Testing general relativity with supermassive black holes using X-ray reflection spectroscopy. (arXiv:1905.08012v1 [gr-qc])

Testing general relativity with supermassive black holes using X-ray reflection spectroscopy. (arXiv:1905.08012v1 [gr-qc]) <a href="http://arxiv.org/find/gr-qc/1/au:+Abdikamalov_A/0/1/0/all/0/1">Askar B. Abdikamalov</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Ayzenberg_D/0/1/0/all/0/1">Dimitry Ayzenberg</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Bambi_C/0/1/0/all/0/1">Cosimo Bambi</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Nampalliwar_S/0/1/0/all/0/1">Sourabh Nampalliwar</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Tripathi_A/0/1/0/all/0/1">Ashutosh Tripathi</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Wong_J/0/1/0/all/0/1">Jelen Wong</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Xu_Y/0/1/0/all/0/1">Yerong Xu</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Yan_J/0/1/0/all/0/1">Jinli Yan</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Yan_Y/0/1/0/all/0/1">Yunfeng Yan</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Yang_Y/0/1/0/all/0/1">Yuchan Yang</a> In this paper, we review our current efforts to test General […]

Occurrence of Great Magnetic Storms on 6-8 March 1582. (arXiv:1905.08017v1 [astro-ph.SR])

Occurrence of Great Magnetic Storms on 6-8 March 1582. (arXiv:1905.08017v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Hattori_K/0/1/0/all/0/1">Kentaro Hattori</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hayakawa_H/0/1/0/all/0/1">Hisashi Hayakawa</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ebihara_Y/0/1/0/all/0/1">Yusuke Ebihara</a> Although knowing the occurrence frequency of severe space weather events is important for a modern society, it is insufficiently known due to the lack of magnetic or sunspot observations, before the Carrington event in 1859 […]

The effects of ionization feedback on star formation: A case study of the M16 H II region. (arXiv:1905.08030v1 [astro-ph.SR])

The effects of ionization feedback on star formation: A case study of the M16 H II region. (arXiv:1905.08030v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Xu_J/0/1/0/all/0/1">Jin-Long Xu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zavagno_A/0/1/0/all/0/1">Annie Zavagno</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yu_N/0/1/0/all/0/1">Naiping Yu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Liu_X/0/1/0/all/0/1">Xiao-Lan Liu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Xu_Y/0/1/0/all/0/1">Ye Xu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Yuan_J/0/1/0/all/0/1">Jinghua Yuan</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_C/0/1/0/all/0/1">Chuan-Peng Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_S/0/1/0/all/0/1">Si-Ju Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_G/0/1/0/all/0/1">Guo-Yin Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ning_C/0/1/0/all/0/1">Chang-Chun Ning</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ju_B/0/1/0/all/0/1">Bing-Gang Ju</a> We aim to […]

Decoding signatures of extra dimensions and estimating spin of quasars from the continuum spectrum. (arXiv:1905.08043v1 [gr-qc])

Decoding signatures of extra dimensions and estimating spin of quasars from the continuum spectrum. (arXiv:1905.08043v1 [gr-qc]) <a href="http://arxiv.org/find/gr-qc/1/au:+Banerjee_I/0/1/0/all/0/1">Indrani Banerjee</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Chakraborty_S/0/1/0/all/0/1">Sumanta Chakraborty</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+SenGupta_S/0/1/0/all/0/1">Soumitra SenGupta</a> Continuum spectrum emitted by the accretion disk around quasars hold a wealth of information regarding the strong gravitational field produced by the massive central object. Such strong gravity regime is […]

An Origin for the Angular Momentum of Molecular Cloud Cores: a Prediction from Filament Fragmentation. (arXiv:1905.08071v1 [astro-ph.GA])

An Origin for the Angular Momentum of Molecular Cloud Cores: a Prediction from Filament Fragmentation. (arXiv:1905.08071v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Misugi_Y/0/1/0/all/0/1">Yoshiaki Misugi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Inutsuka_S/0/1/0/all/0/1">Shu-ichiro Inutsuka</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Arzoumanian_D/0/1/0/all/0/1">Doris Arzoumanian</a> The angular momentum of a molecular cloud core plays a key role in star formation, since it is directly related to the outflow and the jet emanating from the […]

Long term variability of Swift J1753.5-0127]{Long term variability of Swift J1753.5-0127: X-ray spectral-temporal correlations during state transitions. (arXiv:1905.08072v1 [astro-ph.HE])

