--- _id: '11583' abstract: - lang: eng text: 'Candidate galaxies at redshifts of z ∼ 10 are now being found in extremely deep surveys, probing very small areas. As a consequence, candidates are very faint, making spectroscopic confirmation practically impossible. In order to overcome such limitations, we have undertaken the CF-HiZELS survey, which is a large-area, medium-depth near-infrared narrow-band survey targeted at z = 8.8 Lyman α (Lyα) emitters (LAEs) and covering 10 deg2 in part of the SSA22 field with the Canada–France–Hawaii Telescope (CFHT). We surveyed a comoving volume of 4.7 × 106 Mpc3 to a Lyα luminosity limit of 6.3 × 1043舁erg舁s−1. We look for Lyα candidates by applying the following criteria: (i) clear emission-line source, (ii) no optical detections (ugriz from CFHTLS), (iii) no visible detection in the optical stack (ugriz > 27), (iv) visually checked reliable NBJ and J detections and (v) J − K ≤ 0. We compute photometric redshifts and remove a significant amount of dusty lower redshift line-emitters at z ∼ 1.4 or 2.2. A total of 13 Lyα candidates were found, of which two are marked as strong candidates, but the majority have very weak constraints on their spectral energy distributions. Using follow-up observations with SINFONI/VLT, we are able to exclude the most robust candidates as LAEs. We put a strong constraint on the Lyα luminosity function at z ∼ 9 and make realistic predictions for ongoing and future surveys. Our results show that surveys for the highest redshift LAEs are susceptible of multiple contaminations and that spectroscopic follow-up is absolutely necessary.' acknowledgement: We thank the anonymous referee for the comments and suggestions which improved both the quality and clarity of this work. DS acknowledges financial support from the Netherlands Organisation for Scientific Research (NWO) through a Veni fellowship. IRS acknowledges support from STFC (ST/I001573/1), a Leverhulme Fellowship, the ERC Advanced Investigator programme DUSTYGAL 321334 and a Royal Society/Wolfson Merit Award. PNB acknowledges support from the Leverhulme Trust. JWK acknowledges the support from the Creative Research Initiative Program, no. 2008- 0060544, of the National Research Foundation of Korea (NRF) funded by the Korean government (MSIP). JPUF and BMJ acknowledge support from the ERC-StG grant EGGS-278202. The Dark Cosmology Centre is funded by the Danish National Research Foundation. This work is based in part on data obtained as part of the UKIRT Infrared Deep Sky Survey. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the Canada–France–Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France and the University of Hawaii. This work is based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. This work was only possible due to OPTICON/FP7 and the access that it granted to the CFHT telescope. The authors also wish to acknowledge the CFHTLS and UKIDSS surveys for their excellent legacy and complementary value – without such high-quality data sets, this research would not have been possible. article_processing_charge: No article_type: original author: - first_name: Jorryt J full_name: Matthee, Jorryt J id: 7439a258-f3c0-11ec-9501-9df22fe06720 last_name: Matthee orcid: 0000-0003-2871-127X - first_name: David full_name: Sobral, David last_name: Sobral - first_name: A. M. full_name: Swinbank, A. M. last_name: Swinbank - first_name: Ian full_name: Smail, Ian last_name: Smail - first_name: P. N. full_name: Best, P. N. last_name: Best - first_name: Jae-Woo full_name: Kim, Jae-Woo last_name: Kim - first_name: Marijn full_name: Franx, Marijn last_name: Franx - first_name: Bo full_name: Milvang-Jensen, Bo last_name: Milvang-Jensen - first_name: Johan full_name: Fynbo, Johan last_name: Fynbo citation: ama: 'Matthee JJ, Sobral D, Swinbank AM, et al. A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys. Monthly Notices of the Royal Astronomical Society. 2014;440(3):2375-2387. doi:10.1093/mnras/stu392' apa: 'Matthee, J. J., Sobral, D., Swinbank, A. M., Smail, I., Best, P. N., Kim, J.