3,275 results on '"Bradshaw J"'
Search Results
2. The ASAS-SN Bright Supernova Catalog -- V. 2018-2020
- Author
-
Neumann, K. D., Holoien, T. W. -S., Kochanek, C. S., Stanek, K. Z., Vallely, P. J., Shappee, B. J., Prieto, J. L., Pessi, T., Jayasinghe, T., Brimacombe, J., Bersier, D., Aydi, E., Basinger, C., Beacom, J. F., Bose, S., Brown, J. S., Chen, P., Clocchiatti, A., Desai, D. D., Dong, Subo, Falco, E., Holmbo, S., Morrell, N., Shields, J. V., Sokolovsky, K. V., Strader, J., Stritzinger, M. D., Swihart, S., Thompson, T. A., Way, Z., Aslan, L., Bishop, D. W., Bock, G., Bradshaw, J., Cacella, P., Castro-Morales, N., Conseil, E., Cornect, R., Cruz, I., Farfan, R. G., Fernandez, J. M., Gabuya, A., Gonzalez-Carballo, J. -L., Kendurkar, M. R., Kiyota, S., Koff, R. A., Krannich, G., Marples, P., Masi, G., Monard, L. A. G., Muñoz, J. A., Nicholls, B., Post, R. S., Pujic, Z., Stone, G., Tomasella, L., Trappett, D. L., and Wiethoff, W. S.
- Subjects
Astrophysics - High Energy Astrophysical Phenomena - Abstract
We catalog the 443 bright supernovae discovered by the All-Sky Automated Survey for Supernovae (ASAS-SN) in $2018-2020$ along with the 519 supernovae recovered by ASAS-SN and 516 additional $m_{peak}\leq18$ mag supernovae missed by ASAS-SN. Our statistical analysis focuses primarily on the 984 supernovae discovered or recovered in ASAS-SN $g$-band observations. The complete sample of 2427 ASAS-SN supernovae includes earlier $V$-band samples and unrecovered supernovae. For each supernova, we identify the host galaxy, its UV to mid-IR photometry, and the offset of the supernova from the center of the host. Updated light curves, redshifts, classifications, and host galaxy identifications supersede earlier results. With the increase of the limiting magnitude to $g\leq18$ mag, the ASAS-SN sample is roughly complete up to $m_{peak}=16.7$ mag and is $90\%$ complete for $m_{peak}\leq17.0$ mag. This is an increase from the $V$-band sample where it was roughly complete up to $m_{peak}=16.2$ mag and $70\%$ complete for $m_{peak}\leq17.0$ mag., Comment: 14 pages, 7 figures, 4 tables. Updated to reflect changes made in the published version. Tables containing the catalog data presented in this submission are included in machine-readable format as ancillary files
- Published
- 2022
- Full Text
- View/download PDF
3. Stellar occultations enable milliarcsecond astrometry for Trans-Neptunian objects and Centaurs
- Author
-
Rommel, F. L., Braga-Ribas, F., Desmars, J., Camargo, J. I. B., Ortiz, J. L., Sicardy, B., Vieira-Martins, R., Assafin, M., Santos-Sanz, P., Duffard, R., Fernández-Valenzuela, E., Lecacheux, J., Morgado, B. E., Benedetti-Rossi, G., Gomes-Júnior, A. R., Pereira, C. L., Herald, D., Hanna, W., Bradshaw, J., Morales, N., Brimacombe, J., Burtovoi, A., Carruthers, T., de Barros, J. R., Fiori, M., Gilmore, A., Hooper, D., Hornoch, K., Jacques, C., Janik, T., Kerr, S., Kilmartin, P., Winkel, Jan Maarten, Naletto, G., Nardiello, D., Nascimbeni, V., Newman, J., Ossola, A., Pál, A., Pimentel, E., Pravec, P., Sposetti, S., Stechina, A., Szákats, R., Ueno, Y., Zampieri, L., Broughton, J., Dunham, J. B., Dunham, D. W., Gault, D., Hayamizu, T., Hosoi, K., Jehin, E., Jones, R., Kitazaki, K., Komžík, R., Marciniak, A., Maury, A., Mikuž, H., Nosworthy, P., Polleri, J. Fábrega, Rahvar, S., Sfair, R., Siqueira, P. B., Snodgrass, C., Sogorb, P., Tomioka, H., Tregloan-Reed, J., and Winter, O. C.
- Subjects
Astrophysics - Earth and Planetary Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
Trans-Neptunian objects (TNOs) and Centaurs are remnants of our planetary system formation, and their physical properties have invaluable information for evolutionary theories. Stellar occultation is a ground-based method for studying these small bodies and has presented exciting results. These observations can provide precise profiles of the involved body, allowing an accurate determination of its size and shape. The goal is to show that even single-chord detections of TNOs allow us to measure their milliarcsecond astrometric positions in the reference frame of the Gaia second data release (DR2). Accurated ephemerides can then be generated, allowing predictions of stellar occultations with much higher reliability. We analyzed data from stellar occultations to obtain astrometric positions of the involved bodies. The events published before the Gaia era were updated so that the Gaia DR2 catalog is the reference. Previously determined sizes were used to calculate the position of the object center and its corresponding error with respect to the detected chord and the International Celestial Reference System (ICRS) propagated Gaia DR2 star position. We derive 37 precise astrometric positions for 19 TNOs and 4 Centaurs. Twenty-one of these events are presented here for the first time. Although about 68\% of our results are based on single-chord detection, most have intrinsic precision at the submilliarcsecond level. Lower limits on the diameter and shape constraints for a few bodies are also presented as valuable byproducts. Using the Gaia DR2 catalog, we show that even a single detection of a stellar occultation allows improving the object ephemeris significantly, which in turn enables predicting a future stellar occultation with high accuracy. Observational campaigns can be efficiently organized with this help, and may provide a full physical characterization of the involved object., Comment: 16 pages, 28 figures. The manuscript was accepted and is to be published
- Published
- 2020
- Full Text
- View/download PDF
4. Crystal structure of 13,27-dichloro-29,30-dihydroxy-3,9,17,23-tetramethyl- 6,20-dioxa-3,9,17,23-tetraazatri-cyclo[23.3.1.111.15]triacontal( 29),11,13,15(30),25,27-hexaene-(aqua)magnesium hydrate, Mg[C28H40Cl2N4O4(H2O)] · H2O
- Author
-
Nazarenko A. Y., Dalley N. K., Bradshaw J. S., Pastushok V. N., and Lamb J. D.
- Subjects
Physics ,QC1-999 ,Crystallography ,QD901-999 - Published
- 2003
- Full Text
- View/download PDF
5. Preclinical Efficacy and Anti-Inflammatory Mechanisms of Action of the Bruton Tyrosine Kinase Inhibitor Rilzabrutinib for Immune-Mediated Disease.
- Author
-
Langrish, Claire L, Bradshaw, J Michael, Francesco, Michelle R, Owens, Timothy D, Xing, Yan, Shu, Jin, LaStant, Jacob, Bisconte, Angelina, Outerbridge, Catherine, White, Stephen D, Hill, Ronald J, Brameld, Ken A, Goldstein, David M, and Nunn, Philip A
- Subjects
Kidney ,Blood Platelets ,Basophils ,Mast Cells ,Animals ,Dogs ,Humans ,Mice ,Nephritis ,Purpura ,Thrombocytopenic ,Idiopathic ,Pemphigus ,Disease Models ,Animal ,Immunoglobulin E ,Anti-Inflammatory Agents ,Protein Kinase Inhibitors ,Drug Evaluation ,Preclinical ,Mice ,129 Strain ,Agammaglobulinaemia Tyrosine Kinase ,Autoimmune Disease ,5.1 Pharmaceuticals ,Development of treatments and therapeutic interventions ,Inflammatory and immune system ,Immunology - Abstract
Bruton tyrosine kinase (BTK) is expressed in B cells and innate immune cells, acting as an essential signaling element in multiple immune cell pathways. Selective BTK inhibition has the potential to target multiple immune-mediated disease pathways. Rilzabrutinib is an oral, reversible, covalent BTK inhibitor designed for immune-mediated diseases. We examined the pharmacodynamic profile of rilzabrutinib and its preclinical mechanisms of action. In addition to potent and selective BTK enzyme and cellular activity, rilzabrutinib inhibited activation and inflammatory activities of B cells and innate cells such as macrophages, basophils, mast cells, and neutrophils, without cell death (in human and rodent assay systems). Rilzabrutinib demonstrated dose-dependent improvement of clinical scores and joint pathology in a rat model of collagen-induced arthritis and demonstrated reductions in autoantibody-mediated FcγR signaling in vitro and in vivo, with blockade of rat Arthus reaction, kidney protection in mouse Ab-induced nephritis, and reduction in platelet loss in mouse immune thrombocytopenia. Additionally, rilzabrutinib inhibited IgE-mediated, FcεR-dependent immune mechanisms in human basophils and mast cell-dependent mouse models. In canines with naturally occurring pemphigus, rilzabrutinib treatment resulted in rapid clinical improvement demonstrated by anti-inflammatory effects visible within 2 wk and all animals proceeding to complete or substantial disease control. Rilzabrutinib is characterized by reversible covalent BTK binding, long BTK residence time with low systemic exposure, and multiple mechanistic and biological effects on immune cells. Rilzabrutinib's unique characteristics and promising efficacy and safety profile support clinical development of rilzabrutinib for a broad array of immune-mediated diseases.
