image image | UUID string | Image ID string | Paper DOI string | Paper Title string | Image Caption string | Image Authors string | References DOIs list | Citing DOIs list |
|---|---|---|---|---|---|---|---|---|
10.3847.2515-5172.adf191_rnaasadf191f1_102595 | rnaasadf191f1 | 10.3847/2515-5172/adf191 | Determination of the Abundance of Mercury from the Hg II Line at 5677.10 Å. XXIII. HD 90264 B (L Car) | Left: synthesis of the Hg II line at 3983.93 Å of HD 90264 B (observed spectrum in black, synthetic spectrum in red), Right: synthesis of the Hg II line at 5677.10 Å. | Authors: Richard Monier | [
"10.3847/2515-5172/ad4483"
] | [] | |
10.3847.2515-5172.ae0d80_rnaasae0d80f1_102596 | rnaasae0d80f1 | 10.3847/2515-5172/ae0d80 | Mass- and Metallicity-dependent Changes in Stellar Hydrogen Luminosity after Low-mass Brown Dwarf Engulfment | Log of stellar hydrogen luminosity over time, from the start of the simulation, for each brown dwarf mass and stellar metallicity. | Authors: Pranav Siddineni, Parker Johnson | [
"10.3847/1538-4365/acae8d",
"10.3847/1538-4357/acbdfc"
] | [] | |
10.3847.2515-5172.adf326_rnaasadf326f1_102597 | rnaasadf326f1 | 10.3847/2515-5172/adf326 | A Weak-moderate Solar Cycle 25 is Confirmed | Comparison of the temporal evolution of the last 25 observed solar cycles. The thick black line represents Solar Cycle 25, based on the observed 13 months smoothed monthly values of the sunspot number. All other solar cycles are overlaid and aligned at their respective starting points to facilitate comparison. | Authors: M. C. Gallego, A. J. P. Aparicio, V. M. S. Carrasco, J. M. Vaquero | [
"10.3847/2515-5172/acebde"
] | [] | |
10.3847.2515-5172.ae0735_rnaasae0735f1_102598 | rnaasae0735f1 | 10.3847/2515-5172/ae0735 | A Case of the Lensed AGN ULAS J081621.49+213442.65 at z ∼ 7.45 Confused with an Asteroid | (a) 88″ × 44″ UKIDSS J-band leavstack cutout from 2008 November 28. The positions of the moving object MObjHK2008-11-27 are marked with crosses. (b) Corresponding difference image between the UKIDSS J-band images of 2008 and 2007. The newly identified object is labeled MObjJ2008-11-28. (A FITS file of the full analyzed... | Authors: Ekaterina Koptelova, Chorng-Yuan Hwang | [
"10.3847/2515-5172/accb5b"
] | [] | |
10.3847.2515-5172.ae317a_rnaasae317af1_102599 | rnaasae317af1 | 10.3847/2515-5172/ae317a | No Turnover Found in Giant-Planet Occurrence Within 3 au Around Low-mass Stars | Occurrence rate of GPs, defined as ﹩dN/d{\rm{ln}}\,a﹩ (number of planets per star per unit ﹩{\rm{ln}}a﹩), as a function of semimajor axis a, in astronomical units. Left: IDEM rates and NGPPS population-synthesis predictions. Right: Median joint occurrence model (black, ﹩\frac{dN}{d{\rm{ln}}a}\propto {a}^{\beta }﹩) with... | Authors: Katherine L. Gonglewski, Galen J. Bergsten, Ilaria Pascucci, Renu Malhotra, Gijs D. Mulders, Jamie Dietrich, Kevin K. Hardegree-Ullman, Rachel B. Fernandes, Remo Burn, Christoph Mordasini | [
"10.3847/1538-3881/adf633",
"10.3847/1538-3881/ac8fea",
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] | [] | |
10.3847.2515-5172.adb584_rnaasadb584f1_102600 | rnaasadb584f1 | 10.3847/2515-5172/adb584 | Determination of the Abundance of Mercury from the Hg II Line at 5677.10 Å in Late B-type Stars. XV. HD 79158 (36 Lyncis) | Left: Comparison of the observed NARVAL I profile of 36 Lyncis in the range 4420–4500 Å (observed profile in black, synthetic spectrum in red), Right: Same comparison in the range 4510–4560 Å. | Authors: Richard Monier | [
