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ASASSN -14lp , the SIMBAD biblio (63 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.28CEST19:02:14 |
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 |
---|---|---|---|---|---|---|---|---|---|
2015ApJS..221...22I | 41 | X | 1 | 12 | 26 | The very early light curve of SN 2015F in NGC 2442: a possible detection of shock-heated cooling emission and constraints on SN Ia progenitor system. | IM M., CHOI C., YOON S.-C., et al. | ||
2015BAVSR..64...34W | O | 2 | ~ | ASASSN-14lp eine helle Supernova in NGC 4666. | WENZEL K. | ||||
2015BAVSR..64...94H | O | 2 | ~ | ASASSN-14lp, die im Januar/Februar 2015 hellste zu beobachtende Supernova. | HAMBSCH F.J. | ||||
2016ApJ...820...67Z | 86 | X | 2 | 10 | 64 | Optical observations of the Type Ia supernova SN 2011fe in M101 for nearly 500 days. | ZHANG K., WANG X., ZHANG J., et al. | ||
2014ATel.6795....1H | 118 | X | 3 | 2 | 3 | ASAS-SN Discovery of A Bright Probable Supernova in NGC 4666. | HOLOIEN T.W.-S., STANEK K.Z., KOCHANEK C.S., et al. | ||
2014ATel.6801....1T | 158 | T | X | 3 | 1 | 3 |
Spectroscopic Classification of ASASSN-14lp as a SN Ia. |
THORSTENSEN J., ALPER E., SHAPPEE B.J., et al. | |
2014ATel.6815....1F | 119 | T | X | 2 | 1 | 2 | HST Observations of ASASSN -14lp. | FOLEY R.J. | |
2016ApJ...822L..16S | 202 | X | 5 | 14 | 17 | Post-maximum near-infrared spectra of SN 2014J: a search for interaction signatures. | SAND D.J., HSIAO E.Y., BANERJEE D.P.K., et al. | ||
2016ApJ...826...96P | 125 | X | 2 | 2 | 91 | Exploring the potential diversity of early type Ia supernova light curves. | PIRO A.L. and MOROZOVA V.S. | ||
2016ApJ...826..144S | 2773 | T K A | D | X C | 68 | 12 | 52 |
The young and bright type Ia supernova ASASSN-14lp: discovery, early-time observations, first-light time, distance to NGC 4666, and progenitor constraints. |
SHAPPEE B.J., PIRO A.L., HOLOIEN T.W.-S., et al. |
2016MNRAS.461.1308F | 844 | K A | D | X C F | 20 | 16 | 22 | Ultraviolet diversity of Type Ia Supernovae. | FOLEY R.J., PAN Y., BROWN P., et al. |
2016MNRAS.462..649B | 361 | A | D | S X C | 8 | 35 | 11 | Progressive redshifts in the late-time spectra of Type Ia supernovae. | BLACK C.S., FESEN R.A. and PARRENT J.T. |
2017MNRAS.464.2672H | 16 | D | 1 | 171 | 29 | The ASAS-SN bright supernova catalogue - I. 2013-2014. | HOLOIEN T.W.-S., STANEK K.Z., KOCHANEK C.S., et al. | ||
2017ApJ...841...48S | 44 | X | 1 | 10 | 34 | Whimper of a bang: documenting the final days of the nearby Type Ia supernova 2011fe. | SHAPPEE B.J., STANEK K.Z., KOCHANEK C.S., et al. | ||
2017ApJ...841...64Z | 81 | X | 2 | 40 | 13 | Discovery and follow-up observations of the young Type Ia supernova 2016coj. | ZHENG W., FILIPPENKO A.V., MAUERHAN J., et al. | ||
2017ApJ...845L..11H | 135 | X C | 2 | 9 | 121 | Early blue excess from the Type Ia supernova 2017cbv and implications for its progenitor. | HOSSEINZADEH G., SAND D.J., VALENTI S., et al. | ||
