14 research outputs found
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Recreating Winchendon Village: A Distinct Destination in Toy Town (Winchendon, MA)
The goal of the Master of Regional Planning Studio is to develop a studentâs techniques for collecting, analyzing, and synthesizing spatial and non-spatial data and then presenting that collective data in a manner (i.e., report, video, presentation, and charettes) that is understandable to academics, professionals, and the public. Planning Studio allows students to integrate knowledge from coursework and research, and apply such knowledge to resolving representative planning problems. At UMASS Amherst, these problems are found in neighborhood, rural, urban, and/or regional settings.
In the fall of 2014, three local governments contracted with the MRP Studio to create separate vision plans that focused on key aspects of community revitalization. For the Town of Winchendon, the graduate student team (Carousel Consulting) created a revitalization plan that addressed declining investment and commercial activity in the Central Street corridor. As the âdowntownâ and commercial center of Winchendon, the strategy for Central Street focused on generating reinvestment through the advancement of commercial development and diversity, infill development and cohesion, place-making and branding, open space and recreation, and circulatory functionality
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Commonwealth of Massachusetts Mill Building Repurposing Pilot Project (Twist Mill - Athol, MA)
The purpose of the UMass Amherst Department of Landscape Architecture and Regional Planningâs participation in this project is to establish a redevelopment action plan that incorporates the ownershipâs clear vision for reuse of the site, proposes solutions to various obstacles that have hindered progress, and serves as a guiding model in terms of improving the feasibility of similar projects throughout the state.
The project team gathered information from a variety of resources, and conducted three distinct phases of analysis in order to complete this redevelopment action plan. The Phase I: Inventory examines the physical, regulatory, and financial context surrounding the current site in order to gauge its condition as a viable location to foster desired economic development for the region.
The Phase II: Assessment utilizes these inventory findings to identify clear challenges that impact the redevelopment potential of the site in an effort to reduce overall project roadblocks. The Phase III: Implementation provides strategies to alleviate these challenges moving forward, in the form of clear recommendations for local, regional, and state level regulatory improvements.
Phases I and II were conducted in the fall of 2013, and Phase III was conducted in the spring of 2014.
Particular thanks for guidance on this project are extended to L.P. Athol Corporation ownership, Dr. John Mullin of the UMass Amherst Center for Economic Development, State Representative Denise Andrews of the Franklin County Second District, State Senator Stephen Brewer, State Senator Stanley Rosenberg, Congressman James McGovern, and the Town of Athol
TOI-836 : a super-Earth and mini-Neptune transiting a nearby K-dwarf
Funding: TGW, ACC, and KH acknowledge support from STFC consolidated grant numbers ST/R000824/1 and ST/V000861/1, and UKSA grant ST/R003203/1.We present the discovery of two exoplanets transiting TOI-836 (TIC 440887364) using data from TESS Sector 11 and Sector 38. TOI-836 is a bright (T = 8.5 mag), high proper motion (âŒ200 mas yrâ1), low metallicity ([Fe/H]ââ0.28) K-dwarf with a mass of 0.68 ± 0.05 Mâ and a radius of 0.67 ± 0.01 Râ. We obtain photometric follow-up observations with a variety of facilities, and we use these data-sets to determine that the inner planet, TOI-836 b, is a 1.70 ± 0.07 Râ super-Earth in a 3.82 day orbit, placing it directly within the so-called âradius valleyâ. The outer planet, TOI-836 c, is a 2.59 ± 0.09 Râ mini-Neptune in an 8.60 day orbit. Radial velocity measurements reveal that TOI-836 b has a mass of 4.5 ± 0.9 Mâ, while TOI-836 c has a mass of 9.6 ± 2.6 Mâ. Photometric observations show Transit Timing Variations (TTVs) on the order of 20 minutes for TOI-836 c, although there are no detectable TTVs for TOI-836 b. The TTVs of planet TOI-836 c may be caused by an undetected exterior planet.Publisher PDFPeer reviewe
TOI-836: A super-Earth and mini-Neptune transiting a nearby K-dwarf
We present the discovery of two exoplanets transiting TOI-836 (TIC 440887364)
using data from TESS Sector 11 and Sector 38. TOI-836 is a bright (