-W., … Fynbo, J. (2014). A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stu392' chicago: 'Matthee, Jorryt J, David Sobral, A. M. Swinbank, Ian Smail, P. N. Best, Jae-Woo Kim, Marijn Franx, Bo Milvang-Jensen, and Johan Fynbo. “A 10 Deg2 Lyman α Survey at Z=8.8 with Spectroscopic Follow-up: Strong Constraints on the Luminosity Function and Implications for Other Surveys.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2014. https://doi.org/10.1093/mnras/stu392.' ieee: 'J. J. Matthee et al., “A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys,” Monthly Notices of the Royal Astronomical Society, vol. 440, no. 3. Oxford University Press, pp. 2375–2387, 2014.' ista: 'Matthee JJ, Sobral D, Swinbank AM, Smail I, Best PN, Kim J-W, Franx M, Milvang-Jensen B, Fynbo J. 2014. A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys. Monthly Notices of the Royal Astronomical Society. 440(3), 2375–2387.' mla: 'Matthee, Jorryt J., et al. “A 10 Deg2 Lyman α Survey at Z=8.8 with Spectroscopic Follow-up: Strong Constraints on the Luminosity Function and Implications for Other Surveys.” Monthly Notices of the Royal Astronomical Society, vol. 440, no. 3, Oxford University Press, 2014, pp. 2375–87, doi:10.1093/mnras/stu392.' short: J.J. Matthee, D. Sobral, A.M. Swinbank, I. Smail, P.N. Best, J.-W. Kim, M. Franx, B. Milvang-Jensen, J. Fynbo, Monthly Notices of the Royal Astronomical Society 440 (2014) 2375–2387. date_created: 2022-07-14T12:33:24Z date_published: 2014-05-21T00:00:00Z date_updated: 2022-08-19T08:30:30Z day: '21' doi: 10.1093/mnras/stu392 extern: '1' external_id: arxiv: - '1402.6697' intvolume: ' 440' issue: '3' keyword: - Space and Planetary Science - Astronomy and Astrophysics - 'galaxies: evolution' - 'galaxies: high-redshift' - 'cosmology: observations' - dark ages - reionization - first stars language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/1402.6697 month: '05' oa: 1 oa_version: Preprint page: 2375-2387 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: eissn: - 1365-2966 issn: - 0035-8711 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: 'A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys' type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 440 year: '2014' ... --- _id: '11582' abstract: - lang: eng text: We have observed a sample of typical z ∼ 1 star-forming galaxies, selected from the HiZELS survey, with the new K-band Multi-Object Spectrograph (KMOS) near-infrared, multi-integral field unit instrument on the Very Large Telescope (VLT), in order to obtain their dynamics and metallicity gradients. The majority of our galaxies have a metallicity gradient consistent with being flat or negative (i.e. higher metallicity cores than outskirts). Intriguingly, we find a trend between metallicity gradient and specific star formation rate (sSFR), such that galaxies with a high sSFR tend to have relatively metal poor centres, a result which is strengthened when combined with data sets from the literature. This result appears to explain the discrepancies reported between different high-redshift studies and varying claims for evolution. From a galaxy evolution perspective, the trend we see would mean that a galaxy's sSFR is governed by the amount of metal-poor gas that can be funnelled into its core, triggered either by merging or through efficient accretion. In fact, merging may play a significant role as it is the starburst galaxies at all epochs, which have the more positive metallicity gradients. Our results may help to explain the origin of the fundamental metallicity relation, in which galaxies at a fixed mass are observed to have lower metallicities at higher star formation rates, especially if the metallicity is measured in an aperture encompassing only the central regions of the galaxy. Finally, we note that this study demonstrates the power of KMOS as an efficient instrument for large-scale resolved galaxy surveys. acknowledgement: First, we acknowledge