- Published
- 2021
6. Author Correction: A dense ring of the trans-Neptunian object Quaoar outside its Roche limit
- Author
-
Morgado, B. E., Sicardy, B., Braga-Ribas, F., Ortiz, J. L., Salo, H., Vachier, F., Desmars, J., Pereira, C. L., Santos-Sanz, P., Sfair, R., de Santana, T., Assafin, M., Vieira-Martins, R., Gomes-Júnior, A. R., Margoti, G., Dhillon, V. S., Fernández-Valenzuela, E., Broughton, J., Bradshaw, J., Langersek, R., Benedetti-Rossi, G., Souami, D., Holler, B. J., Kretlow, M., Boufleur, R. C., Camargo, J. I. B., Duffard, R., Beisker, W., Morales, N., Lecacheux, J., Rommel, F. L., Herald, D., Benz, W., Jehin, E., Jankowsky, F., Marsh, T. R., Littlefair, S. P., Bruno, G., Pagano, I., Brandeker, A., Collier-Cameron, A., Florén, H. G., Hara, N., Olofsson, G., Wilson, T. G., Benkhaldoun, Z., Busuttil, R., Burdanov, A., Ferrais, M., Gault, D., Gillon, M., Hanna, W., Kerr, S., Kolb, U., Nosworthy, P., Sebastian, D., Snodgrass, C., Teng, J. P., and de Wit, J.
- Published
- 2024
- Full Text
- View/download PDF
7. A dense ring of the trans-Neptunian object Quaoar outside its Roche limit
- Author
-
Morgado, B. E., Sicardy, B., Braga-Ribas, F., Ortiz, J. L., Salo, H., Vachier, F., Desmars, J., Pereira, C. L., Santos-Sanz, P., Sfair, R., de Santana, T., Assafin, M., Vieira-Martins, R., Gomes-Júnior, A. R., Margoti, G., Dhillon, V. S., Fernández-Valenzuela, E., Broughton, J., Bradshaw, J., Langersek, R., Benedetti-Rossi, G., Souami, D., Holler, B. J., Kretlow, M., Boufleur, R. C., Camargo, J. I. B., Duffard, R., Beisker, W., Morales, N., Lecacheux, J., Rommel, F. L., Herald, D., Benz, W., Jehin, E., Jankowsky, F., Marsh, T. R., Littlefair, S. P., Bruno, G., Pagano, I., Brandeker, A., Collier-Cameron, A., Florén, H. G., Hara, N., Olofsson, G., Wilson, T. G., Benkhaldoun, Z., Busuttil, R., Burdanov, A., Ferrais, M., Gault, D., Gillon, M., Hanna, W., Kerr, S., Kolb, U., Nosworthy, P., Sebastian, D., Snodgrass, C., Teng, J. P., and de Wit, J.
- Published
- 2023
- Full Text
- View/download PDF
8. The collective impact of childhood abuse, psychache, and interpersonal needs on suicidal ideation among individuals with bipolar disorder: A discriminant analysis
- Author
-
Kapoor, S., Freitag, S., Bradshaw, J., Valencia, G.T., and Lamis, D.A.
- Published
- 2023
- Full Text
- View/download PDF
9. The Proteome‐Wide Potential for Reversible Covalency at Cysteine
- Author
-
Senkane, Kristine, Vinogradova, Ekaterina V, Suciu, Radu M, Crowley, Vincent M, Zaro, Balyn W, Bradshaw, J Michael, Brameld, Ken A, and Cravatt, Benjamin F
- Subjects
Biotechnology ,Development of treatments and therapeutic interventions ,5.1 Pharmaceuticals ,Generic health relevance ,Amino Acid Sequence ,Cysteine ,Gene Expression Regulation ,Enzymologic ,Phosphotransferases ,Proteome ,activity-based protein profiling ,proteomics ,reactive cysteines ,reversible covalency ,alpha-cyanoacrylamides ,α-cyanoacrylamides ,Chemical Sciences ,Organic Chemistry - Abstract
Reversible covalency, achieved with, for instance, highly electron-deficient olefins, offers a compelling strategy to design chemical probes and drugs that benefit from the sustained target engagement afforded by irreversible compounds, while avoiding permanent protein modification. Reversible covalency has mainly been evaluated for cysteine residues in individual kinases and the broader potential for this strategy to engage cysteines across the proteome remains unexplored. Herein, we describe a mass-spectrometry-based platform that integrates gel filtration with activity-based protein profiling to assess cysteine residues across the human proteome for both irreversible and reversible interactions with small-molecule electrophiles. Using this method, we identify numerous cysteine residues from diverse protein classes that are reversibly engaged by cyanoacrylamide fragment electrophiles, revealing the broad potential for reversible covalency as a strategy for chemical-probe discovery.
- Published
- 2019
10. The structure of Chariklo's rings from stellar occultations
- Author
-
Bérard, D., Sicardy, B., Camargo, J. I. B., Desmars, J., Braga-Ribas, F., Ortiz, J. L., Duffard, R., Morales, N., Meza, E., Leiva, R., Benedetti-Rossi, G., Vieira-Martins, R., Gomes-Júnior, A. R., Assafin, M., Colas, F., Dauvergne, J. L., Kervella, P., Lecacheux, J., Maquet, L., Vachier, F., Renner, S., Monard, B., Sickafoose, A. A., Breytenbach, H., Genade, A., Beisker, W., Bath, K. L., Bode, H. J., Backes, M., Ivanov, V. D., Jehin, E., Gillon, M., Manfroid, J., Pollock, J., Tancredi, G., Roland, S., Salvo, R., Vanzi, L., Herald, D., Gault, D., Kerr, S., Pavlov, H., Hill, K. M., Bradshaw, J., Barry, M. A., Cool, A., Lade, B., Cole, A., Broughton, J., Newman, J., Horvart, R., Maybour, D., Giles, D., Davis, L., Paton, R. A., Loader, B., Pennell, A., Jaquiery, P. D., Brillant, S., Selman, F., Dumas, C., Herrera, C., Carraro, G., Monaco, L., Maury, A., Peyrot, A., Teng-Chuen-Yu, J. P., Richichi, A., Irawati, P., De Witt, C., Schoenau, P., Prager, R., Colazo, C., Melia, R., Spagnotto, J., Blain, A., Alonso, S., Román, A, Santos-Sanz, P., Rizos, J. L., Maestre, J. L., and Dunham, D.
- Subjects
Astrophysics - Earth and Planetary Astrophysics - Abstract
Two narrow and dense rings (called C1R and C2R) were discovered around the Centaur object (10199) Chariklo during a stellar occultation observed on 2013 June 3. Following this discovery, we planned observations of several occultations by Chariklo's system in order to better characterize the physical properties of the ring and main body. Here, we use 12 successful occulations by Chariklo observed between 2014 and 2016. They provide ring profiles (physical width, opacity, edge structure) and constraints on the radii and pole position. Our new observations are currently consistent with the circular ring solution and pole position, to within the $\pm 3.3$ km formal uncertainty for the ring radii derived by Braga-Ribas et al. The six resolved C1R profiles reveal significant width variations from $\sim 5$ to 7.5 km. The width of the fainter ring C2R is less constrained, and may vary between 0.1 and 1 km. The inner and outer edges of C1R are consistent with infinitely sharp boundaries, with typical upper limits of one kilometer for the transition zone between the ring and empty space. No constraint on the sharpness of C2R's edges is available. A 1$\sigma$ upper limit of $\sim 20$ m is derived for the equivalent width of narrow (physical width <4 km) rings up to distances of 12,000 km, counted in the ring plane.
- Published
- 2017
- Full Text
- View/download PDF
11. Study of the plutino object (208996) 2003 AZ84 from stellar occultations: size, shape and topographic features
- Author
-
Dias-Oliveira, A., Sicardy, B., Ortiz, J. L., Braga-Ribas, F., Leiva, R., Vieira-Martins, R., Benedetti-Rossi, G., Camargo, J. I. B., Assafin, M., Gomes-Junior, A. R., Baug, T., Chandrasekhar, T., Desmars, J., Duffard, R., Santos-Sanz, P., Ergang, Z., Ganesh, S., Ikari, Y., Irawati, P., Jain, J., Liying, Z., Richichi, A., Shengbang, Q., Behrend, R., Benkhaldoun, Z., Brosch, N., Daassou, A., Frappa, E., Gal-Yam, A., Garcia-Lozano, R., Gillon, M., Jehin, E., Kaspi, S., Klotz, A., Lecacheux, J., Mahasena, P., Manfroid, J., Manulis, I., Maury, A., Mohan, V., Morales, N., Ofek, E., Rinner, C., Sharma, A., Sposetti, S., Tanga, P., Thirouin, A., Vachier, F., Widemann, T., Asai, A., Watanabe, Hayato, Watanabe, Hiroyuki, Owada, M., Yamamura, H., Hayamizu, T., Bradshaw, J., Kerr, S., Tomioka, H., Andersson, S., Dangl, G., Haymes, T., Naves, R., and Wortmann, G
- Subjects
Astrophysics - Earth and Planetary Astrophysics - Abstract
We present results derived from four stellar occultations by the plutino object (208996) 2003~AZ$_{84}$, detected at January 8, 2011 (single-chord event), February 3, 2012 (multi-chord), December 2, 2013 (single-chord) and November 15, 2014 (multi-chord). Our observations rule out an oblate spheroid solution for 2003~AZ$_{84}$'s shape. Instead, assuming hydrostatic equilibrium, we find that a Jacobi triaxial solution with semi axes $(470 \pm 20) \times (383 \pm 10) \times (245 \pm 8)$~km % axis ratios $b/a= 0.82 \pm 0.05$ and $c/a= 0.52 \pm 0.02$, can better account for all our occultation observations. Combining these dimensions with the rotation period of the body (6.75~h) and the amplitude of its rotation light curve, we derive a density $\rho=0.87 \pm 0.01$~g~cm$^{-3}$ a geometric albedo $p_V= 0.097 \pm 0.009$. A grazing chord observed during the 2014 occultation reveals a topographic feature along 2003~AZ$_{84}$'s limb, that can be interpreted as an abrupt chasm of width $\sim 23$~km and depth $> 8$~km or a smooth depression of width $\sim 80$~km and depth $\sim 13$~km (or an intermediate feature between those two extremes).
