Literature DB >> 32401816

Why do biting horseflies prefer warmer hosts? tabanids can escape easier from warmer targets.

Gábor Horváth1, Ádám Pereszlényi1,2, Ádám Egri3,4, Tímea Tóth1, Imre Miklós Jánosi5.   

Abstract

Blood-sucking horseflies (tabanids) prefer warmer (sunlit, darker) host animals and generally attack them in sunshine, the reason for which was unknown until now. Recently, it was hypothesized that blood-seeking female tabanids prefer elevated temperatures, because their wing muscles are quicker and their nervous system functions better at a warmer body temperature brought about by warmer microclimate, and thus they can more successfully avoid the host's parasite-repelling reactions by prompt takeoffs. To test this hypothesis, we studied in field experiments the success rate of escape reactions of tabanids that landed on black targets as a function of the target temperature, and measured the surface temperature of differently coloured horses with thermography. We found that the escape success of tabanids decreased with decreasing target temperature, that is escape success is driven by temperature. Our results explain the behaviour of biting horseflies that they prefer warmer hosts against colder ones. Since in sunshine the darker the host the warmer its body surface, our results also explain why horseflies prefer sunlit dark (brown, black) hosts against bright (beige, white) ones, and why these parasites attack their hosts usually in sunshine, rather than under shaded conditions.

Entities:  

Year:  2020        PMID: 32401816      PMCID: PMC7219777          DOI: 10.1371/journal.pone.0233038

Source DB:  PubMed          Journal:  PLoS One        ISSN: 1932-6203            Impact factor:   3.240


Introduction

Blood-sucking horseflies (tabanids) prefer warmer (sunlit, darker) host animals against colder (shaded, brighter) ones and generally attack them in sunshine [1, 2, 3, 4, 5]. Tabanids attack black cattle more frequently than white ones [6]. Among white, brown and black cattle, black individuals are the preferred targets of Tabanus spp. horsefly attacks [7]. The attractiveness of sunlit brown horses to tabanids is about four times larger than that of sunlit white ones, and in comparison with a white horse, a brown horse spends two times longer in a tabanid-free shaded forest than in a sunny field with intense tabanid attacks [1]. The most effective tabanid traps use shiny black decoys [8, 9, 10, 11, 12, 13, 14, 15]. The so-called H-traps (composed of a bright tent with a shiny black sphere suspended below it) placed in sunny sites capture significantly more female tabanids than at shaded sites [16]. The reason for this is that sunlit shiny dark targets reflect light at the Brewster’s angle with higher degrees of linear polarization d than shaded ones [17, 18], and host-seeking female tabanids prefer high d-values independent of the direction of polarization [19]. Thus, shiny black decoys used to catch horseflies work due to their colour and reflected degree of polarization, rather than their temperature. After these experimental and observational findings concerning tabanid thermal preference, Horváth et al. [20] showed that Tabanus tergestinus horseflies prefer sunlit warm shiny black targets over sunlit or shaded cold ones with the same optical characteristics. Furthermore, they hypothesized that a blood-seeking female tabanid prefers elevated temperatures, because her wing muscles are quicker and her nervous system functions better in a warmer microclimate, and thus she can more successfully avoid the host’s parasite-repelling reactions by prompt takeoffs. Of course, there could also be other reasons why blood-sucking horseflies might prefer to attack warmer host animals. For example, to increase sweating, the capillaries could be enlarged near the epidermis of warmer hosts, which could be advantageous for blood-sucking insects. The prediction of the hypothesis of Horváth et al. [20] is that the escape success of horseflies that land on host animals increases with increasing surface temperature. To test this prediction, we studied the escape success of tabanids that landed on black targets as a function of the surface temperature, and measured the coat temperature of differently coloured sunlit and shaded horses with thermography. The results of our field experiments presented here corroborated prediction which explains why blood-seeking horseflies prefer sunlit dark (warmer) host animals.

Results

As expected, the surface temperature T of the sunlit back of horses decreased in the colour order black > brown > beige > white, and the mean temperature of the bellies had a smaller standard deviation ΔT than the backs (Fig 1, S1–S4 Figs). The minimum and maximum surface temperatures of horses were: black: 30.9–54.6°C, brown: 31.2–44.6°C, beige: 32.6–46.2°C, white: 31.0–46.6°C. The range Tmax—Tmin and ΔT increased with increasing (Fig 2, S1–S4 Tables).
Fig 1

Thermograms of horses.

Photographs and thermograms of sunlit black, brown, beige and white horses. In the thermograms the black perimeters of the back and belly areas are shown where the surface temperature T was averaged.

Fig 2

Surface temperatures of horses.

Minimum (Tmin), maximum (Tmax), average () and standard deviation (ΔT) of the surface temperature of the back and belly of black, brown, beige and white horses measured with thermography under different illumination conditions (S1–S4 Tables, S1–S4 Figs). shaded: shaded side of a sunlit horse, sunlit: sunlit side of a sunlit horse, cloudy: the horse was illuminated by skylight when the sun was occluded by clouds.

Thermograms of horses.

Photographs and thermograms of sunlit black, brown, beige and white horses. In the thermograms the black perimeters of the back and belly areas are shown where the surface temperature T was averaged.

Surface temperatures of horses.

Minimum (Tmin), maximum (Tmax), average () and standard deviation (ΔT) of the surface temperature of the back and belly of black, brown, beige and white horses measured with thermography under different illumination conditions (S1–S4 Tables, S1–S4 Figs). shaded: shaded side of a sunlit horse, sunlit: sunlit side of a sunlit horse, cloudy: the horse was illuminated by skylight when the sun was occluded by clouds. Fig 3 displays the surface temperature range Tmin ≤ T ≤ Tmax of barrels and the proportions of escape success and capture rate of tabanids that landed on the barrels under different illumination and thermal conditions. Considering experiments 1–3, the escape success was the highest on the sunlit air-filled barrel (85.4%, χ2 = 48.167, df = 1, p < 0.001), it was the lowest on the shaded water-filled barrel (28%, χ2 = 4.84, df = 1, p = 0.02781), and on the shaded air-filled barrel it was in between the former two (54.5%, χ2 = 0.36364, df = 1, p = 0.5465). Under sunlit conditions in experiment 4, the escape success on the air-filled barrel (81.3%) was significantly higher by a factor of 2.3 (χ2 = 34.9634, df = 1, p < 0.001) than that on the water-filled barrel (35.6%). In experiment 5, tabanids could escape also with a significantly higher success (χ2 = 32.5403, df = 1, p < 0.001) from the sunlit side of the air-filled barrel (86.4%) than from its shaded side (39.5%), similarly to the sunlit (45%) and shaded (29.4%) sides of the water-filled barrel (χ2 = 3.1832, df = 1, p = 0.074398). The numbers of captured and escaped tabanids were not significantly different in the following situations: shaded side of the air-filled barrel in experiment 2, shaded side of the air-filled barrel in experiment 5, and sunlit side of the water-filled barrel in experiment 5 (Fig 3, S5 Table). As illustrated in Fig 3 (S6–S10 Tables), the surface of air-filled barrels was always warmer than that of water-filled ones, and the sunlit surface of a given barrel was warmer than its shaded side. All these results support our hypothesis that tabanids can escape more successfully from warmer targets than from cooler ones.
Fig 3

Escape success of horseflies in experiments 1–5.

Surface temperature range Tmin ≤ T ≤ Tmax of barrels and the proportion of escape success of tabanids (grey bars) that landed on the barrels under different illumination and thermal conditions in experiments 1–5 (S6–S10 Tables). The results of χ2 test are indicated: n.s: not significant, p > 0.05, *: 0.01 < p < 0.05, **: 0.001 < p < 0.01, ***: p < 0.001 (S5 Table). Grey and black bars illustrate the escape and capture rates, the proportion values of which are given in the columns.

