Find research datasets worth reusing

opencc-by-4.0Nov 2004View details →

Figs 8–13. 8–12 in New Species Of Cynipid Gall Wasps From Iran And Turkey (Hymenoptera: Cynipidae: Cynipini)

Figs 8–13. 8–12 = Andricus lucidus, asexual female: 8 = head, front view, 9 = head, posterior view, 10 = antenna, 11 = fore wing, 12 = metanotum and propodeum, dorsal view. 13 = A. megalucidus,

opencc-by-4.0Nov 2004View details →

Fig. 31 in New Species Of Cynipid Gall Wasps From Iran And Turkey (Hymenoptera: Cynipidae: Cynipini)

Fig. 31. Aphelonyx persica galls on Q. brantii. The white scale bar is 10 mm long (photo by G. STONE)

Latitudinal Asymmetry in the Dayside Atmosphere of WASP-43b

This repository contains data inputs and analysis products for the manuscript "Latitudinal Asymmetry in the Dayside Atmosphere of WASP-43b" (Challener et al., 2024) accepted for publication in The Astrophysical Journal Letters. The archive contains a README with further description of the included files and an example of how to make use of them. If you make use of these data in your work, please cite our paper: <a href="https://ui.adsabs.harvard.edu/abs/2024arXiv240610207C/abstract">https://ui.adsabs.harvard.edu/abs/2024arXiv240610207C/abstract</a>

Associated data for "The Roasting Marshmallows Program with IGRINS on Gemini South II -- WASP-121 b has super-stellar C/O and refractory-to-volatile ratios" Published in The Astronomical Journal

<table> <tbody> <tr> <td>File Name</td> <td>Description</td> </tr> <tr> <td>w121_1DRC_H2O_ONLY.txt</td> <td>Self consistent, solar composition model spectrum with only H2O opacity.</td> </tr> <tr> <td>w121_1DRC_OH_ONLY.txt</td> <td>Self consistent, solar composition model spectrum with only OH opacity.</td> </tr> <tr> <td>w121_1DRC_CO_ONLY.txt</td> <td>Self consistent, solar composition model spectrum with only CO opacity.</td> </tr> <tr> <td>w121_1DRC_EVERYTHING.txt</td> <td>Self consistent, solar composition model spectrum with all sources of opacity.</td> </tr> <tr> <td>pre_.pic</td> <td>Pre-eclipse data in data cuboid of shape N_order, N_frame, N_pixel</td> </tr> <tr> <td>pre_variance.pic</td> <td>Associated per-pixel variance for the pre-eclipse data.</td> </tr> <tr> <td>post_cube.pic</td> <td>Post-eclipse data in data cuboid of shape N_order, N_frame, N_pixel</td> </tr> <tr> <td>pre_time_BJD.pic</td> <td>Average frame time in BJD for the pre-eclipse sequence.</td> </tr> <tr> <td>pre_rvel.pic</td> <td>Stellar radial velocity, including barycentric correction, per frame for the pre-eclipse sequence.</td> </tr> <tr> <td>post_ph.pic</td> <td>Orbital phase per frame for the post-eclipse sequence.</td> </tr> <tr> <td>post_time_BJD.pic</td> <td>Average frame time in BJD for the post-eclipse sequence.</td> </tr> <tr> <td>post_rvel.pic</td> <td>Stellar radial velocity, including barycentric correction, per frame for the post-eclipse sequence</td> </tr> </tbody> </table>

opencc-by-4.0Mar 2017View details →

FIGURE 3 in Trap-nesting bees and wasps (Hymenoptera, Aculeata) in a Semidecidual Seasonal Forest fragment, southern Brazil

FIGURE 3: Phenology of most common trap-nesting Aculeata in Parque Estadual São Camilo (Palotina, Paraná), (A) from September 2014 to March 2014, (B) from October 2014 to March 2015.

opencc-by-4.0Mar 2017View details →

FIGURE 2 in Trap-nesting bees and wasps (Hymenoptera, Aculeata) in a Semidecidual Seasonal Forest fragment, southern Brazil

FIGURE 2: Trap nests in Parque Estadual São Camilo (Palotina, Paraná), (A) Centris analis, (B) Megachile susurrans, (C) Monobia angulosa, (D) Pachodynerus grandis, (E) Pachodynerus guadulpensis, (F) Zethus smithii. Scale bars: 1 cm.

