cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25550/1q-x80r
title: The interconnected relationships between middle ear bulla size, cavitation defects and chronic otitis media revealed in a syndromic mouse model

description: High incidence of chronic otitis media is associated with human craniofacial syndromes, suggesting that defects in the formation of the middle ear and associated structures can have a knock-on effect on the susceptibility to middle ear inflammation. Patients with branchio-oto-renal (BOR) syndrome have several defects in the ear leading to both sensorineural and conductive hearing loss, including otitis media. 40% of BOR syndrome cases are due to Eya1 haploinsufficiency, with mouse models lacking Eya1, mimicking many of the defects found in patients. Here, we characterize the onset, consequences, and underlying causes of chronic otitis media in Eya1 heterozygous mice. Cavitation defects were evident in these mice from postnatal day (P) 11 onwards, with mesenchyme around the promontory and attic regions of the middle ear space. This mesenchyme was still prominent in adult Eya1 heterozygous mice, while the wild-type littermates had fully aerated ears from P14 onwards. MicroCT analysis highlighted a significantly smaller bulla, confirming the link between bulla size defects and the ability of the mesenchyme to retract successfully. Otitis media was observed from P14, often presenting unilaterally, resulting in hyperplasia of the middle ear mucosa, expansion of secretory cells, defects in the motile cilia, and changes in basal epithelial cell markers. A high incidence of otitis media was identified in older mice but only associated with ears while retaining mesenchyme. To understand the impact of the environment, the mouse line was rederived onto a super-clean environment. Cavitation defects were still evident at early stages, but these generally resolved over time, and importantly, no signs of otitis media were observed at 6 weeks. In conclusion, we show that a small bulla size is closely linked to the defects in cavitation and the presence of retained mesenchyme. A delay in retraction of the mesenchyme predates the onset of otitis media, making the ears susceptible to its development. Early exposure to OM appears to exacerbate the cavitation defect, with mesenchyme evident in the middle ear throughout the animal’s life. This highlights that permanent damage to the middle ear can arise as a consequence of the early onset of OM.
DOI: 10.6084/m9.figshare.20553333
title: Dataset.csv

description: Alibaba social media advert
DOI: 10.5281/zenodo.1184620
title: DeepSlides dataset

description: DeepSlides dataset. please cite: <pre>@article{senaras2018deepfocus, title={DeepFocus: detection of out-of-focus regions in whole slide digital images using deep learning}, author={Senaras, Caglar and Niazi, M Khalid Khan and Lozanski, Gerard and Gurcan, Metin N}, journal={PloS one}, volume={13}, number={10}, pages={e0205387}, year={2018}, publisher={Public Library of Science San Francisco, CA USA} }</pre>
DOI: 10.5281/zenodo.1184621
title: DeepSlides dataset

description: DeepSlides dataset. please cite: <pre>@article{senaras2018deepfocus, title={DeepFocus: detection of out-of-focus regions in whole slide digital images using deep learning}, author={Senaras, Caglar and Niazi, M Khalid Khan and Lozanski, Gerard and Gurcan, Metin N}, journal={PloS one}, volume={13}, number={10}, pages={e0205387}, year={2018}, publisher={Public Library of Science San Francisco, CA USA} }</pre>
DOI: 10.5281/zenodo.7016550
title: Ring-shear experiments with strain markers