Escape success of horseflies in experiments 1–5.

Surface temperature range Tmin ≤ T ≤ Tmax of barrels and the proportion of escape success of tabanids (grey bars) that landed on the barrels under different illumination and thermal conditions in experiments 1–5 (S6–S10 Tables). The results of χ2 test are indicated: n.s: not significant, p > 0.05, *: 0.01 < p < 0.05, **: 0.001 < p < 0.01, ***: p < 0.001 (S5 Table). Grey and black bars illustrate the escape and capture rates, the proportion values of which are given in the columns. As illustrated in Fig 4A, the number Ne of escaped tabanids that landed on barrels has a maximum at around 41°C, drops to zero at 17°C and decreases almost to zero at 62°C. The drop of Ne at lower surface temperatures was the result of (i) less tabanids landing on colder surfaces, and (ii) the escape success is lower on them (see Fig 4C). Since the landing events shorter than 10 seconds were not registered, Ne droped with increasing T. In Fig 4B, the number Nc of captured tabanids that landed on barrels exhibits a clear decreasing trend with increasing Tbarrel for both temperature intervals of 17°C ≤ T ≤ 62°C and Tmin = 31°C ≤ T ≤ Tmax,BL = 55°C. In Fig 4C the increasing tendency of the normalized escape succes e = Ne/(Ne + Nc) with increasing barrel surface temperature Tbarrel is clear. Fig 4C also illustrates that the systematic increase of the escape success e is also present in the temperature range Tmin = 31°C ≤ T ≤ Tmax,BL = 55°C that is typical for the surface temperature of horses.
Fig 4

Escape success of horseflies versus surface temperature.

Number Ne of escaped (A) and number Nc of captured (B) tabanids that landed on barrels as a function of the surface temperature Tbarrel (oC). In B a continuous straight line indicates the linear fit to all Nc(Tbarrel) data (black circles in the interval 17°C ≤ T ≤ 62°C), and a dark grey band around this fit shows the 95% confidence interval. (C) Normalized escape success e = Ne/(Ne + Nc) versus Tbarrel (oC). A continuous straight line and a dark grey band illustrate the linear fit to all e(Tbarrel) data (white squares in the interval 17°C ≤ T ≤ 62°C) with 95% confidence interval. The vertical light and medium grey columns denote the interval Tmin = 31°C ≤ T ≤ Tmax,BBW = 47°C of the surface temperature of brown, beige and white horses (BBW) and the interval Tmin = 31°C ≤ T ≤ Tmax,BL = 55°C of black (BL) horses measured by thermography (Fig 2). In B and C a dotted straight line and a 95% confidence interval with dotted perimeter illustrate the linear fit to the data within the 31°C ≤ T ≤ 55°C interval.

Escape success of horseflies versus surface temperature.

Number Ne of escaped (A) and number Nc of captured (B) tabanids that landed on barrels as a function of the surface temperature Tbarrel (oC). In B a continuous straight line indicates the linear fit to all Nc(Tbarrel) data (black circles in the interval 17°C ≤ T ≤ 62°C), and a dark grey band around this fit shows the 95% confidence interval. (C) Normalized escape success e = Ne/(Ne + Nc) versus Tbarrel (oC). A continuous straight line and a dark grey band illustrate the linear fit to all e(Tbarrel) data (white squares in the interval 17°C ≤ T ≤ 62°C) with 95% confidence interval. The vertical light and medium grey columns denote the interval Tmin = 31°C ≤ T ≤ Tmax,BBW = 47°C of the surface temperature of brown, beige and white horses (BBW) and the interval Tmin = 31°C ≤ T ≤ Tmax,BL = 55°C of black (BL) horses measured by thermography (Fig 2). In B and C a dotted straight line and a 95% confidence interval with dotted perimeter illustrate the linear fit to the data within the 31°C ≤ T ≤ 55°C interval. Fig 5A shows that Tbarrel and Tair correlate positively. Similarly, there was a positive correlation between the normalized escape success e = Ne/(Ne + Nc) and Tair if we take into consideration the results of all five experiments (Fig 5B). Since Tair and Tbarrel correlate positively (Fig 5A) and e increases with increasing Tbarrel (Fig 4C), it could also be expected that e increases with increasing Tair as seen in Fig 5B. However, applying a linear regression for e-values measured at air temperatures lower than 33°C only (this way the warmest observations are eliminated when only sunlit air-filled warm barrels were used in experiment 1 resulting in a strong bias in the escape success e), the regression line becomes horizontal (Fig 5C). In this case there is no correlation between e and Tair. This suggests that the descended horseflies spent sufficient time (10 seconds) on the barrel so that Tbarrel determined the escape success, rather than Tair.
Fig 5

Normalized escape success versus temperatures.

(A) The barrel surface temperature Tbarrel (oC) versus air temperature Tair (oC) in field experiments 1–5. A straight line indicates the linear fit to the Tbarrel (Tair) data (black circles). (B) Normalized escape success e versus Tair (oC) for all five experiments. (C) As B, but only for Tair ≤ 32°C. (D) Normalized escape success e versus Tbarrel—Tair (oC) for all five experiments. In B-D continuous straight lines indicate the linear fit to the data (black circles), and dark grey bands around the fit show the 95% confidence intervals.

Normalized escape success versus temperatures.

(A) The barrel surface temperature Tbarrel (oC) versus air temperature Tair (oC) in field experiments 1–5. A straight line indicates the linear fit to the Tbarrel (Tair) data (black circles). (B) Normalized escape success e versus Tair (oC) for all five experiments. (C) As B, but only for Tair ≤ 32°C. (D) Normalized escape success e versus Tbarrel—Tair (oC) for all five experiments. In B-D continuous straight lines indicate the linear fit to the data (black circles), and dark grey bands around the fit show the 95% confidence intervals. Fig 5D illustrates that the normalized escape success e positively correlates with the temperature difference ΔT = Tbarrel—Tair (oC) for all five experiments. Note that the 17–62°C range of Tbarrel is larger than the 23–38°C range of Tair. This means that if ΔT is low/high, then Tbarrel is also low/high. Thus, the result in Fig 5D is similar to that in Fig 4C, because only the temperature range (horizontal axis) was changed, which resulted in some blur due to the relatively small variation Tair. Fig 6A shows the results of a logistic regression show a highly significant (p < 0.0001) positive correlation between Tbarrel and the escape probability ε of descended tabanids (S11 Table). The effect of Tbarrel in the logistic regression was also significant (p = 0.000395) for the temperature range 31–55°C (S12 Table). The logistic regression in Fig 6B displays a positive correlation between the air temperature Tair and the escape probability ε of tabanids, and the effect of Tair was highly significant (p < 0.0001, S13 Table). Fig 6C shows the highly significant (p < 0.0001) positive correlation between the difference Tbarrel—Tair and the escape probability ε of tabanids (S14 Table). These findings correspond to the results of the linear regressions.
Fig 6

Results of logistic regressions.

(A) Top: Number Ne of escaped horseflies versus the barrel surface temperature Tbarrel. Middle: Escape probability ε of horseflies, where the logistic curve is fitted to the dots showing the surface temperatures at which tabanids were escaped (ε = 100%) and captured (ε = 0%) within the 17°C ≤ Tbarrel ≤ 62°C interval. A dotted curve illustrates the logistic fit to the data within the 31°C ≤ Tbarrel ≤ 55°C interval. Bottom: Number Nc of captured horseflies versus Tbarrel. The vertical light and medium grey columns denote the interval Tmin = 31°C ≤ T ≤ Tmax,BBW = 47°C of the surface temperature of brown, beige and white (BBW) horses and the interval Tmin = 31°C ≤ T ≤ Tmax,BL = 55°C of black (BL) horses measured by thermography (Fig 2). (B) As A versus the air temperature Tair. (C) As A versus the difference Tbarrel—Tair.