CRIRES+ reduced spectroscopic observations of WASP-178

<h1>Reduced CRIRES+ spectroscopy observations of WASP-178 from 2023-05-25</h1> This records contains the reduced data as used in the publication of Cont et al. 2024 "Exploring the ultra-hot Jupiter WASP-178b. Constraints on atmospheric chemistry and dynamics from a joint retrieval of VLT/CRIRES+ and space photometric data" currently in press with Astronomy & Astrophysics and available as preprint on arXiv. Links to the publication: <ol> <li>ADS: <a href="https://ui.adsabs.harvard.edu/abs/2024arXiv240608166C/abstract">https://ui.adsabs.harvard.edu/abs/2024arXiv240608166C/abstract</a></li> <li>arXiv: <a href="https://arxiv.org/abs/2406.08166">https://arxiv.org/abs/2406.08166</a></li> </ol> The raw data from the CRIRES+ instrument were reduced using the instrument pipeline and the reduction steps are described in the article (see Section 3). <h2>Acknowledgements</h2> If you make use of this data in your research, please cite the Cont et al. 2024 article and this record with its DOI (10.5281/zenodo.11637332) and its reference, the bibtex reference is: <pre><code>@dataset{lavail_2024_11637332, author = {Lavail, Alexis}, title = {{CRIRES+ reduced spectroscopic observations of WASP-178}}, month = jun, year = 2024, publisher = {Zenodo}, version = {1.0}, doi = {10.5281/zenodo.11637332}, url = {https://doi.org/10.5281/zenodo.11637332} }</code></pre>  Note also that ESO requests an acknowledgement, which in this case would be: "Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 111.254J". This data is released under a Creative Commons Attribution 4.0 International license. <h2>Format of the data</h2> The data are contained in a pickle file. Instructions on how to read pickle files can be found on the python wiki at <a href="https://wiki.python.org/moin/UsingPickle">https://wiki.python.org/moin/UsingPickle</a>: <pre><code>import pickle data = pickle.load(open('wasp178-230524.pickle', 'rb'))</code></pre> The data consists of a dictionary, the keys can be explored with the following command: <pre><code>print(data.keys())</code></pre> The keys are the following: <ul> <li>script_version</li> <li>nodpos</li> <li>rawfilename</li> <li>nodpair</li> <li>wave</li> <li>wave_model</li> <li>spec</li> <li>err</li> <li>snr</li> <li>airmass</li> <li>bjd_tdb</li> <li>berv</li> <li>orders</li> <li>rawheaders</li> <li>slitfunctionFWHM-det1</li> <li>slitfunctionFWHM-det2</li> <li>slitfunctionFWHM-det3</li> </ul> The keys in boldface (wave, spec, err) contain the reduced data, respectively the wavelength (expressed in vacuum in nanometres), the extracted spectrum (in ADU), and the error spectrum (in ADU). The other keys contain metadata and supplementary information as explained below. Each key contains either a numPy array or a string ("script_version") . The shape of the arrays can be expressed using three sizes: <ol> <li>n_obs = 52: the number of observations in the dataset</li> <li>n_pix = 2008: the number of pixels in each segment</li> <li>n_orders  = 21: the numbers of segment (each spectral order is split over three detectors creating three segments)</li> </ol> The size of each array can be investigated with e.g <pre><code>for key in data.keys(): try: print(key,':', data[key].shape) except: print(key) </code> which results in</pre> <pre><code>script_version nodpos : (52,) rawfilename : (52,) nodpair : (52,) wave : (21, 52, 2008) wave_model : (21, 52, 2008) spec : (21, 52, 2008) err : (21, 52, 2008) snr : (21, 52) airmass : (52,) bjd_tdb : (52,) berv : (52,) orders : (21,) rawheaders : (52, 2484, 3) slitfunctionFWHM-det1 : (52, 8, 3) slitfunctionFWHM-det2 : (52, 8, 3) slitfunctionFWHM-det3 : (52, 8, 3) </code></pre> <h2>What's in the data?</h2> <ul> <li>script_version: version number of the python script used to produce the data</li> <li>nodpos: string, ('A' or 'B') the nodding position of the observation</li> <li>rawfilename: string, the filename of the raw science file from the ESO archive </li> <li>nodpair: string, ('pairNN') where NN is the number of nodding pair used in the data reduction: science files are reduced in pair with one nodding 'A' spectrum and one 'B'</li> <li>wave: array containing the pipeline-derived wavelength solution for the spectrum in nanometers in vacuum </li> <li>wave_model: refined and more precise wavelength solution using molecfit fitting the telluric spectrum as explained in Sect. 2.1 of the paper</li> <li>spec: reduced spectrum in ADU from the CRIRES+ pipeline. The spectra have been divided by the blaze spectrum (extracted spectrum from the flat-field lamp) to rectify the shape of the continuum and simplify spectrum, normalization </li> <li>err: the error spectrum in ADU corresponding to the spec (signal to noise ration can be computed using spec/err) </li> <li>snr: median signal to noise ratio for each segment/observation</li> <li>airmass: airmass for each observation taken from the raw file header (mean of airmass at start and end of each exposure)</li> <li>bjd_tdb: bjd_tdb (barycentric julian date expressed in temps dynamique barycentrique) time at the middle of the exposure computed with barycorrpy (<a href="https://github.com/shbhuk/barycorrpy">https://github.com/shbhuk/barycorrpy</a>)</li> <li>berv: berv correction at middle of exposure computed with barycorrpy</li> <li>orders: string (D-OO) identifying the segment where D is the detector number (1-3) and OO is the order number (02-08)</li> <li>rawheaders: the fits header from the raw science files</li> <li>slitfunctionFWHM-det1: contains information on the FWHM of the slit function taken from the reduced file headers for the orders of detector 1</li> <li>slitfunctionFWHM-det2: same for detector 2</li> <li>slitfunctionFWHM-det3: same for detector 3</li> </ul>

