The DOI matches its Crossref record; 55 of the 55 references it cites were found in a registry or an index.
THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE
Open accessAbstract
The Carnegie Supernova Project (CSP) was a five-year observational survey conducted at Las Campanas Observatory that obtained, among other things, high-quality light curves of ∼100 low-redshift Type Ia supernovae (SNe Ia). Presented here is the second data release of nearby SN Ia photometry consisting of 50 objects, with a subset of 45 having near-infrared follow-up observations. Thirty-three objects have optical pre-maximum coverage with a subset of 15 beginning at least five days before maximum light. In the near-infrared, 27 objects have coverage beginning before the epoch of B -band maximum, with a subset of 13 beginning at least five days before maximum. In addition, we present results of a photometric calibration program to measure the CSP optical ( uBgVri ) bandpasses with an accuracy of ∼1%. Finally, we report the discovery of a second SN Ia, SN 2006ot, similar in its characteristics to the peculiar SN 2006bt.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R. L., Hogan, C. J., Jha, S., Kirshner, R. P., et al. (1998) · The Astronomical Journal · doi:10.1086/300499 · Cited by 19,704
Self-citationMeasurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
Self-citationSchlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
UBVRI photometric standard stars in the magnitude range 11.5-16.0 around the celestial equator
Landolt, A. U. (1992) · The Astronomical Journal · doi:10.1086/116242 · Cited by 4,168
The Sloan Digital Sky Survey Photometric System
Fukugita, M., Ichikawa, T., Gunn, J. E., Doi, M., Shimasaku, K., & Schneider, D. P. (1996) · The Astronomical Journal · doi:10.1086/117915 · Cited by 3,033
Astier, P., Guy, J., Regnault, N., Pain, R., Aubourg, E., Balam, D., Basa, S., Carlberg, R. G., Fabbro, S., Fouchez, D., et al. (2006) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20054185 · Cited by 2,434
The absolute magnitudes of Type IA supernovae
Phillips, M. M. (1993) · The Astrophysical Journal · doi:10.1086/186970 · Cited by 2,111
Self-citationDunkley, J., Komatsu, E., Nolta, M. R., Spergel, D. N., Larson, D., Hinshaw, G., Page, L., Bennett, C. L., Gold, B., Jarosik, N., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/306 · Cited by 1,787
Riess, A. G., Strolger, L., Casertano, S., Ferguson, H. C., Mobasher, B., Gold, B., Challis, P. J., Filippenko, A. V., Jha, S., Li, W., et al. (2007) · The Astrophysical Journal · doi:10.1086/510378 · Cited by 1,758 · cited 1×
“The current data have revealed that the equation-of- state parameter of the dark energy, w = P/(ρc2), is consistent with a cosmological constant, w = −1 (Astier et al. 2006; Wood-Vasey et al. 2007; Riess et al. 2007; Freedman et al. 2009; Sullivan et al. 2011).”
BackgroundSelf-citationSmith, J. A., Tucker, D. L., Kent, S., Richmond, M. W., Fukugita, M., Ichikawa, T., Ichikawa, S.-I., Jorgensen, A. M., Uomoto, A., Gunn, J. E., et al. (2002) · The Astronomical Journal · doi:10.1086/339311 · Cited by 1,621
Cited by
Alam, S., Aubert, M., Avila, S., Balland, C., Bautista, J. E., Bershady, M. A., Bizyaev, D., Blanton, M. R., Bolton, A. S., Bovy, J., et al. (2021) · Physical Review D · doi:10.1103/physrevd.103.083533 · Cited by 1,337
The Pantheon+ Analysis: The Full Data Set and Light-curve Release
Scolnic, D., Brout, D., Carr, A., Riess, A. G., Davis, T. M., Dwomoh, A., Jones, D. O., Ali, N., Charvu, P., Chen, R., et al. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac8b7a · Cited by 939
Self-citationFreedman, W. L., Madore, B. F., Hatt, D., Hoyt, T. J., Jang, I. S., Beaton, R. L., Burns, C. R., Lee, M. G., Monson, A. J., Neeley, J. R., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab2f73 · Cited by 839
Self-citation
Metadata
- Authors
- Stritzinger, M. D., Phillips, M. M., Boldt, L. N., Burns, C., Campillay, A., Contreras, C., Gonzalez, S., Folatelli, G., Morrell, N., Krzeminski, W., Roth, M., Salgado, F., DePoy, D. L., Hamuy, M., Freedman, W. L., Madore, B. F., Marshall, J. L., Persson, S. E., Rheault, J.-P., Suntzeff, N. B., Villanueva, S., Li, W., & Filippenko, A. V.
- Venue
- The Astronomical Journal
- Publisher
- American Astronomical Society
- Published
- 2011-10-03
- Volume
- 142
- Issue
- 5
- Pages
- 156
- ISSN
- 0004-6256 (ISSN-L)
- 1538-3881
- OpenAlex
- W2082378517
- Cited by
- 286
- References
- 55
- FWCI
- 10.02
- Type
- journal article
- Language
- en
- Open access
- bronze
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE. https://app.cochat.ai/papers/10.1088/0004-6256/142/5/156
- The paper
- Stritzinger, M. D., Phillips, M. M., Boldt, L. N., Burns, C., Campillay, A., Contreras, C., Gonzalez, S., Folatelli, G., Morrell, N., Krzeminski, W., Roth, M., Salgado, F., DePoy, D. L., Hamuy, M., Freedman, W. L., Madore, B. F., Marshall, J. L., Persson, S. E., Rheault, J.-P., . . . Filippenko, A. V. (2011). THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE. The Astronomical Journal. https://doi.org/10.1088/0004-6256/142/5/156
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