Results of logistic regressions.

(A) Top: Number Ne of escaped horseflies versus the barrel surface temperature Tbarrel. Middle: Escape probability ε of horseflies, where the logistic curve is fitted to the dots showing the surface temperatures at which tabanids were escaped (ε = 100%) and captured (ε = 0%) within the 17°C ≤ Tbarrel ≤ 62°C interval. A dotted curve illustrates the logistic fit to the data within the 31°C ≤ Tbarrel ≤ 55°C interval. Bottom: Number Nc of captured horseflies versus Tbarrel. The vertical light and medium grey columns denote the interval Tmin = 31°C ≤ T ≤ Tmax,BBW = 47°C of the surface temperature of brown, beige and white (BBW) horses and the interval Tmin = 31°C ≤ T ≤ Tmax,BL = 55°C of black (BL) horses measured by thermography (Fig 2). (B) As A versus the air temperature Tair. (C) As A versus the difference Tbarrel—Tair.

Discussion

Female tabanids prefer to attack sunlit against shaded dark host animals, and dark against bright hosts for a blood meal, the exact reasons for which were unknown. Our results presented here show that the surface temperature of sunlit darker horses is higher than that of sunlit brighter horses. This result corresponds to previous measurements [21, 22, 23, 24, 25, 26, 27]. The differences in surface temperatures of dark and bright as well as sunlit and shaded hosts may partly explain their different attractiveness to tabanids. Horváth et al. [20] found that Tabanus tergestinus horseflies prefer sunlit warm shiny black targets against sunlit or shaded cold ones with the same optical characteristics. They hypothesized that blood-sucking female tabanids prefer higher temperatures, because their wing muscles are quicker and their nervous system functions better in a warmer microclimate [28], therefore they can avoid the parasite-repelling reactions of host animals by prompt takeoffs. Since the thermoreceptors of tabanids (as in Diptera in general) are in their legs, antennae and mouthpart [28, 29, 30], they cannot sense (e.g. by infrareceptors) the temperature of a target remotely. They can sense the surface temperature of a substrate/host only after physical contact (landing). However, based on the leg/antenna/mouth-sensed temperature of the boundary layer around a target, tabanids can decide whether the target’s surface is or is not warm enough for alighting [20]. The blood meal from warm-blooded animals is used by biting female horseflies as an energy source for the maturation of their eggs [25, 28, 29, 30]. For this purpose, the blood of any warm-blooded host is sufficient, regardless of whether a host is dark- or bright-coloured, shaded or sunlit. In spite of this, blood-seeking female tabanids prefer dark and sunlit hosts [1, 2, 3, 4, 5, 6, 7], and this is the reason why horsefly traps usually have black decoys and are most effective in sunshine [8, 9, 10, 11, 12, 13, 14, 15, 16]. Our main assumption was that blood-seeking tabanids prefer to land on sunlit dark hosts to keep their body warm, which aids their rapid escape when the host performs such typical antiparasite reactions as removing horseflies from their coats with tail brushing, stamping and dislodging the flies, or by nibbling their skin [1, 28]. These fly-repelling reactions are dangerous for blood-sucking tabanids, therefore have to be avoided by a quick flying away. In this work we analysed the results of our field experiments for the whole tabanid population of the study area without considering differences between tabanid species/genus, because species/genus identification was not feasible in the field. However, there may be differences between species/genus in landing, daily activity and responses to environmental parameters that might influence their escape success. For example, Haematopota species might be more active in the late afternoon when Tair decreases. It is also unknown whether the influence of Tair on host preference for Haematopota sp. is lower than that for Tabanus or Atylotus sp. To test these hypotheses could be the focus of further studies. What we know from our field experiments is the following: (i) apart from Tair (S6–S10 Tables) the weather situation (calm with no meteorological fronts) was the same during our field experiments. (ii) There was no correlation between the escape success e of descended horseflies and Tair < 33°C (Fig 5C). In this case Tbarrel determined the escape success e, rather than Tair. According to earlier field experiments [31, 32] in the same experimental site (a Hungarian horse farm in Szokolya) with the same tabanid species (Tabanus tergestinus, T. bromius, T. bovinus, T. autumnalis, Atylotus fulvus, A. loewianus, A. rusticus, Haematopota italica) as in the present field experiments, the daily activity of different tabanid species and the effect of weather variables on their flight activity were slightly different. Herczeg et al. [32], for example, found the following: (i) rainfall, air temperature, and sunshine were the three most important factors influencing the number of tabanids trapped. (ii) The effect of relative air humidity H on tabanids was indirect through the Tair: H ≈ 35% (corresponding to T ≈ 32°C) was optimal for tabanid capture, and tabanids were not captured at H ≥ 80% (corresponding to T ≤ 18°C). (iii) A fast decrease in the air pressure enhanced the trap success for horseflies. (iv) Wind velocities exceeding 10 km/h drastically reduced the number of trapped tabanids. In our field experiments 4 and 5 warm and cold sunlit barrels were used simultaneously, while in experiments 1–3 the cold and the warm barrels were tested separately (experiment 1: sunlit air-filled barrels, experiment 2: shaded air-filled barrels, experiment 3: shaded water-filled barrels). This was, however, not a problem, because apart from the air temperature (S6–S10 Tables) the environmental conditions (calm with no meteorological fronts) were practically identical on all experimental days. Thus, the slightly different environmental factors in our field experiments could have resulted in only small differences in the activity of a given tabanid species. In our field experiments the investigator waited 10 seconds before he tried to capture a tabanid that landed on a barrel. This 10-second period turned out to be optimal: it was neither too short, nor too long. Within a period shorter than 10 s the flight muscles of descended tabanids could not warm up or cool down to the surface temperature of barrels [33]. On the other hand, when a tabanid recognizes that the barrel is not a host animal after landing, it flies away after a certain period. If too much time had elapsed after tabanids landed before the counting was initiated, many of these events would have been missed. Since Tair did not correlate with the escape success (Fig 5C), 10 s was sufficiently long to warm the wing muscles of flies that landed on the barrel. On the other hand, if a tabanid lands on a sunlit dark (warm) surface, then it will not cool down, contrary to a bright (colder) surface where its wing muscles can cool down. It is reasonable to suppose that during flight the wing muscles are appropriately warm. Furthermore, according to Heinrich [33], many Dipteran species (including true flies and also tsetse flies) can be heterothermic, or generate a certain amount of heat which can then be used to improve their performance. However, as far as we know, practically nothing is known about the thermoregulation in horseflies. Thus, without knowing the horsefly thermal physiology, we restricted our study to the correlation between (air/barrel) temperature and escape success with a waiting period of 10 seconds before the experimenter tried to capture a tabanid that landed on a barrel. During the field experiments all barrels were optically uniformly attractive to host-seeking horseflies. Our air-filled sunlit warm barrels (37–62°C) thermally imitated sunlit black horses (31–55°C), while our water-filled sunlit cold barrels (19–29°C) were cooler than sunlit brown, beige and white horses (31–47°C). Although the measured low escape successes in the case of our water-filled cold barrels were associated with temperatures that were lower than those on the studied horse bodies, the positive correlation between escape success e and surface temperature T (i.e. increasing e with increasing T) is also evident in the interval Tmin = 31°C ≤ T ≤ Tmax,BL = 55°C as clearly shown by the dotted curves of Figs 4C and 6A. Thus, the results of our field experiments show that the escape success of tabanids depends on the host’s surface temperature T: the higher the T, the larger the escape success of horseflies. The average surface temperature of the studied sunlit black horses was between 48 and 55°C. Almost all tabanids managed to escape in this temperature range. In Figs 4 and 6A, the 100% escape successes at surface temperatures T > 50°C are associated with very small absolute numbers of horseflies and also with hot air temperatures ranging from 33 to 38°C (S6 Table). The reason for this is that only the minority of tabanids landing on hot (T > 55°C) surfaces spent periods longer than 2 seconds on them, and the waiting time until a catch attempt was 10 seconds after a tabanid landed on a barrel. In experiment 1 the weather was very warm (Tair ≤ 38°C) and the surface temperature of the warm barrel was above 45°C the whole day (S6 Table). Larger horseflies can tolerate extreme temperatures for a short time, and are also intrinsically faster [28]. The thermal transfer between a horsefly and a surface could be very different in the following two cases: (i) When a fly lands on a horse, the grip is maintained by the insect’s legs holding on the hairs, leaving plenty of insulating air between the two animals. (ii) When a fly lands on a plastic barrel, its legs must remain attached to a much less convenient substrate. In the future, an important task could be to measure both types of thermal transfer. It has been shown that dark-bodied host animals have a much stronger reflection-polarization signature than bright-bodied ones, which is an important visual sign, leading to horsefly attacks [18]. The high degrees of polarization of reflected light helps tabanids to select sunlit dark host animals from the dark patches of their visual environment. A strong polarization signature could also advertise a hot animal and greater chances of escape of tabanids, but both traits could be also dissociated, all depending on the thermal transfer and the thermal physiology of horseflies.