description: <strong>Experiment overview</strong> ID Shearing velocity [mm/min] Effective normal stress [kPa] mdt4 7.00 6 mdt5 0.70 6 mdt6 0.07 6 mdt7 7.00 50 mdt8 0.70 50 mdt9 0.07 50 <br> <strong>Apparatus and material</strong> These experiments were conducted in a ring-shear apparatus at the Department of Geoscience, Aarhus University, with a sample chamber volume of 14,48 l. The till was Mid-Danish Till deposited at the Last Glacial Maximum, and sampled at Knud Strand, Denmark. All shearing commenced under water-saturated conditions, and I used BB-gun pellets as strain markers. Please see the following publication for more technical details on the ring-shear apparaturs: Damsgaard, A., D. L. Egholm, J. A. Piotrowski, S. Tulaczyk, N. K. Larsen, and K. Tylmann (2013), Discrete element modeling of subglacial sediment deformation, J. Geophys. Res. Earth Surf., 118, 2230–2242, doi:10.1002/2013JF002830. <br> <strong>Data files and format</strong> <em>Sensor data during shear</em> These data files are named in the style "&lt;ID&gt;-stress-shear.tsv", where<br> ID refers to the experiment ID seen in the table above. The values are tab-separated, with the following columns and units: Shearing distance [mm] Normal stress [kPa] Shear stress [kPa] Dilation [mm] Important!: The shear stress readings are unreliable due to sensor failure. <em>Strain marker data</em> These data files are named in the style "&lt;ID&gt;-shear-disp.tsv". The values are tab-separated, with the following columns and units: Marker position along shear direction [mm] Marker depth [mm] <br> <strong>Author and funding</strong> Anders Damsgaard &lt;anders@adamsgaard.dk&gt;, Department of Geoscience, Aarhus University This dataset is part of a project that has received funding from the European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No 897967.
DOI: 10.5281/zenodo.7016549
title: Ring-shear experiments with strain markers

description: <strong>Experiment overview</strong> ID Shearing velocity [mm/min] Effective normal stress [kPa] mdt4 7.00 6 mdt5 0.70 6 mdt6 0.07 6 mdt7 7.00 50 mdt8 0.70 50 mdt9 0.07 50 <br> <strong>Apparatus and material</strong> These experiments were conducted in a ring-shear apparatus at the Department of Geoscience, Aarhus University, with a sample chamber volume of 14,48 l. The till was Mid-Danish Till deposited at the Last Glacial Maximum, and sampled at Knud Strand, Denmark. All shearing commenced under water-saturated conditions, and I used BB-gun pellets as strain markers. Please see the following publication for more technical details on the ring-shear apparaturs: Damsgaard, A., D. L. Egholm, J. A. Piotrowski, S. Tulaczyk, N. K. Larsen, and K. Tylmann (2013), Discrete element modeling of subglacial sediment deformation, J. Geophys. Res. Earth Surf., 118, 2230–2242, doi:10.1002/2013JF002830. <br> <strong>Data files and format</strong> <em>Sensor data during shear</em> These data files are named in the style "&lt;ID&gt;-stress-shear.tsv", where<br> ID refers to the experiment ID seen in the table above. The values are tab-separated, with the following columns and units: Shearing distance [mm] Normal stress [kPa] Shear stress [kPa] Dilation [mm] Important!: The shear stress readings are unreliable due to sensor failure. <em>Strain marker data</em> These data files are named in the style "&lt;ID&gt;-shear-disp.tsv". The values are tab-separated, with the following columns and units: Marker position along shear direction [mm] Marker depth [mm] <br> <strong>Author and funding</strong> Anders Damsgaard &lt;anders@adamsgaard.dk&gt;, Department of Geoscience, Aarhus University This dataset is part of a project that has received funding from the European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No 897967.
DOI: 10.25574/02297
title: Chandra X-ray Observatory ObsId 2297

description: THE MOLECULAR FRACTION AND ABUNDANCES OF GAS IN THE GALAXY
DOI: 10.25574/02304
title: Chandra X-ray Observatory ObsId 2304

description: HETG OBSERVATIONS OF EXTREME NARROW-LINE SEYFERT 1 GALAXIES
DOI: 10.25574/02305
title: Chandra X-ray Observatory ObsId 2305

description: ARE B STAR X-RAY SOURCES WIND-CORONAL HYBRIDS?
DOI: 10.25574/02306
title: Chandra X-ray Observatory ObsId 2306