Long term variability of Swift J1753.5-0127]{Long term variability of Swift J1753.5-0127: X-ray spectral-temporal correlations during state transitions. (arXiv:1905.08072v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Bu_Q/0/1/0/all/0/1">Qingcui Bu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tao_L/0/1/0/all/0/1">Lian Tao</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lu_Y/0/1/0/all/0/1">Yu Lu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_S/0/1/0/all/0/1">Shuangnan Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zhang_L/0/1/0/all/0/1">Liang Zhang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Huang_Y/0/1/0/all/0/1">Yue Huang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_L/0/1/0/all/0/1">Li Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Qu_J/0/1/0/all/0/1">Jinlu Qu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ma_X/0/1/0/all/0/1">Xiang Ma</a> We studied the long-term evolution of the spectral-temporal correlated […]

Density jump as a function of magnetic field for collisionless shocks in pair plasmas: the perpendicular case. (arXiv:1905.08079v1 [physics.plasm-ph])

Density jump as a function of magnetic field for collisionless shocks in pair plasmas: the perpendicular case. (arXiv:1905.08079v1 [physics.plasm-ph]) <a href="http://arxiv.org/find/physics/1/au:+Bret_A/0/1/0/all/0/1">Antoine Bret</a>, <a href="http://arxiv.org/find/physics/1/au:+Narayan_R/0/1/0/all/0/1">Ramesh Narayan</a> In the absence of frequent binary collisions to isotropize the plasma, the fulfillment of the magnetohydrodynamic (MHD) Rankine-Hugoniot jump conditions by collisionless shocks is not trivial. In particular, the presence […]

Constraints on Bianchi type-I spacetime extension of the standard $Lambda$CDM model. (arXiv:1905.06949v1 [astro-ph.CO])

Constraints on Bianchi type-I spacetime extension of the standard $Lambda$CDM model. (arXiv:1905.06949v1 [astro-ph.CO]) <a href="http://arxiv.org/find/astro-ph/1/au:+Akarsu_O/0/1/0/all/0/1">Ozgur Akarsu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kumar_S/0/1/0/all/0/1">Suresh Kumar</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sharma_S/0/1/0/all/0/1">Shivani Sharma</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tedesco_L/0/1/0/all/0/1">Luigi Tedesco</a> We consider the simplest anisotropic generalization, as a correction, to the standard $Lambda$CDM model, by replacing the spatially flat Robertson-Walker metric by the Bianchi type-I metric, which brings in a […]

Extreme CO Isotopologue Line Ratios in ULIRGS: Evidence for a top-heavy IMF. (arXiv:1905.06950v1 [astro-ph.GA])

Extreme CO Isotopologue Line Ratios in ULIRGS: Evidence for a top-heavy IMF. (arXiv:1905.06950v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Brown_T/0/1/0/all/0/1">Toby Brown</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wilson_C/0/1/0/all/0/1">Christine Wilson</a> We present high-resolution ALMA observations of the C$^{18}$O, $^{13}$CO and $^{12}$CO $J$=1-0 isotopologues in 3 nearby ultra-luminous infrared galaxies (ULIRGS; Arp 220, IRAS 13120-5453, IRAS 17208-0014) and 1 nearby post-merger galaxy (NGC 2623). In all […]

Dark Matter Targets for Axion-like Particle Searches. (arXiv:1905.06952v1 [hep-ph])

Dark Matter Targets for Axion-like Particle Searches. (arXiv:1905.06952v1 [hep-ph]) <a href="http://arxiv.org/find/hep-ph/1/au:+Blinov_N/0/1/0/all/0/1">Nikita Blinov</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Dolan_M/0/1/0/all/0/1">Matthew J. Dolan</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Draper_P/0/1/0/all/0/1">Patrick Draper</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Kozaczuk_J/0/1/0/all/0/1">Jonathan Kozaczuk</a> Many existing and proposed experiments targeting QCD axion dark matter (DM) can also search for a broad class of axion-like particles (ALPs). We analyze the experimental sensitivities to electromagnetically-coupled ALP DM in different […]

Prospects for Observing the Cosmic Web in Lyman-{alpha} Emission. (arXiv:1905.06954v1 [astro-ph.GA])