the referee for their comments, which have improved the clarity of this paper. JPS and IRS acknowledge support from STFC (ST/I001573/1). IRS also acknowledges support from the ERC Advanced Investigator programme DUSTYGAL and a Royal Society/Wolfson Merit Award. DS acknowledges financial support from NWO through a Veni fellowship and from FCT through the award of an FCT-IF starting grant. PNB acknowledges STFC for financial support. article_processing_charge: No article_type: original author: - first_name: John P. full_name: Stott, John P. last_name: Stott - first_name: David full_name: Sobral, David last_name: Sobral - first_name: A. M. full_name: Swinbank, A. M. last_name: Swinbank - first_name: Ian full_name: Smail, Ian last_name: Smail - first_name: Richard full_name: Bower, Richard last_name: Bower - first_name: Philip N. full_name: Best, Philip N. last_name: Best - first_name: Ray M. full_name: Sharples, Ray M. last_name: Sharples - first_name: James E. full_name: Geach, James E. last_name: Geach - first_name: Jorryt J full_name: Matthee, Jorryt J id: 7439a258-f3c0-11ec-9501-9df22fe06720 last_name: Matthee orcid: 0000-0003-2871-127X citation: ama: Stott JP, Sobral D, Swinbank AM, et al. A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS. Monthly Notices of the Royal Astronomical Society. 2014;443(3):2695-2704. doi:10.1093/mnras/stu1343 apa: Stott, J. P., Sobral, D., Swinbank, A. M., Smail, I., Bower, R., Best, P. N., … Matthee, J. J. (2014). A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stu1343 chicago: Stott, John P., David Sobral, A. M. Swinbank, Ian Smail, Richard Bower, Philip N. Best, Ray M. Sharples, James E. Geach, and Jorryt J Matthee. “A Relationship between Specific Star Formation Rate and Metallicity Gradient within z ∼ 1 Galaxies from KMOS-HiZELS.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2014. https://doi.org/10.1093/mnras/stu1343. ieee: J. P. Stott et al., “A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS,” Monthly Notices of the Royal Astronomical Society, vol. 443, no. 3. Oxford University Press, pp. 2695–2704, 2014. ista: Stott JP, Sobral D, Swinbank AM, Smail I, Bower R, Best PN, Sharples RM, Geach JE, Matthee JJ. 2014. A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS. Monthly Notices of the Royal Astronomical Society. 443(3), 2695–2704. mla: Stott, John P., et al. “A Relationship between Specific Star Formation Rate and Metallicity Gradient within z ∼ 1 Galaxies from KMOS-HiZELS.” Monthly Notices of the Royal Astronomical Society, vol. 443, no. 3, Oxford University Press, 2014, pp. 2695–704, doi:10.1093/mnras/stu1343. short: J.P. Stott, D. Sobral, A.M. Swinbank, I. Smail, R. Bower, P.N. Best, R.M. Sharples, J.E. Geach, J.J. Matthee, Monthly Notices of the Royal Astronomical Society 443 (2014) 2695–2704. date_created: 2022-07-14T12:16:10Z date_published: 2014-09-21T00:00:00Z date_updated: 2022-08-19T08:27:25Z day: '21' doi: 10.1093/mnras/stu1343 extern: '1' external_id: arxiv: - '1407.1047' intvolume: ' 443' issue: '3' keyword: - Space and Planetary Science - Astronomy and Astrophysics - 'galaxies: abundances' - 'galaxies: evolution' - 'galaxies: kinematics and dynamics' language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/1407.1047 month: '09' oa: 1 oa_version: Preprint page: 2695-2704 publication: Monthly Notices of the Royal Astronomical Society publication_identifier: eissn: - 1365-2966 issn: - 0035-8711 publication_status: published publisher: Oxford University Press quality_controlled: '1' scopus_import: '1' status: public title: A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 443 year: '2014' ... --- _id: '11750' abstract: - lang: eng text: We report on the magnetic properties of a hot-pressed FeSb 2 sample. We find a significant increase in the magnetic susceptibility in our sample when compared with the values previously reported for the polycrystalline sample. The pronounced Curie tail at low temperature corresponds to 0.2% of Fe 2+ impurities per mole. In the intrinsic