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There is some apprehension on how to write the body of the PDF a= ttachment. The following examples keep to the Proposer Guidelines in Anonymou= s Reviews, and are meant as additional guides in crafting your own prop= osals.
Here is an example of text from a sample proposal:
Over the last five years, we have used in= frared photometry from 2MASS to compile a census of nearby ultracool M and = L dwarfs (Cruz et al, 2003; 2006). We have identified 87 L dwarfs in 80 sys= tems with nominal distances less than 20 parsecs from the Sun. This is the = first true L dwarf census =E2=80=93 a large-scale, volume-limited sample. M= ost distances are based on spectroscopic parallaxes, accurate to 20%, which= is adequate for present purposes. Fifty systems already have high-resoluti= on imaging, including our Cycle 9 and 13 snapshot programs, #8581 and #1014= 3; nine are in binary or multiple systems, including six new discoveries. W= e propose to target the remaining sources via the current pro= posal. We will combine those data with X-ray measurements made in our Cycle= 14 Chandra proposal #2095.
Here is the same text, re-worked following the anonymizing guidelines:= p>
Over the last five years, 2MASS infrared = photometry has been used to compile a census of nearby ultracool M and L dw= arfs (Cruz et al, 2003; 2006). 87 L dwarfs in 80 systems have been identifi= ed with nominal distances less than 20 parsecs from the Sun. This is the fi= rst true L dwarf census =E2=80=93 a large-scale, volume-limited sample. Mos= t distances are based on spectroscopic parallaxes, accurate to 20%, which i= s adequate for present purposes. Fifty systems already have high-resolution= imaging, including the Cycle 9 and 13 snapshot programs, #8581 and #10143;= nine are in binary or multiple systems, including six new discoveries. We = propose to target the remaining sources via the current propo= sal. Those data will be combined with Chandra X-ray measurements from progr= am #2095 (Reid, priv. comm.).
Here is another example of text from a sample proposal:
In Rogers et al. (2014), we concluded tha= t the best explanation for the dynamics of the shockwave and the spectra fr= om both the forward-shocked ISM and the reverse-shocked ejecta is that a Ty= pe Ia supernova exploded into a preexisting wind-blown cavity. This object = is the only known example of such a phenomenon, and it thus provides a uniq= ue opportunity to illuminate the nature of Type Ia supernovae and the proge= nitors. If our model from Rogers et al. (2014) is correct, then the single-= degenerate channel for SNe Ia production must exist. We propose here for a = second epoch of observations which we will compare with our first epoch obt= ained in 2007 to measure the proper motion of the shock wave.
Here is the same text, again re-worked following the anonymizing guideli= nes:
= Rogers et al. (2014) concluded that the best explanation for the dynamics o= f the shockwave and the spectra from both the forward-shocked ISM and the r= everse-shocked ejecta is that a Type Ia supernova exploded into a preexisti= ng wind-blown cavity. This object is the only known example of such a pheno= menon, and it thus provides a unique opportunity to illuminate the nature o= f Type Ia supernovae and the progenitors. If the model from Rogers et al. (= 2014) is correct, then the single-degenerate channel for SNe Ia production = must exist. We propose here f= or a second epoch of observations which we will compare with a first epoch = obtained in 2007 to measure the proper motion of the shock wave.
As further example, here's an excerpted sample from an Archival proposal= :