- Published
- 2017
- Full Text
- View/download PDF
12. PRN473, an inhibitor of Bruton's tyrosine kinase, inhibits neutrophil recruitment via inhibition of macrophage antigen‐1 signalling
- Author
-
Herter, Jan M, Margraf, Andreas, Volmering, Stephanie, Correia, Benedito Eduardo, Bradshaw, J Michael, Bisconte, Angelina, Hill, Ronald J, Langrish, Claire L, Lowell, Clifford A, and Zarbock, Alexander
- Subjects
Pharmacology and Pharmaceutical Sciences ,Biomedical and Clinical Sciences ,Digestive Diseases ,Liver Disease ,Underpinning research ,1.1 Normal biological development and functioning ,Inflammatory and immune system ,Agammaglobulinaemia Tyrosine Kinase ,Animals ,Chemical and Drug Induced Liver Injury ,Dose-Response Relationship ,Drug ,Macrophage-1 Antigen ,Mice ,Mice ,Inbred C57BL ,Mice ,Knockout ,Neutrophil Infiltration ,Neutrophils ,Protein Kinase Inhibitors ,Protein-Tyrosine Kinases ,Signal Transduction ,Pharmacology & Pharmacy ,Pharmacology and pharmaceutical sciences - Abstract
Background and purposeFollowing inflammatory stimuli, neutrophils are recruited to sites of inflammation and exert effector functions that often have deleterious effects on tissue integrity, which can lead to organ failure. Bruton's tyrosine kinase (Btk) is expressed in neutrophils and constitutes a promising pharmacological target for neutrophil-mediated tissue damage. Here, we evaluate a selective reversible inhibitor of Btk, PRN473, for its ability to dampen neutrophil influx via inhibition of adhesion receptor signalling pathways.Experimental approachIn vitro assays were used to assess fMLP receptor 1 (Fpr-1)-mediated binding of ligands to the adhesion receptors macrophage antigen-1 (Mac-1) and lymphocyte function antigen-1. Intravital microscopy of the murine cremaster was used to evaluate post-adhesion strengthening and endoluminal crawling. Finally, neutrophil influx was visualized in a clinically relevant model of sterile liver injury in vivo. Btk knockout animals were used as points of reference for Btk functions.Key resultsPharmacological inhibition of Btk by PRN473 reduced fMLP-induced phosphorylation of Btk and Mac-1 activation. Biochemical experiments demonstrated the specificity of the inhibitor. PRN473 (20 mg·kg-1 ) significantly reduced intravascular crawling and neutrophil recruitment into inflamed tissue in a model of sterile liver injury, down to levels seen in Btk-deficient animals. A higher dose did not provide additional reduction of intravascular crawling and neutrophil recruitment.Conclusions and implicationsPRN473, a highly selective inhibitor of Btk, potently attenuates sterile liver injury by inhibiting the activation of the β2 -integrin Mac-1 and subsequently neutrophil recruitment into inflamed tissue.
- Published
- 2018
13. Pluto's atmosphere from the 29 June 2015 ground-based stellar occultation at the time of the New Horizons flyby
- Author
-
Sicardy, B., Talbot, J., Meza, E., Camargo, J. I. B., Desmars, J., Gault, D., Herald, D., Kerr, S., Pavlov, H., Braga-Ribas, F., Assafin, M., Benedetti-Rossi, G., Dias-Oliveira, A., Ramos-Gomes-Jr., A., Vieira-Martins, R., Berard, D., Kervella, P., Lecacheux, J., Lellouch, E., Beisker, W., Dunham, D., Jelinek, M., Duffard, R., Ortiz, J. L., Castro-Tirado, A. J., Cunniffe, R., Querel, R., Yock, P. A., Cole, A. A., Giles, A. B., Hill, K. M., Beaulieu, J. P., Harnisch, M., Jansen, R., Pennell, A., Todd, S., Allen, W. H., Graham, P. B., Loader, B., McKay, G., Milner, J., Parker, S., Barry, M. A., Bradshaw, J., Broughton, J., Davis, L., Devillepoix, H., Drummond, J., Field, L., Forbes, M., Giles, D., Glassey, R., Groom, R., Hooper, D., Horvat, R., Hudson, G., Idaczyk, R., Jenke, D., Lade, B., Newman, J., Nosworthy, P., Purcell, P., Skilton, P. F., Streamer, M., Unwin, M., Watanabe, H., White, G. L., and Watson, D.
- Subjects
Astrophysics - Earth and Planetary Astrophysics - Abstract
We present results from a multi-chord Pluto stellar occultation observed on 29 June 2015 from New Zealand and Australia. This occurred only two weeks before the NASA New Horizons flyby of the Pluto system and serves as a useful comparison between ground-based and space results. We find that Pluto's atmosphere is still expanding, with a significant pressure increase of 5$\pm$2\% since 2013 and a factor of almost three since 1988. This trend rules out, as of today, an atmospheric collapse associated with Pluto's recession from the Sun. A central flash, a rare occurrence, was observed from several sites in New Zealand. The flash shape and amplitude are compatible with a spherical and transparent atmospheric layer of roughly 3~km in thickness whose base lies at about 4~km above Pluto's surface, and where an average thermal gradient of about 5 K~km$^{-1}$ prevails. We discuss the possibility that small departures between the observed and modeled flash are caused by local topographic features (mountains) along Pluto's limb that block the stellar light. Finally, using two possible temperature profiles, and extrapolating our pressure profile from our deepest accessible level down to the surface, we obtain a possible range of 11.9-13.7~$\mu$bar for the surface pressure., Comment: 16 pages, 2 tables, 3 figures
- Published
- 2016
- Full Text
- View/download PDF
14. Prolonged and tunable residence time using reversible covalent kinase inhibitors
- Author
-
Bradshaw, J Michael, McFarland, Jesse M, Paavilainen, Ville O, Bisconte, Angelina, Tam, Danny, Phan, Vernon T, Romanov, Sergei, Finkle, David, Shu, Jin, Patel, Vaishali, Ton, Tony, Li, Xiaoyan, Loughhead, David G, Nunn, Philip A, Karr, Dane E, Gerritsen, Mary E, Funk, Jens Oliver, Owens, Timothy D, Verner, Erik, Brameld, Ken A, Hill, Ronald J, Goldstein, David M, and Taunton, Jack
- Subjects
Acrylamides ,Agammaglobulinaemia Tyrosine Kinase ,Animals ,B-Lymphocytes ,Cell Line ,Tumor ,Crystallography ,X-Ray ,Cyanoacrylates ,Dasatinib ,Female ,Gene Expression ,Humans ,Ligands ,Molecular Docking Simulation ,Protein Kinase Inhibitors ,Protein Structure ,Tertiary ,Protein-Tyrosine Kinases ,Pyrimidines ,Rats ,Rats ,Sprague-Dawley ,Recombinant Proteins ,Sf9 Cells ,Spodoptera ,Structure-Activity Relationship ,Substrate Specificity ,Thiazoles ,Time Factors ,Medicinal and Biomolecular Chemistry ,Biochemistry and Cell Biology ,Biochemistry & Molecular Biology - Abstract
Drugs with prolonged on-target residence times often show superior efficacy, yet general strategies for optimizing drug-target residence time are lacking. Here we made progress toward this elusive goal by targeting a noncatalytic cysteine in Bruton's tyrosine kinase (BTK) with reversible covalent inhibitors. Using an inverted orientation of the cysteine-reactive cyanoacrylamide electrophile, we identified potent and selective BTK inhibitors that demonstrated biochemical residence times spanning from minutes to 7 d. An inverted cyanoacrylamide with prolonged residence time in vivo remained bound to BTK for more than 18 h after clearance from the circulation. The inverted cyanoacrylamide strategy was further used to discover fibroblast growth factor receptor (FGFR) kinase inhibitors with residence times of several days, demonstrating the generalizability of the approach. Targeting of noncatalytic cysteines with inverted cyanoacrylamides may serve as a broadly applicable platform that facilitates 'residence time by design', the ability to modulate and improve the duration of target engagement in vivo.
- Published
- 2015
15. Diagnosis and management of a ruptured 20-week anencephalic cornual ectopic pregnancy undergoing termination: implications of interstate travel due to restrictive abortion law
- Author
-
Sutton, O.M., primary, Berman, D.J., additional, Vaught, A.J., additional, Bradshaw, J., additional, and Johns, R.A., additional
- Published
- 2023
- Full Text
- View/download PDF
16. ITK and RLK Inhibitor PRN694 Improves Skin Disease in Two Mouse Models of Psoriasis
- Author
-
Fuhriman, Jessica M., Winge, Mårten C.G., Haberstock-Debic, Helena, Funk, Jens Oliver, Bradshaw, J. Michael, and Marinkovich, M. Peter
- Published
- 2018
- Full Text
- View/download PDF
17. An Ultrasensitive Ca 2+ /Calmodulin-Dependent Protein Kinase II-Protein Phosphatase 1 Switch Facilitates Specificity in Postsynaptic Calcium Signaling
- Author
-
Bradshaw, J. Michael, Kubota, Yoshi, Meyer, Tobias, and Schulman, Howard
- Published
- 2003
18. Life History and Laboratory Rearing of Emesaya b. brevipennis (Heteroptera: Reduviidae) in Southern Illinois
- Author
-
Hagerty, A. M., Mcpherson, J. E., and Bradshaw, J. D.
- Published
- 2001
- Full Text
- View/download PDF
19. Central/eastern North Pacific photochemical precursor distributions for fall/spring seasons as defined by airborne field studies
- Author
-
DiNunno, B, Davis, D, Chen, G, Gregory, G, Sachse, G, Anderson, B, Vay, S, Avery, M, Ridley, B, Carroll, M, Walega, J, Montzka, D, Grahek, F, Bradshaw, J, Sandholm, S, Kondo, Y, Kok, G, Blake, D, Blake, N, Barrick, J, Fuelberg, H, Martin, B, and Balok, A
- Subjects
ozone ,Pacific ,troposphere ,photochemistry ,Meteorology & Atmospheric Sciences - Published
- 2003
20. Oncogenic activation of JAK3-STAT signaling confers clinical sensitivity to PRN371, a novel selective and potent JAK3 inhibitor, in natural killer/T-cell lymphoma
- Author
-
Nairismägi, M. -L., Gerritsen, M. E., Li, Z. M., Wijaya, G. C., Chia, B. K. H., Laurensia, Y., Lim, J. Q., Yeoh, K. W., Yao, X. S., Pang, W. L., Bisconte, A., Hill, R. J., Bradshaw, J. M., Huang, D., Song, T. L. L., Ng, C. C. Y., Rajasegaran, V., Tang, T., Tang, Q. Q., Xia, X. J., Kang, T. B., Teh, B. T., Lim, S. T., Ong, C. K., and Tan, J.