conductivity region, the susceptibility due to free carriers shows thermally activated behavior and is consistent with the data reported for single crystal FeSb 2 . Based on our data and analysis, while the enhanced magnetic susceptibility in our sample comes mainly from a small amount of unreacted Fe, the contribution from the enhanced carrier density due to lattice and strain defects arising from the ball milling process is also significant. Existence of an unreacted Fe phase is evidenced by small coercivity values of ~100 observed at 50 and 300 K. article_number: '6675864' article_processing_charge: No article_type: original author: - first_name: Mani full_name: Pokharel, Mani last_name: Pokharel - first_name: Huaizhou full_name: Zhao, Huaizhou last_name: Zhao - first_name: Kimberly A full_name: Modic, Kimberly A id: 13C26AC0-EB69-11E9-87C6-5F3BE6697425 last_name: Modic orcid: 0000-0001-9760-3147 - first_name: Zhifeng full_name: Ren, Zhifeng last_name: Ren - first_name: Cyril full_name: Opeil, Cyril last_name: Opeil citation: ama: Pokharel M, Zhao H, Modic KA, Ren Z, Opeil C. Magnetic properties of hot-pressed FeSb2. IEEE Transactions on Magnetics. 2014;50(5). doi:10.1109/TMAG.2013.2292607 apa: Pokharel, M., Zhao, H., Modic, K. A., Ren, Z., & Opeil, C. (2014). Magnetic properties of hot-pressed FeSb2. IEEE Transactions on Magnetics. Institute of Electrical and Electronics Engineers. https://doi.org/10.1109/TMAG.2013.2292607 chicago: Pokharel, Mani, Huaizhou Zhao, Kimberly A Modic, Zhifeng Ren, and Cyril Opeil. “Magnetic Properties of Hot-Pressed FeSb2.” IEEE Transactions on Magnetics. Institute of Electrical and Electronics Engineers, 2014. https://doi.org/10.1109/TMAG.2013.2292607. ieee: M. Pokharel, H. Zhao, K. A. Modic, Z. Ren, and C. Opeil, “Magnetic properties of hot-pressed FeSb2,” IEEE Transactions on Magnetics, vol. 50, no. 5. Institute of Electrical and Electronics Engineers, 2014. ista: Pokharel M, Zhao H, Modic KA, Ren Z, Opeil C. 2014. Magnetic properties of hot-pressed FeSb2. IEEE Transactions on Magnetics. 50(5), 6675864. mla: Pokharel, Mani, et al. “Magnetic Properties of Hot-Pressed FeSb2.” IEEE Transactions on Magnetics, vol. 50, no. 5, 6675864, Institute of Electrical and Electronics Engineers, 2014, doi:10.1109/TMAG.2013.2292607. short: M. Pokharel, H. Zhao, K.A. Modic, Z. Ren, C. Opeil, IEEE Transactions on Magnetics 50 (2014). date_created: 2022-08-08T08:26:02Z date_published: 2014-05-01T00:00:00Z date_updated: 2022-08-11T09:51:22Z day: '01' doi: 10.1109/TMAG.2013.2292607 extern: '1' intvolume: ' 50' issue: '5' language: - iso: eng month: '05' oa_version: None publication: IEEE Transactions on Magnetics publication_identifier: eissn: - 1941-0069 issn: - 0018-9464 publication_status: published publisher: Institute of Electrical and Electronics Engineers quality_controlled: '1' scopus_import: '1' status: public title: Magnetic properties of hot-pressed FeSb2 type: journal_article user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 50 year: '2014' ... --- _id: '11789' abstract: - lang: eng text: "We study a weighted online bipartite matching problem: G(V 1, V 2, E) is a weighted bipartite graph where V 1 is known beforehand and the vertices of V 2 arrive online. The goal is to match vertices of V 2 as they arrive to vertices in V 1, so as to maximize the sum of weights of edges in the matching. If assignments to V 1 cannot be changed, no bounded competitive ratio is achievable. We study the weighted online matching problem with free disposal, where vertices in V 1 can be assigned multiple times, but only get credit for the maximum weight edge assigned to them over the course of the algorithm. For this problem, the greedy algorithm is 0.5-competitive and determining whether a better competitive ratio is achievable is a well known open problem.