FIGURE 1 in Redescription and phylogenetic placement of the Cretaceous wasp Parviformosus wohlrabeae (Hymenoptera: Proctotrupomorpha)

FIGURE 1. Scanning electron microscopic images of Parviformosus wohlrabeae Barling et al., 2013. (1) Complete habitus. (2) Mesosoma. (3) Metasoma excluding ovipositor. (4) Ovipositor (arrow) engulfed in mineral ridge. (5) Metasoma, broken posterior tip with individual layers of Mt7 and Mt8 (arrow) visible. (6) Anterolateral view of mesosoma, head to right, dashed line marks posterior margin of pronotum. Scales (1) 1 mm; (2, 3) 0.1 mm; (4–6) 0.02 mm. Abbreviations: msc = mesoscutum, Mt6/7 = metasomal tergite 6/7, no1 = pronotum, pl2 = mesopleuron.

FIGURE 3 in Redescription and phylogenetic placement of the Cretaceous wasp Parviformosus wohlrabeae (Hymenoptera: Proctotrupomorpha)

FIGURE 3. Parviformosus wohlrabeae, habitus, lateral view; Abbreviations: le = left eye, lfe3? = probable left metafemur, lti2/3 = left meso- or metatibia, man = mandible, mc = median carina, msc = mesoscutum, Mt = metasomal tergite, no1 = pronotum, no3 = metanotum, not = notaulus, ovp = ovipositor, pl2 = mesopleuron, ppd = propodeum, rcx1 = right procoxa, rcx3 = right metacoxa, rfe3 = right metafemur, rfw? = probably remnant of right forewing, rtro3 = right metatrochanter, sct = mesoscutellum, spr = spiracle, wa = wing articulation, wf = wing fragment; Scale: 1 mm.