"10.3847/2515-5172/ad4483"
] | [] | |
10.3847.2515-5172.adbbeb_rnaasadbbebf1_102601 | rnaasadbbebf1 | 10.3847/2515-5172/adbbeb | Determination of the Abundance of Mercury from the Hg II Line at 5677.10 Å in Late B-type Stars. XVI. HD 33904 (μ Lep) | Left: synthesis of the Hg II line at 5677.10 Å (observed FEROS spectrum of μ Lep in black, synthetic spectra in red) Right: synthesis of the the same line in a HARPS spectrum of μ Lep. | Authors: Richard Monier | [
"10.3847/1538-3881/acdb50",
"10.3847/2515-5172/ad4483"
] | [] | |
10.3847.2515-5172.adf059_rnaasadf059f1_102602 | rnaasadf059f1 | 10.3847/2515-5172/adf059 | Palomar and Apache Point Spectrophotometry of Interstellar Comet 3I/ATLAS | Left: Palomar and Apache Point imaging and spectroscopy. 3I/ATLAS has a red spectrum in the visible that becomes more neutral at longer wavelengths. Right: comparison between our combined and binned 3I/ATLAS spectrum and 1I from A. Fitzsimmons et al. (2018) and 2I from J. de León et al. (2020). 3I/ATLAS appears roughly... | Authors: Matthew Belyakov, Christoffer Fremling, Matthew J. Graham, Bryce T. Bolin, Mukremin Kilic, Gracyn Jewett, Carey M. Lisse, Carl Ingebretsen, M. Ryleigh Davis, Ian Wong | [
"10.3847/2041-8213/adf49a"
] | [
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10.3847.2515-5172.adef49_rnaasadef49f1_102603 | rnaasadef49f1 | 10.3847/2515-5172/adef49 | Updated Mutual Inclination Measurement for 14 Her b and c | Panel (a): Best-fit to RVs of various instruments. Panel (b): RV residuals. Panel (c): Best-fit to Hipparcos, Gaia DR2 and DR3 astrometry. The black thick line denotes the optimal orbit of 14 Her, while the arrow indicates its direction of motion. Panel (d): Zoom in on the rectangle region of panel (c) where depicts th... | Authors: Guang-Yao Xiao, Fabo Feng | [
"10.3847/2041-8213/ade30f",
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] | [] | |
10.3847.2515-5172.adf83e_rnaasadf83ef1_102604 | rnaasadf83ef1 | 10.3847/2515-5172/adf83e | Peculiar Stellar Ages of the Peculiar Dwarf Galaxy NGC 5474 | Top left: the broadband B image of NGC 5474 (J. C. Mihos et al. 2013). Top right: the narrowband continuum-subtracted Hβ image; white indicates emission and black indicates absorption. In both panels, the blue circle defines the bulge, the inner green circle defines the main disk and the outer circle defines the outer ... | Authors: Liv Moody, Ray Garner | [
"10.3847/1538-4357/aca27a",
"10.3847/1538-4357/ad8b1e"
] | [] | |
10.3847.2515-5172.adaf90_rnaasadaf90f1_102605 | rnaasadaf90f1 | 10.3847/2515-5172/adaf90 | XRISM Observations of the Cooling Flow Cluster A2029 Support Heating by Mixing | A temperature map with radio contours of A2029 adapted from T. E. Clarke et al. (2004). The temperature scale is by the color bar in keV; 1″ corresponds to 1.45 kpc. I draw the approximate distance to which the turbulence can carry hot gas within one (black) and two (red) cooling times, where τcool(0) = 6 × 107 yr. | Authors: Noam Soker | [
"10.3847/2041-8213/ada7cd"
] | [] | |