Conclusion

We presented the results of our field experiment studying the dependence of tabanid escape success on the temperature of the landing surface. The temperature of artificial landing sites was parallelled by the analysis of thermal imaging measurements of surface temperatures of different body parts of differently coloured horses. Not surprisingly, fur temperatures were higher in darker horses and lower in bright coloured ones. The tabanid escape success strongly depended on the surface temperature; the highest escape success occurred on surfaces having temperatures similar to those recorded in black horses, i.e. above 50°C. We conclude that the warmer (also darker) host animals allow higher escape success of blood-sucking horseflies. This supports our hypothesis that the preference of horseflies to dark hosts has partly evolved due to higher survival success.

Materials and methods

Animal ethics statement and field study permits

Csaba Viski permitted us to photograph his horses in his horse farm in Szokolya. For the location and activities of our field study no specific permissions were required.

Thermography of horses

On a warm day (6 July 2019) 46 thermograms of 2 black, 2 brown, 2 beige and 2 white horses were obtained with an infrared camera (VarioCAM®, Jenoptik Laser Optik Systeme GmbH, Jena, Germany, nominal precision of ±1.5°C) under sunny and cloudy conditions. The validation and calibration of this thermocamera with a contact thermometer (GAO Digital Multitester EM392B 06554H, EverFlourish Europe Gmbh., Friedrichsthal, Germany, nominal precision of ±1°C) are described in the Supporting Material of [20].

Field experiments

Field experiments 1–5 were performed on 1, 2, 3, 4 and 11 July 2019 on a Hungarian horse farm in Szokolya (47o 52' North, 19o 00' East), where horseflies were present. All five experimental days were windless, and only weak local winds blew in the early afternoons. Meteorological fronts did not move through the study site. Thus, apart from the air temperature (according to S6–S10 Tables, in experiment 1 the air temperatures were warmer than on the other four experimental days), the environmental conditions were practically the same. In the mornings, the weather was sunny, warm and cloudless, however in the afternoons a few cumulus clouds formed. In these experiments the escape success of tabanids that landed on shiny black cylindrical plastic barrels (height = 42 cm, diameter = 30 cm, wall thickness = 5 mm) of different surface temperatures (set with warm air or cold water load) but with the same optical characteristics was studied under sunlit and shaded conditions. The purpose of these barrels was to imitate warm and cold dark host animals of tabanids. Sufficiently large temperature differences between the warm and cold barrels could easily be ensured with air-filled warm and water-filled cold barrels. An experimenter, who was "blind" to the predictions of the experiment tried to capture the tabanids that landed on the barrels with a hemispherical tea-strainer of diameter 15 cm. The time allowed to elapse before a capture attempt was 10 seconds (measured with a stopwatch) after a tabanid landed on a barrel. This 10-second period turned out to be optimal: it was neither too short, nor too long (a more detailed explanation of the choice of this optimal 10-second value can be read in the Discussion). In experiment 1 (1 July 2019, 10:20–17:00 hour = local summer time = UTC + 2 h) two air-filled sunlit black barrels were used, which thermally modelled sunlit black host animals (e.g. horses) for tabanids. The two barrels were put on top of each other, and both were placed on a four-legged white plastic stand (height = 46 cm) at a sunlit site without any shade cast by vegetation or other objects. Only tabanids that landed on the sunlit side of the barrels were taken into account. In experiment 2 (2 July 2019, 9:40–16:00 h) two air-filled barrels under shadow were used, which modelled shaded hosts. The barrels were put on top of each other and the white stand was in the shade of trees during the experiment. Only tabanids that landed on the side of the barrels facing toward the open field were considered. In experiment 3 (3 July 2019, 9:50–16:00 h) two cold-water-filled shaded barrels were used, which modelled cool shaded hosts. The barrels were continuously in the shadow of trees. Both barrels were filled with tap water and 10 frozen ice packs (Aspico G40, 0.25 litre, 0.76 kg). The experimenter tried to capture only tabanids that landed on the side of the barrels facing toward the open field. In experiment 4 (4 July 2019, 10:00–12:00 h) two sunlit air-filled barrels and two sunlit cold-water-filled barrels were used which thermally modelled sunlit and shaded hosts, respectively. Both barrels were continuously exposed to sunlight. Only tabanids that landed on the sunlit side of the barrels were tried to capture. Experiment 5 (11 July 2019, 10:20–16:00 h) was technically the same as experiment 4, but all tabanids landing on both sunlit and shaded sides of barrels were subject of attack. The experimenter wore white clothes and a hat against direct sunshine and to minimize his visual attractiveness to tabanids. He was sitting on a chair during the experiments next to the barrels (50 cm) in such a way that he could easily reach the tabanids on the barrels with the tea-strainer. After the fly was successfully caught, it was released. After each capture trial the air temperature (Tair) and the surface temperature of the barrel (Tbarrel) at the tabanid’s landing location was measured with a contact thermometer (GAO Digital Multitester EM392B 06554H, EverFlourish Europe Gmbh., Friedrichsthal, Germany, nominal precision of ±1°C). For this part of the study, the use of thermography was not possible, because (i) the thermocamera needed about two minutes for self-calibration after each switch on, whilst the next tabanids could land on the barrels, and (ii) on the recorded thermograms it would have been impossible to localize the exact landing sites of tabanids. The experimenter was the same person throughout all experiments, who had practised the capture of tabanids during a pilot experiment. Due to the low number of flying tabanids in the vicinity of the barrels, only single tabanids landed on the barrels at any given time. Thus, the experimenter’s attention could focus entirely on one fly at a time. An in situ identification of the species of tabanids that landed on the barrels was not feasible. It was obvious, however, that they were tabanids (Diptera: Tabanidae). In previous field experiments [31, 32], the following tabanid species occurred at the same study site: Tabanus tergestinus, T. bromius, T. bovinus, T. autumnalis, Atylotus fulvus, A. loewianus, A. rusticus, Haematopota italica. Since we could record the escape success of different tabanid species, our results can be considered as the average escape success of the tabanid population of the experimental site. Since the reflection-polarization characteristics of the dry barrel surface are independent of its temperature in the visible spectral range, all optical parameters (radiance, degree of linear polarization and angle of polarization) of our warm and cool barrels were identical.