2017A&A...603A.136P | 41 | X | 1 | 15 | 1 | Testing for redshift evolution of Type Ia supernovae using the strongly lensed PS1-10afx at z = 1.4. | PETRUSHEVSKA T., AMANULLAH R., BULLA M., et al. | ||
2017ApJ...848...66Z | 260 | D | X | 7 | 66 | 4 | An empirical fitting method for Type Ia supernova light curves. II. Estimating the first-light time and rise time. | ZHENG W., KELLY P.L. and FILIPPENKO A.V. | |
2017MNRAS.472.2787N | 44 | X | 1 | 9 | 32 | Early light curves for Type Ia supernova explosion models. | NOEBAUER U.M., KROMER M., TAUBENBERGER S., et al. | ||
2017Sci...358.1574S | 38 | 6 | 228 | Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger. | SHAPPEE B.J., SIMON J.D., DROUT M.R., et al. | ||||
2018ApJ...855....6S | 126 | X | 3 | 14 | 44 | Strong evidence against a non-degenerate companion in SN 2012cg. | SHAPPEE B.J., PIRO A.L., STANEK K.Z., et al. | ||
2018ApJ...859...79G | 42 | X | 1 | 13 | 15 | Observations of SN 2015F suggest a correlation between the intrinsic luminosity of Type Ia supernovae and the shape of their light curves >900 days after explosion. | GRAUR O., ZUREK D.R., REST A., et al. | ||
2018ApJ...864L..35S | 17 | D | 1 | 26 | 51 | Red versus blue: early observations of thermonuclear supernovae reveal two distinct populations? | STRITZINGER M.D., SHAPPEE B.J., PIRO A.L., et al. | ||
2018MNRAS.479..517P | 165 | C F | 3 | 82 | 6 | Swift UVOT grism observations of nearby Type Ia supernovae - I. Observations and data reduction. | PAN Y.-C., FOLEY R.J., FILIPPENKO A.V., et al. | ||
2018ApJ...865..149J | 222 | D | X C | 5 | 54 | 13 | Surface radioactivity or interactions? Multiple origins of early-excess Type Ia supernovae and associated subclasses. | JIANG J.-A., DOI M., MAEDA K., et al. | |
2018ApJ...866...10G | 1712 | T K A | X C | 40 | 7 | 5 |
Late-time observations of ASASSN-14lp strengthen the case for a correlation between the peak luminosity of Type Ia supernovae and the shape of their late-time light curves. |
GRAUR O., ZUREK D.R., CARA M., et al. | |
2019ApJ...870L...1D | 48 | X | 1 | 14 | 84 | K2 observations of SN 2018oh reveal a two-component rising light curve for a Type Ia supernova. | DIMITRIADIS G., FOLEY R.J., REST A., et al. | ||
2019ApJ...870...13S | 46 | X | 1 | 17 | 71 | Seeing double: ASASSN-18bt exhibits a two-component rise in the early-time K2 light curve. | SHAPPEE B.J., HOLOIEN T.W.-S., DROUT M.R., et al. | ||
2019ApJ...870...14G | 268 | D | X | 7 | 7 | 6 | Late-time observations of the Type Ia supernova SN 2014J with the Hubble Space Telescope Wide Field Camera 3. | GRAUR O. | |
2019ApJ...870L..14D | 43 | X | 1 | 8 | 11 | Nebular spectroscopy of Kepler's brightest supernova. | DIMITRIADIS G., ROJAS-BRAVO C., KILPATRICK C.D., et al. | ||
2019MNRAS.483.1114B | 878 | A | D | S X C | 20 | 25 | 4 | Narrow transient absorptions in late-time optical spectra of type Ia supernovae: evidence for large clumps of iron-rich ejecta? | BLACK C.S., FESEN R.A. and PARRENT J.T. |
2019ApJ...872...14Z | 460 | X C | 10 | 13 | 1 | Observations of a fast-expanding and uv-bright Type Ia supernova SN 2013gs. | ZHANG T., WANG X., ZHAO X., et al. | ||