mag), high proper motion ( mas yr), low metallicity
([Fe/H]) K-dwarf with a mass of M and a
radius of R. We obtain photometric follow-up
observations with a variety of facilities, and we use these data-sets to
determine that the inner planet, TOI-836 b, is a R
super-Earth in a 3.82 day orbit, placing it directly within the so-called
'radius valley'. The outer planet, TOI-836 c, is a R
mini-Neptune in an 8.60 day orbit. Radial velocity measurements reveal that
TOI-836 b has a mass of M , while TOI-836 c has a mass
of M. Photometric observations show Transit Timing
Variations (TTVs) on the order of 20 minutes for TOI-836 c, although there are
no detectable TTVs for TOI-836 b. The TTVs of planet TOI-836 c may be caused by
an undetected exterior planet
Two warm Neptunes transiting HIP 9618 revealed by TESS and Cheops
peer reviewedHIP 9618 (HD 12572, TOI-1471, TIC 306263608) is a bright (G = 9.0 mag) solar analogue. TESS photometry revealed the star to have two candidate planets with radii of 3.9 ± 0.044 R (HIP 9618 b) and 3.343 ± 0.039 R (HIP 9618 c). While the 20.77291 d period of HIP 9618 b was measured unambiguously, HIP 9618 c showed only two transits separated by a 680-d gap in the time series, leaving many possibilities for the period. To solve this issue, CHEOPS performed targeted photometry of period aliases to attempt to recover the true period of planet c, and successfully determined the true period to be 52.56349 d. High-resolution spectroscopy with HARPS-N, SOPHIE, and CAFE revealed a mass of 10.0 ± 3.1M for HIP 9618 b, which, according to our interior structure models, corresponds to a 6.8 ± 1.4 per cent gas fraction. HIP 9618 c appears to have a lower mass than HIP 9618 b, with a 3-sigma upper limit of 50 d, opening the door for the atmospheric characterization of warm (Teq < 750 K) sub-Neptunes
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A close-in puffy Neptune with hidden friends : the enigma of TOI 620
We present the validation of a transiting low-density exoplanet orbiting the M2.5 dwarf TOI 620 discovered by the NASA Transiting Exoplanet Survey Satellite (TESS) mission. We utilize photometric data from both TESS and ground-based follow-up observations to validate the ephemerides of the 5.09 day transiting signal and vet false-positive scenarios. High-contrast imaging data are used to resolve the stellar host and exclude stellar companions at separations âł0farcs2. We obtain follow-up spectroscopy and corresponding precise radial velocities (RVs) with multiple precision radial velocity (PRV) spectrographs to confirm the planetary nature of the transiting exoplanet. We calculate a 5Ï upper limit of MP < 7.1 Mâ and ÏP < 0.74 g cmâ3, and we identify a nontransiting 17.7 day candidate. We also find evidence for a substellar (1â20 MJ) companion with a projected separation âČ20 au from a combined analysis of Gaia, adaptive optics imaging, and RVs. With the discovery of this outer companion, we carry out a detailed exploration of the possibilities that TOI 620 b might instead be a circum-secondary planet or a pair of eclipsing binary stars orbiting the host in a hierarchical triple system. We find, under scrutiny, that we can exclude both of these scenarios from the multiwavelength transit photometry, thus validating TOI 620 b as a low-density exoplanet transiting the central star in this system. The low density of TOI 620 b makes it one of the most amenable exoplanets for atmospheric characterization, such as with the James Webb Space Telescope and Ariel, validated or confirmed by the TESS mission to date
TOI-836:A super-Earth and mini-Neptune transiting a nearby K-dwarf
We present the discovery of two exoplanets transiting TOI-836 (TIC 440887364) using data from TESS Sector 11 and Sector 38. TOI-836 is a bright (T=8.5mag), high proper motion (âŒ200 mas yrâ1), low metallicity ([Fe/H]ââ0.28) K-dwarf with a mass of 0.68±0.05 Mâ and aradius of 0.67±0.01 Râ. We obtain photometric follow-upobservations with a variety of facilities, and we use these data-sets todetermine that the inner planet, TOI-836 b, is a 1.70±0.07 Râsuper-Earth in a 3.82 day orbit, placing it directly within the so-called'radius valley'. The outer planet, TOI-836 c, is a 2.59±0.09 Râmini-Neptune in an 8.60 day orbit. Radial velocity measurements reveal thatTOI-836 b has a mass of 4.5±0.9 Mâ , while TOI-836 c has a massof 9.6±2.6 Mâ. Photometric observations show Transit TimingVariations (TTVs) on the order of 20 minutes for TOI-836 c, although there areno detectable TTVs for TOI-836 b. The TTVs of planet TOI-836 c may be caused byan undetected exterior planet