- Published
- 2018
- Full Text
- View/download PDF
21. Supplementary Table and Supplementary Figures 1-2 from The Irreversible Covalent Fibroblast Growth Factor Receptor Inhibitor PRN1371 Exhibits Sustained Inhibition of FGFR after Drug Clearance
- Author
-
Venetsanakos, Eleni, primary, Brameld, Ken A., primary, Phan, Vernon T., primary, Verner, Erik, primary, Owens, Timothy D., primary, Xing, Yan, primary, Tam, Danny, primary, LaStant, Jacob, primary, Leung, Kwan, primary, Karr, Dane E., primary, Hill, Ronald J., primary, Gerritsen, Mary E., primary, Goldstein, David M., primary, Funk, Jens Oliver, primary, and Bradshaw, J. Michael, primary
- Published
- 2023
- Full Text
- View/download PDF
22. Data from The Irreversible Covalent Fibroblast Growth Factor Receptor Inhibitor PRN1371 Exhibits Sustained Inhibition of FGFR after Drug Clearance
- Author
-
Venetsanakos, Eleni, primary, Brameld, Ken A., primary, Phan, Vernon T., primary, Verner, Erik, primary, Owens, Timothy D., primary, Xing, Yan, primary, Tam, Danny, primary, LaStant, Jacob, primary, Leung, Kwan, primary, Karr, Dane E., primary, Hill, Ronald J., primary, Gerritsen, Mary E., primary, Goldstein, David M., primary, Funk, Jens Oliver, primary, and Bradshaw, J. Michael, primary
- Published
- 2023
- Full Text
- View/download PDF
23. An Assessment of HOx Chemistry in the Tropical pacific Boundary Layer: Comparison of Model Simulations with Observations Recorded During PEM Tropics A
- Author
-
Blake, DR, Chen, G, Davis, D, Crawford, J, Heikes, B, O’Sullivan, D, Lee, M, Eisele, F, Mauldin, L, Tanner, D, Collins, J, Barrick, J, Anderson, B, Bradshaw, J, Sandholm, S, Carroll, M, Albercook, G, and Clarke, A
- Subjects
Physical Chemistry (incl. Structural) ,Other Chemical Sciences ,Meteorology & Atmospheric Sciences - Published
- 2001
24. A dense ring of the trans-Neptunian object Quaoar outside its Roche limit
- Author
-
Morgado, B. E. (B. E.), Sicardy, B. (B.), Braga-Ribas, F. (F.), Ortiz, J. L. (J. L.), Salo, H. (H.), Vachier, F. (F.), Desmars, J. (J.), Pereira, C. L. (C. L.), Santos-Sanz, P. (P.), Sfair, R. (R.), de Santana, T. (T.), Assafin, M. (M.), Vieira-Martins, R. (R.), Gomes-Júnior, A. R. (A. R.), Margoti, G. (G.), Dhillon, V. S. (V. S.), Fernández-Valenzuela, E. (E.), Broughton, J. (J.), Bradshaw, J. (J.), Langersek, R. (R.), Benedetti-Rossi, G. (G.), Souami, D. (D.), Holler, B. J. (B. J.), Kretlow, M. (M.), Boufleur, R. C. (R. C.), Camargo, J. I. (J. I. B.), Duffard, R. (R.), Beisker, W. (W.), Morales, N. (N.), Lecacheux, J. (J.), Rommel, F. L. (F. L.), Herald, D. (D.), Benz, W. (W.), Jehin, E. (E.), Jankowsky, F. (F.), Marsh, T. R. (T. R.), Littlefair, S. P. (S. P.), Bruno, G. (G.), Pagano, I. (I.), Brandeker, A. (A.), Collier-Cameron, A. (A.), Florén, H. G. (H. G.), Hara, N. (N.), Olofsson, G. (G.), Wilson, T. G. (T. G.), Benkhaldoun, Z. (Z.), Busuttil, R. (R.), Burdanov, A. (A.), Ferrais, M. (M.), Gault, D. (D.), Gillon, M. (M.), Hanna, W. (W.), Kerr, S. (S.), Kolb, U. (U.), Nosworthy, P. (P.), Sebastian, D. (D.), Snodgrass, C. (C.), Teng, J. P. (J. P.), de Wit, J. (J.), Morgado, B. E. (B. E.), Sicardy, B. (B.), Braga-Ribas, F. (F.), Ortiz, J. L. (J. L.), Salo, H. (H.), Vachier, F. (F.), Desmars, J. (J.), Pereira, C. L. (C. L.), Santos-Sanz, P. (P.), Sfair, R. (R.), de Santana, T. (T.), Assafin, M. (M.), Vieira-Martins, R. (R.), Gomes-Júnior, A. R. (A. R.), Margoti, G. (G.), Dhillon, V. S. (V. S.), Fernández-Valenzuela, E. (E.), Broughton, J. (J.), Bradshaw, J. (J.), Langersek, R. (R.), Benedetti-Rossi, G. (G.), Souami, D. (D.), Holler, B. J. (B. J.), Kretlow, M. (M.), Boufleur, R. C. (R. C.), Camargo, J. I. (J. I. B.), Duffard, R. (R.), Beisker, W. (W.), Morales, N. (N.), Lecacheux, J. (J.), Rommel, F. L. (F. L.), Herald, D. (D.), Benz, W. (W.), Jehin, E. (E.), Jankowsky, F. (F.), Marsh, T. R. (T. R.), Littlefair, S. P. (S. P.), Bruno, G. (G.), Pagano, I. (I.), Brandeker, A. (A.), Collier-Cameron, A. (A.), Florén, H. G. (H. G.), Hara, N. (N.), Olofsson, G. (G.), Wilson, T. G. (T. G.), Benkhaldoun, Z. (Z.), Busuttil, R. (R.), Burdanov, A. (A.), Ferrais, M. (M.), Gault, D. (D.), Gillon, M. (M.), Hanna, W. (W.), Kerr, S. (S.), Kolb, U. (U.), Nosworthy, P. (P.), Sebastian, D. (D.), Snodgrass, C. (C.), Teng, J. P. (J. P.), and de Wit, J. (J.)
- Abstract
Planetary rings are observed not only around giant planets¹, but also around small bodies such as the Centaur Chariklo² and the dwarf planet Haumea³. Up to now, all known dense rings were located close enough to their parent bodies, being inside the Roche limit, where tidal forces prevent material with reasonable densities from aggregating into a satellite. Here we report observations of an inhomogeneous ring around the trans-Neptunian body (50000) Quaoar. This trans-Neptunian object has an estimated radius⁴ of 555 km and possesses a roughly 80-km satellite⁵ (Weywot) that orbits at 24 Quaoar radii⁶,⁷. The detected ring orbits at 7.4 radii from the central body, which is well outside Quaoar’s classical Roche limit, thus indicating that this limit does not always determine where ring material can survive. Our local collisional simulations show that elastic collisions, based on laboratory experiments⁸, can maintain a ring far away from the body. Moreover, Quaoar’s ring orbits close to the 1/3 spin–orbit resonance9 with Quaoar, a property shared by Chariklo’s ²,¹⁰,¹¹ and Haumea’s³ rings, suggesting that this resonance plays a key role in ring confinement for small bodies.
- Published
- 2023
25. Summary of Publications Featuring Talking Mats™
- Author
-
Hayden, N., Bradshaw, J., Hayward, S., Murphy, J., Hayden, N., Bradshaw, J., Hayward, S., and Murphy, J.
- Abstract
The Talking Mats™ Research Network has produced this summary of studies and reports that reported using Talking Mats. Suggested citation: Hayden, N. K., Bradshaw, J., Hayward, S., Murphy, J., Boa, S., Eden, V., Mischo, S., Pampoulo, E., Macrae, A.-M., Reid, J., Darvell, C., auer, N., Mundt, I., Clark, L., Nagawa, M., Duner, A., and Talking Mats Research Network (2023). Summary of Talking Mats Studies. Talking Mats.
- Published
- 2023
26. Characterizing relationships among fecal indicator bacteria, microbial source tracking markers, and associated waterborne pathogen occurrence in stream water and sediments in a mixed land use watershed
- Author
-
Bradshaw, J. Kenneth, Snyder, Blake J., Oladeinde, Adelumola, Spidle, David, Berrang, Mark E., Meinersmann, Richard J., Oakley, Brian, Sidle, Roy C., Sullivan, Kathleen, and Molina, Marirosa
- Published
- 2016
- Full Text
- View/download PDF
27. Biomass burning influences on the composition of the remote South Pacific troposphere: analysis based on observations from PEM-Tropics-A
- Author
-
Singh, HB, Viezee, W, Chen, Y, Bradshaw, J, Sandholm, S, Blake, D, Blake, N, Heikes, B, Snow, J, Talbot, R, Browell, E, Gregory, G, Sachse, G, and Vay, S
- Subjects
Climate Action ,trace chemicals ,biomass burning pollution ,remote atmospheres ,Statistics ,Atmospheric Sciences ,Environmental Engineering ,Meteorology & Atmospheric Sciences - Abstract
Airborne, in situ measurements from PEM-Tropics-A (September/October 1996) are analyzed to show the presence of distinct pollution plumes in the middle-tropical troposphere of the remote South Pacific (10-30°S). These elevated plumes cause a relative maximum at about 5-7km altitude in the vertical distribution of primary and secondary species characteristic of fuel combustion and biomass burning (CO, C2H2, C2H6, CH3Cl, PAN, O3). Similar plumes were also observed at mid-latitudes in the middle troposphere during three flights east of New Zealand (40-45°S). In all, pollution plumes with CO larger than 100 ppb were observed 24 times on seven separate flight days south of the equator. The observed plumes were frequently embedded in very dry air. Ten-day back trajectory analysis supports the view that these originated from the biomass burning regions of South Africa (and South America) and were transported to the South Pacific along long-distance subsiding trajectories. The chemical composition of the southern Pacific troposphere analyzed from the PEM-Tropics-A data is compared with data from the tropical regions of the northern Pacific (PEM-West-A) and southern Atlantic (TRACE-A) during the same Sept/Oct time period. Sizable perturbations in the abundance of ozone and its key precursors, resulting from the transport of pollution originating from biomass burning sources, are observed in much of the Southern Hemispheric troposphere. Copyright (C) 2000 Elsevier Science B.V.