description: HIGH RESOLUTION LINE SPECTROSCOPY OF THREE YOUNG SUPERNOVA REMNANTS IN THE LARGE MAGELLANIC CLOUD
DOI: 10.25574/02307
title: Chandra X-ray Observatory ObsId 2307

description: BROAD-BAND HIGH RESOLUTION SPECTROSCOPY OF SS CYGNI IN OUTBURST
DOI: 10.25574/02308
title: Chandra X-ray Observatory ObsId 2308

description: MULTIWAVELENGTH TOO OBSERVATIONS OF BRIGHT NOVAE IN OUTBURST
DOI: 10.25574/02310
title: Chandra X-ray Observatory ObsId 2310

description: FINDING THE BARYONS IN THE LOW REDSHIFT UNIVERSE.
DOI: 10.25574/02311
title: Chandra X-ray Observatory ObsId 2311

description: FINDING THE BARYONS IN THE LOW REDSHIFT UNIVERSE.
DOI: 10.14457/tu.the.2021.92
title: Implementing lean information management: case study on service organization

description: This research is to study problems that arise in the work process of a service organization. Which serves as an official distributor of Japanese standard aluminum doors and windows in Thailand. By using a lean thinking process and lean tools to improve information management and the work system of employees regarding internal information, and to have a better standard of work, reduce the problem of loss, and delay in the work. All solutions to this problem are based on knowledge, understanding and tools related to lean management, Kaizen system and value stream mapping. The results of this research will help organizations reduce waste and shorter lead times to gain an advantage over competitors in sales and service. This research can reduce the loss incurred by the organization by at least 5% of the total waste that occurs. And all employees are satisfied in the lean management not less than 80% of the total workforce.
DOI: 10.14457/tu.the.2021.97
title: Guidelines for selecting the appropriate health-related product: case study lumbar support pillow

description: Computers with desks and chairs are a hugely important part of human work. The worker may have to analyze the many data in a limited time. It calls for long, intensive hours of concentrated and repetitive work with the desk and chairs. Health back is also a popular option to support back when they sit in the wrong position. However, health back also easily accumulates the wrong position of ergonomic. They have almost some defectsof existing product reference from ergonomic when they sit in the chair. Through the research, present to recommend a method of study that identifies an aspect of the analysis of the product on the market with ergonomic and engineering design, by comparison, existing product and found the best model to recommendation. Then the recommended design of the product, which can both satisfy customer demand and balance between production and cost. A recommend design may relieve low back pain by the existing production the market. Adapt and compare the good things from the existing product with the correct ergonomic and can fit any chairs. Then applied the technique of modified size and supportive ergonomic to long-term health when you work in the same position for a long time. Since the product is well designed to support the correct ergonomic, we hope that this recommended product from the existing model will be using the memory foam material and can adjust to fix in any chairs and may relieve low back pain.
DOI: 10.25574/02318
title: Chandra X-ray Observatory ObsId 2318

description: OBSERVATION OF SNR RCW103
DOI: 10.25574/02330
title: Chandra X-ray Observatory ObsId 2330

description: ACIS-S/HETG OBSERVATIONS OF THE CENTRAL REGION OF THE HYDRA A CLUSTER OF GALAXIES
DOI: 10.25574/02331
title: Chandra X-ray Observatory ObsId 2331

description: ACIS-S/HETG OBSERVATIONS OF THE CENTRAL REGION OF THE HYDRA A CLUSTER OF GALAXIES
DOI: 10.25574/02332
title: Chandra X-ray Observatory ObsId 2332

description: ACIS-S/HETG OBSERVATIONS OF THE CENTRAL REGION OF THE HYDRA A CLUSTER OF GALAXIES
DOI: 10.25574/02333
title: Chandra X-ray Observatory ObsId 2333

description: ACIS-S/HETG OBSERVATIONS OF THE CENTRAL REGION OF THE HYDRA A CLUSTER OF GALAXIES
DOI: 10.25574/02334
title: Chandra X-ray Observatory ObsId 2334