10.3847.2515-5172.adcd6c_rnaasadcd6cf1_102606 | rnaasadcd6cf1 | 10.3847/2515-5172/adcd6c | Discovery of Photodissociation Region in Overlapping Galaxy Pair VV 191 with HST and JWST | Top left: the AV map of the PDR. Top right: the ﹩{R}_{\widetilde{VI}}﹩ (see Equation (2)) map. Bottom left: the JWST F356W image of the PDR, circled in gold. Bottom right: the ICA map from the JWST F356W and F444W filters. On the AV and ICA maps, the HST F336W intensity is overlaid as a contour where: cyan = 0.003 coun... | Authors: Clayton D. Robertson, Benne W. Holwerda, Jessica M. Berkheimer, Kyle W. Cook, William C. Keel, Rogier A. Windhorst | [
"10.3847/2041-8213/ad0387",
"10.3847/1538-3881/ad39c4",
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] | [] | |
10.3847.2515-5172.ae0293_rnaasae0293f1_102607 | rnaasae0293f1 | 10.3847/2515-5172/ae0293 | SPHEREx Discovery of Strong Water Ice Absorption and an Extended Carbon Dioxide Coma in 3I/ATLAS | (a) SPHEREx 0.75–5.0 μm 2 pixel radius aperture spectrophotometry (left) and solar spectrum corrected reflectance (right) for 3I. Red arrows denote possible significant background contamination due to known background sources. The arrows start at the measured flux+1σ. For the reflectance, the NASA-IRTF/SpeX 0.7–2.5 μm ... | Authors: C. M. Lisse, Y. P. Bach, S. Bryan, B. P. Crill, A. Cukierman, O. Doré, B. Fabinsky, A. Faisst, P. M. Korngut, G. Melnick, Z. Rustamkulov, V. Tolls, M. Werner, M. L. Sitko, C. Champagne, M. Connelley, J. P. Emery, Y. R. Fernandez, B. Yang | [
"10.3847/PSJ/ac6097",
"10.3847/2041-8213/adf8d8",
"10.3847/1538-4365/ae04cc",
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"10.3847/2041-8213/ae08a7",
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"10.3847/2041-8213/ae1232",
"10.3847/1538-4357/ae11b2"
] | |
10.3847.2515-5172.ae031c_rnaasae031cf1_102608 | rnaasae031cf1 | 10.3847/2515-5172/ae031c | Mapping Gamma-Ray Bursts: Distinguishing Progenitor Systems Through Machine Learning | (a) Top left: GRBs with known radio afterglow classification; radio-bright GRBs are shown in gold, radio-dark in navy. (b) Top right: low-luminosity GRBs (llGRBs) with L < 1049 erg s−1, overlaid in purple (c) Bottom: continuous gradient of T90 durations for all 2511 GRBs; the longest duration GRBs appear to cluster in ... | Authors: Sharleen N. Espinoza, Nicole M. Lloyd-Ronning, Michela Negro, Roseanne M. Cheng, Nicoló Cibrario | [
"10.3847/1538-4357/ae04e7"
] | [] | |
10.3847.2515-5172.ae0c9e_rnaasae0c9ef1_102609 | rnaasae0c9ef1 | 10.3847/2515-5172/ae0c9e | A Refined Orbital Ephemeris for the Intermediate Polar FO Aquarii and Evidence for a Period Derivative | Left: The dark points show one of the recent light curves of a FO Aqr obtained from the SLKT. This light curve covers approximately one binary orbit, while the rapid modulation results from the spinning white dwarf. The solid line plotted on the points is a light curve model constructed from L–S analysis. The differenc... | Authors: Peter Garnavich, Jordan Tweddale, Colin Littlefield | [
"10.3847/2515-5172/ac9bf7"
] | [] | |
10.3847.2515-5172.ae1448_rnaasae1448f1_102610 | rnaasae1448f1 | 10.3847/2515-5172/ae1448 | Comparison of Australasian Tektites with Australasian Microtektites and BeLaU Spherules Recovered from the Ocean | Panel (a) Primitive-mantle normalized (using W. F. McDonough & S. S. Sun 1995 values) elemental compositions of Australasian tektites compared to the UCC (R. L. Rudnick & S. Gao 2014), arranged in order of most incompatible to most compatible elements. Panel (b): The UCC-normalized elemental patterns of the individual ... | Authors: Eugenia Hyung, Emma Levy, Loralei Cook, Stein B. Jacobsen, Abraham Loeb, Jayden Squire, Juraj Farkas | [