- Published
- 2000
28. Characterization of the chemical signatures of air masses observed during the PEM experiments over the western Pacific
- Author
-
Smyth, S, Sandholm, S, Shumaker, B, Mitch, W, Kanvinde, A, Bradshaw, J, Liu, S, McKeen, S, Gregory, G, Anderson, B, Talbot, R, Blake, D, Rowland, S, Browell, E, Fenn, M, Merrill, J, Bachmeier, S, Sachse, G, and Collins, J
- Subjects
Climate Action ,Meteorology & Atmospheric Sciences - Abstract
Extensive observations of tropospheric trace species during the second NASA Global Tropospheric Experiment Western Pacific Exploratory Mission (PEM-West B) in February-March 1994 showed significant seasonal variability in comparison with the first mission (PEM-West A), conducted in September-October 1991. In this study we adopt a previously established analytical method, i.e., the ratio C2H2/CO as a measure of the relative degree of atmospheric processing, to elucidate the key similarities and variations between the two missions. In addition, the C2H2/CO ratio scheme is combined with the back-trajectory-based and the LIDAR-based air mass classification schemes, respectively, to make in-depth analysis of the seasonal variation between PEM-West A and PEM-West B (hereinafter referred to as PEM-WA and PEM-WB). A large number of compounds, including long-lived NMHCs, CH4, and CO2, are, as expected, well correlated with the ratio C2H2/CO. In comparison with PEM-WA, a significantly larger range of observed C2H2/CO values at the high end for the PEM-WB period indicates that the western Pacific was more impacted by "fresher" source emissions, i.e., faster or more efficient continental outflow. As in the case of PEM-WA, the C2H2/CO scheme complements the back-trajectory air mass classification scheme very well. By combining the two schemes, we found that the atmospheric processing in the region is dominated by atmospheric mixing for the trace species analyzed. This PEM-WB wintertime result is similar to that found in PEM-WA for the autumn. In both cases, photochemical reactions are found to play a significant role in determining the background mixing ratios of trace gases, and in this way the two processes are directly related and dependent upon each other. This analysis also indicates that many of the upper tropospheric air masses encountered over the western Pacific during PEM-WB may have had little impact from eastern Asia's continental surface sources. NOx mixing ratios were significantly enhanced during PEM-WB when compared with PEM-WA, in the upper troposphere's more atmospherically processed air masses. These high levels of NOx resulted in a substantial amount of photochemical production of O3. A lack of corresponding enhancements in surface emission tracers strongly implies that in situ atmospheric sources such as lightning are responsible for the enhanced upper tropospheric NOx. The similarity in NOx values between the northern (higher air traffic) and southern continental air masses together with the indications of a large seasonal shift suggests that aircraft emissions are not the dominant source. However, photochemical recycling cannot be ruled out as this in situ source of NOx. Copyright 1999 by the American Geophysical Union.
- Published
- 1999
29. Implications of large scale shifts in tropospheric NO x levels in the remote tropical Pacific
- Author
-
Crawford, JH, Davis, DD, Chen, G, Bradshaw, J, Sandholm, S, Kondo, Y, Merrill, J, Liu, S, Browell, E, Gregory, G, Anderson, B, Sachse, G, Barrick, J, Blake, D, Talbot, R, and Pueschel, R
- Subjects
Meteorology & Atmospheric Sciences - Abstract
A major observation recorded during NASA's western Pacific Exploratory Mission (PEM-West B) was the large shift in tropical NO levels as a function of geographical location. High-altitude NO levels exceeding 100 pptv were observed during portions of tropical flights 5-8, while values almost never exceeded 20 pptv during tropical flights 9 and 10. The geographical regions encompassing these two flight groupings are here labeled "high" and "low" NOx regimes. A comparison of these two regimes, based on back trajectories and chemical tracers, suggests that air parcels in both were strongly influenced by deep convection. The low NOx regime appears to have been predominantly impacted by marine convection, whereas the high NOx regime shows evidence of having been more influenced by deep convection over a continental land mass. DMSP satellite observations point strongly toward lightning as the major source of NOx in the latter regime. Photochemical ozone formation in the high NOx regime exceeded that for low NOx by factors of 2 to 6, whereas O3 destruction in the low NOx regime exceeded that for high NOx by factors of up to 3. Taking the tropopause height to be 17 km, estimates of the net photochemical effect on the O3 column revealed that the high NOx regime led to a small net production. By contrast, the low NOx regime was shown to destroy O3 at the rate of 3.4% per day. One proposed mechanism for off-setting this projected large deficit would involve the transport of O3 rich midlatitude air into the tropics. Alternatively, it is suggested that O3 within the tropics may be overall near self-sustaining with respect to photochemical activity. This scenario would require that some tropical regions, unsampled at the time of PEM-B, display significant net column O3 production, leading to an overall balanced budget for the "greater" tropical Pacific basin. Details concerning the chemical nature of such regimes are discussed.
- Published
- 1997
30. An assessment of ozone photochemistry in the extratropical western North Pacific: Impact of continental outflow during the late winter/early spring
- Author
-
Crawford, J, Davis, D, Chen, G, Bradshaw, J, Sandholm, S, Kondo, Y, Liu, S, Browell, E, Gregory, G, Anderson, B, Sachse, G, Collins, J, Barrick, J, Blake, D, Talbot, R, and Singh, H
- Subjects
Meteorology & Atmospheric Sciences - Abstract
This study examines the influence of photochemical processes on tropospheric ozone distributions over the extratropical western North Pacific. The analysis presented ere is based on data collected during the Pacific Exploratory Mission-West Phase B (PEM-West B) field study conducted in February-March 1994. Sampling in the study region involved altitudes of 0-12 km and latitudes of 10°S to 50°N. The extratropical component of the data set (i.e., 20-50°N) was defined by markedly different photochemical environments north and south of 30°N. This separation was clearly defined by an abrupt decrease in the tropopause height near 30°N and a concomitant increase in total O3 column density. This shift in overhead O3 led to highly reduced rates of O3 formation and destruction for the 30-50°N latitude regime. Both latitude ranges, however, stili exhibited net O3 production at all altitudes. Of special significance was the finding that net O3 production prevailed even at boundary layer and lower free tropospheric altitudes (e.g., < 4 km), a condition uncommon to Pacific marine environments. These results reflect the strong impact of continental outflow of O3 precursors (e.g., NO and NMHCs) into the northwestern Pacific Basin. Comparisons with PEM-West A, which sampled the same region in a different season (September-October), revealed major differences at altitudes below 4 km, the altitude range most influenced by continental outflow. The resulting net rate of increase in the tropospheric O3 column for PEM-West B was 1-3% per day, while for PEM-West A it was approximately zero. Unique to the PEM-West B study is the finding that even under wintertime conditions substantial column production of tropospheric O3 can occur at subtropical and mid-latitudes. While such impacts may not be totally unexpected at near coast locations, the present study suggests that the impact from continental outflow on the marine BL could extend out to distances of more than 2000 km from the Asian Pacific Rim.
- Published
- 1997
31. Implications of large scale shifts in tropospheric NOx levels in the remote tropical Pacific
- Author
-
Crawford, JH, Davis, DD, Chen, G, Bradshaw, J, Sandholm, S, Kondo, Y, Merrill, J, Liu, S, Browell, E, Gregory, G, Anderson, B, Sachse, G, Barrick, J, Blake, D, Talbot, R, and Pueschel, R
- Subjects
Meteorology & Atmospheric Sciences - Abstract
A major observation recorded during NASA's western Pacific Exploratory Mission (PEM-West B) was the large shift in tropical NO levels as a function of geographical location. High-altitude NO levels exceeding 100 pptv were observed during portions of tropical flights 5-8, while values almost never exceeded 20 pptv during tropical flights 9 and 10. The geographical regions encompassing these two flight groupings are here labeled "high" and "low" NOx regimes. A comparison of these two regimes, based on back trajectories and chemical tracers, suggests that air parcels in both were strongly influenced by deep convection. The low NOx regime appears to have been predominantly impacted by marine convection, whereas the high NOx regime shows evidence of having been more influenced by deep convection over a continental land mass. DMSP satellite observations point strongly toward lightning as the major source of NOx in the latter regime. Photochemical ozone formation in the high NOx regime exceeded that for low NOx by factors of 2 to 6, whereas O3 destruction in the low NOx regime exceeded that for high NOx by factors of up to 3. Taking the tropopause height to be 17 km, estimates of the net photochemical effect on the O3 column revealed that the high NOx regime led to a small net production. By contrast, the low NOx regime was shown to destroy O3 at the rate of 3.4% per day. One proposed mechanism for off-setting this projected large deficit would involve the transport of O3 rich midlatitude air into the tropics. Alternatively, it is suggested that O3 within the tropics may be overall near self-sustaining with respect to photochemical activity. This scenario would require that some tropical regions, unsampled at the time of PEM-B, display significant net column O3 production, leading to an overall balanced budget for the "greater" tropical Pacific basin. Details concerning the chemical nature of such regimes are discussed.