Prospects for Observing the Cosmic Web in Lyman-{alpha} Emission. (arXiv:1905.06954v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Witstok_J/0/1/0/all/0/1">Joris Witstok</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Puchwein_E/0/1/0/all/0/1">Ewald Puchwein</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kulkarni_G/0/1/0/all/0/1">Girish Kulkarni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Smit_R/0/1/0/all/0/1">Renske Smit</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Haehnelt_M/0/1/0/all/0/1">Martin G. Haehnelt</a> Mapping the intergalactic medium (IGM) in Lyman-$alpha$ emission would yield unprecedented tomographic information on the large-scale distribution of baryons and potentially provide new constraints on the UV background […]

AGN in Dusty Starbursts at Z=2: Feedback Still To Kick In. (arXiv:1905.06955v1 [astro-ph.GA])

AGN in Dusty Starbursts at Z=2: Feedback Still To Kick In. (arXiv:1905.06955v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Rodighiero_G/0/1/0/all/0/1">G. Rodighiero</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Enia_A/0/1/0/all/0/1">A. Enia</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Delvecchio_I/0/1/0/all/0/1">I. Delvecchio</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lapi_A/0/1/0/all/0/1">A. Lapi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Magdis_G/0/1/0/all/0/1">G. E. Magdis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rujopakarn_W/0/1/0/all/0/1">W. Rujopakarn</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mancini_C/0/1/0/all/0/1">C. Mancini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Rodriguez_Munoz_L/0/1/0/all/0/1">L. Rodriguez-Munoz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Carraro_R/0/1/0/all/0/1">R. Carraro</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Iani_E/0/1/0/all/0/1">E. Iani</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Negrello_M/0/1/0/all/0/1">M. Negrello</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Franceschini_A/0/1/0/all/0/1">A. Franceschini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Renzini_A/0/1/0/all/0/1">A. Renzini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gruppioni_C/0/1/0/all/0/1">C. […]

A deep learning model to emulate simulations of cosmic reionization. (arXiv:1905.06958v1 [astro-ph.CO])

A deep learning model to emulate simulations of cosmic reionization. (arXiv:1905.06958v1 [astro-ph.CO]) <a href="http://arxiv.org/find/astro-ph/1/au:+Chardin_J/0/1/0/all/0/1">Jonathan Chardin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Uhlrich_G/0/1/0/all/0/1">Gr&#xe9;goire Uhlrich</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Aubert_D/0/1/0/all/0/1">Dominique Aubert</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Deparis_N/0/1/0/all/0/1">Nicolas Deparis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gillet_N/0/1/0/all/0/1">Nicolas Gillet</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ocvirk_P/0/1/0/all/0/1">Pierre Ocvirk</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lewis_J/0/1/0/all/0/1">Joseph Lewis</a> We present a deep learning model trained to emulate the radiative transfer during the epoch of cosmological reionization. CRADLE (Cosmological Reionization And […]

Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2. (arXiv:1905.06960v1 [astro-ph.GA])

Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2. (arXiv:1905.06960v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Lang_P/0/1/0/all/0/1">P. Lang</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Schinnerer_E/0/1/0/all/0/1">E. Schinnerer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Smail_I/0/1/0/all/0/1">Ian Smail</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dudzeviciute_U/0/1/0/all/0/1">U. Dudzevi&#x10d;i&#x16b;t&#x117;</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Swinbank_A/0/1/0/all/0/1">A.M. Swinbank</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Liu_D/0/1/0/all/0/1">Daizhong Liu</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Leslie_S/0/1/0/all/0/1">S. K. Leslie</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Almaini_O/0/1/0/all/0/1">O. Almaini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+An_F/0/1/0/all/0/1">Fang Xia An</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bertoldi_F/0/1/0/all/0/1">F. Bertoldi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Blain_A/0/1/0/all/0/1">A. W. Blain</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chapman_S/0/1/0/all/0/1">S. C. Chapman</a>, […]

CO Emission in Infrared-Selected Active Galactic Nuclei. (arXiv:1905.06961v1 [astro-ph.GA])

CO Emission in Infrared-Selected Active Galactic Nuclei. (arXiv:1905.06961v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Kirkpatrick_A/0/1/0/all/0/1">Allison Kirkpatrick</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Sharon_C/0/1/0/all/0/1">Chelsea Sharon</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Keller_E/0/1/0/all/0/1">Erica Keller</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pope_A/0/1/0/all/0/1">Alexandra Pope</a> In order to better understand how active galactic nuclei (AGN) effect the interstellar media of their host galaxies, we perform a meta-analysis of the CO emission for a sample of $z=0.01-4$ galaxies from the […]