"10.3847/1538-4357/ac8eac"
] | [] | |
10.3847.2515-5172.ae06a2_rnaasae06a2f1_102612 | rnaasae06a2f1 | 10.3847/2515-5172/ae06a2 | JAM 1: Discovery of a New Candidate Evolved Planetary Nebula in Deep [O III] and Hα Imaging | Discovery images of the candidate planetary nebula JAM 1. | Authors: J. A. Manuel, D. Jones, M. Santander-García | [
"10.3847/2515-5172/acaf7e",
"10.3847/1538-3881/adf3af"
] | [] | |
10.3847.2515-5172.adde46_rnaasadde46f1_102613 | rnaasadde46f1 | 10.3847/2515-5172/adde46 | Modeling Supernova 2023ixf: Lightcurve Degeneracies and Morphological Differences | Left: Families for SN 2023ixf: Mej(top), Menv(middle), and ﹩{E}_{{\rm{\exp }}}﹩(bottom) as a function of R, shading the 11% modeling uncertainty (GBP19). The GB20 stellar model grid is overlaid, with color indicating MZAMS from 10 to 25M⊙ (lighter colors = lower MZAMS). Upper Right: Lightcurve for the explosion of an M... | Authors: Shannon Forde, Jared A. Goldberg | [
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10.3847.2515-5172.adbbe9_rnaasadbbe9f1_102614 | rnaasadbbe9f1 | 10.3847/2515-5172/adbbe9 | SKYSURF-7: Exploring PSF Contamination in Diffuse Sky Measurements with HST | Comparison of the difference between recovered and input sky-SB as a function of the sky-SB level for a modeled Gaussian PSF, and an empirical HST PSF. Each data point represents a single image. The blue triangles represent realistic HST PSF data, and the red squares represent the modeled data. We calculate the PSF lea... | Authors: Logan R. Conrad, Rosalia O'Brien, Delondrae Carter, Alex Pigarelli, Rogier A. Windhorst, Timothy Carleton, Seth H. Cohen, Rolf A. Jansen, Rafael Ortiz | [
"10.3847/1538-4357/ad7798",
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10.3847.2515-5172.adbca2_rnaasadbca2f1_102615 | rnaasadbca2f1 | 10.3847/2515-5172/adbca2 | Upper Limits on GeV Gamma-Ray Flux from the Ultra-long Period Neutron Star PSR J0901−4046 | The gamma-ray luminosity vs. spin-down power of PSR J0901−4046 (upper limit) and the third Fermi pulsar catalog (D. A. Smith et al. 2023). | Authors: Anne Duerr, Henrike Fleischhack, David Kieda | [
"10.3847/1538-4357/acee67",
"10.3847/1538-4365/ac6751"
] | [] | |
10.3847.2515-5172.adc4e7_rnaasadc4e7f1_102616 | rnaasadc4e7f1 | 10.3847/2515-5172/adc4e7 | Apparent Change in Comet 103P/Hartley 2’s Rotation Period During 2023/2024 Measured via Aperture Photometry | Top: Calibrated apparent magnitude in a 5000 km radius aperture using the green filter. The size of points approximately corresponds to the average uncertainty of a magnitude estimate (2σ level). The line represents a model curve ﹩m=14.2+5{\rm{log}}(\Delta )+4.5\ast 2.5{\rm{log}}({r}_{{\rm{H}}})﹩ where Δ is geocentric ... | Authors: Thomas Lehmann | [] | [
"10.3847/PSJ/ae018e"
] | |