- Published
- 1997
32. Ozone, hydroperoxides, oxides of nitrogen, and hydrocarbon budgets in the marine boundary layer over the South Atlantic
- Author
-
Heikes, B, Lee, M, Jacob, D, Talbot, R, Bradshaw, J, Singh, H, Blake, D, Anderson, B, Fuelberg, H, and Thompson, AM
- Subjects
Meteorology & Atmospheric Sciences - Abstract
The NASA GTE TRACE A mission sampled air over the South Atlantic and western Indian Oceans. Thirteen flight legs were flown within the marine boundary layer (MBL). The MBL was typically the cleanest air sampled (e.g., CH4 < 1680 ppb, CO < 70 ppb, C2H6 < 400 ppt, C3H8 < 40 ppt, NOx < 15 ppt, and midday NO < 5 ppt) but was overlain by polluted air. The photochemistry of the MBL was influenced by oceanic emissions, surface deposition, and entrainment of pollutants from aloft. Chemical budgets were constructed for several species in the MBL in order to investigate these effects and are presented for ethane, ethylene, propane, propylene, n-butane, formic acid (HFo), methylhydroperoxide (CH3OOH), oxides of nitrogen (i.e., NO, NO2, PAN, HNO3), hydrogen peroxide (H2O2), and ozone (O3). A photochemical point model was used to evaluate local chemical production and loss. An entrainment model was used to assess material exchange between the lower free troposphere (FT) and the MBL and a resistance deposition model was used to evaluate material exchange across the air-sea interface. The results suggested the ocean to be the source of measured alkenes in the MBL and to be the most likely source of the shorter-lived alkanes: propane and n-butane. Ethane was the only hydrocarbon for which input from aloft may have exceeded its photochemical destruction. The estimated hydrocarbon sources from the ocean were in agreement with prior analyses. Transport from the lower FT together with surface loss could not account for measured concentrations of CH2O, HFo, and HNO3. The transport of peroxyacetylnitrate (PAN) from the FT to the MBL exceeded the rate of HNO3 production and was more than sufficient to maintain observed NOx levels without having to invoke an oceanic source for NO. The flux of NOx, PAN, and HNO3 was in balance with the surface deposition flux of HNO3. However, the predicted rates of HNO3 formation from the oxidation of NO2 and HNO3 entrainment from aloft were inadequate to maintain observed levels of HNO3 unless HNO3 was partitioned between the gas phase and a more slowly depositing aerosol phase. The estimated dry deposition flux of HNO3 to the South Atlantic during TRACE A, 2-4 × 109 molecules cm-2 s-1, was about 10 times the annual average estimate for this region. The destruction of O3 within the MBL was found to be exceeded by transport into the MBL from aloft, 6 ±2 × 1010 compared to 11 ± 10 × 1010 molecules cm-2 s-1. The principal O3 destruction process was mediated by the formation and surface deposition of H2O2 and CH3OOH, 4 ± 4 × 1010 and 1.1 ± 0.5 × 1010 molecules cm-2 s-1. The direct loss of O3 to the sea surface was estimated to be 1.7 ± 0.2 × 1010 molecules cm-2 s-1. CH3OOH was lost to the sea and transported into the FT from the MBL. Its first-order loss rate was estimated to be 7 × 10-6 s-1 for a mean MBL height of 700 m. H2O2 and CH2O losses from the MBL were estimated at rates of 1.3 × 10-5 s-1 for both species. The inclusion of surface deposition improved the agreement between predicted and measured concentrations of HNO3, CH3OOH, H2O2, and CH2O. However, model CH2O remained significantly greater than that measured in the MBL.
- Published
- 1996
33. Understanding Cation-Macrocycle Binding Selectivity in Single-Solvent, Extraction, and Liquid Membrane Systems by Quantifying Thermodynamic Interactions
- Author
-
Bruening, R. L., primary, Izatt, R. M., additional, and Bradshaw, J. S., additional
- Published
- 2018
- Full Text
- View/download PDF
34. A comparison of aircraft and ground-based measurements at Mauna Loa observatory, Hawaii, during GTE PEM-west and MLOPEX 2
- Author
-
Atlas, E, Ridley, B, Walega, J, Greenberg, J, Kok, G, Staffelbach, T, Schauffler, S, Lind, J, Hubler, G, Norton, R, Liu, S, Davis, D, Bandy, A, Blake, D, Bradshaw, J, Browell, E, Collins, JE, Gregory, G, Heikes, B, Kondo, Y, Sachse, G, Sandholm, S, Singh, H, Talbot, B, Dlugokencky, E, Elkins, J, Oltmans, S, Mackay, G, and Karecki, D
- Subjects
Meteorology & Atmospheric Sciences - Published
- 1996
35. The paradoxical world of the dog.
- Author
-
Bradshaw, J., primary and Hiby, E., additional
- Published
- 2018
- Full Text
- View/download PDF
36. Hydrogen peroxide and methylhydroperoxide distributions related to ozone and odd hydrogen over the North Pacific in the fall of 1991
- Author
-
Heikes, Brian G, Lee, Meehye, Bradshaw, J, Sandholm, S, Davis, DD, Crawford, J, Rodriguez, Jose, Liu, S, McKeen, S, Thornton, D, Bandy, A, Gregory, G, Talbot, R, and Blake, D
- Subjects
Meteorology & Atmospheric Sciences - Abstract
Hydrogen peroxide and methylhydroperoxide were measured in the troposphere over the western North Pacific as part of the airborne portion of NASA's Global Tropospheric Experiment/Pacific Exploratory Mission-West A field mission. The flights circled the North Pacific, focusing on the western Pacific, and extended from 300 to 13,000 m altitude. The hydroperoxides were uniquely separated and quantified using a high-pressure liquid chromatography system in conjunction with a continuous enzyme fluorometric instrument. Results show a latitudinal gradient in both peroxides at all altitudes; for example, between 3 and 5 km, H2O2 median values decrease from 1700 to 500 parts per trillion by volume (pptv) in going from 0°-15°N to 45°-60°N, and the corresponding decrease in CH3OOH was 1100 to 200 pptv. Concentration maxima are observed in both species at altitudes of 2 to 3 km with H2O2 concentrations below 1 km lower by 30%, 10% for CH3OOH, and even lower, by a factor of 10, for both above 9 km. The H2O2 to CH3OOH ratio increased with altitude and latitude with ratios 2 at midlatitude high altitude. Highest peroxide concentrations were encountered over the Celebes Sea in air which was impacted by aged biomass fire and urban pollutants. CH3OOH was below the level of detection in stratospheric air. H2O2 exceeded SO2 95% of the time, with the exceptions generally above 9 km. Above 3 km, O3 increases with decreasing H2O2 and CH3OOH. Below 3 km the O3-CH3OOH trend is the same but O3 increases with increasing H2O2. The measurements are compared with predictions based upon a photochemical steady state zero-dimensional model and a three-dimensional mesoscale time-dependent model. These models capture observed trends in H2O2 and CH3OOH, with the possible exception of H2O2 below 2 km where surface removal is important. A surface removal lifetime of 3.5 days brings the observed and zero-dimensional model-estimated H2O2 into agreement. The steady state model suggests a strong correlation between the ratios of NO/CO or HO2/HO and the ratio of H2O2/CH3OOH. The observed hydroperoxide ratios bracket the modeled relationship with occasionally much lower H2O2 than expected. Copyright 1996 by the American Geophysical Union.
- Published
- 1996
37. Comparison of free tropospheric western Pacific air mass classification schemes for the PEM‐West A experiment
- Author
-
Smyth, S, Bradshaw, J, Sandholm, S, Liu, S, McKeen, S, Gregory, G, Anderson, B, Talbot, R, Blake, D, Rowland, S, Browell, E, Fenn, M, Merrill, J, Bachmeier, S, Sachse, G, Collins, J, Thornton, D, Davis, D, and Singh, H
- Subjects
Climate Action ,Meteorology & Atmospheric Sciences - Abstract
During September/October 1991, NASA's Global Tropospheric Experiment (GTE) conducted an airborne field measurement program (PEM-West A) in the troposphere over the western Pacific Ocean. In this paper we describe and use the relative abundance of the combustion products C2H2 and CO to classify air masses encountered during PEM-West A based on the degree that these tracers were processed by the combined effects of photochemical reactions and dynamical mixing (termed the degree of atmospheric processing). A large number of trace compounds (e.g., C2H6, C3H8, C6H6, NOy, and O3) are found to be well correlated with the degree of atmospheric processing that is reflected by changes in the ratio of C2H2/CO over the range of values from ∼0.3 to 2.0 (parts per trillion volume) C2H2/ (parts per billion volume) CO. This C2H2/CO-based classification scheme is compared to model simulations and to two independent classification schemes based on air mass back-trajectory analyses and lidar profiles of O3 and aerosols. In general, these schemes agree well, and in combination they suggest that the functional dependence that other observed species exhibit with respect to the C2H2/CO atmospheric processing scale can be used to study the origin, sources, and sinks of trace species and to derive several important findings. First, the degree of atmospheric processing is found to be dominated by dilution associated with atmospheric mixing, which is found to primarily occur through the vertical mixing of relatively recent emissions of surface layer trace species. Photochemical reactions play their major role by influencing the background concentrations of trace species that are entrained during the mixing (i.e., dilution) process. Second, a significant noncontinental source(s) of NO (and NOx) in the free troposphere is evident. In particular, the enhanced NO mixing ratios that were observed in convected air masses are attributed to either emissions from lightning or the rapid recycling of NOy compounds. Third, nonsoluble trace species emitted in the continental boundary layer, such as CO and hydrocarbons, are vertically transported to the upper troposphere as efficiently as they are to the midtroposphere. In addition, the mixing ratios of CO and hydrocarbons in the upper troposphere over the western Pacific may reflect a significant contribution from northern hemisphere land areas other than Asia. Finally, we believe that these results can be valuable for the quantitative evaluation of the vertical transport processes that are usually parameterized in models. Copyright 1996 by the American Geophysical Union.
