Hubble Residuals of Nearby SN Ia Are Correlated with Host Galaxy Masses

By Patrick L. Kelly, Menlo Park Kipac, M. Hicken, Harvard-Smithsonian Ctr. Astrophys., D. Burke, Kaisey S. Mandel, R. Kirshner. 2009

204 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/ee8218ec6e55569281c0cdc1c1e979a0f4ef6943

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TYPE Ia SUPERNOVA LIGHT CURVE INFERENCE: HIERARCHICAL MODELS IN THE OPTICAL AND NEAR-INFRARED (2010, background): “Observables that are not derived from light curve data, such as host galaxy masses (e.g., Kelly et al. 2010; Sullivan et al. 2010) or spectroscopic measurements (e.g., Bailey et al. 2009; Blondin et al. 2011; Foley & Kasen 2011), can be correlated with the intrinsic absolute light curves.”
A 2.4% DETERMINATION OF THE LOCAL VALUE OF THE HUBBLE CONSTANT (2016, methodology): “As in R11, we make use of several studies (Hicken et al. 2009b; Kelly et al. 2010; Lampeitl et al. 2010; Sullivan et al. 2010) which have shown the existence of a small step brighter for the corrected SN magnitude for hosts more massive than ~Mlog 10stellar .”
CONFIRMATION OF A STAR FORMATION BIAS IN TYPE Ia SUPERNOVA DISTANCES AND ITS EFFECT ON THE MEASUREMENT OF THE HUBBLE CONSTANT (2014, methodology): “…global or nuclear host-galaxy properties have been fruitful in revealing environmental dependencies that remain even after SNe Ia are standardized using their lightcurve widths and colors (e.g., Kelly et al. 2010; Sullivan et al. 2010; Lampeitl et al. 2010; Gupta et al. 2011; D’Andrea et al. 2011).”
The VISTA deep extragalactic observations (VIDEO) survey (2012, background): “…a key role in the cosmological analyses (Sullivan et al. 2011), will improve substantially when the optical DES data are used in conjunction with the deep VIDEO near-IR data, and aid in the determination of host galaxy stellar masses (Kelly et al. 2010; Lampeitl et al. 2010; Sullivan et al. 2010).”
COSMOLOGICAL CONSTRAINTS FROM MEASUREMENTS OF TYPE Ia SUPERNOVAE DISCOVERED DURING THE FIRST 1.5 yr OF THE Pan-STARRS1 SURVEY (2013, background): “…et al. 2009; Foley & Kasen 2011; Foley et al. 2011), other spectral features (Foley et al. 2008; Bailey et al. 2009; Blondin et al. 2011; Silverman et al. 2012b; Foley & Kirshner 2013), and host galaxy properties (Kelly et al. 2010; Lampeitl et al. 2010; Sullivan et al. 2010; Hayden et al. 2012).”
The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample (2017, background): “These tests include probing relations between luminosity and properties of the host galaxies of the SNe (e.g., Kelly et al. 2010; Lampeitl et al. 2010; Sullivan et al. 2010) and analyses of the light-curve fit parameters of SNe and how these parameters relate to luminosity (e.g., Mandel et al.…”
Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples (2014, methodology): “Kelly et al. (2010), Lampeitl et al. (2010b) and Sullivan et al. (2010) have found, in independent samples, a correlation between the shape and color corrected luminosities of type Ia supernovae and the stellar mass of their host galaxies (respectively for low-z, SDSS-II, and SNLS SNe).”
THE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III (2012, background): “The new classification will also enable a large statistical study of the correlated properties between SNe Ia and their host galaxies (e.g., Kelly et al. 2010; Sullivan et al. 2010; Lampeitl et al. 2010; Brandt et al. 2010).”
THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. V. IMPROVING THE DARK-ENERGY CONSTRAINTS ABOVE z > 1 AND BUILDING AN EARLY-TYPE-HOSTED SUPERNOVA SAMPLE (2011, background): “Host Mass Correction to SN Ia Luminosities There is evidence that SN Ia luminosity correlates with the mass of the host galaxy, even after the corrections for color and light curve width have been applied (Kelly et al. 2010; Sullivan et al. 2010; Lampeitl et al. 2010).”
CfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE (2012, unknown): “The CfA3 sample was also instrumental in providing the data for Kelly et al. (2010), who first detected the small but real relation between SN Ia host-galaxy masses and the residuals from the distance predictions based on SN Ia light curves.”
Evidence of Environmental Dependencies of Type Ia Supernovae from the Nearby Supernova Factory indicated by Local H$\alpha$ (2013, methodology): “We compare this model to mass steps measured using literature SNe from SNLS, SDSS and non-SNfactory lowz datasets (Sullivan et al. 2010; Gupta et al. 2011; Kelly et al. 2010, respectively) from the combined dataset of Childress et al. (2013a).”
Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters (2017, background): “Host Galaxy Masses It has been shown that after shape and color correction, SNe Ia are ∼ 0.05-0.1 mag brighter in high mass host galaxies (log(M∗/M ) > 10) than in lower-mass host galaxies at the same redshifts (∆M ; Kelly et al. 2010; Lampeitl et al. 2010; Sullivan et al. 2010).”