FIGURE 2 in Redescription and phylogenetic placement of the Cretaceous wasp Parviformosus wohlrabeae (Hymenoptera: Proctotrupomorpha)

FIGURE 2. Scanning electron microscopic images of the mesosoma of Parviformosus wohlrabeae. (1) Posterior part of mesosoma with potential forewing fragment (arrow), right lateral view. (2–4) Metanotum and propodeum, (2) dorsal view, arrow indicates metanotum submedially overlapping propodeum; (3) left dorsolateral view; (4) right dorsolateral view. Scales (1–3) 0.1 mm; (4) 0.05 mm. Abbreviations: lti2/3 = left meso- or metatibia, no3 = metanotum, ppd = propodeum, rfe3 = right metafemur, rfw? = probably remnant of right forewing, scta = mesoscutellar arm, spr = spiracle, wf = wing fragment.

Products and Models for "A benchmark JWST near-infrared spectrum for the exoplanet WASP-39 b"

Publication Here: https://www.nature.com/articles/s41550-024-02292-x Observing exoplanets through transmission spectroscopy supplies detailed information on their atmospheric composition, physics, and chemistry. Prior to JWST, these observations were limited to a narrow wavelength range across the near-ultraviolet to near-infrared, alongside broadband photometry at longer wavelengths. To understand more complex properties of exoplanet atmospheres, improved wavelength coverage and resolution are necessary to robustly quantify the influence of a broader range of absorbing molecular species. Here we show a combined analysis of JWST transmission spectroscopy across four different instrumental modes spanning 0.5–5.2 micron using Early Release Science observations of the Saturn-mass exoplanet WASP-39b. Our uniform analysis constrains the orbital and stellar parameters within sub-percent precision, including matching the precision obtained by the most precise asteroseismology measurements of stellar density to-date. Leveraging the advantages of a uniform light curve analysis, we improve the agreement between the transmission spectra of all modes, except for the NIRSpec PRISM, which is affected by partial saturation of the detector.  Together, these collected data constitute the most comprehensive transmission spectrum of an exoplanet to date, providing unparalleled access to atmospheric absorbers including Na, K, H2O, CO, CO2, and SO2.

Figure B1 in †Cretolixon - a remarkable new genus of rhopalosomatid wasps (Hymenoptera: Vespoidea: Rhopalosomatidae) from chemically tested, mid-Cretaceous Burmese (Kachin) amber supports the monophyly of Rhopalosomatinae

Figure B1. Molecules identified in the pyrolysates of Burmese amber. Individual compounds are labeled according to the identification of peaks in Figs. 1 and B2 and Table A1.

Figure B2 in †Cretolixon - a remarkable new genus of rhopalosomatid wasps (Hymenoptera: Vespoidea: Rhopalosomatidae) from chemically tested, mid-Cretaceous Burmese (Kachin) amber supports the monophyly of Rhopalosomatinae

Figure B2. Total ion chromatograms from the THM–GC–MS analysis of Burmese ambers. Numbered peaks refer to identified compounds in Table A1 and Fig. B1.

Figure 10 in †Cretolixon - a remarkable new genus of rhopalosomatid wasps (Hymenoptera: Vespoidea: Rhopalosomatidae) from chemically tested, mid-Cretaceous Burmese (Kachin) amber supports the monophyly of Rhopalosomatinae

Figure 10. Distribution of the discussed characters among Rhopalosomatidae. The tree topology of the recent genera is based on Brothers and Carpenter (1993), Brothers (1999) (both: "rhopalosomatids" sister to Olixon), Guidotti (1999), and unpublished molecular data (Blaschke et al., unpublished results) (both: Olixon + (Liosphex + (Rhopalosoma + Paniscomima))).

Figure 8 in †Cretolixon - a remarkable new genus of rhopalosomatid wasps (Hymenoptera: Vespoidea: Rhopalosomatidae) from chemically tested, mid-Cretaceous Burmese (Kachin) amber supports the monophyly of Rhopalosomatinae

Figure 8. Cretolixon alatum gen. et sp. nov., female, paratype (VL-Bu-04; UMB). (a) Basal half of left antenna. (b) Details of mouth parts (maxillary palpus highlighted in grey). (c) Details of mouth parts (labial palpus highlighted in grey). Abbreviations: FI, FII, FIII – flagellomere 1, flagellomere 2, flagellomere 3; G – gena; lp1,..., lp4 – labial palpomere 1,..., labial palpomere 4; M – mandible; mp2,..., mp6 – maxillary palpomere 2,..., maxillary palpomere 6; p – pedicel; sc – scape. Drawings based on Fig. 5b.