10.3847.2515-5172.addac5_rnaasaddac5f1_102617 | rnaasaddac5f1 | 10.3847/2515-5172/addac5 | Kast Optical Spectra of Unclassified Stars Within 20 pc of the Sun | (a) Gaia-2MASS color–magnitude diagram for our sample, with symbol colors indicating spectral type. Median errors shown are σG−J = 0.02 and ﹩{\sigma }_{{M}_{G}}﹩ = 0.004. (b) Kast spectrum of UPM J1425+2540 (black line) compared to its best-fit M7 template (magenta line), with main spectral features labeled. (c) Distri... | Authors: Marylin Loritsch, Adam Burgasser, Madison Fierro, Emma Softich, Christopher Theissen, Preethi Karpoor, Chih-Chun Hsu, Roman Gerasimov | [
"10.3847/1538-4365/ad24e2",
"10.3847/1538-4365/ac9b28"
] | [] | |
10.3847.2515-5172.ae3177_rnaasae3177f1_102618 | rnaasae3177f1 | 10.3847/2515-5172/ae3177 | Determination of the Abundance of Mercury from the Hg II Line at 5677.10 Å in Late B-type Stars. XXVI. HD 173524 B (46 Dra B) | Left: Synthesis of the Hg II line at 5677.10 for 46 Dra B (observed spectrum in black, synthetic in red) Right: Synthesis of the Pt II line at 4514.17 Å. | Authors: Richard Monier | [
"10.3847/2515-5172/ad4483",
"10.3847/2515-5172/ad76b1"
] | [] | |
10.3847.2515-5172.ae2120_rnaasae2120f1_102619 | rnaasae2120f1 | 10.3847/2515-5172/ae2120 | Detectability of Dust and Ion Tails of Interstellar Comet 3I/ATLAS by Europa Clipper | Simulated dust and pickup ion tails of interstellar comet 3I/ATLAS at various epochs along its trajectory (panels (a) and (b)). The views from the Earth (c) and the Europa Clipper (d) on 2025 November 5th are generated for future comparison with actual observations. The orbits of Mars, the Europa Clipper, and Jupiter a... | Authors: Hsiang-Wen Hsu, Jan Deca, Mihaly Horanyi, Sascha Kempf, Corey J. Cochrane, Xianzhe Jia, Cynthia B. Phillips | [
"10.3847/2041-8213/adfd4d",
"10.3847/2515-5172/ae109f",
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10.3847.2515-5172.ae23c8_rnaasae23c8f1_102620 | rnaasae23c8f1 | 10.3847/2515-5172/ae23c8 | Tracking the Activity of the Interstellar Object 3I/ATLAS through Its Perihelion | 3I/ATLAS magnitude data from a variety of sources, together with the November 6th prediction models in Equations (3) and (4). | Authors: T. Marshall Eubanks, Craig E. DeForest, Kevin J. Walsh, Simon Porter, Thomas Lehmann, Bruce G. Bills, Adam Hibberd, W. Paul Blase, Andreas M. Hein, Robert G. Kennedy, Adrien Coffinet, Pierre Kervella, Carlos Gomez de Olea Ballester | [
"10.3847/2041-8213/ae0647"
] | [] | |
10.3847.2515-5172.ae2a22_rnaasae2a22f1_102621 | rnaasae2a22f1 | 10.3847/2515-5172/ae2a22 | An SMA Survey of UV-driven Chemical Tracers in Transition Disks | Top: disk-integrated spectra extracted using Keplerian masks. Bottom: violin plots of distance-normalized CN and HCO+ fluxes sub-divided by the presence and radial size of dust cavities. Points are individual measurements from our SMA data and the literature. Black bars show the interquartile range, and violin widths a... | Authors: Shantanusinh Parmar, Charles J. Law | [
"10.3847/1538-3881/ad26ff",
"10.3847/2041-8213/adc43b"
] | [] | |
10.3847.2515-5172.ae2a24_rnaasae2a24f1_102622 | rnaasae2a24f1 | 10.3847/2515-5172/ae2a24 | Evidence for No Orbital Decay in the Hot Jupiter XO-3b from Transit-timing Analysis | Transit time deviation plot of XO-3b with data from all sources (left) and Spitzer and TESS only (right), with quadratic and linear fit models. | Authors: Jinyi Zhou | [
"10.3847/1538-4365/ac545b",
"10.3847/1538-4365/ac3a10",
"10.3847/1538-4365/ac9da4"
] | [] | |