\r\n\r\nWe identify an interesting special case where the edge weights are decomposable as the product of two factors, one corresponding to each end point of the edge. This is analogous to the well studied related machines model in the scheduling literature, although the objective functions are different. For this case of decomposable edge weights, we design a 0.5664 competitive randomized algorithm in complete bipartite graphs. We show that such instances with decomposable weights are non-trivial by establishing upper bounds of 0.618 for deterministic and 0.8 for randomized algorithms.\r\n\r\nA tight competitive ratio of 1 − 1/e ≈ 0.632 was known previously for both the 0-1 case as well as the case where edge weights depend on the offline vertices only, but for these cases, reassignments cannot change the quality of the solution. Beating 0.5 for weighted matching where reassignments are necessary has been a significant challenge. We thus give the first online algorithm with competitive ratio strictly better than 0.5 for a non-trivial case of weighted matching with free disposal." alternative_title: - LNCS article_processing_charge: No author: - first_name: Moses full_name: Charikar, Moses last_name: Charikar - first_name: Monika H full_name: Henzinger, Monika H id: 540c9bbd-f2de-11ec-812d-d04a5be85630 last_name: Henzinger orcid: 0000-0002-5008-6530 - first_name: Huy L. full_name: Nguyễn, Huy L. last_name: Nguyễn citation: ama: 'Charikar M, Henzinger MH, Nguyễn HL. Online bipartite matching with decomposable weights. In: 22nd Annual European Symposium on Algorithms. Vol 8737. Springer Nature; 2014:260-271. doi:10.1007/978-3-662-44777-2_22' apa: 'Charikar, M., Henzinger, M. H., & Nguyễn, H. L. (2014). Online bipartite matching with decomposable weights. In 22nd Annual European Symposium on Algorithms (Vol. 8737, pp. 260–271). Wroclaw, Poland: Springer Nature. https://doi.org/10.1007/978-3-662-44777-2_22' chicago: Charikar, Moses, Monika H Henzinger, and Huy L. Nguyễn. “Online Bipartite Matching with Decomposable Weights.” In 22nd Annual European Symposium on Algorithms, 8737:260–71. Springer Nature, 2014. https://doi.org/10.1007/978-3-662-44777-2_22. ieee: M. Charikar, M. H. Henzinger, and H. L. Nguyễn, “Online bipartite matching with decomposable weights,” in 22nd Annual European Symposium on Algorithms, Wroclaw, Poland, 2014, vol. 8737, pp. 260–271. ista: 'Charikar M, Henzinger MH, Nguyễn HL. 2014. Online bipartite matching with decomposable weights. 22nd Annual European Symposium on Algorithms. ESA: Annual European Symposium on Algorithms, LNCS, vol. 8737, 260–271.' mla: Charikar, Moses, et al. “Online Bipartite Matching with Decomposable Weights.” 22nd Annual European Symposium on Algorithms, vol. 8737, Springer Nature, 2014, pp. 260–71, doi:10.1007/978-3-662-44777-2_22. short: M. Charikar, M.H. Henzinger, H.L. Nguyễn, in:, 22nd Annual European Symposium on Algorithms, Springer Nature, 2014, pp. 260–271. conference: end_date: 2014-09-10 location: Wroclaw, Poland name: 'ESA: Annual European Symposium on Algorithms' start_date: 2014-09-08 date_created: 2022-08-11T10:41:47Z date_published: 2014-09-01T00:00:00Z date_updated: 2023-02-13T11:16:24Z day: '01' doi: 10.1007/978-3-662-44777-2_22 extern: '1' external_id: arxiv: - '1409.2139' intvolume: ' 8737' language: - iso: eng main_file_link: - open_access: '1' url: https://arxiv.org/abs/1409.2139 month: '09' oa: 1 oa_version: Preprint page: 260 - 271 publication: 22nd Annual European Symposium on Algorithms publication_identifier: isbn: - 978-366244776-5 issn: - 0302-9743 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Online bipartite matching with decomposable weights type: conference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 8737 year: '2014' ... --- _id: '11790' abstract: - lang: eng text: "Assume a seller wants to sell a digital product in a social network where a buyer’s valuation of the item has positive network externalities from her neighbors that already have the item. The goal of the seller is to maximize his revenue. Previous work on this problem [7] studies the case where clients are offered the item in sequence and have to pay personalized prices. This is highly infeasible in large scale networks such as the Facebook graph: (1) Offering items to the clients one after the other consumes a large amount of time, and (2) price-discrimination of clients could appear unfair to them and result in negative client reaction or could conflict with legal requirements.