Figure 9 in †Cretolixon - a remarkable new genus of rhopalosomatid wasps (Hymenoptera: Vespoidea: Rhopalosomatidae) from chemically tested, mid-Cretaceous Burmese (Kachin) amber supports the monophyly of Rhopalosomatinae

Figure 9. Some characters of Rhopalosomatidae. (a) Rhopalosomatidae, gen. et sp. indet., Burmese (Kachin) amber (ZMB; MB.I 6501), basal section of hind wing. (b) Liosphex boreus Lohrmann (in Lohrmann and Ohl, 2010), basal section of hind wing. (c) Rhopalosoma nearcticum Brues, 1943, basal section of hind wing. (d) Olixon banksii (Brues, 1922), mouthparts. (e) Liosphex longicornis Lohrmann (in Lohrmann and Ohl, 2010), mouthparts. (f) Paniscomima kilombero Lohrmann, 2011, mouthparts. (g) Paniscomima opposita Guidotti, 2007, male, paratype, head in dorsal view. (h) Paniscomima seyrigi (Berland, 1951), female, head in dorsal view. (i) Liosphex varius Townes, 1977, female, holotype, head in dorsal view. Abbreviations: ab – apical bristle; lp1,..., lp4 – labial palpomere 1,..., labial palpomere 4; mp1,..., mp6 – maxillary palpomere 1,..., maxillary palpomere 6. Panel (i) is reproduced with permission from copyright holder and was first published in Zootaxa (Lohrmann and Ohl, 2010); photo by David Wahl.

Figure 7 in †Cretolixon - a remarkable new genus of rhopalosomatid wasps (Hymenoptera: Vespoidea: Rhopalosomatidae) from chemically tested, mid-Cretaceous Burmese (Kachin) amber supports the monophyly of Rhopalosomatinae

Figure 7. Cretolixon alatum gen. et sp. nov., male, holotype (MB.I 6500; ZMB). Venation of fore and hind wings (microtrichia omitted, drawing based on a photograph with a perspective similar to that of Fig. 4e).

Figure 4 in †Cretolixon - a remarkable new genus of rhopalosomatid wasps (Hymenoptera: Vespoidea: Rhopalosomatidae) from chemically tested, mid-Cretaceous Burmese (Kachin) amber supports the monophyly of Rhopalosomatinae

Figure 4. Cretolixon alatum gen. et sp. nov., male, holotype (MB.I 6500; ZMB). (a) Habitus in lateral view. (b) Head in slightly oblique frontal view. (c) Mesosoma in lateral view. (d) Partial right antenna. (e) Wings. Abbreviations: ab – apical bristle; FI, FII, FIII – flagellomere 1, flagellomere 2, flagellomere 3; lo – lateral ocellus; oc – occipital carina; p – pedicel; sc – scape. The arrowheads indicate the apical bristles on third maxillary palpomeres (c) and basal flagellomeres (d).

Figure 5 in †Cretolixon - a remarkable new genus of rhopalosomatid wasps (Hymenoptera: Vespoidea: Rhopalosomatidae) from chemically tested, mid-Cretaceous Burmese (Kachin) amber supports the monophyly of Rhopalosomatinae

Figure 5. Cretolixon alatum gen. et sp. nov., female, paratype (VL-Bu-04, UMB). (a) Habitus in lateral view. (b) Head and basal halves of antennae in oblique lateral view. (c) Mesosoma in lateral view. (d) Right protibia and protarsus. (e) Wings. The arrowheads indicate the apical bristles on second labial and third maxillary palpomeres (b).

Figure 1 in †Cretolixon - a remarkable new genus of rhopalosomatid wasps (Hymenoptera: Vespoidea: Rhopalosomatidae) from chemically tested, mid-Cretaceous Burmese (Kachin) amber supports the monophyly of Rhopalosomatinae

Figure 1. Total ion chromatogram from the THM–GC–MS analysis of the Burmese amber MB.I 6500. Numbered peaks refer to identified compounds in Table A1 and Fig. B1.