Long-Term Returns Predictability Following Stock Splits: The Blind Side

2016 ◽  
Author(s):  
Ahmed M. Elnahas ◽  
Lei Gao ◽  
Ghada M. Ismail

2015 ◽  
Vol 21 (1) ◽  
Author(s):  
Wei Wu ◽  
Robert Couch ◽  
Yulianto Suharto ◽  
Mark J. Ahn

Using an effectuation theory lens, we study reverse stock splits in the biotech industry where significant uncertainty makes specific scenarios of success difficult to predict. We conjecture and find that, in contrast to other environments where there is less uncertainty, reverse stock splits in the biotech industry are followed by positive abnormal returns over the subsequent 1- to 12-months. Also consistent with our effectuation-based predictions, we find that these returns are positively related to the reverse split ratio, size, cash holding, and long-term debt, and negatively related to the market-to-book ratio and firm age. We also find that liquidity increases after a reverse stock split. These results suggest that the concept of effectuation theory is better suited to analyzing reverse stock splits in the biotech industry. 



2009 ◽  
Vol 7 (2) ◽  
pp. 420-439
Author(s):  
Michael Gombola ◽  
Amy Yueh-Fang Ho ◽  
Yi-Kai Chen

This study investigates earnings management and long-term stock performance surrounding reverse stock splits. It is designed to provide evidence on the role of managerial pessimism and discretionary current accruals. Discretionary current accruals are used to measure earnings management. These discretionary current accruals are measured in our study using the balance sheet approach as well as the cash flow statement approach. We find consistent evidence of negative discretionary current accruals prior to reverse stock splits. Such negative discretionary accruals are consistent with managerial pessimism prior to a reverse stock split. Such pessimism is warranted by the observed negative market reaction to a reverse split announcement and the negative abnormal returns observed after reverse splits. Negative discretionary current accruals are also consistent with smoothing of earnings during difficult and challenging periods for the firm. Our study might provide an alternative to the opportunism explanation. It also provides additional evidence buttressing the role of managerial optimism and pessimism in explaining earnings management.



1995 ◽  
Vol 19 (3) ◽  
pp. 119-134
Author(s):  
Aigbe Akhigbe ◽  
Jeff Madura ◽  
Stephen P. Zera


2012 ◽  
Vol 18 (4) ◽  
pp. 439-449 ◽  
Author(s):  
Jae-Kwang Hwang ◽  
Young Dimkpah ◽  
Alex I. Ogwu


2010 ◽  
Vol 13 (03) ◽  
pp. 403-416 ◽  
Author(s):  
Li-Hsun Wang ◽  
Chu-Hsiung Lin ◽  
Hsien-Ming Chen

This study examines the application of CEO turnover on reverse stock splits firms. Using Taiwanese samples, we find that non-CEO turnover firms receive negative long-term abnormal returns, and their financial performances continue to decline following reverse splits. These findings are consistent with prior studies. Contrarily, neither significantly negative long-term abnormal returns nor changes on financial performance were found for CEO turnover firms. This study concludes that applying CEO turnover is suggestive in reverse splits. Additionally, we find that reverse split firms raise debt and concern with their short-term solvency following splits.



2019 ◽  
Vol 42 ◽  
Author(s):  
John P. A. Ioannidis

AbstractNeurobiology-based interventions for mental diseases and searches for useful biomarkers of treatment response have largely failed. Clinical trials should assess interventions related to environmental and social stressors, with long-term follow-up; social rather than biological endpoints; personalized outcomes; and suitable cluster, adaptive, and n-of-1 designs. Labor, education, financial, and other social/political decisions should be evaluated for their impacts on mental disease.



2016 ◽  
Vol 39 ◽  
Author(s):  
Mary C. Potter

AbstractRapid serial visual presentation (RSVP) of words or pictured scenes provides evidence for a large-capacity conceptual short-term memory (CSTM) that momentarily provides rich associated material from long-term memory, permitting rapid chunking (Potter 1993; 2009; 2012). In perception of scenes as well as language comprehension, we make use of knowledge that briefly exceeds the supposed limits of working memory.



1999 ◽  
Vol 173 ◽  
pp. 189-192
Author(s):  
J. Tichá ◽  
M. Tichý ◽  
Z. Moravec

AbstractA long-term photographic search programme for minor planets was begun at the Kleť Observatory at the end of seventies using a 0.63-m Maksutov telescope, but with insufficient respect for long-arc follow-up astrometry. More than two thousand provisional designations were given to new Kleť discoveries. Since 1993 targeted follow-up astrometry of Kleť candidates has been performed with a 0.57-m reflector equipped with a CCD camera, and reliable orbits for many previous Kleť discoveries have been determined. The photographic programme results in more than 350 numbered minor planets credited to Kleť, one of the world's most prolific discovery sites. Nearly 50 per cent of them were numbered as a consequence of CCD follow-up observations since 1994.This brief summary describes the results of this Kleť photographic minor planet survey between 1977 and 1996. The majority of the Kleť photographic discoveries are main belt asteroids, but two Amor type asteroids and one Trojan have been found.



1994 ◽  
Vol 144 ◽  
pp. 29-33
Author(s):  
P. Ambrož

AbstractThe large-scale coronal structures observed during the sporadically visible solar eclipses were compared with the numerically extrapolated field-line structures of coronal magnetic field. A characteristic relationship between the observed structures of coronal plasma and the magnetic field line configurations was determined. The long-term evolution of large scale coronal structures inferred from photospheric magnetic observations in the course of 11- and 22-year solar cycles is described.Some known parameters, such as the source surface radius, or coronal rotation rate are discussed and actually interpreted. A relation between the large-scale photospheric magnetic field evolution and the coronal structure rearrangement is demonstrated.



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