST GALAXIES OF TYPE Ia SUPERNOVAE FROM THE NEARBY SUPERNOVA FACTORY
journal, May 2013

Diversity of common envelope jets supernovae and the fast transient AT2018cow
journal, February 2019

The Universal Relation of Galactic Chemical Evolution: the Origin of the Mass-Metallicity Relation
journal, August 2014

Light Curves of Hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory
journal, June 2018

A HIGHLY CONSISTENT FRAMEWORK FOR THE EVOLUTION OF THE STAR-FORMING “MAIN SEQUENCE” FROM z ∼ 0-6
journal, September 2014

A very energetic supernova associated with the γ-ray burst of 29 March 2003
journal, June 2003

Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies
journal, March 2015

Stellar masses and star formation histories for 10 ⁵ galaxies from the Sloan Digital Sky Survey
journal, May 2003

A SPECTROSCOPIC STUDY OF TYPE Ibc SUPERNOVA HOST GALAXIES FROM UNTARGETED SURVEYS
journal, October 2012

The Seventh data Release of the Sloan Digital sky Survey
journal, May 2009

Luminous Supernovae
journal, August 2012

Stellar population synthesis at the resolution of 2003
journal, October 2003

Matplotlib: A 2D Graphics Environment
journal, January 2007

Aperture Effects on the Oxygen Abundance Determinations from Califa data
journal, July 2016

Studying the environment of AT 2018cow with MUSE
journal, May 2020

GAMA: towards a physical understanding of galaxy formation
journal, October 2009

The Koala: A Fast Blue Optical Transient with Luminous Radio Emission from a Starburst Dwarf Galaxy at z = 0.27
journal, May 2020

iPTF 16asu: A Luminous, Rapidly Evolving, and High-velocity Supernova
journal, December 2017

Aperture corrections for disk galaxy properties derived from the CALIFA survey: Balmer emission lines in spiral galaxies
journal, May 2013

The mystery of photometric twins DES17X1boj and DES16E2bjy
journal, April 2020

OzDES multifibre spectroscopy for the Dark Energy Survey: 3-yr results and first data release
journal, July 2017

Hydrogen-Poor Superluminous Supernovae and Long-Duration Gamma-Ray Bursts have Similar host Galaxies
journal, May 2014

Optical Spectra of Supernovae
journal, September 1997

Evidence for Late-stage Eruptive Mass Loss in the Progenitor to SN2018gep, a Broad-lined Ic Supernova: Pre-explosion Emission and a Rapidly Rising Luminous Transient
journal, December 2019

Classification parameters for the emission-line spectra of extragalactic objects
journal, February 1981

Host Galaxies of Type Ic and Broad-lined Type Ic Supernovae from the Palomar Transient Factory: Implications for Jet Production
journal, April 2020

Dependence of Type Ia supernova luminosities on their local environment
journal, July 2018

Chemical abundances in high-redshift galaxies: a powerful new emission line diagnostic
journal, January 2016

A Wind-driven Model: Application to Peculiar Transients AT2018cow and iPTF14hls
journal, July 2020

Fast-rising blue optical transients and AT2018cow following electron-capture collapse of merged white dwarfs
journal, July 2019