description: ACIS-S/HETG OBSERVATIONS OF THE CENTRAL REGION OF THE HYDRA A CLUSTER OF GALAXIES
DOI: 10.25574/02336
title: Chandra X-ray Observatory ObsId 2336

description: THE NATURE OF CLASSICAL SYMBIOTIC OUTBURSTS
DOI: 10.25574/02337
title: Chandra X-ray Observatory ObsId 2337

description: CAPTURING WR140 AT PERIASTRON WITH THE CHANDRA HETG
DOI: 10.25574/02338
title: Chandra X-ray Observatory ObsId 2338

description: CAPTURING WR140 AT PERIASTRON WITH THE CHANDRA HETG
DOI: 10.25574/02341
title: Chandra X-ray Observatory ObsId 2341

description: HRC-I FOCUS CHECK
DOI: 10.6084/m9.figshare.20553234.v2
title: Intrapulmonary shunting is a key contributor to hypoxia in COVID-19: an update on the pathophysiology

description: Data from every patient over 18 years old admitted to the two centres for clinically and/or laboratory-confirmed COVID-19 was recorded. Patients were only included if they were hypoxic on admission and required supplemental oxygen. Patients were excluded if they were pregnant, self-discharged against medical advice before treatment completion, or if there was no documentation of oxygen saturations on admission. Oxygen saturations measured using fingertip pulse oximetry by the ambulance crew and emergency departments were collected. Oxygen flow (litres/min) was converted to FiO2 according to predetermined conversion charts. Baseline saturations on air followed by saturations after administration of oxygen were collected and used to construct the oxygen dissociation curve (ODC). The calculation has been previously described in detail. Intrapulmonary shunt and VA/Q mismatch were estimated using software based on the algorithm developed by Lockwood et al which produces ODCs using a two-compartment model. Epidemiological, clinical, laboratory, and radiological characteristics were collected in addition to treatments and outcome (discharge or death).
DOI: 10.25574/02374
title: Chandra X-ray Observatory ObsId 2374

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02375
title: Chandra X-ray Observatory ObsId 2375

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02376
title: Chandra X-ray Observatory ObsId 2376

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02377
title: Chandra X-ray Observatory ObsId 2377

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02378
title: Chandra X-ray Observatory ObsId 2378

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02379
title: Chandra X-ray Observatory ObsId 2379

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02380
title: Chandra X-ray Observatory ObsId 2380

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02381
title: Chandra X-ray Observatory ObsId 2381

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02382
title: Chandra X-ray Observatory ObsId 2382

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02383
title: Chandra X-ray Observatory ObsId 2383

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02384
title: Chandra X-ray Observatory ObsId 2384

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02385
title: Chandra X-ray Observatory ObsId 2385

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02388
title: Chandra X-ray Observatory ObsId 2388

description: COORDINATED AXAF AND HST SPECTROSCOPY OF FLARES ON PROXIMA CENTAURI
DOI: 10.25574/02389
title: Chandra X-ray Observatory ObsId 2389

description: THE DETAILED X-RAY SPECTRA OF ELLIPTICAL GALAXIES
DOI: 10.25574/02390
title: Chandra X-ray Observatory ObsId 2390

description: X-RAY SPECTROSCOPY OF COMET C/1999 T1
DOI: 10.25574/02391
title: Chandra X-ray Observatory ObsId 2391

description: X-RAY SPECTROSCOPY OF COMET C/1999 T1
DOI: 10.25574/02392
title: Chandra X-ray Observatory ObsId 2392

description: X-RAY SPECTROSCOPY OF COMET C/1999 T1
DOI: 10.25574/02393
title: Chandra X-ray Observatory ObsId 2393

description: X-RAY SPECTROSCOPY OF COMET C/1999 T1
DOI: 10.25574/02398
title: Chandra X-ray Observatory ObsId 2398