2019PASP..131a4001P | 59 | D | X | 2 | 416 | 58 | Carnegie Supernova Project-II: extending the near-infrared Hubble diagram for Type Ia supernovae to z ∼ 0.1. | PHILLIPS M.M., CONTRERAS C., HSIAO E.Y., et al. | |
2019PASP..131a4002H | 100 | D | C | 4 | 173 | 56 | Carnegie Supernova Project-II: the near-infrared spectroscopy program. | HSIAO E.Y., PHILLIPS M.M., MARION G.H., et al. | |
2019MNRAS.484.3785B | 17 | D | 1 | 918 | 27 | The relative specific Type Ia supernovae rate from three years of ASAS-SN. | BROWN J.S., STANEK K.Z., HOLOIEN T.W.-S., et al. | ||
2019ApJ...875L..14A | 268 | D | X C | 6 | 16 | 3 | Carnegie supernova Project-II: using near-infrared spectroscopy to determine the location of the outer 56Ni in Type Ia supernovae. | ASHALL C., HSIAO E.Y., HOEFLICH P., et al. | |
2019ApJ...878...86A | 84 | F | 1 | 14 | 3 | A physical basis for the H-band blue-edge velocity and light-curve shape correlation in context of Type Ia supernova explosion physics. | ASHALL C., HOEFLICH P., HSIAO E.Y., et al. | ||
2019MNRAS.487.2372V | 43 | X | 1 | 28 | 53 | ASASSN-18tb: a most unusual Type Ia supernova observed by TESS and SALT. | VALLELY P.J., FAUSNAUGH M., JHA S.W., et al. | ||
2019A&A...627A.174H | 42 | X | 1 | 19 | 15 | Discovery and progenitor constraints on the Type Ia supernova 2013gy. | HOLMBO S., STRITZINGER M.D., SHAPPEE B.J., et al. | ||
2019ApJ...882...30L | 42 | X | 1 | 15 | ~ | Observations of Type Ia supernova 2014J for nearly 900 days and constraints on its progenitor system. | LI W., WANG X., HU M., et al. | ||
2020MNRAS.491.2902F | 43 | X | 1 | 68 | 46 | Sub-Chandrasekhar progenitors favoured for Type Ia supernovae: evidence from late-time spectroscopy. | FLORS A., SPYROMILIO J., TAUBENBERGER S., et al. | ||
2020MNRAS.491.5897P | 60 | D | X | 2 | 59 | ~ | Swift UVOT grism observations of nearby Type Ia supernovae - II. Probing the progenitor metallicity of SNe Ia with ultraviolet spectra. | PAN Y.-C., FOLEY R.J., JONES D.O., et al. | |
2020MNRAS.492.4325S | 17 | D | 3 | 247 | 24 | Berkeley supernova Ia program: data release of 637 spectra from 247 Type Ia supernovae. | STAHL B.E., ZHENG W., DE JAEGER T., et al. | ||
2020A&A...634A..37M | 230 | D | X | 6 | 35 | 32 | Determining the 56Ni distribution of type Ia supernovae from observations within days of explosion. | MAGEE M.R., MAGUIRE K., KOTAK R., et al. | |
2020AJ....159..167L | 17 | D | 1 | 639 | 53 | The AMUSING++ nearby galaxy compilation. I. Full sample characterization and galactic-scale outflow selection. | LOPEZ-COBA C., SANCHEZ S.F., ANDERSON J.P., et al. | ||
2020ApJ...900L..27S | 44 | X | 1 | 17 | 27 | Strong calcium emission indicates that the ultraviolet-flashing SN Ia 2019yvq was the result of a sub-Chandrasekar-mass double-detonation explosion. | SIEBERT M.R., DIMITRIADIS G., POLIN A., et al. | ||
2020ApJS..250...12C | 570 | D | S X C | 12 | 39 | ~ | Artificial intelligence-assisted inversion (AIAI) of synthetic Type Ia supernova spectra. | CHEN X., HU L. and WANG L. | |
