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| SN 2009D , the SIMBAD biblio (43 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST09:59:45 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2009CBET.1647....1L | 37 | T | O X | 2 | 0 | Supernovae 2009C and 2009D. | LI W., CENKO S.B. and FILIPPENKO A.V. | ||
| 2009CBET.1647....2C | 37 | T | O X | 2 | 0 | Supernovae 2009C and 2009D. | CHALLIS P. and CALKINS M. | ||
|
2012ApJ...745...74F |
15 | D | 1 | 55 | 61 | Unburned material in the ejecta of type Ia supernovae. | FOLATELLI G., PHILLIPS M.M., MORRELL N., et al. | ||
|
2012A&A...538A.120L |
15 | D | 1 | 5598 | 37 | A unified supernova catalogue. | LENNARZ D., ALTMANN D. and WIEBUSCH C. | ||
|
2012ApJS..200...12H |
15 | D | 1 | 188 | 159 | CfA4: light curves for 94 type Ia supernovae. | HICKEN M., CHALLIS P., KIRSHNER R.P., et al. | ||
|
2013ApJ...773...53F |
15 | D | 1 | 101 | 121 | Spectroscopy of type Ia supernovae by the Carnegie Supernova Project. | FOLATELLI G., MORRELL N., PHILLIPS M.M., et al. | ||
|
2014ApJ...795...44R |
15 | D | 1 | 346 | 306 | Cosmological constraints from measurements of type Ia supernovae discovered during the first 1.5 yr of the Pan-STARRS1 survey. | REST A., SCOLNIC D., FOLEY R.J., et al. | ||
| 2015Sci...347.1459K | 87 | 31 | Distances with <4% precision from type Ia supernovae in young star-forming environments. | KELLY P.L., FILIPPENKO A.V., BURKE D.L., et al. | |||||
|
2015ApJS..220....9F |
16 | D | 5 | 315 | 64 | CfAIR2: near-infrared light curves of 94 Type Ia supernovae. | FRIEDMAN A.S., WOOD-VASEY W.M., MARION G.H., et al. | ||
|
2015ApJS..220...20Z |
16 | D | 1 | 209 | 14 | The silicon and calcium high-velocity features in Type Ia supernovae from early to maximum phases. | ZHAO X., WANG X., MAEDA K., et al. | ||
|
2015ApJ...812...31J |
16 | D | 1 | 337 | 27 | Reconsidering the effects of local star formation on type Ia supernova cosmology. | JONES D.O., RIESS A.G. and SCOLNIC D.M. | ||
|
2017AJ....154..211K |
16 | D | 3 | 348 | 140 | The Carnegie Supernova Project. I. Third photometry data release of low-redshift Type Ia supernovae and other white dwarf explosions. | KRISCIUNAS K., CONTRERAS C., BURNS C.R., et al. | ||
|
2018ApJ...859..101S |
17 | D | 1 | 1047 | 1682 | The complete light-curve sample of spectroscopically confirmed SNe Ia from Pan-STARRS1 and cosmological constraints from the combined Pantheon Sample. | SCOLNIC D.M., JONES D.O., REST A., et al. | ||
|
2018ApJ...869...56B |
16 | D | 1 | 176 | 128 | The Carnegie Supernova Project: absolute calibration and the Hubble constant. | BURNS C.R., PARENT E., PHILLIPS M.M., et al. | ||
| 2018PASP..130k4504P | 16 | D | 1 | 116 | 10 | Extending supernova spectral templates for next-generation Space Telescope observations. | PIEREL J.D.R., RODNEY S., AVELINO A., et al. | ||
|
2019ApJ...874..150B |
16 | D | 2 | 329 | 108 | First cosmology results using SNe Ia from the dark Energy Survey: analysis, systematic uncertainties, and validation. | BROUT D., SCOLNIC D., KESSLER R., et al. | ||
|
2019MNRAS.485.2343P |
16 | D | 1 | 263 | 3 | Characterizing the secondary maximum in the r-band for Type Ia supernovae: diagnostic for the ejecta mass. | PAPADOGIANNAKIS S., DHAWAN S., MOROSIN R., et al. | ||
| 2019ApJ...887..106A | 16 | D | 6 | 179 | 31 | Type Ia supernovae are excellent standard candles in the near-infrared. | AVELINO A., FRIEDMAN A.S., MANDEL K.S., et al. | ||
| 2019MNRAS.490.3882S | 179 | D | X F | 4 | 182 | 57 | Lick Observatory Supernova Search follow-up program: photometry data release of 93 Type Ia supernovae. | STAHL B.E., ZHENG W., DE JAEGER T., et al. | |
|
2020MNRAS.492.4325S |
16 | D | 4 | 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. | ||
| 2020ApJ...895L...3A | 16 | D | 1 | 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...896L...4R |
16 | D | 1 | 259 | ~ | Evidence for cosmic acceleration is robust to observed correlations between Type Ia supernova luminosity and stellar age. | ROSE B.M., RUBIN D., CIKOTA A., et al. | ||