Angular momentum transport by the GSF instability: nonlinear simulations at the equator. (arXiv:1905.06962v1 [astro-ph.SR])

Angular momentum transport by the GSF instability: nonlinear simulations at the equator. (arXiv:1905.06962v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Barker_A/0/1/0/all/0/1">Adrian J. Barker</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jones_C/0/1/0/all/0/1">Chris A. Jones</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tobias_S/0/1/0/all/0/1">Steven M. Tobias</a> We present an investigation into the nonlinear evolution of the Goldreich-Schubert-Fricke (GSF) instability using axisymmetric and three-dimensional simulations near the equator of a differentially rotating radiation zone. This instability […]

Broad-band X-ray analysis of local mid-infrared selected Compton-thick AGN candidates. (arXiv:1905.06964v1 [astro-ph.GA])

Broad-band X-ray analysis of local mid-infrared selected Compton-thick AGN candidates. (arXiv:1905.06964v1 [astro-ph.GA]) <a href="http://arxiv.org/find/astro-ph/1/au:+Caria_M/0/1/0/all/0/1">M.-M. La Caria</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vignali_C/0/1/0/all/0/1">C. Vignali</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lanzuisi_G/0/1/0/all/0/1">G. Lanzuisi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gruppioni_C/0/1/0/all/0/1">C. Gruppioni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pozzi_F/0/1/0/all/0/1">F. Pozzi</a> The estimate of the number and space density of obscured AGN over cosmic time still represents an open issue. While the obscured AGN population is a key […]

Magnetogenesis from rotating scalar: `a la scalar chiral magnetic effect. (arXiv:1905.06966v1 [hep-ph])

Magnetogenesis from rotating scalar: `a la scalar chiral magnetic effect. (arXiv:1905.06966v1 [hep-ph]) <a href="http://arxiv.org/find/hep-ph/1/au:+Kamada_K/0/1/0/all/0/1">Kohei Kamada</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Shin_C/0/1/0/all/0/1">Chang Sub Shin</a> The chiral magnetic effect is a phenomenon that an electric current parallel to the magnetic fields is induced in the presence of the chiral asymmetry in the fermionic system. In this article we point out that […]

When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster. (arXiv:1905.06974v1 [astro-ph.SR])

When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster. (arXiv:1905.06974v1 [astro-ph.SR]) <a href="http://arxiv.org/find/astro-ph/1/au:+Jerabkova_T/0/1/0/all/0/1">Tereza Jerabkova</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Beccari_G/0/1/0/all/0/1">Giacomo Beccari</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Boffin_H/0/1/0/all/0/1">Henri M.J. Boffin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Petr_Gotzens_M/0/1/0/all/0/1">Monika G. Petr-Gotzens</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Manara_C/0/1/0/all/0/1">Carlo F. Manara</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Moroni_P/0/1/0/all/0/1">Pier Giorgio Prada Moroni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tognelli_E/0/1/0/all/0/1">Emanuele Tognelli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+DeglInnocenti_S/0/1/0/all/0/1">Scilla Degl&#x27;Innocenti</a> The high-quality OmegaCAM photometry of the 3×3 deg around […]

GROWTH on S190426c. II. Real-Time Search for a Counterpart to the Probable Neutron Star-Black Hole Merger using an Automated Difference Imaging Pipeline for DECam. (arXiv:1905.06980v1 [astro-ph.HE])

GROWTH on S190426c. II. Real-Time Search for a Counterpart to the Probable Neutron Star-Black Hole Merger using an Automated Difference Imaging Pipeline for DECam. (arXiv:1905.06980v1 [astro-ph.HE]) <a href="http://arxiv.org/find/astro-ph/1/au:+Goldstein_D/0/1/0/all/0/1">Daniel A. Goldstein</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Andreoni_I/0/1/0/all/0/1">Igor Andreoni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Nugent_P/0/1/0/all/0/1">Peter E. Nugent</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kasliwal_M/0/1/0/all/0/1">Mansi M. Kasliwal</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Coughlin_M/0/1/0/all/0/1">Michael W. Coughlin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Anand_S/0/1/0/all/0/1">Shreya Anand</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bloom_J/0/1/0/all/0/1">Joshua S. Bloom</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Martinez_Palomera_J/0/1/0/all/0/1">Jorge Mart&#xed;nez-Palomera</a>, […]