2020MNRAS.499.1424H | 17 | D | 1 | 408 | ~ | Supernovae and their host galaxies - VII. The diversity of Type Ia supernova progenitors. | HAKOBYAN A.A., BARKHUDARYAN L.V., KARAPETYAN A.G., et al. | ||
2021MNRAS.501.3122C | 17 | D | 1 | 116 | ~ | The delay time distribution of supernovae from integral-field spectroscopy of nearby galaxies. | CASTRILLO A., ASCASIBAR Y., GALBANY L., et al. | ||
2021ApJ...910..151M | 44 | X | 1 | 20 | ~ | Rapidly declining hostless Type Ia supernova KSP-OT-201509b from the KMTNet Supernova Program: transitional nature and constraint on 56Ni distribution and progenitor Type. | MOON D.-S., NI Y.Q., DROUT M.R., et al. | ||
2021PASP..133d4002B | 17 | D | 2 | 142 | ~ | Low-redshift Type Ia supernova from the LSQ/LCO collaboration. | BALTAY C., GROSSMAN L., HOWARD R., et al. | ||
2021MNRAS.504.2073K | 45 | X | 1 | 35 | 51 | A cool and inflated progenitor candidate for the Type Ib supernova 2019yvr at 2.6 yr before explosion. | KILPATRICK C.D., DROUT M.R., AUCHETTL K., et al. | ||
2021MNRAS.506..415B | 2089 | T K A | D | S X C | 46 | 9 | ~ |
ASASSN-14lp: two possible solutions for the observed ultraviolet suppression. |
BARNA B., PEREIRA T., TAUBENBERGER S., et al. |
2021MNRAS.508.1590P | 44 | X | 1 | 13 | ~ | Prospects of direct detection of 48V gamma-rays from thermonuclear supernovae. | PANTHER F.H., SEITENZAHL I.R., RUITER A.J., et al. | ||
2022MNRAS.510.3701S | 45 | X | 1 | 17 | 15 | An environmental analysis of the Type Ib SN 2019yvr and the possible presence of an inflated binary companion. | SUN N.-C., MAUND J.R., CROWTHER P.A., et al. | ||
2022MNRAS.511..691G | 46 | X | 1 | 17 | 17 | How much hydrogen is in Type Ib and IIb supernova progenitors? | GILKIS A. and ARCAVI I. | ||
2022ApJ...930...70H | 45 | X | 1 | 19 | 10 | Spectroscopic Studies of Type Ia Supernovae Using LSTM Neural Networks. | HU L., CHEN X. and WANG L. | ||
2022MNRAS.515.3703T | 134 | X | 3 | 14 | 4 | The late-time light curves of Type Ia supernovae: confronting models with observations. | TIWARI V., GRAUR O., FISHER R., et al. | ||
2022A&A...665A.123M | 90 | C | 1 | 6 | 3 | Testing the homogeneity of type Ia Supernovae in near-infrared for accurate distance estimations. | MULLER-BRAVO T.E., GALBANY L., KARAMEHMETOGLU E., et al. | ||
2023MNRAS.521.1162D | 47 | X | 1 | 30 | 9 | SN 2021zny: an early flux excess combined with late-time oxygen emission suggests a double white dwarf merger event. | DIMITRIADIS G., MAGUIRE K., KARAMBELKAR V.R., et al. | ||
2023MNRAS.522.3481D | 998 | K | D | X C F | 20 | 24 | 3 | SN 2021fxy: mid-ultraviolet flux suppression is a common feature of Type Ia supernovae. | DERKACY J.M., PAUGH S., BARON E., et al. |
2024ApJ...962...17W | 200 | X C | 3 | 18 | ~ | Flight of the Bumblebee: the Early Excess Flux of Type Ia Supernova 2023bee Revealed by TESS, Swift, and Young Supernova Experiment Observations. | WANG Q., REST A., DIMITRIADIS G., et al. | ||
2024ApJ...962..125C | 300 | X C | 5 | 9 | ~ | Artificial Intelligence Assisted Inversion (AIAI): Quantifying the Spectral Features of 56Ni of Type Ia Supernovae. | CHEN X., WANG L., HU L., et al. |