- Published
- 1996
38. Assessment of ozone photochemistry in the western North Pacific as inferred from PEM‐West A observations during the fall 1991
- Author
-
Davis, DD, Crawford, J, Chen, G, Chameides, W, Liu, S, Bradshaw, J, Sandholm, S, Sachse, G, Gregory, G, Anderson, B, Barrick, J, Bachmeier, A, Collins, J, Browell, E, Blake, D, Rowland, S, Kondo, Y, Singh, H, Talbot, R, Heikes, B, Merrill, J, Rodriguez, J, and Newell, RE
- Subjects
Meteorology & Atmospheric Sciences - Abstract
This study examines the influence of photochemical processes on ozone distributions in the western North Pacific. The analysis is based on data generated during NASA's western Pacific Exploratory Mission (PEM-West A) during the fall of 1991. Ozone trends were best described in terms of two geographical domains: the western North Pacific rim (WNPR) and the western tropical North Pacific (WTNP). For both geographical regions, ozone photochemical destruction, D(O3), decreased more rapidly with altitude than did photochemical formation, F(O3). Thus the ozone tendency, P(O3), was typically found to be negative for z 6-8 km. For nearly all altitudes and latitudes, observed nonmethane hydrocarbon (NMHC) levels were shown to be of minor importance as ozone precursor species. Air parcel types producing the largest positive values of P(O3) included fresh continental boundary layer (BL) air and high-altitude (z > 7 km) parcels influenced by deep convection/lightning. Significant negative P(O3) values were found when encountering clean marine BL air or relatively clean lower free-tropospheric air. Photochemical destruction and formation fluxes for the Pacific rim region were found to exceed average values cited for marine dry deposition and stratospheric injection in the northern hemisphere by nearly a factor of 6. This region was also found to be in near balance with respect to column-integrated O3 photochemical production and destruction. By contrast, for the tropical regime column-integrated O3 showed photochemical destruction exceeding production by nearly 80%. Both transport of O3 rich midlatitude air into the tropics as well as very high-altitude (10-17 km) photochemical O3 production were proposed as possible additional sources that might explain this estimated deficit. Results from this study further suggest that during the fall time period, deep convection over Asia and Malaysia/Indonesia provided a significant source of high-altitude NOx to the western Pacific. Given that the high-altitude NOx lifetime is estimated at between 3 and 9 days, one would predict that this source added significantly to high altitude photochemical O3 formation over large areas of the western Pacific. When viewed in terms of strong seasonal westerly flow, its influence would potentially span a large part of the Pacific. Copyright 1996 by the American Geophysical Union.
- Published
- 1996
39. The ASAS-SN bright supernova catalogue – V. 2018–2020
- Author
-
Neumann, K D, primary, Holoien, T W-S, additional, Kochanek, C S, additional, Stanek, K Z, additional, Vallely, P J, additional, Shappee, B J, additional, Prieto, J L, additional, Pessi, T, additional, Jayasinghe, T, additional, Brimacombe, J, additional, Bersier, D, additional, Aydi, E, additional, Basinger, C, additional, Beacom, J F, additional, Bose, S, additional, Brown, J S, additional, Chen, P, additional, Clocchiatti, A, additional, Desai, D D, additional, Dong, Subo, additional, Falco, E, additional, Holmbo, S, additional, Morrell, N, additional, Shields, J V, additional, Sokolovsky, K V, additional, Strader, J, additional, Stritzinger, M D, additional, Swihart, S, additional, Thompson, T A, additional, Way, Z, additional, Aslan, L, additional, Bishop, D W, additional, Bock, G, additional, Bradshaw, J, additional, Cacella, P, additional, Castro-Morales, N, additional, Conseil, E, additional, Cornect, R, additional, Cruz, I, additional, Farfan, R G, additional, Fernandez, J M, additional, Gabuya, A, additional, Gonzalez-Carballo, J-L, additional, Kendurkar, M R, additional, Kiyota, S, additional, Koff, R A, additional, Krannich, G, additional, Marples, P, additional, Masi, G, additional, Monard, L A G, additional, Muñoz, J A, additional, Nicholls, B, additional, Post, R S, additional, Pujic, Z, additional, Stone, G, additional, Tomasella, L, additional, Trappett, D L, additional, and Wiethoff, W S, additional
- Published
- 2023
- Full Text
- View/download PDF
40. Co‐inhibition of immunoproteasome subunits LMP2 and LMP7 is required to block autoimmunity
- Author
-
Basler, Michael, Lindstrom, Michelle M, LaStant, Jacob J, Bradshaw, J Michael, Owens, Timothy D, Schmidt, Christian, Maurits, Elmer, Tsu, Christopher, Overkleeft, Herman S, Kirk, Christopher J, Langrish, Claire L, and Groettrup, Marcus
- Published
- 2018
- Full Text
- View/download PDF
41. A dense ring of the trans-Neptunian object Quaoar outside its Roche limit
- Author
-
Morgado, B E, Sicardy, B, Braga-Ribas, F, Ortiz, J L, Salo, H, Vachier, F, Desmars, J, Pereira, C L, Santos-Sanz, P, Sfair, R, de Santana, T, Assafin, M, Vieira-Martins, R, Gomes-Júnior, A R, Margoti, G, Dhillon, V S, Fernández-Valenzuela, E, Broughton, J, Bradshaw, J, Langersek, R, Benedetti-Rossi, G, Souami, D, Holler, B J, Kretlow, M, Boufleur, R C, Camargo, J I B, Duffard, R, Beisker, W, Morales, N, Lecacheux, J, Rommel, F L, Herald, D, Benz, Willy, Jehin, E, Jankowsky, F, Marsh, T R, Littlefair, S P, Bruno, G, Pagano, I, Brandeker, A, Collier-Cameron, A, Florén, H G, Hara, N, Olofsson, G, Wilson, T G, Benkhaldoun, Z, Busuttil, R, Burdanov, A, Ferrais, M, Gault, D, Gillon, M, Hanna, W, Kerr, S, Kolb, U, Nosworthy, P, Sebastian, D, Snodgrass, C, Teng, J P, de Wit, J, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Polytechnique des Sciences Avancées (IPSA), Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Science & Technology Facilities Council, University of St Andrews. St Andrews Centre for Exoplanet Science, University of St Andrews. School of Physics and Astronomy, Ministerio de Ciencia e Innovación (España), Junta de Andalucía, European Research Council, European Commission, and Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (Brasil)
- Subjects
MCC ,QC Physics ,Multidisciplinary ,[SDU]Sciences of the Universe [physics] ,QB Astronomy ,520 Astronomie ,3rd-DAS ,530 Physik ,AC ,QC ,QB - Abstract
Full list of authors: Morgado, B. E.; Sicardy, B.; Braga-Ribas, F.; Ortiz, J. L.; Salo, H.; Vachier, F.; Desmars, J.; Pereira, C. L.; Santos-Sanz, P.; Sfair, R.; de Santana, T.; Assafin, M.; Vieira-Martins, R.; Gomes-Junior, A. R.; Margoti, G.; Dhillon, V. S.; Fernandez-Valenzuela, E.; Broughton, J.; Bradshaw, J.; Langersek, R.; Benedetti-Rossi, G.; Souami, D.; Holler, B. J.; Kretlow, M.; Boufleur, R. C.; Camargo, J. I. B.; Duffard, R.; Beisker, W.; Morales, N.; Lecacheux, J.; Rommel, F. L.; Herald, D.; Benz, W.; Jehin, E.; Jankowsky, F.; Marsh, T. R.; Littlefair, S. P.; Bruno, G.; Pagano, I.; Brandeker, A.; Collier-Cameron, A.; Floren, H. G.; Hara, N.; Olofsson, G.; Wilson, T. G.; Benkhaldoun, Z.; Busuttil, R.; Burdanov, A.; Ferrais, M.; Gault, D.; Gillon, M.; Hanna, W.; Kerr, S.; Kolb, U.; Nosworthy, P.; Sebastian, D.; Snodgrass, C.; Teng, J. P.; de Wit, J., Planetary rings are observed not only around giant planets1, but also around small bodies such as the Centaur Chariklo2 and the dwarf planet Haumea3. Up to now, all known dense rings were located close enough to their parent bodies, being inside the Roche limit, where tidal forces prevent material with reasonable densities from aggregating into a satellite. Here we report observations of an inhomogeneous ring around the trans-Neptunian body (50000) Quaoar. This trans-Neptunian object has an estimated radius4 of 555 km and possesses a roughly 80-km satellite5 (Weywot) that orbits at 24 Quaoar radii6,7. The detected ring orbits at 7.4 radii from the central body, which is well outside Quaoar’s classical Roche limit, thus indicating that this limit does not always determine where ring material can survive. Our local collisional simulations show that elastic collisions, based on laboratory experiments8, can maintain a ring far away from the body. Moreover, Quaoar’s ring orbits close to the 1/3 spin–orbit resonance9 with Quaoar, a property shared by Chariklo’s2,10,11 and Haumea’s3 rings, suggesting that this resonance plays a key role in ring confinement for small bodies. © 2023, The Author(s), under exclusive licence to Springer Nature Limited., This work was carried out under the Lucky Star umbrella that agglomerates the efforts of the Paris, Granada and Rio teams, which is funded by the ERC under the European Community’s H2020 (ERC grant agreement no. 669416). Part of the results were obtained using CHEOPS data. CHEOPS is an ESA mission in partnership with Switzerland with important contributions to the payload and the ground segment from Austria, Belgium, France, Germany, Hungary, Italy, Portugal, Spain, Sweden and the UK. The CHEOPS Consortium gratefully acknowledge the support received by all the agencies, offices, universities and industries involved. Their flexibility and willingness to explore new approaches were essential to the success of this mission. The design and construction of HiPERCAM was supported by the ERC under the European Union’s Seventh Framework Programme (FP/2007-2013) under ERC-2013-ADG grant agreement no. 340040 (HiPERCAM). HiPERCAM operations and V.S.D. are funded by the Science and Technology Facilities Council (grant no. ST/V000853/1). The GTC is installed at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias, on the island of La Palma. This work has made use of data from the ESA mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). This study was financed in part by the National Institute of Science and Technology of the e-Universe project (INCT do e-Universo, CNPq grant no. 465376/2014-2). This study was financed in part by CAPES - Finance Code 001. The following authors acknowledge the respective (1) CNPq grants to B.E.M. no. 150612/2020-6; F.B.