\r\n\r\nWe study a setting dealing with these issues. Specifically, the item is offered in parallel to multiple clients at the same time and at the same price. This is called a round. We show that with O(logn) rounds, where n is the number of clients, a constant factor of the revenue with price discrimination can be achieved and that this is not possible with o(logn) rounds. Moreover we show that it is APX-hard to maximize the revenue and we give constant factor approximation algorithms for various further settings of limited price discrimination." alternative_title: - LNCS article_processing_charge: No author: - first_name: Luděk full_name: Cigler, Luděk last_name: Cigler - first_name: Wolfgang full_name: Dvořák, Wolfgang last_name: Dvořák - first_name: Monika H full_name: Henzinger, Monika H id: 540c9bbd-f2de-11ec-812d-d04a5be85630 last_name: Henzinger orcid: 0000-0002-5008-6530 - first_name: Martin full_name: Starnberger, Martin last_name: Starnberger citation: ama: 'Cigler L, Dvořák W, Henzinger MH, Starnberger M. Limiting price discrimination when selling products with positive network externalities. In: 10th International Conference of Web and Internet Economics. Vol 8877. Springer Nature; 2014:44-57. doi:10.1007/978-3-319-13129-0_4' apa: 'Cigler, L., Dvořák, W., Henzinger, M. H., & Starnberger, M. (2014). Limiting price discrimination when selling products with positive network externalities. In 10th International Conference of Web and Internet Economics (Vol. 8877, pp. 44–57). Beijing, China: Springer Nature. https://doi.org/10.1007/978-3-319-13129-0_4' chicago: Cigler, Luděk, Wolfgang Dvořák, Monika H Henzinger, and Martin Starnberger. “Limiting Price Discrimination When Selling Products with Positive Network Externalities.” In 10th International Conference of Web and Internet Economics, 8877:44–57. Springer Nature, 2014. https://doi.org/10.1007/978-3-319-13129-0_4. ieee: L. Cigler, W. Dvořák, M. H. Henzinger, and M. Starnberger, “Limiting price discrimination when selling products with positive network externalities,” in 10th International Conference of Web and Internet Economics, Beijing, China, 2014, vol. 8877, pp. 44–57. ista: 'Cigler L, Dvořák W, Henzinger MH, Starnberger M. 2014. Limiting price discrimination when selling products with positive network externalities. 10th International Conference of Web and Internet Economics. WINE: International Conference on Web and Internet Economics, LNCS, vol. 8877, 44–57.' mla: Cigler, Luděk, et al. “Limiting Price Discrimination When Selling Products with Positive Network Externalities.” 10th International Conference of Web and Internet Economics, vol. 8877, Springer Nature, 2014, pp. 44–57, doi:10.1007/978-3-319-13129-0_4. short: L. Cigler, W. Dvořák, M.H. Henzinger, M. Starnberger, in:, 10th International Conference of Web and Internet Economics, Springer Nature, 2014, pp. 44–57. conference: end_date: 2014-12-17 location: Beijing, China name: 'WINE: International Conference on Web and Internet Economics' start_date: 2014-12-14 date_created: 2022-08-11T10:58:44Z date_published: 2014-12-01T00:00:00Z date_updated: 2023-02-13T11:18:30Z day: '01' doi: 10.1007/978-3-319-13129-0_4 extern: '1' intvolume: ' 8877' language: - iso: eng month: '12' oa_version: None page: 44 - 57 publication: 10th International Conference of Web and Internet Economics publication_identifier: issn: - 0302-9743 publication_status: published publisher: Springer Nature quality_controlled: '1' scopus_import: '1' status: public title: Limiting price discrimination when selling products with positive network externalities type: conference user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87 volume: 8877 year: '2014' ...