RESULTS OF THE LICK OBSERVATORY SUPERNOVA SEARCH FOLLOW-UP PHOTOMETRY PROGRAM: BVRI LIGHT CURVES OF 165 TYPE Ia SUPERNOVAE

By M. Ganeshalingam, Weidong Li, A. Filippenko, C. Anderson, G. Foster, E. Gates, C. Griffith, B. Grigsby, N. Joubert, J. Leja and 5 more. 2010

198 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/32c0c1b38e1d5e86c92bfb39c308690f17abb0a5

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In Astronomy and Astrophysics

1. A. Filippenko
2. A. Riess
3. N. Smith
4. Ryan Chornock
5. S. Jha
6. Weidong Li
7. R. Kirshner
8. E. Berger

In Nuclear and High Energy Physics

1. N. Smith
2. A. Filippenko
3. Ryan Chornock
4. A. Gal-yam
5. Weidong Li
6. R. Kirshner
7. S. Jha
8. D. Kasen

Citations in the corpus

• Berkeley Supernova Ia Program – I. Observations, data reduction and spectroscopic sample of 582 low-redshift Type Ia supernovae (2012, methodology): “This likely comes from the fact that for most of the project’s lifetime, BSNIP has had a strong focus on spectroscopically monitoring SNe Ia that were being concurrently observed photometrically as part of the sample presented by Ganeshalingam et al. (2010).”
• The Pantheon+ Analysis: The Full Data Set and Light-curve Release (2021, background): “The largest increase in the number of SNe for the Pantheon+ sample is at low redshift owing to the addition of the Foundation, LOSS1, LOSS2, SOUSA, and CNIa0.”
• TYPE Iax SUPERNOVAE: A NEW CLASS OF STELLAR EXPLOSION (2012, methodology): “As a part of the LOSS photometric follow-up effort, filtered photometry of SN 2008A was obtained and presented by Ganeshalingam et al. (2010).”
• TYPE Ia SUPERNOVAE STRONGLY INTERACTING WITH THEIR CIRCUMSTELLAR MEDIUM (2013, background): “The gray shaded region is the range of SNe Ia that follow the Phillips relation, about −19.7 to −18.5 mag (e.g., Ganeshalingam et al. 2010).”
• THE SPECTROSCOPIC DIVERSITY OF TYPE Ia SUPERNOVAE (2000, methodology): “…SN Ia light curves have already been published (Hamuy et al. 1996; Riess et al. 1999; Jha et al. 2006; Hicken et al. 2009; Contreras et al. 2010; Ganeshalingam et al. 2010; Stritzinger et al. 2011), but until the recent publication of 432 spectra of 32 SN Ia by Matheson et al. (2008), there had…”
• A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THE HUBBLE SPACE TELESCOPE AND WIDE FIELD CAMERA 3 (2011, background): “Ganeshalingam et al. (2010) recently published light curves of a large sample of SNe Ia from the Lick Observatory Supernova Search, but there is a large overlap with those given by Hicken et al. (2009b).”
• The Pantheon+ Analysis: Cosmological Constraints (2022, background): “…Digital Sky Survey (SDSS; Sako et al. 2011), Hubble Space Telescope (HST; Gilliland et al. 1999; Riess et al. 2001, 2004, 2007; Suzuki et al. 2012; Riess et al. 2018), and Low-z (grouped together as LOSS_11; Ganeshalingam et al. 2010; LOSS_21; Stahl et al. 2019; SOUSA135; Brown et al. 2014; CNIa0.”
• Luminous blue variable eruptions and related transients: diversity of progenitors and outburst properties (2010, methodology): “These template images and calibrations are then used in the KAIT photometry pipeline (Ganeshalingam et al. 2010) to perform image subtraction on the image data and calibration to the standard photometry system.”
• THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE (2010, background): “The light curves presented here are a significant addi- tion to a growing sample of low-z SNe Ia that have been observed in well-understood and stable photometric systems (Wood-Vasey et al. 2008; Hicken et al. 2009; Contreras et al. 2010; Ganeshalingam et al. 2010).”
• Nearby Supernova Rates from the Lick Observatory Supernova Search. II. The Observed Luminosity Functions and Fractions of Supernovae in a Complete Sample (2010, methodology): “In the left panel of Figure 1, we plot the R-band light curves of a sample of 83 well-observed SNe Ia in the LOSS photometry database (solid lines; Ganeshalingam et al. 2010).”
• Nearby supernova rates from the Lick Observatory Supernova Search – I. The methods and data base (2010, methodology): “The data are automatically processed through an imagesubtraction pipeline (Ganeshalingam et al. 2010; Filippenko et al. 2011), and candidate SNe are flagged.”
• Sub-Chandrasekhar-mass White Dwarf Detonations Revisited (2017, background): “Also overlaid for comparison in gray are three well-observed SNe Ia: the subluminous 1991bg-like SN 1999by (Garnavich et al. 2004; Stritzinger 2005; Ganeshalingam et al. 2010), the normal SN 2011fe (Munari et al. 2013; Pereira et al. 2013; Tsvetkov et al. 2013), and the over-luminous 1991T-like SN…”
• CfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE (2012, methodology): “More recently, the Sloan Digital Sky Survey (SDSS) published 19 SNe Ia with z < 0.100 (Holtzman et al. 2008) as part of the SDSS-II program, and the Lick Observatory Supernova Search (LOSS) published optical photometry of 165 SNe Ia (Ganeshalingam et al. 2010).”