SN 2016hnk , the SIMBAD biblio

SN 2016hnk , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.14CEST13:02:18


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Title First 3 Authors
2018ApJ...855..107G viz 16       D               1 285 86 PISCO: the PMAS/PPak Integral-field Supernova hosts COmpilation. GALBANY L., ANDERSON J.P., SANCHEZ S.F., et al.
2018MNRAS.475L.111S 354 T   A     X         8 7 6 Chandra X-ray constraints on the candidate Ca-rich gap transient
SN 2016hnk.
SELL P.H., ARUR K., MACCARONE T.J., et al.
2016ATel.9685....1T 40           X         1 24 ~ ATLAS discoveries of optical transients. TONRY J., DENNEAU L., STALDER B., et al.
2016ATel.9703....1C 241 T         X         5 2 ~ Spectroscopic observations of
AT2016hnk by NUTS (NOT Un-biased Transient Survey).
CANNIZZARO G., FRASER M., BENETTI S., et al.
2016ATel.9704....1D 80           X         2 7 ~ PESSTO spectroscopic classification of optical transients. DIMITRIADIS G., PURSIAINEN M., SMITH M., et al.
2016ATel.9705....1P 482 T         X         11 5 ~ Spectroscopy of
SN 2016hnk (=
ATLAS16dpc) with SOAR and SALT: A Peculiar Type-Ia Supernova Similar to PTF09dav.
PAN Y.-C., DUARTE A.S., FOLEY R.J., et al.
2019A&A...630A..76G viz 7005   K A S   X C       166 45 31 Evidence for a Chandrasekhar-mass explosion in the Ca-strong 1991bg-like type Ia supernova 2016hnk. GALBANY L., ASHALL C., HOFLICH P., et al.
2019ApJ...885..136A 42           X         1 3 ~ Nuclear ignition of white dwarf stars by relativistic encounters with rotating intermediate mass black holes. ANNINOS P., HOFFMAN R.D., GREWAL M., et al.
2019ApJ...887..180S 100       D     X         3 20 ~ The progenitors of calcium-strong transients. SHEN K.J., QUATAERT E. and PAKMOR R.
2020ApJ...895L...3A 102       D       C       2 142 ~ Carnegie supernova Project-II: a new method to photometrically identify sub-types of extreme Type Ia supernovae. ASHALL C., LU J., BURNS C., et al.
2020ApJ...896..165J viz 9603 T   A     X C       224 21 ~ Ca hnk: the calcium-rich transient
Supernova 2016hnk from a helium shell detonation of a sub-Chandrasekhar white dwarf.
JACOBSON-GALAN W.V., POLIN A., FOLEY R.J., et al.
2020ApJ...898..166J viz 342           X C       7 32 44 SN 2019ehk: a double-peaked Ca-rich transient with luminous X-ray emission and shock-ionized spectral features. JACOBSON-GALAN W.V., MARGUTTI R., KILPATRICK C.D., et al.
2020ApJ...900L..27S 256           X         6 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.
2020ApJ...905...58D viz 1762       D     X C       41 68 64 The Zwicky Transient Facility Census of the Local Universe. I. Systematic search for calcium-rich gap transients reveals three related spectroscopic subclasses. DE K., KASLIWAL M.M., TZANIDAKIS A., et al.
2021ApJ...908L..32J 218           X C       4 14 13 Late-time observations of calcium-rich transient SN 2019ehk reveal a pure radioactive decay power source. JACOBSON-GALAN W.V., MARGUTTI R., KILPATRICK C.D., et al.
2021ApJ...922..186H viz 219           X C       4 12 13 Measuring an off-center detonation through infrared line profiles: the peculiar Type Ia supernova SN 2020qxp/ASASSN-20jq. HOEFLICH P., ASHALL C., BOSE S., et al.
2021ApJ...923..267D viz 17       D               3 379 11 The Foundation Supernova Survey: photospheric velocity correlations in Type Ia supernovae. DETTMAN K.G., JHA S.W., DAI M., et al.
2022ApJ...927..199D 421       D     X         10 38 5 Physical Properties of the Host Galaxies of Ca-rich Transients. DONG Y., MILISAVLJEVIC D., LEJA J., et al.
2022ApJS..259...53C viz 18       D               1 291 15 The First Data Release of CNIa0.02-A Complete Nearby (Redshift <0.02) Sample of Type Ia Supernova Light Curves. CHEN P., DONG S., KOCHANEK C.S., et al.
2022ApJ...925L..12K 48           X         1 6 19 Discovery of a Double-detonation Thermonuclear Supernova Progenitor. KUPFER T., BAUER E.B., VAN ROESTEL J., et al.
2022ApJ...932...58J 224           X C       4 29 14 The Circumstellar Environments of Double-peaked, Calcium-strong Transients 2021gno and 2021inl. JACOBSON-GALAN W.V., VENKATRAMAN P., MARGUTTI R., et al.
2022ApJ...934..102D 672           X C       14 12 5 SN 2016dsg: A Thermonuclear Explosion Involving a Thick Helium Shell. DONG Y., VALENTI S., POLIN A., et al.
2023ApJ...944...22Z 187           X C       3 15 6 The Origins of Calcium-rich Supernovae From Disruptions of CO White Dwarfs by Hybrid He-CO White Dwarfs. ZENATI Y., PERETS H.B., DESSART L., et al.
2023ApJ...946...83L 746           X C       15 23 4 SN 2020jgb: A Peculiar Type Ia Supernova Triggered by a Helium-shell Detonation in a Star-forming Galaxy. LIU C., MILLER A.A., POLIN A., et al.
2023MNRAS.522.6264S 1745       D S   X C F     35 19 ~ The γ-ray deposition histories of calcium-rich supernovae. SHARON A. and KUSHNIR D.
2023ApJ...950...17L 513           X C       10 13 ~ SN 2016ije: An SN 2002es-like Type Ia Supernova Exploded in a Metal-poor and Low-surface Brightness Galaxy. LI Z., ZHANG T., WANG X., et al.
2023ApJ...953...25P 700           X C       14 19 ~ Peculiar Spectral Evolution of the Type I Supernova 2019eix: A Possible Double Detonation from a Helium Shell on a Sub-Chandrasekhar-mass White Dwarf. PADILLA GONZALEZ E., HOWELL D.A., BURKE J., et al.
2023MNRAS.526..279E 93             C       1 22 ~ SN 2021gno: a calcium-rich transient with double-peaked light curves. ERTINI K., FOLATELLI G., MARTINEZ L., et al.
2023ApJ...958..173S 47           X         1 19 ~ An Asymmetric Double-degenerate Type Ia Supernova Explosion with a Surviving Companion Star. SIEBERT M.R., FOLEY R.J., ZENATI Y., et al.
2023ApJ...958..178L 47           X         1 19 ~ SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation. LIU C., MILLER A.A., BOOS S.J., et al.
2024ApJ...961..187D 100           X         2 18 ~ JWST MIRI/Medium Resolution Spectrograph (MRS) Observations and Spectral Models of the Underluminous Type Ia Supernova 2022xkq. DERKACY J.M., ASHALL C., HOEFLICH P., et al.

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