-R. no. 314772/2020-0; R.V.-M. no. 307368/2021-1; M.A. nos. 427700/2018-3, 310683/2017-3 and 473002/2013-2; and J.I.B.C. nos. 308150/2016-3 and 305917/2019-6. (2) CAPES/Cofecub grant to B.E.M. no. 394/2016-05. (3) FAPERJ grant no. M.A. E-26/111.488/2013. (4) FAPESP (Fundação de Amparo à Pesquisa do Estado de São Paulo) grants to A.R.G.-J. no. 2018/11239-8 and R.S. no. 2016/24561-0. (5) CAPES-PrInt Program grant to G.B.-R. no. 88887.310463/2018-00, mobility number 88887.571156/2020-00. (6) DFG (the German Research Foundation) grant to R.S. no. 446102036. P.S-S. and R.D. acknowledge financial support by the Spanish grant no. AYA-RTI2018-098657-J-I00 ‘LEO-SBNAF’ (MCIU/AEI/FEDER, UE). J.L.O., P.S-S., R.D. and N.M. acknowledge financial support from the State Agency for Research of the Spanish MCIU through the ‘Center of Excellence Severo Ochoa’ award for the Instituto de Astrofísica de Andalucía (grant no. SEV-2017-0709), and they also acknowledge the financial support by the Spanish grant nos. AYA-2017-84637-R and PID2020-112789GB-I00, and the Proyectos de Excelencia de la Junta de Andalucía grant nos. 2012-FQM1776 and PY20-01309. G.B-R. and I.P. acknowledge support from CHEOPS ASI-INAF agreement no. 2019-29-HH.0. A.B. was supported by the SNSA. A.C.-C. and T.G.W. acknowledge support from STFC consolidated grant nos. ST/R000824/1 and ST/V000861/1, and UK Space Agency grant no. ST/R003203/1. U.K. and R.B. acknowledge support by The OpenSTEM Laboratories, an initiative funded by the Higher Education Funding Council for England and the Wolfson Foundation. J.W. gratefully acknowledges financial support from the Heising-Simons Foundation, C. Masson and P. A. Gilman for Artemis, the first telescope of the SPECULOOS network situated in Tenerife, Spain. The ULiege’s contribution to SPECULOOS has received funding from the ERC under the European Union’s Seventh Framework Programme (FP/2007-2013) (grant agreement no. 336480/SPECULOOS), from the Balzan Prize and Francqui Foundations, from the Belgian Scientific Research Foundation (F.R.S.-FNRS; grant no. T.0109.20), from the University of Liege and from the ARC grant for Concerted Research Actions financed by the Wallonia-Brussels Federation. TRAPPIST is a project funded by the Belgian Fonds (National) de la Recherche Scientique (F.R.S.-FNRS) under grant no. PDR T.0120.21. TRAPPIST-North is a project funded by the University of Liege, in collaboration with the Cadi Ayyad University of Marrakech (Morocco). E.J. is FNRS Senior Research Associate., With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2021-001131-S).
- Published
- 2023
- Full Text
- View/download PDF
42. Summertime partitioning and budget of NOycompounds in the troposphere over Alaska and Canada: ABLE 3B
- Author
-
Sandholm, S, Olson, J, Bradshaw, J, Talbot, R, Singh, H, Gregory, G, Blake, D, Anderson, B, Sachse, G, Barrick, J, Collins, J, Klemm, K, Lefer, B, Klemm, O, Gorzelska, K, Herlth, D, and O'Hara, D
- Subjects
Meteorology & Atmospheric Sciences - Published
- 1994
43. Summertime partitioning and budget of NOy compounds in the troposphere over Alaska and Canada: ABLE 3B
- Author
-
Sandholm, S, Olson, J, Bradshaw, J, Talbot, R, Singh, H, Gregory, G, Blake, D, Anderson, B, Sachse, G, Barrick, J, Collins, J, Klemm, K, Lefer, B, Klemm, O, Gorzelska, K, Herlth, D, and O'Hara, D
- Subjects
Meteorology & Atmospheric Sciences - Published
- 1994
44. A photostationary state analysis of the NO2‐NO system based on airborne observations from the subtropical/tropical North and South Atlantic
- Author
-
Davis, DD, Chen, G, Chameides, W, Bradshaw, J, Sandholm, S, Rodgers, M, Schendal, J, Madronich, S, Sachse, G, Gregory, G, Anderson, B, Barrick, J, Shipham, M, Collins, J, Wade, L, and Blake, D
- Subjects
Meteorology & Atmospheric Sciences - Published
- 1993
45. A PHOTOSTATIONARY STATE ANALYSIS OF THE NO2-NO SYSTEM BASED ON AIRBORNE OBSERVATIONS FROM THE SUBTROPICAL TROPICAL NORTH AND SOUTH-ATLANTIC
- Author
-
DAVIS, DD, CHEN, G, CHAMEIDES, W, BRADSHAW, J, SANDHOLM, S, RODGERS, M, SCHENDAL, J, MADRONICH, S, SACHSE, G, GREGORY, G, ANDERSON, B, BARRICK, J, SHIPHAM, M, COLLINS, J, WADE, L, and BLAKE, D
- Subjects
Meteorology & Atmospheric Sciences - Published
- 1993
46. The ASAS-SN Bright Supernova Catalog -- V. 2018-2020
- Author
-
Holoien, T. W. -S., Kochanek, C. S., Stanek, K. Z., Vallely, P. J., Shappee, B. J., Prieto, J. L., Pessi, T., Jayasinghe, T., Brimacombe, J., Bersier, D., Aydi, E., Basinger, C., Beacom, J. F., Bose, S., Brown, J. S., Chen, P., Clocchiatti, A., Desai, D. D., Dong, S., Falco, E., Holmbo, S., Morrell, N., Shields, J. V., Sokolovsky, K., Strader, J., Stritzinger, M. D., Swihart, S., Thompson, T. A., Way, Z., Aslan, L., Bishop, D. W., Bock, G., Bradshaw, J., Cacella, P., Castro, N., Conseil, E., Cornect, R., Cruz, I., Farfan, R. G., Gabuya, A., Gonzalez-Carballo, J. -L., Kendurkar, M. R., Kiyota, S., Koff, R. A., Krannich, G., Marples, P., Masi, G., Monard, L. A. G., Muñoz, J. A., Nicholls, B., Post, R. S., Pujic, Z., Stone, G., Tomasella, L., Trappett, D. L., and Wiethoff, W. S.
- Subjects
astro-ph.HE - Abstract
We catalog the 443 bright supernovae discovered by the All-Sky Automated Survey for Supernovae (ASAS-SN) in $2018-2020$ along with the 519 supernovae recovered by ASAS-SN and 516 additional $m_{peak}\leq18$ mag supernovae missed by ASAS-SN. Our statistical analysis focuses primarily on the 984 supernovae discovered or recovered in ASAS-SN $g$-band observations. The complete sample of 2427 ASAS-SN supernovae includes earlier $V$-band samples and unrecovered supernovae. For each supernova, we identify the host galaxy, its UV to mid-IR photometry, and the offset of the supernova from the center of the host. Updated light curves, redshifts, classifications, and host galaxy identifications supersede earlier results. With the increase of the limiting magnitude to $g\leq18$ mag, the ASAS-SN sample is roughly complete up to $m_{peak}=16.7$ mag and is $90\%$ complete for $m_{peak}\leq17.0$ mag. This is an increase from the $V$-band sample where it was roughly complete up to $m_{peak}=16.2$ mag and $70\%$ complete for $m_{peak}\leq17.0$ mag.
- Published
- 2022
47. The Quest to Identify a New Virus Disease of Sunflower from Nebraska
- Author
-
Harveson, R. M., primary, Al Rwahnih, M., additional, Tian, T., additional, Karasev, A., additional, Gulya, T. J., additional, and Bradshaw, J. D., additional
- Published
- 2022
- Full Text
- View/download PDF
48. Pre-Operative vs. Post-Operative Fractionated Stereotactic Radiotherapy: A Single-Institution Analysis of 534 Resected Metastases
- Author
-
Perlow, H.K., Hennings, S., Bradshaw, J., Reddy, S., Luu, S., Matsui, J.K., Klamer, B., Dibs, K., Harrell, M.R., McGregor, J., Lonser, R.R., Prevedello, D., Elder, J.B., Wu, K., Prabhu, R.S., Zhu, S., Singh, R., Beyer, S., Grecula, J.C., Blakaj, D.M., Thomas, E.M., Raval, R., and Palmer, J.D.
- Published
- 2024
- Full Text
- View/download PDF
49. Pre-Operative Single Fraction vs. Fractionated Stereotactic Radiotherapy: A Single-Institution Analysis of 299 Resected Metastases
- Author
-
Perlow, H.K., Luu, S., Reddy, S., Bradshaw, J., Hennings, S., Matsui, J.K., Klamer, B., Upadhyay, R., Oliver, A., McGregor, J., Lonser, R.R., Prevedello, D., Elder, J.B., Wu, K., Prabhu, R.S., Zhu, S., Singh, R., Beyer, S., Grecula, J.C., Blakaj, D.M., Thomas, E.M., Raval, R., and Palmer, J.D.
- Published
- 2024
- Full Text
- View/download PDF
50. Reduced Treatment Volumes for Glioblastoma Result in Lower Rates of Radionecrosis and Lymphopenia: A Pooled Analysis
- Author
-
Matsui, J.K., Swanson, D., Allen, P.K., Perlow, H.K., Bradshaw, J., Beckham, T., Tom, M.C., Wang, C., Perni, S., Yeboa, D.N., Ghia, A.J., McAleer, M.F., Li, J., Palmer, J.D., and McGovern, S.L.
- Published
- 2024
- Full Text
- View/download PDF
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.