10.3847.2515-5172.ae1a66_rnaasae1a66f1_102623 | rnaasae1a66f1 | 10.3847/2515-5172/ae1a66 | High-spectral Resolution, Multi-wavelength Center-to-limb Observations of the Sun | GONG Hα full-disk image obtained at 10:49:11 UT. The grayscale insert is an Hα line-core VTT drift scan image taken at 10:48:53 UT (top-left). Spectroheliograms were taken at seven positions along the Hα line, and the labels to the right indicate the wavelength offset from the line center (top-right). The Hα quiet-Sun ... | Authors: Meetu Verma, Carsten Denker, Alexander G. M. Pietrow, Robert Kamlah, Dominique J. M. Petit dit de la Roche | [] | [
"10.3847/2515-5172/ae230b"
] | |
10.3847.2515-5172.ae1ae5_rnaasae1ae5f1_102624 | rnaasae1ae5f1 | 10.3847/2515-5172/ae1ae5 | Further Identification of δ Scuti, γ Doradus Stars, and Eclipsing Binaries with TESS | Examples of newly identified δ Sct, γ Dor stars and hybrid pulsators. | Authors: Ai-Ying Zhou | [
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10.3847.2515-5172.adbf14_rnaasadbf14f1_102625 | rnaasadbf14f1 | 10.3847/2515-5172/adbf14 | Variability Census of Legacy Catalogs. IV. 3600+ New δ Scuti and γ Doradus Stars | Example TESS light curves and periodograms of newly identified: γ Dor stars (top two rows: HD 49152, HD 52087), δ Sct-γ Dor hybrid (rows 3–4: TYC 1854-93-1, HD 281579), eclipsing binaries with δ Sct (rows 5–6: HD 355359, HD 292868A) and γ Dor (bottom row: HD 337051, HD 290580) primary components. | Authors: Ai-Ying Zhou | [
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10.3847.2515-5172.adc12f_rnaasadc12ff1_102626 | rnaasadc12ff1 | 10.3847/2515-5172/adc12f | IAU CPS Satellite Optical Brightness Recommendation: Rationale | Comparison between (1) the IAU CPS recommendation based on the altitude ratio approximation and (2) the full expression using rates. The approximation is favored for the recommendation due to its simplicity. | Authors: Aaron C. Boley, Richard Green, Meredith L. Rawls, Siegfried Eggl | [] | [
"10.3847/1538-3881/adfbef"
] | |
10.3847.2515-5172.adc453_rnaasadc453f1_102627 | rnaasadc453f1 | 10.3847/2515-5172/adc453 | Observations and Characterization of the New Active Centaur 2023 RS61 | Left: cropped archival Pan-STARRS1 images taken on (Top) 2017 September 21 in w-band recalibrated against G/Gaia-DR2 with brightness G ∼ 23.5, and on (Bottom) 2017 October 10 in i-band, with G ∼ 19.1 during an apparent outburst. Right blue panels display data taken on 2025 January 2 with LDT in SDSS ﹩{r}^{{\prime} }﹩... | Authors: Eva Lilly, Charles A. Schambeau, Audrey Thirouin, Peter Jevčák, Robert Weryk, Richard J. Wainscoat | [] | [
"10.3847/2515-5172/ae122b"
] | |
10.3847.2515-5172.adc25f_rnaasadc25ff1_102628 | rnaasadc25ff1 | 10.3847/2515-5172/adc25f | Prediction and Observation of a Stellar Occultation by Haumea’s Satellite Namaka | Predictions of the stellar occultations by (a) Haumea and (b) Namaka. Solid blue lines denote the estimated diameters of the objects and dashed red lines show the 1σ uncertainties. Panel (c) presents the normalized occultation light curve, and panel (d) presents the on-sky projection of the chords for Haumea and Namaka... | Authors: Flavia L. Rommel, Benjamin C. N. Proudfoot, Bryan J. Holler, Jose L. Ortiz, Estela Fernández-Valenzuela | [
"10.3847/PSJ/ad26e9",
"10.3847/PSJ/acdd5f"
] | [] |