Statistical analysis

For comparison of the numbers of escaped and captured tabanids that landed on test surfaces of various temperatures, we applied χ2 tests of homogeneity, where the escape versus non-escape ratio was tested against the predicted 50/50 ratio. These χ2 tests were performed to compare escape/non-escape numbers for a given barrel or barrel side (sunlit or shaded). Thus, the compared escape/non-escape numbers corresponded to the same barrel temperature and there was no comparison between data originating from different barrel temperatures. In other words, χ2 test was used to detect whether a given barrel temperature had an effect on tabanid escape success. Linear regressions were applied to find a trend of the escape success of horseflies as a function of Tbarrel, Tair and Tbarrel—Tair. The independent variables were Tbarrel, Tair and Tbarrel—Tair, while the dependent variable was the normalized escape success e = Ne/(Ne + Nc, where Ne is the number of escaped tabanids and Nc is the number of captured horseflies. We also applied logistic regression to model the probability of escape as a function of Tbarrel, Tair and Tbarrel—Tair. We also applied the linear and logistic regressions as a funciton of Tbarrel using the data within the 31°C ≤ T ≤ 55°C interval. Logistic regression was also used to find whether there is a correlation between Tair and Tbarrel. The R statistical package 3.0.2 [34] was used for statistical analyses.

Temperatures of black horses measured with thermography on shaded and sunlit sides of the back and belly, and when the sun was occluded by clouds (cloudy).

: average, ±ΔT: standard deviation, Tmin: minimum, Tmax: maximum. (DOC) Click here for additional data file.

Temperatures of brown horses measured with thermography on shaded and sunlit sides of the back and belly, and when the sun was occluded by clouds (cloudy).

: average, ±ΔT: standard deviation, Tmin: minimum, Tmax: maximum. (DOC) Click here for additional data file.

Temperatures of beige horses measured with thermography on shaded and sunlit sides of the back and belly, and when the sun was occluded by clouds (cloudy).

: average, ±ΔT: standard deviation, Tmin: minimum, Tmax: maximum. (DOC) Click here for additional data file.

Temperatures of white horses measured with thermography on shaded and sunlit sides of the back and belly, and when the sun was occluded by clouds (cloudy).

: average, ±ΔT: standard deviation, Tmin: minimum, Tmax: maximum. (DOC) Click here for additional data file.

Results of χ2 tests comparing the sums of S6–S10 Tables obtained in experiments 1–5.

(DOC) Click here for additional data file.

Capture success (-: Not captured, +: Captured) of horseflies, and temperatures of the air (Tair) and the surface of the air-filled sunlit barrel (Tbarrel) in experiment 1 on 1 July 2019.

(DOC) Click here for additional data file.

Capture success (-: Not captured, +: Captured)) of horseflies, and temperatures of the air (Tair) and the surface of the air-filled shaded barrel (Tbarrel) in experiment 2 on 2 July 2019.

(DOC) Click here for additional data file.

Capture success (-: Not captured, +: Captured) of horseflies, and temperatures of the air (Tair) and the surface of the cold-water-filled shaded barrel (Tbarrel) in experiment 3 on 3 July 2019.

(DOC) Click here for additional data file.

Capture success (-: Not captured, +: Captured) of horseflies, and temperatures of the air (Tair) and the sunlit side of the surface of the air-filled warm barrel (Twarm) and the water-filled cold barrel (Tcold) in experiment 4 on 4 July 2019.

(DOC) Click here for additional data file.

Capture success (-: Not captured, +: Captured) of horseflies, and temperatures of the air (Tair) and the surface of the air-filled sunlit barrel (Twarm) and the cold-water-filled sunlit barrel (Tcold) in experiment 5 on 11 July 2019.

(DOC) Click here for additional data file.

Summary of the logistic regression.

The escape probability ε of tabanids depends highly significantly on the barrel surface temperature Tbarrel in the interval 17°C ≤ Tbarrel ≤ 62°C. The large difference between the null deviance and the residual deviance suggests that the logistic regression model is accurate. (DOC) Click here for additional data file. The escape probability ε of tabanids depends highly significantly on the barrel surface temperature Tbarrel in the interval 31°C ≤ Tbarrel ≤ 55°C. (DOC) Click here for additional data file. The escape probability ε of tabanids depends highly significantly on the air temperature Tair. (DOC) Click here for additional data file. The escape probability ε of tabanids depends highly significantly on the temperature difference Tbarrel—Tair. (DOC) Click here for additional data file.

Photographs, thermograms and thermograms with selected back and belly areas of black horses under different illumination conditions.

Shaded: shaded side of the sunlit horse. sunlit: sunlit side of the sunlit horse. cloudy: illuminated by skylight when the sun was occluded by clouds. (DOC) Click here for additional data file.

Photographs, thermograms and thermograms with selected back and belly areas of brown horses under different illumination conditions.

Shaded: shaded side of the sunlit horse. sunlit: sunlit side of the sunlit horse. cloudy: illuminated by skylight when the sun was occluded by clouds. (DOC) Click here for additional data file.

Photographs, thermograms and thermograms with selected back and belly areas of a beige horse under different illumination conditions.

Shaded: shaded side of the sunlit horse. sunlit: sunlit side of the sunlit horse. cloudy: illuminated by skylight when the sun was occluded by clouds. (DOC) Click here for additional data file.

Photographs, thermograms and thermograms with selected back and belly areas of white horses under different illumination conditions.

