The DOI matches its Crossref record; 9 of the 9 references it cites were found in a registry or an index.
THE CLUSTER LENSING AND SUPERNOVA SURVEY WITH HUBBLE: AN OVERVIEW
Open accessAbstract
The Cluster Lensing And Supernova survey with Hubble (CLASH) is a 524-orbit Multi-Cycle Treasury Program to use the gravitational lensing properties of 25 galaxy clusters to accurately constrain their mass distributions. The survey, described in detail in this paper, will definitively establish the degree of concentration of dark matter in the cluster cores, a key prediction of structure formation models. The CLASH cluster sample is larger and less biased than current samples of space-based imaging studies of clusters to similar depth, as we have minimized lensing-based selection that favors systems with overly dense cores. Specifically, 20 CLASH clusters are solely X-ray selected. The X-ray-selected clusters are massive ( kT > 5 keV) and, in most cases, dynamically relaxed. Five additional clusters are included for their lensing strength (θ Ein > 35'' at z s = 2) to optimize the likelihood of finding highly magnified high- z ( z > 7) galaxies. A total of 16 broadband filters, spanning the near-UV to near-IR, are employed for each 20-orbit campaign on each cluster. These data are used to measure precise (σ z ∼ 0.02(1 + z )) photometric redshifts for newly discovered arcs. Observations of each cluster are spread over eight epochs to enable a search for Type Ia supernovae at z > 1 to improve constraints on the time dependence of the dark energy equation of state and the evolution of supernovae. We present newly re-derived X-ray luminosities, temperatures, and Fe abundances for the CLASH clusters as well as a representative source list for MACS1149.6+2223 ( z = 0.544).
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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
Schlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
The Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 1×
“Functional forms that fit such a profile well include the “NFW” profile (Navarro et al. 1996, 1997) and the Einasto / Sérsic profile (Sérsic 1963; Einasto 1965; Navarro et al. 2004, 2010).”
BackgroundRiess, A. G., Strolger, L., Tonry, J., Casertano, S., Ferguson, H. C., Mobasher, B., Challis, P., Filippenko, A. V., Jha, S., Li, W., et al. (2004) · The Astrophysical Journal · doi:10.1086/383612 · Cited by 4,315 · cited 1×
“From the 23 SNe Ia at z > 1 with HST data (Riess et al. 2004, 2007) we have learned: 1) that cosmic expansion was once decelerating before it recently began accelerating, 2) that dark energy, i.e., an energy density with w < 0, was already present during this prior decelerating phase, 3) that SNe…”
MethodSelf-citationRiess, 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×
“From the 23 SNe Ia at z > 1 with HST data (Riess et al. 2004, 2007) we have learned: 1) that cosmic expansion was once decelerating before it recently began accelerating, 2) that dark energy, i.e., an energy density with w < 0, was already present during this prior decelerating phase, 3) that SNe…”
MethodSelf-citationThe statistics of CDM halo concentrations
Neto, A. F., Gao, L., Bett, P., Cole, S., Navarro, J. F., Frenk, C. S., White, S. D. M., Springel, V., & Jenkins, A. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.12381.x · Cited by 764
Duffy, A. R., Schaye, J., Kay, S. T., Vecchia, C. D., Battye, R. A., & Booth, C. M. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16613.x · Cited by 186
Cited by
Bouwens, R. J., Illingworth, G. D., Oesch, P. A., Labbé, I., van Dokkum, P. G., Trenti, M., Franx, M., Smit, R., Gonzalez, V., & Magee, D. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/793/2/115 · Cited by 406
Self-citationDust in the Reionization Era: ALMA Observations of a z = 8.38 Gravitationally Lensed Galaxy
Laporte, N., Ellis, R. S., Boone, F., Bauer, F. E., Quénard, D., Roberts-Borsani, G. W., Pelló, R., Pérez-Fournon, I., & Streblyanska, A. (2017) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aa62aa · Cited by 319
A magnified young galaxy from about 500 million years after the Big Bang
Zheng, W., Postman, M., Zitrin, A., Moustakas, J., Shu, X., Jouvel, S., Høst, O., Molino, A., Bradley, L., Coe, D., et al. (2012) · Nature · doi:10.1038/nature11446 · Cited by 313
Self-citationvon der Linden, A., Allen, M. T., Applegate, D. E., Kelly, P. L., Allen, S. W., Ebeling, H., Burchat, P. R., Burke, D. L., Donovan, D., Morris, R. G., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1945 · Cited by 259
THE MUSIC OF CLASH: PREDICTIONS ON THE CONCENTRATION-MASS RELATION
Meneghetti, M., Rasia, E., Vega, J., Merten, J., Postman, M., Yepes, G., Sembolini, F., Donahue, M., Ettori, S., Umetsu, K., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/797/1/34 · Cited by 144
Self-citation
Metadata
- Authors
- Postman, M., Coe, D., Benítez, N., Bradley, L., Broadhurst, T., Donahue, M., Ford, H., Graur, O., Graves, G., Jouvel, S., Koekemoer, A., Lemze, D., Medezinski, E., Molino, A., Moustakas, L., Ogaz, S., Riess, A., Rodney, S., Rosati, P., Umetsu, K., Zheng, W., Zitrin, A., Bartelmann, M., Bouwens, R., Czakon, N., Golwala, S., Host, O., Infante, L., Jha, S., Jimenez-Teja, Y., Kelson, D., Lahav, O., Lazkoz, R., Maoz, D., McCully, C., Melchior, P., Meneghetti, M., Merten, J., Moustakas, J., Nonino, M., Patel, B., Regös, E., Sayers, J., Seitz, S., & Van der Wel, A.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 2012-03-14
- Volume
- 199
- Issue
- 2
- Pages
- 25
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W1501370474
- Cited by
- 849
- References
- 9
- FWCI
- 40.40
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Postman, M., Coe, D., Benítez, N., Bradley, L., Broadhurst, T., Donahue, M., Ford, H., Graur, O., Graves, G., Jouvel, S., Koekemoer, A., Lemze, D., Medezinski, E., Molino, A., Moustakas, L., Ogaz, S., Riess, A., Rodney, S., Rosati, P., . . . Van der Wel, A. (2012). THE CLUSTER LENSING AND SUPERNOVA SURVEY WITH HUBBLE: AN OVERVIEW. The Astrophysical Journal Supplement Series. https://doi.org/10.1088/0067-0049/199/2/25
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