description: ACIS OBSERVATIONS OF JUPITER
DOI: 10.25574/02399
title: Chandra X-ray Observatory ObsId 2399

description: ACIS OBSERVATIONS OF JUPITER
DOI: 10.25574/02400
title: Chandra X-ray Observatory ObsId 2400

description: ACIS OBSERVATIONS OF JUPITER
DOI: 10.25574/02401
title: Chandra X-ray Observatory ObsId 2401

description: ACIS OBSERVATIONS OF JUPITER
DOI: 10.21227/yskj-v875
title: Buried Object Characterization Using Ground Penetrating Radar 

description: Ground Penetrating Radar (GPR) has a wide range of applications such as detection of buried mines, pipes and wires. GPR has been used as a near-surface remote sensing technique, and its working principle is based on electromagnetic (EM) wave theory. Here proposed data set is meant for data driven surrogate modelling based Buried Object Characterization. The considered problem of estimating geophysical parameters of a buried object is 2D. The training and testing scenarios include B-scan images (2D data), which contain 16 pairs of A-scan (concatenated forms of A-scans). Each A-scan is a time-varying normalized power amplitude signal obtained at the one point along the synthetic aperture. In other words, the scanning path length is 600. In addition, A-scan combination was presented as the A-scan ID according to points at the scanning path (400 mm). The data consists of 600 time-varying amplitudes and the A-scan ID (601x1). Here, the A-scan ID is an integer between 1 and 16. The training and testing datasets consist of 315 linearly samples scenarios, and 63 randomly selected scenarios, respectively, with the data acquired using a full wave EM simulator. Each data set contains 16 A scan signals (the total of 5040 and 1008 A-scans for training and test data sets respectively).For more detailed information please check [1]. [1] R. Yurt, H. Torpi, P. Mahouti, A. Kızılay and S. Koziel, “Buried Object Characterization Using Ground Penetrating Radar Assisted by Data-Driven Surrogate-Models,” to be published in IEEE Access.
DOI: 10.25574/02407
title: Chandra X-ray Observatory ObsId 2407

description: ACIS OBSERVATIONS OF JUPITER
DOI: 10.25574/02408
title: Chandra X-ray Observatory ObsId 2408

description: ACIS OBSERVATIONS OF JUPITER
DOI: 10.25574/02410
title: Chandra X-ray Observatory ObsId 2410

description: HIGH RESOLUTION SPECTRA OF YOUNG SUPERNOVA REMNANTS
DOI: 10.25574/02411
title: Chandra X-ray Observatory ObsId 2411

description: VENUS AND MARS: THE CLOSEST PLANETARY ANALOGUES TO COMETS
DOI: 10.25574/02414
title: Chandra X-ray Observatory ObsId 2414

description: VENUS AND MARS: THE CLOSEST PLANETARY ANALOGUES TO COMETS
DOI: 10.25574/02415
title: Chandra X-ray Observatory ObsId 2415

description: CHANDRA OBSERVATIONS OF CYGNUS X-1 IN A RARE, SUSTAINED HIGH/SOFT STATE
DOI: 10.25574/02416
title: Chandra X-ray Observatory ObsId 2416

description: HIGH RESOLUTION SPECTRA OF YOUNG SUPERNOVA REMNANTS
DOI: 10.25574/02417
title: Chandra X-ray Observatory ObsId 2417

description: ACIS STUDY OF GRAVITATIONALLY LENSED QUASARS
DOI: 10.25574/02418
title: Chandra X-ray Observatory ObsId 2418

description: FINDING THE BARYONS IN THE LOW REDSHIFT UNIVERSE.
DOI: 10.25574/02420
title: Chandra X-ray Observatory ObsId 2420

description: COLLIDING STELLAR WINDS IN IOTA ORIONIS.
DOI: 10.25574/02429
title: Chandra X-ray Observatory ObsId 2429

description: HIGH RESOLUTION SPECTROSCOPY OF THE POSSIBLE JETS IN GRS 1758-258
DOI: 10.25574/02440
title: Chandra X-ray Observatory ObsId 2440