Shaded: shaded side of the sunlit horse. sunlit: sunlit side of the sunlit horse. cloudy: illuminated by skylight when the sun was occluded by clouds. (DOC) Click here for additional data file. 16 Mar 2020 PONE-D-20-04024 Why Do Biting Horseflies Prefer Warmer Hosts? Tabanids can Escape Easier from Warmer Targets PLOS ONE Dear Prof. Horvath, Thank you for submitting your manuscript to PLOS ONE. After careful consideration, we feel that it has merit but does not fully meet PLOS ONE’s publication criteria as it currently stands. Therefore, we invite you to submit a revised version of the manuscript that addresses the points raised during the review process. The reviewers agree that this is an interesting manuscript but also express some concerns about the methodology employed that need to be addressed carefully. These include the lack of taxonomic identification at least to genus level of the tabanids observed and the varying conditions under which data for the various experiments were collected. Importantly though, thermal measurements of real hosts and the barrels used appear to be different which may question the conclusions drawn from the data. In addition, there are a number of apparent contradictions throughout the manuscript which should also be shortened. In their revisions the authors should carefully address the comments by the reviewers provided below. We would appreciate receiving your revised manuscript by Apr 30 2020 11:59PM. When you are ready to submit your revision, log on to https://www.editorialmanager.com/pone/ and select the 'Submissions Needing Revision' folder to locate your manuscript file. If you would like to make changes to your financial disclosure, please include your updated statement in your cover letter. To enhance the reproducibility of your results, we recommend that if applicable you deposit your laboratory protocols in protocols.io, where a protocol can be assigned its own identifier (DOI) such that it can be cited independently in the future. For instructions see: http://journals.plos.org/plosone/s/submission-guidelines#loc-laboratory-protocols Please include the following items when submitting your revised manuscript: A rebuttal letter that responds to each point raised by the academic editor and reviewer(s). This letter should be uploaded as separate file and labeled 'Response to Reviewers'. A marked-up copy of your manuscript that highlights changes made to the original version. This file should be uploaded as separate file and labeled 'Revised Manuscript with Track Changes'. An unmarked version of your revised paper without tracked changes. This file should be uploaded as separate file and labeled 'Manuscript'. Please note while forming your response, if your article is accepted, you may have the opportunity to make the peer review history publicly available. The record will include editor decision letters (with reviews) and your responses to reviewer comments. If eligible, we will contact you to opt in or out. We look forward to receiving your revised manuscript. Kind regards, Heike Lutermann, PhD Academic Editor PLOS ONE Journal Requirements: When submitting your revision, we need you to address these additional requirements. 1. Please ensure that your manuscript meets PLOS ONE's style requirements, including those for file naming. The PLOS ONE style templates can be found at http://www.journals.plos.org/plosone/s/file?id=wjVg/PLOSOne_formatting_sample_main_body.pdf and http://www.journals.plos.org/plosone/s/file?id=ba62/PLOSOne_formatting_sample_title_authors_affiliations.pdf 2. PLOS requires an ORCID iD for the corresponding author in Editorial Manager on papers submitted after December 6th, 2016. Please ensure that you have an ORCID iD and that it is validated in Editorial Manager. To do this, go to ‘Update my Information’ (in the upper left-hand corner of the main menu), and click on the Fetch/Validate link next to the ORCID field. This will take you to the ORCID site and allow you to create a new iD or authenticate a pre-existing iD in Editorial Manager. Please see the following video for instructions on linking an ORCID iD to your Editorial Manager account: https://www.youtube.com/watch?v=_xcclfuvtxQ 3. Your ethics statement must appear in the Methods section of your manuscript. If your ethics statement is written in any section besides the Methods, please move it to the Methods section and delete it from any other section. Please also ensure that your ethics statement is included in your manuscript, as the ethics section of your online submission will not be published alongside your manuscript. [Note: HTML markup is below. Please do not edit.] Reviewers' comments: Reviewer's Responses to Questions Comments to the Author 1. Is the manuscript technically sound, and do the data support the conclusions? The manuscript must describe a technically sound piece of scientific research with data that supports the conclusions. Experiments must have been conducted rigorously, with appropriate controls, replication, and sample sizes. The conclusions must be drawn appropriately based on the data presented. Reviewer #1: Yes Reviewer #2: Yes Reviewer #3: Partly ********** 2. Has the statistical analysis been performed appropriately and rigorously? Reviewer #1: Yes Reviewer #2: Yes Reviewer #3: Yes ********** 3. Have the authors made all data underlying the findings in their manuscript fully available? The PLOS Data policy requires authors to make all data underlying the findings described in their manuscript fully available without restriction, with rare exception (please refer to the Data Availability Statement in the manuscript PDF file). The data should be provided as part of the manuscript or its supporting information, or deposited to a public repository. For example, in addition to summary statistics, the data points behind means, medians and variance measures should be available. If there are restrictions on publicly sharing data—e.g. participant privacy or use of data from a third party—those must be specified. Reviewer #1: Yes Reviewer #2: Yes Reviewer #3: Yes ********** 4. Is the manuscript presented in an intelligible fashion and written in standard English? PLOS ONE does not copyedit accepted manuscripts, so the language in submitted articles must be clear, correct, and unambiguous. Any typographical or grammatical errors should be corrected at revision, so please note any specific errors here. Reviewer #1: Yes Reviewer #2: Yes Reviewer #3: Yes ********** 5. Review Comments to the Author Please use the space provided to explain your answers to the questions above. You may also include additional comments for the author, including concerns about dual publication, research ethics, or publication ethics. (Please upload your review as an attachment if it exceeds 20,000 characters) Reviewer #1: This is a very interesting and important manuscript. Manuscript comprises important data which are well represented, illustrated and commented. However, I have one comment in chapter Introduction; last part of last sentence line 82 to 85 is not clear “though the blood of shady or bright (cooler) hosts would also good for the development of tabanid eggs”. I would like to suggest delete this in the last sentence. Blood meal of warm blooded animals biting female horseflies use as source of energy for egg maturation, regardless if hosts are dark or bright colour or in shady place or in sunlit. Everything else is excellent (abstract, introduction, materials and methods, results, discussion, conclusions and statistical analyses as well as English language). Reviewer #2: Dear Editor, The article is about tabanid preferences to darker hosts. The authors tested the hypothesis that tabanids prefer dark sunlit warm hosts because high temperatures might increase wing muscle and nervous system performance so that tabanid females escape easily and quickly in case of host defensive reactions. First, the authors estimated surface temperatures of horses with different coat colour. Then, they compared tabanid escape success in the field using different barrels modelling horse surface temperatures. This study provides an interesting approach to explain why tabanid are attracted by warm hosts or targets since it is well-known that host attractivity is dependant on olfactive, visual and thermal cues. However, here are some minor concerns about the study: - The authors analysed the results for all the tabanid population of the study area without considering differences between species. I understand that species identification is not feasible in the field, however the authors could have identified tabanid at the genus level. Tabanus, Atylotus and Haematopota have main characteristics that allow to discriminate them. There are differences between species in landing, daily activity and responses to environmental parameters that might influence their escape success. For example, Haematopota species might be more active in late afternoon when temperatures decrease. Maybe, the influence of temperatures on host preference for Haematopota sp. is lower than for Tabanus sp. or Atylotus sp. I think that this point should be discussed by the authors. - Field experiment setting: only the experiments 4 and 5 are well set to compare tabanid escape success between the two types of barrels modelling hosts with different temperatures in the same conditions. In experiments 1, 2 and 3, the two barrels were not tested simultaneously. They were used different days with different environmental conditions. However, factors other than temperatures (for example, wind) have an effect on tabanid activity and these other factors might also influenced escape success. - Statistical analysis : the authors used a Khi 2 test to compare the escape/non escape ratio versus the 50/50 ratio. This test did not allow to compare warm barrel versus cold barrel. - Discussion (lines 191-194) : I suggest to develop this part and to cite some references about tabanid landings and host defensive reactions. - I am not English-native speaker, but I think that the manuscript might be improved by an English speaker review. Reviewer #3: The paper by Horváth et al. deals with the interesting hypothesis, demonstrated by the Authors, that horseflies, after landing, would prefer to walk around and feed on warmer hosts as this would allow them to be more reactive and ready to take off, escaping hosts defensive reactions. The paper is interesting for an entomologist working on horseflies, English language is very good, methods are sound and provided data strong, but there are some major concerns affecting the manuscript, to be evaluated before taking a decision regarding its publication on PLOS ONE. The first one regards the exceedingly excessive length of the manuscript that is really redundant and rambling. Whole sections should be reduced or totally deleted. Authors spent a lot of words both in materials and methods and results dealing with very obvious statements regarding horse temperatures, that should be considered not a for its own sake section, but just something functional to experiments on horseflies. As a consequence, all the sections dealing with horse temperatures should be reduced to few lines, also considering that results are very obvious: a dark horse is warmer than a white one, a horse in sunlight is warmer than a horse in the shadow, the belly is cooler than the back, and other similar things. This is very boring for the reader. Also figures, photos and graphs on this subject should be eliminated. The whole manuscript needs to be simpler and slenderer to make it really interesting. But, there are also some logic and methodological problems, with contradictory statements and results. There is a methodological problem, which in theory could impair a big part of the results, needing an explanation by the Authors. I hereby detail the problems I revealed during the review, problems that have to be addressed by Authors with a very thorough revision, to make the manuscript deserving publication on PLOS ONE. 1. Manuscript Length: a) Lines 93-110: reduce to 3-5 lines at maximum, as they are very obvious results, which should be only functional to the experiments on horseflies. Moreover, remove figures and graphs only dealing with horse temperatures; b) Lines 145-149: these lines should be deleted, as results of this analysis are clear enough also without this heavy introduction; c) Lines 197-201: delete these lines. Not necessary and only making the discussion heavier; d) Lines 209-218: delete these lines. They are an unnecessary and really unexplainable repetition of things already said elsewhere in the manuscript. They are Introduction, Materials and Methods, not a Discussion at all; e) Lines 265-278: the same as for point a). Reduce to 3 lines. This section is not for its own sake, but only functional to experiments on tabanids. Moreover, most part of relative results are very obvious. Again, shorten all the sections regarding horse temperatures and remove graphs, pics. They all make the paper very strenuous to read; f) Lines 290-292: not necessary. Delete; g) Lines 295-296: not necessary. Delete; h) Lines 326-329: shorten this explanation. It was not possible for technical problems. Most part of readers will be entomologists!!!; i) Lines 342-345: Delete these lines. Authors just said that from an optical point of view the barrels were the same, this is enough. 