|
2020MNRAS.498.2703B |
16 | D | 1 | 474 | 54 | Cosmic flows in the nearby Universe: new peculiar velocities from SNe and cosmological constraints. | BORUAH S.S., HUDSON M.J. and LAVAUX G. | ||
| 2020ApJ...901..143U | 16 | D | 3 | 249 | 43 | The Carnegie Supernova Project-I: correlation between Type Ia supernovae and their host galaxies from optical to near-infrared bands. | UDDIN S.A., BURNS C.R., PHILLIPS M.M., et al. | ||
| 2020ApJ...901..154B | 16 | D | 1 | 130 | ~ | Carnegie Supernova Project: classification of Type Ia supernovae. | BURROW A., BARON E., ASHALL C., et al. | ||
|
2020ApJ...902...14S |
16 | D | 1 | 1047 | 22 | Effects of supernova redshift uncertainties on the determination of cosmological parameters. | STEINHARDT C.L., SNEPPEN A. and SEN B. | ||
|
2020MNRAS.499.1424H |
16 | 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. | ||
| 2020MNRAS.499.5121P | 16 | D | 1 | 631 | 16 | The dependence of Type Ia Supernovae SALT2 light-curve parameters on host galaxy morphology. | PRUZHINSKAYA M.V., NOVINSKAYA A.K., PAUNA N., et al. | ||
|
2021ApJ...923..197P |
17 | D | 1 | 441 | ~ | Are Type Ia supernovae in rest-frame H brighter in more massive galaxies? | PONDER K.A., WOOD-VASEY W.M., WEYANT A., et al. | ||
|
2021ApJ...923..267D |
17 | D | 2 | 379 | 11 | The Foundation Supernova Survey: photospheric velocity correlations in Type Ia supernovae. | DETTMAN K.G., JHA S.W., DAI M., et al. | ||
|
2022MNRAS.509.5275S |
17 | D | 2 | 544 | 8 | The ZTF-BTS Type Ia supernovae luminosity function is consistent with a single progenitor channel for the explosions. | SHARON A. and KUSHNIR D. | ||
| 2022MNRAS.510.3939M | 17 | D | 1 | 91 | 33 | A hierarchical Bayesian SED model for Type Ia supernovae in the optical to near-infrared. | MANDEL K.S., THORP S., NARAYAN G., et al. | ||
| 2022MNRAS.510.4779S | 17 | D | 2 | 445 | ~ | Type Ia supernova magnitude step from the local dark matter environment. | STEIGERWALD H., RODRIGUES D., PROFUMO S., et al. | ||
| 2022MNRAS.510.4929P | 102 | D | F | 2 | 56 | 3 | Carnegie Supernova Project: kinky i-band light curves of Type Ia supernovae. | PESSI P.J., HSIAO E.Y., FOLATELLI G., et al. | |
|
2022ApJ...930...70H |
17 | D | 1 | 363 | 10 | Spectroscopic Studies of Type Ia Supernovae Using LSTM Neural Networks. | HU L., CHEN X. and WANG L. | ||
|
2022ApJ...938..110B |
17 | D | 3 | 1534 | 204 | The Pantheon+ Analysis: Cosmological Constraints. | BROUT D., SCOLNIC D., POPOVIC B., et al. | ||
|
2022PASA...39...46C |
17 | D | 1 | 2242 | 36 | The Pantheon+ analysis: Improving the redshifts and peculiar velocities of type Ia supernovae used in cosmological analyses. | CARR A., DAVIS T.M., SCOLNIC D., et al. | ||
|
2022A&A...668A..34H |
17 | D | 1 | 1045 | 24 | Inference of the cosmic rest-frame from supernovae Ia. | HORSTMANN N., PIETSCHKE Y. and SCHWARZ D.J. | ||
| 2023MNRAS.524..235D | 17 | D | 1 | 136 | ~ | A BayeSN distance ladder: H0 from a consistent modelling of Type Ia supernovae from the optical to the near-infrared. | DHAWAN S., THORP S., MANDEL K.S., et al. | ||
|
2024A&A...687A.108G |
18 | D | 1 | 1820 | ~ | Narrow absorption lines from intervening material in supernovae I. Measurements and temporal evolution. | GONZALEZ-GAITAN S., GUTIERREZ C.P., ANDERSON J.P., et al. | ||
| 2025MNRAS.536.1752L | 19 | D | 1 | 8 | ~ | Cosmological foundations revisited with Pantheon+. | LANE Z.G., SEIFERT A., RIDDEN-HARPER R., et al. | ||
| 2025ApJ...985..122I | 19 | D | 1 | 141 | ~ | North+Lone Star Supernova Host Survey. I. Local Host-galaxy Hα Surface Brightness and the Hubble Residuals of Type Ia Supernovae. | ISAACS A.M., KELLY P.L. and WHEELER J.C. | ||
| 2025MNRAS.540.3247S | 19 | D | 1 | 48 | ~ | All known Type Ia supernovae models fail to reproduce the observed bolometric luminosity-width correlation. | SHARON A., KUSHNIR D. and WYGODA N. |