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02441
title: Chandra X-ray Observatory ObsId 2441

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02442
title: Chandra X-ray Observatory ObsId 2442

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02443
title: Chandra X-ray Observatory ObsId 2443

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02444
title: Chandra X-ray Observatory ObsId 2444

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02445
title: Chandra X-ray Observatory ObsId 2445

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02446
title: Chandra X-ray Observatory ObsId 2446

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02447
title: Chandra X-ray Observatory ObsId 2447

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02448
title: Chandra X-ray Observatory ObsId 2448

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02449
title: Chandra X-ray Observatory ObsId 2449

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02450
title: Chandra X-ray Observatory ObsId 2450

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02451
title: Chandra X-ray Observatory ObsId 2451

description: HRC-I CALIBRATION OBSERVATIONS OF ARLAC
DOI: 10.25574/02458
title: Chandra X-ray Observatory ObsId 2458

description: IMMEDIATE POST-GIANT FLARE OBSERVATIONS OF SGR 1900+14
DOI: 10.25574/02459
title: Chandra X-ray Observatory ObsId 2459

description: TOO OBSERVATIONS OF SGR 1900+14 IN AN ACTIVE STATE
DOI: 10.25574/02462
title: Chandra X-ray Observatory ObsId 2462

description: AO3 CALIBRATION OBSERVATIONS OF 3C273
DOI: 10.25574/02463
title: Chandra X-ray Observatory ObsId 2463

description: AO3 CALIBRATION OBSERVATIONS OF 3C273
DOI: 10.25574/02464
title: Chandra X-ray Observatory ObsId 2464

description: AO3 CALIBRATION OBSERVATIONS OF 3C273
DOI: 10.25574/02468
title: Chandra X-ray Observatory ObsId 2468

description: ACIS DARK CURRENT CALIBARTION ON DARK MOON
DOI: 10.25574/02469
title: Chandra X-ray Observatory ObsId 2469

description: ACIS DARK CURRENT CALIBARTION ON DARK MOON
DOI: 10.25574/02471
title: Chandra X-ray Observatory ObsId 2471

description: AO3 CALIBRATION OBSERVATIONS OF 3C273
DOI: 10.25574/02472
title: Chandra X-ray Observatory ObsId 2472

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02473
title: Chandra X-ray Observatory ObsId 2473

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02474
title: Chandra X-ray Observatory ObsId 2474

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02475
title: Chandra X-ray Observatory ObsId 2475

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02476
title: Chandra X-ray Observatory ObsId 2476

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02477
title: Chandra X-ray Observatory ObsId 2477

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02478
title: Chandra X-ray Observatory ObsId 2478

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02479
title: Chandra X-ray Observatory ObsId 2479

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02480
title: Chandra X-ray Observatory ObsId 2480

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02481
title: Chandra X-ray Observatory ObsId 2481

description: SOLVING THE PUZZLE OF COMETARY X-RAY ORIGIN: OBSERVATIONS OF COMET 10P/TEMPEL 2
DOI: 10.25574/02487
title: Chandra X-ray Observatory ObsId 2487

description: ACIS DARK CURRENT CALIBARTION ON DARK MOON
DOI: 10.25574/02488
title: Chandra X-ray Observatory ObsId 2488

description: ACIS DARK CURRENT CALIBARTION ON DARK MOON
DOI: 10.25574/02489
title: Chandra X-ray Observatory ObsId 2489

description: ACIS DARK CURRENT CALIBARTION ON DARK MOON
DOI: 10.25574/02490
title: Chandra X-ray Observatory ObsId 2490

description: ACIS DARK CURRENT CALIBARTION ON DARK MOON
DOI: 10.25574/02491
title: Chandra X-ray Observatory ObsId 2491

description: DOPPLER-SHIFTED EMISSION LINES FROM THE JETS OF 1E1740.7-2942?