2. Methodological problem: What reported at lines 89-92 is quite strange and needs to be explained by the Authors. In fact, while warm and cold barrels ranges of temperatures don't overlap, warm and “cold horses” are highly overlapping. Moreover, while warm barrels are, for the most part, in the range of temperatures of “warm horses”, cold barrels temperatures are lower than those of “colder horses”, totally out of the range of temperature of “cold horses”. This is very strange. Standing this situation, it seems that authors used cold barrels too cold, don't reflecting a real situation and hence possibly producing wrong results. This is really very relevant. The use of so cold barrels could invalidate the whole study. Authors should explain this choice and why, in their opinion, this is not affecting the validity of the work. 3. Contradictory Statements and Needed Explanations: a) Lines 66-68: if it is true, as Authors say in another part of the manuscript, that tabanids are not able to feel temperature of an object before landing on it, what stated in these lines is in contradiction with what Authors try to demonstrate in the paper. Black decoys used for catching horseflies would work not for their temperature, but for their colour; b) Lines 129-144: the whole paragraph is very mixed up, difficult to read and understand. Furthermore, Authors don’t explain some of the findings. Why there is a drop of escaped tabanids at very high temperatures? Zero at 62°C? Why fewer tabanids landed on cold barrels if they feel temperature only after landing? Why the specification at lines 139-140? All these things are quite obscure for the reader. Authors should greatly simplify this section, explain these points and report only the relevant results; c) Line 294: Why 10 seconds? In Materials and Methods Authors should explain this choice; d) Lines 331-333: it is not clear how Authors prevented the simultaneous landing of two or more tabanids on barrels. They give it for granted, but it is not. At Line 62, “spp.” not in italics; At line 84 “would also good for” should be changed in “would also be good for” In conclusion, the paper by Horváth et al. could deserve publication on PLOS ONE only after major changes regarding its length and some logic inconsistency that Authors should modify or better explain. ********** 6. PLOS authors have the option to publish the peer review history of their article (what does this mean?). If published, this will include your full peer review and any attached files. If you choose “no”, your identity will remain anonymous but your review may still be made public. Do you want your identity to be public for this peer review? For information about this choice, including consent withdrawal, please see our Privacy Policy. Reviewer #1: No Reviewer #2: No Reviewer #3: No [NOTE: If reviewer comments were submitted as an attachment file, they will be attached to this email and accessible via the submission site. Please log into your account, locate the manuscript record, and check for the action link "View Attachments". If this link does not appear, there are no attachment files to be viewed.] While revising your submission, please upload your figure files to the Preflight Analysis and Conversion Engine (PACE) digital diagnostic tool, https://pacev2.apexcovantage.com/. PACE helps ensure that figures meet PLOS requirements. To use PACE, you must first register as a user. Registration is free. Then, login and navigate to the UPLOAD tab, where you will find detailed instructions on how to use the tool. If you encounter any issues or have any questions when using PACE, please email us at figures@plos.org. Please note that Supporting Information files do not need this step. 31 Mar 2020 All specific reviewer and editor comments are responded in detail in the following uploaded file: +TabanidThermalTrapping_PLoS-One-response.doc Submitted filename: +TabanidThermalTrapping_PLoS-One-response.doc Click here for additional data file. 16 Apr 2020 PONE-D-20-04024R1 Why Do Biting Horseflies Prefer Warmer Hosts? Tabanids can Escape Easier from Warmer Targets PLOS ONE Dear Prof. Horvath, Thank you for submitting your manuscript to PLOS ONE. After careful consideration, we feel that it has merit but does not fully meet PLOS ONE’s publication criteria as it currently stands. Therefore, we invite you to submit a revised version of the manuscript that addresses the points raised during the review process. ============================== Both reviewers are satiesfied with the way the authors have addressed there previous comments but there are still a few matters that need to be addressed before this manuscript can be considered for publication in PLoS One. The authors may want to seek help with grammatical editing. Given that PLoS One does not provide any editorial service after acceptance at minimum the authors should address the grammatical concerns raised in the annotated pdf. These include 1. the replacement of the term 'shady' with 'shaded' as well as 2. the inclusion of 'that' before 'landed' on many occasions. 3. In addition, the authors should use their abbreviations (i.e. Tair, Tbarrel, ΔTbarrel-Tair) consistently after once brielfly introducing them at first mention. Please find a few additional comments that require addressing in your revision in the annotated pdf attached. ============================== We would appreciate receiving your revised manuscript by May 31 2020 11:59PM. When you are ready to submit your revision, log on to https://www.editorialmanager.com/pone/ and select the 'Submissions Needing Revision' folder to locate your manuscript file. If you would like to make changes to your financial disclosure, please include your updated statement in your cover letter. To enhance the reproducibility of your results, we recommend that if applicable you deposit your laboratory protocols in protocols.io, where a protocol can be assigned its own identifier (DOI) such that it can be cited independently in the future. For instructions see: http://journals.plos.org/plosone/s/submission-guidelines#loc-laboratory-protocols Please include the following items when submitting your revised manuscript: A rebuttal letter that responds to each point raised by the academic editor and reviewer(s). This letter should be uploaded as separate file and labeled 'Response to Reviewers'. A marked-up copy of your manuscript that highlights changes made to the original version. This file should be uploaded as separate file and labeled 'Revised Manuscript with Track Changes'. An unmarked version of your revised paper without tracked changes. This file should be uploaded as separate file and labeled 'Manuscript'. Please note while forming your response, if your article is accepted, you may have the opportunity to make the peer review history publicly available. The record will include editor decision letters (with reviews) and your responses to reviewer comments. If eligible, we will contact you to opt in or out. We look forward to receiving your revised manuscript. Kind regards, Heike Lutermann, PhD Academic Editor PLOS ONE [Note: HTML markup is below. Please do not edit.] Reviewers' comments: Reviewer's Responses to Questions Comments to the Author 1. If the authors have adequately addressed your comments raised in a previous round of review and you feel that this manuscript is now acceptable for publication, you may indicate that here to bypass the “Comments to the Author” section, enter your conflict of interest statement in the “Confidential to Editor” section, and submit your "Accept" recommendation. Reviewer #2: All comments have been addressed Reviewer #3: All comments have been addressed ********** 2. Is the manuscript technically sound, and do the data support the conclusions? The manuscript must describe a technically sound piece of scientific research with data that supports the conclusions. Experiments must have been conducted rigorously, with appropriate controls, replication, and sample sizes. The conclusions must be drawn appropriately based on the data presented. Reviewer #2: Yes Reviewer #3: Yes ********** 3. Has the statistical analysis been performed appropriately and rigorously? Reviewer #2: Yes Reviewer #3: Yes ********** 4. Have the authors made all data underlying the findings in their manuscript fully available? The PLOS Data policy requires authors to make all data underlying the findings described in their manuscript fully available without restriction, with rare exception (please refer to the Data Availability Statement in the manuscript PDF file). The data should be provided as part of the manuscript or its supporting information, or deposited to a public repository. For example, in addition to summary statistics, the data points behind means, medians and variance measures should be available. If there are restrictions on publicly sharing data—e.g. participant privacy or use of data from a third party—those must be specified. Reviewer #2: Yes Reviewer #3: Yes ********** 5. Is the manuscript presented in an intelligible fashion and written in standard English? PLOS ONE does not copyedit accepted manuscripts, so the language in submitted articles must be clear, correct, and unambiguous. Any typographical or grammatical errors should be corrected at revision, so please note any specific errors here. Reviewer #2: Yes Reviewer #3: Yes ********** 6. Review Comments to the Author Please use the space provided to explain your answers to the questions above. You may also include additional comments for the author, including concerns about dual publication, research ethics, or publication ethics. (Please upload your review as an attachment if it exceeds 20,000 characters) Reviewer #2: Dear Editor the authors have adressed all the comments of the three referees. The manuscript is now suitable for publication. Sincerely, Reviewer #3: All my comments in review round 1 have been adequately addressed hence, in my opinion, the manuscript in this new version deserves pubblication on PLOS ONE ********** 7. PLOS authors have the option to publish the peer review history of their article (what does this mean?). If published, this will include your full peer review and any attached files. If you choose “no”, your identity will remain anonymous but your review may still be made public. Do you want your identity to be public for this peer review? For information about this choice, including consent withdrawal, please see our Privacy Policy. Reviewer #2: No Reviewer #3: No [NOTE: If reviewer comments were submitted as an attachment file, they will be attached to this email and accessible via the submission site. Please log into your account, locate the manuscript record, and check for the action link "View Attachments". If this link does not appear, there are no attachment files to be viewed.] While revising your submission, please upload your figure files to the Preflight Analysis and Conversion Engine (PACE) digital diagnostic tool, https://pacev2.apexcovantage.com/. PACE helps ensure that figures meet PLOS requirements. To use PACE, you must first register as a user. Registration is free. Then, login and navigate to the UPLOAD tab, where you will find detailed instructions on how to use the tool. If you encounter any issues or have any questions when using PACE, please email us at figures@plos.org. Please note that Supporting Information files do not need this step. Submitted filename: PONE-D-20-04024_R1 editor feedback.pdf Click here for additional data file. 22 Apr 2020 Our response is uploaded as a separate file. Submitted filename: +PONE-D-20-04024-R2_response.doc Click here for additional data file. 28 Apr 2020 Why Do Biting Horseflies Prefer Warmer Hosts? Tabanids can Escape Easier from Warmer Targets PONE-D-20-04024R2 Dear Dr. Horvath, We are pleased to inform you that your manuscript has been judged scientifically suitable for publication and will be formally accepted for publication once it complies with all outstanding technical requirements. Within one week, you will receive an e-mail containing information on the amendments required prior to publication. When all required modifications have been addressed, you will receive a formal acceptance letter and your manuscript will proceed to our production department and be scheduled for publication. Shortly after the formal acceptance letter is sent, an invoice for payment will follow. To ensure an efficient production and billing process, please log into Editorial Manager at https://www.editorialmanager.com/pone/, click the "Update My Information" link at the top of the page, and update your user information. If you have any billing related questions, please contact our Author Billing department directly at authorbilling@plos.org. If your institution or institutions have a press office, please notify them about your upcoming paper to enable them to help maximize its impact. If they will be preparing press materials for this manuscript, you must inform our press team as soon as possible and no later than 48 hours after receiving the formal acceptance. Your manuscript will remain under strict press embargo until 2 pm Eastern Time on the date of publication. For more information, please contact onepress@plos.org. With kind regards, Heike Lutermann, PhD Academic Editor PLOS ONE Additional Editor Comments (optional): Reviewers' comments: 30 Apr 2020 PONE-D-20-04024R2 Why Do Biting Horseflies Prefer Warmer Hosts? Tabanids can Escape Easier from Warmer Targets Dear Dr. Horváth: I am pleased to inform you that your manuscript has been deemed suitable for publication in PLOS ONE. Congratulations! Your manuscript is now with our production department. If your institution or institutions have a press office, please notify them about your upcoming paper at this point, to enable them to help maximize its impact. If they will be preparing press materials for this manuscript, please inform our press team within the next 48 hours. Your manuscript will remain under strict press embargo until 2 pm Eastern Time on the date of publication. For more information please contact onepress@plos.org. For any other questions or concerns, please email plosone@plos.org. Thank you for submitting your work to PLOS ONE. With kind regards, PLOS ONE Editorial Office Staff on behalf of Dr Heike Lutermann Academic Editor PLOS ONE
  16 in total

1.  Polarotactic tabanids find striped patterns with brightness and/or polarization modulation least attractive: an advantage of zebra stripes.

Authors:  Adám Egri; Miklós Blahó; György Kriska; Róbert Farkas; Mónika Gyurkovszky; Susanne Akesson; Gábor Horváth
Journal:  J Exp Biol       Date:  2012-03-01       Impact factor: 3.312

2.  A horizontally polarizing liquid trap enhances the tabanid-capturing efficiency of the classic canopy trap.

Authors:  Á Egri; M Blahó; D Száz; G Kriska; J Majer; T Herczeg; M Gyurkovszky; R Farkas; G Horváth
Journal:  Bull Entomol Res       Date:  2013-06-28       Impact factor: 1.750

3.  Thermographic measurements of the surface temperatures of animals.

Authors:  K Cena; J A Clark
Journal:  J Mammal       Date:  1973-11       Impact factor: 2.416

4.  An unexpected advantage of whiteness in horses: the most horsefly-proof horse has a depolarizing white coat.

Authors:  Gábor Horváth; Miklós Blahó; György Kriska; Ramón Hegedüs; Balázs Gerics; Róbert Farkas; Susanne Akesson
Journal:  Proc Biol Sci       Date:  2010-02-03       Impact factor: 5.349

5.  Seasonality and daily activity of male and female tabanid flies monitored in a Hungarian hill-country pasture by new polarization traps and traditional canopy traps.

Authors:  Tamás Herczeg; Miklós Blahó; Dénes Száz; György Kriska; Mónika Gyurkovszky; Róbert Farkas; Gábor Horváth
Journal:  Parasitol Res       Date:  2014-09-06       Impact factor: 2.289

6.  Spottier targets are less attractive to tabanid flies: on the tabanid-repellency of spotty fur patterns.

Authors:  Miklos Blaho; Adam Egri; Lea Bahidszki; Gyorgy Kriska; Ramon Hegedus; Susanne Akesson; Gabor Horvath
Journal:  PLoS One       Date:  2012-08-02       Impact factor: 3.240

7.  Efficiency of colored modified box traps for sampling of tabanids.

Authors:  Stjepan Krčmar; Vanja Radolić; Petar Lajoš; Igor Lukačević
Journal:  Parasite       Date:  2014-12-17       Impact factor: 3.000

8.  Why do horseflies need polarization vision for host detection? Polarization helps tabanid flies to select sunlit dark host animals from the dark patches of the visual environment.

Authors:  Gábor Horváth; Tamás Szörényi; Ádám Pereszlényi; Balázs Gerics; Ramón Hegedüs; András Barta; Susanne Åkesson
Journal:  R Soc Open Sci       Date:  2017-11-08       Impact factor: 2.963

9.  Experimental evidence that stripes do not cool zebras.

Authors:  Gábor Horváth; Ádám Pereszlényi; Dénes Száz; András Barta; Imre M Jánosi; Balázs Gerics; Susanne Åkesson
Journal:  Sci Rep       Date:  2018-06-19       Impact factor: 4.379

10.  Attractiveness of thermally different, uniformly black targets to horseflies: Tabanus tergestinus prefers sunlit warm shiny dark targets.

Authors:  Gábor Horváth; Ádám Pereszlényi; Tímea Tóth; Szabolcs Polgár; Imre M Jánosi
Journal:  R Soc Open Sci       Date:  2019-10-23       Impact factor: 2.963

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  2 in total

1.  Sunlit zebra stripes may confuse the thermal perception of blood vessels causing the visual unattractiveness of zebras to horseflies.

Authors:  Péter Takács; Dénes Száz; Miklós Vincze; Judit Slíz-Balogh; Gábor Horváth
Journal:  Sci Rep       Date:  2022-08-04       Impact factor: 4.996

2.  A new argument against cooling by convective air eddies formed above sunlit zebra stripes.

Authors:  Ádám Pereszlényi; Dénes Száz; Imre M Jánosi; Gábor Horváth
Journal:  Sci Rep       Date:  2021-08-04       Impact factor: 4.379

  2 in total

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